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Magnetism
Magnetism
from Wikipedia
The shape of a bar magnet's magnetic field is revealed by the orientation of iron filings sprinkled on the table around it.

Magnetism is the class of physical attributes that occur through a magnetic field, which allows objects to attract or repel each other. Because both electric currents and magnetic moments of elementary particles give rise to a magnetic field, magnetism is one of two aspects of electromagnetism.

The most familiar effects occur in ferromagnetic materials, which are strongly attracted by magnetic fields and can be magnetized to become permanent magnets, producing magnetic fields themselves. Demagnetizing a magnet is also possible. Only a few substances are ferromagnetic; the most common ones are iron, cobalt, nickel, and their alloys.

All substances exhibit some type of magnetism. Magnetic materials are classified according to their bulk susceptibility.[1] Ferromagnetism is responsible for most of the effects of magnetism encountered in everyday life, but there are actually several types of magnetism. Paramagnetic substances, such as aluminium and oxygen, are weakly attracted to an applied magnetic field; diamagnetic substances, such as copper and carbon, are weakly repelled; while antiferromagnetic materials, such as chromium, have a more complex relationship with a magnetic field.[vague] The force of a magnet on paramagnetic, diamagnetic, and antiferromagnetic materials is usually too weak to be felt and can be detected only by laboratory instruments, so in everyday life, these substances are often described as non-magnetic.

The strength of a magnetic field always decreases with distance from the magnetic source,[2] though the exact mathematical relationship between strength and distance varies. Many factors can influence the magnetic field of an object including the magnetic moment of the material, the physical shape of the object, both the magnitude and direction of any electric current present within the object, and the temperature of the object.

History

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Lodestone, a natural magnet, attracting iron nails. Ancient humans discovered the property of magnetism from lodestone.
An illustration from Gilbert's 1600 De Magnete showing one of the earliest methods of making a magnet. A blacksmith holds a piece of red-hot iron in a north–south direction and hammers it as it cools. The magnetic field of the Earth aligns the domains, leaving the iron a weak magnet.
Drawing of a medical treatment using magnetic brushes. Charles Jacque 1843, France.

Magnetism was first discovered in the ancient world when people noticed that lodestones, naturally magnetized pieces of the mineral magnetite, could attract iron.[3] The word magnet comes from the Greek term μαγνῆτις λίθος magnētis lithos,[4] "the Magnesian stone, lodestone".[5] In ancient Greece, Aristotle attributed the first of what could be called a scientific discussion of magnetism to the philosopher Thales of Miletus, who lived from about 625 BCE to about 545 BCE.[6] The ancient Indian medical text Sushruta Samhita describes using magnetite to remove arrows embedded in a person's body.[7]

In ancient China, the earliest literary reference to magnetism lies in a 4th-century BCE book named after its author, Guiguzi.[8] The 2nd-century BCE annals, Lüshi Chunqiu, also notes: "The lodestone makes iron approach; some (force) is attracting it."[9] The earliest mention of the attraction of a needle is in a 1st-century work Lunheng (Balanced Inquiries): "A lodestone attracts a needle."[10] The 11th-century Chinese scientist Shen Kuo was the first person to write—in the Dream Pool Essays—of the magnetic needle compass and that it improved the accuracy of navigation by employing the astronomical concept of true north. By the 12th century, the Chinese were known to use the lodestone compass for navigation. They sculpted a directional spoon from lodestone in such a way that the handle of the spoon always pointed south.

Alexander Neckam, by 1187, was the first in Europe to describe the compass and its use for navigation. In 1269, Peter Peregrinus de Maricourt wrote the Epistola de magnete, the first extant treatise describing the properties of magnets. In 1282, the properties of magnets and the dry compasses were discussed by Al-Ashraf Umar II, a Yemeni physicist, astronomer, and geographer.[11]

Leonardo Garzoni's only extant work, the Due trattati sopra la natura, e le qualità della calamita (Two treatises on the nature and qualities of the magnet), is the first known example of a modern treatment of magnetic phenomena. Written in years near 1580 and never published, the treatise had a wide diffusion. In particular, Garzoni is referred to as an expert in magnetism by Niccolò Cabeo, whose Philosophia Magnetica (1629) is just a re-adjustment of Garzoni's work. Garzoni's treatise was known also to Giovanni Battista Della Porta.

In 1600, William Gilbert published his De Magnete, Magneticisque Corporibus, et de Magno Magnete Tellure (On the Magnet and Magnetic Bodies, and on the Great Magnet the Earth). In this work he describes many of his experiments with his model earth called the terrella. From his experiments, he concluded that the Earth was itself magnetic and that this was the reason compasses pointed north whereas, previously, some believed that it was the pole star Polaris or a large magnetic island on the north pole that attracted the compass.

An understanding of the relationship between electricity and magnetism began in 1819 with work by Hans Christian Ørsted, a professor at the University of Copenhagen, who discovered, by the accidental twitching of a compass needle near a wire, that an electric current could create a magnetic field. This landmark experiment is known as Ørsted's Experiment. Jean-Baptiste Biot and Félix Savart, both of whom in 1820 came up with the Biot–Savart law giving an equation for the magnetic field from a current-carrying wire. Around the same time, André-Marie Ampère carried out numerous systematic experiments and discovered that the magnetic force between two DC current loops of any shape is equal to the sum of the individual forces that each current element of one circuit exerts on each other current element of the other circuit.

In 1831, Michael Faraday discovered that a time-varying magnetic flux induces a voltage through a wire loop. In 1835, Carl Friedrich Gauss hypothesized, based on Ampère's force law in its original form, that all forms of magnetism arise as a result of elementary point charges moving relative to each other.[12] Wilhelm Eduard Weber advanced Gauss's theory to Weber electrodynamics.

From around 1861, James Clerk Maxwell synthesized and expanded many of these insights into Maxwell's equations, unifying electricity, magnetism, and optics into the field of electromagnetism. However, Gauss's interpretation of magnetism is not fully compatible with Maxwell's electrodynamics. In 1905, Albert Einstein used Maxwell's equations in motivating his theory of special relativity,[13] requiring that the laws hold true in all inertial reference frames. Gauss's approach of interpreting the magnetic force as a mere effect of relative velocities thus found its way back into electrodynamics to some extent.

Electromagnetism has continued to develop into the 21st century, being incorporated into the more fundamental theories of gauge theory, quantum electrodynamics, electroweak theory, and finally the Standard Model.

Sources

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Magnetism, at its root, arises from three sources:

  1. Electric current
  2. Spin magnetic moments of elementary particles
  3. Changing electric fields

The magnetic properties of materials are mainly due to the magnetic moments of their atoms' orbiting electrons. The magnetic moments of the nuclei of atoms are typically thousands of times smaller than the electrons' magnetic moments, so they are negligible in the context of the magnetization of materials. Nuclear magnetic moments are nevertheless very important in other contexts, particularly in nuclear magnetic resonance (NMR) and magnetic resonance imaging (MRI).

Ordinarily, the enormous number of electrons in a material are arranged such that their magnetic moments (both orbital and intrinsic) cancel out. This is due, to some extent, to electrons combining into pairs with opposite intrinsic magnetic moments as a result of the Pauli exclusion principle (see electron configuration), and combining into filled subshells with zero net orbital motion. In both cases, the electrons preferentially adopt arrangements in which the magnetic moment of each electron is canceled by the opposite moment of another electron. Moreover, even when the electron configuration is such that there are unpaired electrons and/or non-filled subshells, it is often the case that the various electrons in the solid will contribute magnetic moments that point in different, random directions so that the material will not be magnetic.

Sometimes—either spontaneously, or owing to an applied external magnetic field—each of the electron magnetic moments will be, on average, lined up. A suitable material can then produce a strong net magnetic field.

The magnetic behavior of a material depends on its structure, particularly its electron configuration, for the reasons mentioned above, and also on the temperature. At high temperatures, random thermal motion makes it more difficult for the electrons to maintain alignment.

Types

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Hierarchy of types of magnetism.[14]

Diamagnetism

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Diamagnetism appears in all materials and is the tendency of a material to oppose an applied magnetic field, and therefore, to be repelled by a magnetic field. However, in a material with paramagnetic properties (that is, with a tendency to enhance an external magnetic field), the paramagnetic behavior dominates.[15] Thus, despite its universal occurrence, diamagnetic behavior is observed only in a purely diamagnetic material. In a diamagnetic material, there are no unpaired electrons, so the intrinsic electron magnetic moments cannot produce any bulk effect. In these cases, the magnetization arises from the electrons' orbital motions, which can be understood classically as follows:

When a material is put in a magnetic field, the electrons circling the nucleus will experience, in addition to their Coulomb attraction to the nucleus, a Lorentz force from the magnetic field. Depending on which direction the electron is orbiting, this force may increase the centripetal force on the electrons, pulling them in towards the nucleus, or it may decrease the force, pulling them away from the nucleus. This effect systematically increases the orbital magnetic moments that were aligned opposite the field and decreases the ones aligned parallel to the field (in accordance with Lenz's law). This results in a small bulk magnetic moment, with an opposite direction to the applied field.

This description is meant only as a heuristic; the Bohr–Van Leeuwen theorem shows that diamagnetism is impossible according to classical physics, and that a proper understanding requires a quantum-mechanical description.

All materials undergo this orbital response. However, in paramagnetic and ferromagnetic substances, the diamagnetic effect is overwhelmed by the much stronger effects caused by the unpaired electrons.

Paramagnetism

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In a paramagnetic material there are unpaired electrons; i.e., atomic or molecular orbitals with exactly one electron in them. While paired electrons are required by the Pauli exclusion principle to have their intrinsic ('spin') magnetic moments pointing in opposite directions, causing their magnetic fields to cancel out, an unpaired electron is free to align its magnetic moment in any direction. When an external magnetic field is applied, these magnetic moments will tend to align themselves in the same direction as the applied field, thus reinforcing it.

Ferromagnetism

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A ferromagnet, like a paramagnetic substance, has unpaired electrons. However, in addition to the electrons' intrinsic magnetic moment's tendency to be parallel to an applied field, there is also in these materials a tendency for these magnetic moments to orient parallel to each other to maintain a lowered-energy state. Thus, even in the absence of an applied field, the magnetic moments of the electrons in the material spontaneously line up parallel to one another.

Every ferromagnetic substance has its own individual temperature, called the Curie temperature, or Curie point, above which it loses its ferromagnetic properties. This is because the thermal tendency to disorder overwhelms the energy-lowering due to ferromagnetic order.

Ferromagnetism only occurs in a few substances; common ones are iron, nickel, cobalt, their alloys, and some alloys of rare-earth metals.

Magnetic domains

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Magnetic domains boundaries (white lines) in ferromagnetic material (black rectangle)
Effect of a magnet on the domains

The magnetic moments of atoms in a ferromagnetic material cause them to behave something like tiny permanent magnets. They stick together and align themselves into small regions of more or less uniform alignment called magnetic domains or Weiss domains. Magnetic domains can be observed with a magnetic force microscope to reveal magnetic domain boundaries that resemble white lines in the sketch. There are many scientific experiments that can physically show magnetic fields.

When a domain contains too many molecules, it becomes unstable and divides into two domains aligned in opposite directions so that they stick together more stably.

When exposed to a magnetic field, the domain boundaries move, so that the domains aligned with the magnetic field grow and dominate the structure (dotted yellow area), as shown at the left. When the magnetizing field is removed, the domains may not return to an unmagnetized state. This results in the ferromagnetic material's being magnetized, forming a permanent magnet.

When magnetized strongly enough that the prevailing domain overruns all others to result in only one single domain, the material is magnetically saturated. When a magnetized ferromagnetic material is heated to the Curie point temperature, the molecules are agitated to the point that the magnetic domains lose the organization, and the magnetic properties they cause cease. When the material is cooled, this domain alignment structure spontaneously returns, in a manner roughly analogous to how a liquid can freeze into a crystalline solid.

Antiferromagnetism

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Antiferromagnetic ordering

In an antiferromagnet, unlike a ferromagnet, there is a tendency for the intrinsic magnetic moments of neighboring valence electrons to point in opposite directions. When all atoms are arranged in a substance so that each neighbor is anti-parallel, the substance is antiferromagnetic. Antiferromagnets have a zero net magnetic moment because adjacent opposite moment cancels out, meaning that no field is produced by them. Antiferromagnets are less common compared to the other types of behaviors and are mostly observed at low temperatures. In varying temperatures, antiferromagnets can be seen to exhibit diamagnetic and ferromagnetic properties.

In some materials, neighboring electrons prefer to point in opposite directions, but there is no geometrical arrangement in which each pair of neighbors is anti-aligned. This is called a canted antiferromagnet or spin ice and is an example of geometrical frustration.

Ferrimagnetism

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Ferrimagnetic ordering

Like ferromagnetism, ferrimagnets retain their magnetization in the absence of a field. However, like antiferromagnets, neighboring pairs of electron spins tend to point in opposite directions. These two properties are not contradictory, because in the optimal geometrical arrangement, there is more magnetic moment from the sublattice of electrons that point in one direction, than from the sublattice that points in the opposite direction.

Most ferrites are ferrimagnetic. The first discovered magnetic substance, magnetite, is a ferrite and was originally believed to be a ferromagnet; Louis Néel disproved this, however, after discovering ferrimagnetism.

Superparamagnetism

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Magnetic orders: comparison between ferro, antiferro and ferrimagnetism

When a ferromagnet or ferrimagnet is sufficiently small, it acts like a single magnetic spin that is subject to Brownian motion. Its response to a magnetic field is qualitatively similar to the response of a paramagnet, but much larger.

Nagaoka magnetism

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Japanese physicist Yosuke Nagaoka conceived of a type of magnetism in a square, two-dimensional lattice where every lattice node had one electron. If one electron was removed under specific conditions, the lattice's energy would be minimal only when all electrons' spins were parallel.

A variation on this was achieved experimentally by arranging the atoms in a triangular moiré lattice of molybdenum diselenide and tungsten disulfide monolayers. Applying a weak magnetic field and a voltage led to ferromagnetic behavior when 100–150% more electrons than lattice nodes were present. The extra electrons delocalized and paired with lattice electrons to form doublons. Delocalization was prevented unless the lattice electrons had aligned spins. The doublons thus created localized ferromagnetic regions. The phenomenon took place at 140 millikelvins.[16]

Other types of magnetism

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Electromagnet

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An electromagnet attracts paper clips when current is applied, creating a magnetic field. The electromagnet loses them when current and magnetic field are removed.

An electromagnet is a type of magnet in which the magnetic field is produced by an electric current.[17] The magnetic field disappears when the current is turned off. Electromagnets usually consist of a large number of closely spaced turns of wire that create the magnetic field. The wire turns are often wound around a magnetic core made from a ferromagnetic or ferrimagnetic material such as iron; the magnetic core concentrates the magnetic flux and makes a more powerful magnet.

The main advantage of an electromagnet over a permanent magnet is that the magnetic field can be quickly changed by controlling the amount of electric current in the winding. However, unlike a permanent magnet that needs no power, an electromagnet requires a continuous supply of current to maintain the magnetic field.

Electromagnets are widely used as components of other electrical devices, such as motors, generators, relays, solenoids, loudspeakers, hard disks, MRI machines, scientific instruments, and magnetic separation equipment. Electromagnets are also employed in industry for picking up and moving heavy iron objects such as scrap iron and steel.[18] Electromagnetism was discovered in 1820.[19]

Magnetism, electricity, and special relativity

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As a consequence of Einstein's theory of special relativity, electricity and magnetism are fundamentally interlinked. Both magnetism lacking electricity, and electricity without magnetism, are inconsistent with special relativity, due to such effects as length contraction, time dilation, and the fact that the magnetic force is velocity-dependent. However, when both electricity and magnetism are taken into account, the resulting theory (electromagnetism) is fully consistent with special relativity.[13][20] In particular, a phenomenon that appears purely electric or purely magnetic to one observer may be a mix of both to another, or more generally the relative contributions of electricity and magnetism are dependent on the frame of reference. Thus, special relativity "mixes" electricity and magnetism into a single, inseparable phenomenon called electromagnetism, analogous to how general relativity "mixes" space and time into spacetime.

All observations on electromagnetism apply to what might be considered to be primarily magnetism, e.g. perturbations in the magnetic field are necessarily accompanied by a nonzero electric field, and propagate at the speed of light.[21]

Magnetic fields in a material

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In vacuum, where μ0 is the vacuum permeability.

In a material,

The quantity μ0M is called magnetic polarization.

If the field H is small, the response of the magnetization M in a diamagnet or paramagnet is approximately linear: the constant of proportionality being called the magnetic susceptibility. If so,

In a hard magnet such as a ferromagnet, M is not proportional to the field and is generally nonzero even when H is zero (see Remanence).

Magnetic force

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Magnetic lines of force of a bar magnet shown by iron filings on paper
Detecting magnetic field with compass and with iron filings

The phenomenon of magnetism is "mediated" by the magnetic field. An electric current or magnetic dipole creates a magnetic field, and that field, in turn, imparts magnetic forces on other particles that are in the fields.

Maxwell's equations, which simplify to the Biot–Savart law in the case of steady currents, describe the origin and behavior of the fields that govern these forces. Therefore, magnetism is seen whenever electrically charged particles are in motion—for example, from movement of electrons in an electric current, or in certain cases from the orbital motion of electrons around an atom's nucleus. They also arise from "intrinsic" magnetic dipoles arising from quantum-mechanical spin.

The same situations that create magnetic fields—charge moving in a current or in an atom, and intrinsic magnetic dipoles—are also the situations in which a magnetic field has an effect, creating a force. Following is the formula for moving charge; for the forces on an intrinsic dipole, see magnetic dipole.

When a charged particle moves through a magnetic field B, it feels a Lorentz force F given by the cross product:[22] where is the electric charge of the particle, and is the velocity vector of the particle.

Because this is a cross product, the force is perpendicular to both the motion of the particle and the magnetic field. The magnitude of the force is where is the angle between v and B.

One tool for determining the direction of the velocity vector of a moving charge, the magnetic field, and the force exerted is labeling the index finger "V"[dubiousdiscuss], the middle finger "B", and the thumb "F" with your right hand. When making a gun-like configuration, with the middle finger crossing under the index finger, the fingers represent the velocity vector, magnetic field vector, and force vector, respectively. See also right-hand rule.

Magnetic dipoles

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All known magnets are dipoles, meaning that they have a "north" and "south" pole, so named as the Earth's magnetic field applies a force to point a magnet's poles toward areas near the Earth's respective North Pole and South Pole, specifically the north magnetic pole and south magnetic pole. A magnet's north pole is attracted to another magnet's south pole.

A magnetic field contains energy, and physical systems move toward configurations with lower energy. When diamagnetic material is placed in a magnetic field, a magnetic dipole tends to align itself in opposed polarity to that field, thereby lowering the net field strength. When ferromagnetic material is placed within a magnetic field, the magnetic dipoles align to the applied field, thus expanding the domain walls of the magnetic domains.

Magnetic monopoles

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Since a bar magnet gets its ferromagnetism from electrons distributed evenly throughout the bar, when a bar magnet is cut in half, each of the resulting pieces is a smaller bar magnet. Even though a magnet is said to have a north pole and a south pole, these two poles cannot be separated from each other. A monopole—if such a thing exists—would be a new and fundamentally different kind of magnetic object. It would act as an isolated north pole, not attached to a south pole, or vice versa. Monopoles would carry "magnetic charge" analogous to electric charge. Despite systematic searches since 1931, they have never been observed.[23]

Nevertheless, some theoretical physics models predict the existence of these magnetic monopoles. Paul Dirac observed in 1931 that, because electricity and magnetism show a certain symmetry, just as quantum theory predicts that individual positive or negative electric charges can be observed without the opposing charge, isolated South or North magnetic poles should be observable. Using quantum theory Dirac showed that if magnetic monopoles exist, then one could explain the quantization of electric charge—that is, why the observed elementary particles carry charges that are multiples of the charge of the electron.

Certain grand unified theories predict the existence of monopoles which, unlike elementary particles, are solitons (localized energy packets). The initial results of using these models to estimate the number of monopoles created in the Big Bang contradicted cosmological observations—the monopoles would have been so plentiful and massive that they would have long since halted the expansion of the universe. However, the idea of inflation (for which this problem served as a partial motivation) was successful in solving this problem, creating models in which monopoles existed but were rare enough to be consistent with current observations.[24]

Units

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SI

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Symbol[25] Name of quantity Unit name Symbol Base units
E energy joule J = C⋅V = W⋅s kg⋅m2⋅s−2
Q electric charge coulomb C A⋅s
I electric current ampere A = C/s = W/V A
J electric current density ampere per square metre A/m2 A⋅m−2
U, ΔV; Δϕ; E, ξ potential difference; voltage; electromotive force volt V = J/C kg⋅m2⋅s−3⋅A−1
R; Z; X electric resistance; impedance; reactance ohm Ω = V/A kg⋅m2⋅s−3⋅A−2
ρ resistivity ohm metre Ω⋅m kg⋅m3⋅s−3⋅A−2
P electric power watt W = V⋅A kg⋅m2⋅s−3
C capacitance farad F = C/V kg−1⋅m−2⋅A2⋅s4
ΦE electric flux volt metre V⋅m kg⋅m3⋅s−3⋅A−1
E electric field strength volt per metre V/m = N/C kg⋅m⋅A−1⋅s−3
D electric displacement field coulomb per square metre C/m2 A⋅s⋅m−2
ε permittivity farad per metre F/m kg−1⋅m−3⋅A2⋅s4
χe electric susceptibility (dimensionless) 1 1
p electric dipole moment coulomb metre C⋅m A⋅s⋅m
G; Y; B conductance; admittance; susceptance siemens S = Ω−1 kg−1⋅m−2⋅s3⋅A2
κ, γ, σ conductivity siemens per metre S/m kg−1⋅m−3⋅s3⋅A2
B magnetic flux density, magnetic induction tesla T = Wb/m2 = N⋅A−1⋅m−1 kg⋅s−2⋅A−1
Φ, ΦM, ΦB magnetic flux weber Wb = V⋅s kg⋅m2⋅s−2⋅A−1
H magnetic field strength ampere per metre A/m A⋅m−1
F magnetomotive force ampere A = Wb/H A
R magnetic reluctance inverse henry H−1 = A/Wb kg−1⋅m−2⋅s2⋅A2
P magnetic permeance henry H = Wb/A kg⋅m2⋅s–2⋅A–2
L, M inductance henry H = Wb/A = V⋅s/A kg⋅m2⋅s−2⋅A−2
μ permeability henry per metre H/m kg⋅m⋅s−2⋅A−2
χ magnetic susceptibility (dimensionless) 1 1
m magnetic dipole moment ampere square meter A⋅m2 = J⋅T−1 A⋅m2
σ mass magnetization ampere square meter per kilogram A⋅m2/kg A⋅m2⋅kg−1

Other

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Living things

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A live frog levitates inside a 32 mm diameter vertical bore of a Bitter solenoid in a very strong magnetic field—about 16 teslas

Some organisms can detect magnetic fields, a phenomenon known as magnetoception. Some materials in living things are ferromagnetic, though it is unclear if the magnetic properties serve a special function or are merely a byproduct of containing iron. For instance, chitons, a type of marine mollusk, produce magnetite to harden their teeth, and even humans produce magnetite in bodily tissue.[26]

Magnetobiology studies the effects of magnetic fields on living organisms; fields naturally produced by an organism are known as biomagnetism. Many biological organisms are mostly made of water, and because water is diamagnetic, extremely strong magnetic fields can repel these living things.

Interpretation of magnetism by means of relative velocities

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In the years after 1820, André-Marie Ampère carried out numerous experiments in which he measured the forces between direct currents. In particular, he also studied the magnetic forces between non-parallel wires.[27] The final result of his work was a force law that is now named after him. In 1835, Carl Friedrich Gauss realized [12] that Ampere's force law in its original form can be explained by a generalization of Coulomb's law.

Gauss's force law states that the electromagnetic force experienced by a point charge, with trajectory , in the vicinity of another point charge, with trajectory , in a vacuum is equal to the central force , where is the distance between the charges and is the relative velocity. Wilhelm Eduard Weber confirmed Gauss's hypothesis in numerous experiments.[28][29][30] By means of Weber electrodynamics it is possible to explain the static and quasi-static effects in the non-relativistic regime of classical electrodynamics without magnetic field and Lorentz force.

Since 1870, Maxwell electrodynamics has been developed, which postulates that electric and magnetic fields exist. In Maxwell's electrodynamics, the actual electromagnetic force can be calculated using the Lorentz force, which, like the Weber force, is speed-dependent. However, Maxwell's electrodynamics is not fully compatible with the work of Ampère, Gauss and Weber in the quasi-static regime. In particular, Ampère's original force law and the Biot-Savart law are only equivalent if the field-generating conductor loop is closed.[31] Maxwell's electrodynamics therefore represents a break with the interpretation of magnetism by Gauss and Weber, since in Maxwell's electrodynamics it is no longer possible to deduce the magnetic force from a central force.

Quantum-mechanical origin of magnetism

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While heuristic explanations based on classical physics can be formulated, diamagnetism, paramagnetism and ferromagnetism can be fully explained only using quantum theory.[32][33] A successful model was developed already in 1927, by Walter Heitler and Fritz London, who derived, quantum-mechanically, how hydrogen molecules are formed from hydrogen atoms, i.e. from the atomic hydrogen orbitals and centered at the nuclei A and B, see below. That this leads to magnetism is not at all obvious, but will be explained in the following.

According to the Heitler–London theory, so-called two-body molecular -orbitals are formed, namely the resulting orbital is:

Here the last product means that a first electron, r1, is in an atomic hydrogen-orbital centered at the second nucleus, whereas the second electron runs around the first nucleus. This "exchange" phenomenon is an expression for the quantum-mechanical property that particles with identical properties cannot be distinguished. It is specific not only for the formation of chemical bonds, but also for magnetism. That is, in this connection the term exchange interaction arises, a term which is essential for the origin of magnetism, and which is stronger, roughly by factors 100 and even by 1000, than the energies arising from the electrodynamic dipole-dipole interaction.

As for the spin function , which is responsible for the magnetism, we have the already mentioned Pauli's principle, namely that a symmetric orbital (i.e. with the + sign as above) must be multiplied with an antisymmetric spin function (i.e. with a − sign), and vice versa. Thus: , I.e., not only and must be substituted by α and β, respectively (the first entity means "spin up", the second one "spin down"), but also the sign + by the − sign, and finally ri by the discrete values si (= ±12); thereby we have and . The "singlet state", i.e. the − sign, means: the spins are antiparallel, i.e. for the solid we have antiferromagnetism, and for two-atomic molecules one has diamagnetism. The tendency to form a (homoeopolar) chemical bond (this means: the formation of a symmetric molecular orbital, i.e. with the + sign) results through the Pauli principle automatically in an antisymmetric spin state (i.e. with the − sign). In contrast, the Coulomb repulsion of the electrons, i.e. the tendency that they try to avoid each other by this repulsion, would lead to an antisymmetric orbital function (i.e. with the − sign) of these two particles, and complementary to a symmetric spin function (i.e. with the + sign, one of the so-called "triplet functions"). Thus, now the spins would be parallel (ferromagnetism in a solid, paramagnetism in two-atomic gases).

The last-mentioned tendency dominates in the metals iron, cobalt and nickel, and in some rare earths, which are ferromagnetic. Most of the other metals, where the first-mentioned tendency dominates, are nonmagnetic (e.g. sodium, aluminium, and magnesium) or antiferromagnetic (e.g. manganese). Diatomic gases are also almost exclusively diamagnetic, and not paramagnetic. However, the oxygen molecule, because of the involvement of π-orbitals, is an exception important for the life-sciences.

The Heitler–London considerations can be generalized to the Heisenberg model of magnetism (Heisenberg 1928).

The explanation of the phenomena is thus essentially based on all subtleties of quantum mechanics, whereas the electrodynamics covers mainly the phenomenology.

See also

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References

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Further reading

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Bibliography

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Magnetism is a fundamental force in physics arising from the motion of electric charges, particularly the orbital and spin motions of electrons within atoms, which produces that exert attractive or repulsive forces on other magnetic materials or currents. These fields are visualized through lines of force, where parallel electric currents attract and opposing currents repel, with permanent magnets like lodestones representing a key manifestation observed since ancient times. At its core, magnetism is intimately linked to , as demonstrated by the production of by electric currents, forming the basis for electromagnetic phenomena essential to both natural processes and modern . The phenomenon has been recognized for millennia, with early discoveries of naturally occurring magnets—lodestones—in regions like Magnesia, Asia Minor, around 600 BCE, and in ancient , leading to their use in primitive devices, such as the south-pointing spoon, by the ancient Chinese for divination and later navigation. Significant advancements came in the 19th century, when in 1821 observed that electric currents deflect compass needles, unifying and magnetism, followed by André-Marie Ampère's explanation of magnetic forces between currents. William Gilbert's 1600 work further established Earth itself as a giant magnet, advancing the scientific understanding of geomagnetism, which was crucial for navigation in the Age of Exploration. Materials exhibit various types of magnetism based on their atomic structure and electron interactions, broadly classified into diamagnetism, paramagnetism, ferromagnetism, ferrimagnetism, and antiferromagnetism. Diamagnetism, a universal weak property, causes materials like to be repelled by magnetic fields due to induced opposing currents, independent of temperature. Paramagnetism results in weak attraction in substances like aluminum, where atomic magnetic moments align with external fields but are disrupted by thermal motion, making it temperature-dependent. Stronger effects occur in ferromagnetism, seen in iron, where spins align spontaneously below the (770°C for iron), enabling permanent magnets. Ferrimagnetism in materials like produces net from unequal opposing moments, while antiferromagnetism features antiparallel alignment of adjacent atomic magnetic moments below the Néel temperature, yielding zero net . Magnetism underpins diverse applications, from everyday devices like refrigerator magnets and electric motors to advanced technologies such as MRI scanners, via (recognized by the 2007 ), and generators for . In nature, it explains cosmic rays, atomic energy levels, and the trapping of charged particles in Earth's Van Allen belts, while the planet's protects against solar radiation, studied through satellite observations. Electromagnetic waves, combining electric and magnetic fields, enable communications like radio and X-rays, revolutionizing and global connectivity.

Fundamentals

Basic Concepts

Magnetism is a fundamental physical force arising from the motion of electric charges, manifesting as attractive or repulsive interactions between certain materials. Specifically, it is the natural force exerted by magnets, which attract ferromagnetic materials like iron, , and , while also producing forces on other moving charges. The electromagnetic force, which encompasses both electric and magnetic interactions, is one of the four fundamental interactions in nature, alongside , the strong , and the weak nuclear force. A key observable phenomenon of magnetism is the behavior of magnetic poles. Every magnet possesses two distinct poles: a north pole and a south pole. Like poles repel each other, whereas unlike poles attract, following the north-south rule where the north pole of one magnet draws toward the south pole of another. This interaction is evident when bar magnets are brought close together, demonstrating the repulsive force between two north poles or two south poles, and the attractive pull between opposite poles. The presence of a magnetic field surrounding magnets is another core concept, often represented by field lines that originate from the and converge toward the outside the . These lines illustrate the direction and relative strength of the field, with denser lines indicating stronger magnetic influence. , a naturally occurring form of the (Fe₃O₄), serves as the earliest known example of a permanent natural , exhibiting these pole behaviors without external influence. On a planetary scale, provides a prominent global example of magnetism, generated by processes in its core and extending into space to form the . This field influences needles, aligning their north poles toward Earth's geographic north (actually the magnetic ), and protects the atmosphere from solar particles.

Magnetic Fields

The magnetic field, denoted as B\mathbf{B}, is a vector field that describes the magnetic influence exerted on a moving , a , or another at any given point in space. It is defined such that the force on a charge qq moving with velocity v\mathbf{v} is F=qv×B\mathbf{F} = q \mathbf{v} \times \mathbf{B}, highlighting its role in mediating magnetic interactions. This vector nature allows B\mathbf{B} to have both magnitude and direction, with the direction conventionally determined by the north-pointing end of a needle placed in the field. Magnetic fields are often visualized using iron filings sprinkled on a surface near a , which align themselves tangent to the field lines due to the torque induced on their small magnetic domains. Alternatively, an array of needles reveals the field's direction at multiple points, with arrows pointing from the toward the of the . The density of these field lines represents the field's strength, being greater where B\mathbf{B} is more intense, such as near the poles of a bar . This visualization underscores that lines form continuous closed loops, never beginning or ending, consistent with the absence of magnetic monopoles. Key properties of the magnetic field include its ability to exert a torque τ=m×B\mathbf{\tau} = \mathbf{m} \times \mathbf{B} on a magnetic dipole moment m\mathbf{m}, which aligns the dipole parallel to the field to minimize potential energy. Unlike electric fields, magnetic fields do no net work on isolated moving charges, as the Lorentz force F=qv×B\mathbf{F} = q \mathbf{v} \times \mathbf{B} is always perpendicular to the velocity v\mathbf{v}, preserving the charge's kinetic energy while altering its direction. On planetary scales, Earth's magnetic field approximates a dipole tilted by about 11° relative to the planet's rotational axis. The geomagnetic poles, defined as the intersections of the best-fit dipole axis with Earth's surface, are located near but distinct from the geographic poles; as of 2025, the north geomagnetic pole is approximately at 80.8°N, 72.8°W in the Arctic Ocean (per IGRF-14). The points where field lines are vertical (magnetic dip poles) are distinct, with the north magnetic dip pole at approximately 85.7°N, 138.6°E. This dipole structure arises primarily from dynamo action in the molten outer core. At large distances from a bar magnet, the magnetic field follows the dipole approximation, treating the magnet as a point dipole with magnetic moment m\mathbf{m}: B(r)=μ04π(3(mr^)r^mr3),\mathbf{B}(\mathbf{r}) = \frac{\mu_0}{4\pi} \left( \frac{3(\mathbf{m} \cdot \hat{r})\hat{r} - \mathbf{m}}{r^3} \right), where μ0\mu_0 is the permeability of free space, r\mathbf{r} is the position vector from the dipole, r=rr = |\mathbf{r}|, and r^=r/r\hat{r} = \mathbf{r}/r. This expression shows the field's 1/r31/r^3 decay and angular dependence, strongest along the dipole axis and zero in the equatorial plane.

Historical Development

Early Observations

One of the earliest recorded observations of magnetic phenomena dates back to ancient during the , around 400 BCE, where —a naturally magnetized form of —was employed in practices. Chinese scholars fashioned rudimentary compasses from spoons balanced on smooth plates, allowing the stone to rotate and align with the , which was interpreted as a tool for and rather than . In the 6th century BCE, Greek philosopher documented the attractive properties of to iron, marking one of the first Western accounts of magnetism. Thales observed that could draw iron fragments without physical contact, attributing this to an innate "soul" within the stone, though he did not distinguish it from electrical effects like the attraction produced by rubbed amber. During the medieval period, magnetic knowledge advanced in both and the Islamic world. In 1088 CE, Chinese polymath described the invention of a suspended magnetic needle in his work , noting its deviation from due to and applying it to improved . This innovation spread to through Arab scholars, who refined lodestone-based devices for maritime use by the 12th century. In 1600, English physician William Gilbert published , a seminal treatise based on extensive experiments with and spherical magnets (terrellae), which he used to model the 's magnetism. Gilbert conclusively distinguished magnetism from —previously conflated as "effluvia"—and proposed that the itself functions as a giant magnet, explaining behavior through its dipolar field. The pivotal link between and magnetism emerged in 1820 when Danish physicist accidentally observed that a current-carrying wire deflected a nearby needle during a demonstration. This serendipitous finding, published promptly, revealed that electric currents produce , laying the empirical foundation for and inspiring subsequent theoretical work.

Theoretical Advancements

In 1820, conducted an experiment demonstrating that an passing through a wire causes a nearby needle to deflect, revealing the intimate connection between and magnetism. This discovery prompted to investigate the forces between current-carrying wires, leading to his formulation in 1820–1822 of the fundamental law of electrodynamics, which quantifies the magnetic force between two current elements as proportional to the product of their currents, the inverse square of their separation, and a cosine dependence on their relative orientation. Ampère's law established that magnetism arises from moving electric charges, providing a mathematical framework for the interactions observed by Ørsted. Building on these insights, discovered in 1831 through experiments showing that a changing induces an in a closed circuit. This principle, known as Faraday's , states that the induced E\mathcal{E} equals the negative rate of change of ΦB\Phi_B through the circuit: E=dΦBdt\mathcal{E} = -\frac{d\Phi_B}{dt}. Faraday's work demonstrated the between electricity and magnetism, as a time-varying generates an , complementing Ørsted's finding that currents produce . In the 1860s, James Clerk Maxwell unified these empirical laws into a comprehensive theoretical framework, culminating in his equations that describe all classical electromagnetic phenomena. One key equation, Ampère's law with Maxwell's addition, relates the curl of the B\mathbf{B} to the J\mathbf{J} and the time derivative of the E\mathbf{E}: ×B=μ0J+μ0ϵ0Et\nabla \times \mathbf{B} = \mu_0 \mathbf{J} + \mu_0 \epsilon_0 \frac{\partial \mathbf{E}}{\partial t}. This term enabled Maxwell to predict electromagnetic waves propagating at the , establishing light as an electromagnetic phenomenon and bridging , magnetism, and . Pierre Curie's investigations into in 1895 revealed that for paramagnetic materials, susceptibility varies inversely with , a relation now known as , and identified a critical —the Curie point—above which ferromagnetic materials lose their permanent magnetization and behave paramagnetically. This temperature-dependent transition provided early evidence of the thermal disruption of magnetic ordering, influencing subsequent theories of magnetism in matter. In 1907, Pierre Weiss proposed the to explain , positing that ferromagnetic materials consist of microscopic regions called domains where atomic magnetic moments align spontaneously due to an internal "molecular field" far stronger than external fields. This theory accounted for the bulk magnetization of ferromagnets as the alignment of these domains under an applied field, while their random orientations in the absence of a field explain the low net magnetism of unmagnetized samples. Weiss's molecular field concept laid the groundwork for understanding cooperative magnetic behavior, bridging with atomic-scale phenomena.

Sources of Magnetism

Permanent Magnets

Permanent magnets are materials capable of producing a in free space without continuous energy input, distinguishing them from temporary magnetic sources. They exhibit , defined as the maximum alignment of atomic magnetic moments—primarily from spins in transition metals or rare-earth elements—achieved under a saturating external field, resulting in a net MsM_s that persists after the field is removed. This property enables permanent magnets to maintain their magnetism indefinitely under normal conditions, provided they are not exposed to demagnetizing influences. Common permanent magnet materials include alloys, developed in the 1930s as the first modern high-performance magnets composed of aluminum, , , and iron, offering good temperature stability up to 550°C. Ferrite magnets, also known as magnets based on or (e.g., SrFe₁₂O₁₉), emerged commercially in the mid-20th century and are valued for their low cost, high , and corrosion resistance despite lower . Neodymium-iron-boron (NdFeB or Nd₂Fe₁₄B) magnets, introduced in the 1980s, represent the strongest commercially available permanent magnets with energy products up to 58 MGOe, revolutionizing applications requiring high density, though they have a lower of 312°C. Two critical factors determine a permanent magnet's resistance to demagnetization: remanence (BrB_r) and coercivity (HcH_c). Remanence is the residual magnetic flux density that remains after the magnet is saturated and the external field is removed, quantifying the magnet's inherent field strength and directly influencing its practical output in devices. Coercivity measures the reverse magnetic field strength required to reduce the flux density to zero, serving as an indicator of the material's stability against opposing fields or thermal fluctuations, with higher values essential for "hard" magnetic materials used in permanent applications. The behavior of permanent magnets is characterized by the B-H hysteresis loop, a graphical representation of the relationship between magnetic flux density BB and applied field HH during magnetization cycles. Starting from zero field, increasing HH aligns magnetic domains to reach saturation, where BB plateaus as all moments are fully aligned. Upon removing the field, the curve traces to BrB_r on the B-axis, reflecting the retained . Applying a reverse field then demagnetizes the material, crossing zero flux at HcH_c on the H-axis, and further reversal leads to negative saturation; the loop closes upon returning to the original direction, with the area enclosed representing energy loss per cycle. For permanent magnets, the second-quadrant portion of this curve is particularly important, guiding design by showing operating limits and BHmaxBH_{\max}. These magnets find essential applications in navigation tools like compasses, where a lightweight permanent magnet aligns with Earth's geomagnetic field to indicate direction. In electric motors, permanent magnets provide the stationary field that interacts with current-carrying coils to produce torque, enabling efficient conversion of electrical to mechanical energy in devices from household appliances to industrial machinery.

Induced Magnetism

Induced magnetism, also known as magnetic induction, occurs when a material becomes temporarily magnetized in the presence of an external magnetic field, with the magnetization aligning parallel to the applied field and vanishing upon removal of the field. This phenomenon arises because the external field causes the alignment of magnetic moments within the material, such as electron spins or atomic currents, without requiring intrinsic permanent dipoles. The degree of induced magnetization, denoted as M\mathbf{M}, is typically proportional to the applied magnetic field strength H\mathbf{H} for small fields, characterized by the material's magnetic susceptibility χm\chi_m, where M=χmH\mathbf{M} = \chi_m \mathbf{H}. A key application of induced magnetism is in , devices that produce strong, controllable magnetic fields using electric currents. An typically consists of a —a helical coil of insulated wire—often wound around a ferromagnetic core, such as iron, which enhances the field through induced magnetization. The B\mathbf{B} inside a long in is given by B=μ0nI\mathbf{B} = \mu_0 n I where μ0=4π×107\mu_0 = 4\pi \times 10^{-7} T·m/A is the permeability of free space, nn is the number of turns per unit length, and II is the current. When a ferromagnetic core is inserted, the induced magnetization in the core amplifies the total field, as the core's permeability μ=μ0(1+χm)\mu = \mu_0 (1 + \chi_m) increases B\mathbf{B} significantly, often by factors of thousands. The field's strength and direction can be precisely adjusted by varying the current, making electromagnets versatile for applications like lifting machinery, magnetic resonance imaging, and particle accelerators. The invention of the practical electromagnet is credited to Joseph Henry in 1831, who constructed one capable of lifting over 750 pounds using insulated wire windings to allow more turns without shorting. The behavior of induced magnetism depends on the material's response to the applied field, particularly its —the reverse field needed to reduce to zero after saturation. Soft magnetic materials, such as pure iron or silicon steel, exhibit low (typically below 1 kA/m), enabling rapid and reversible induction ideal for temporary magnetism in transformers and inductors. In contrast, hard magnetic materials like alloys have high (often exceeding 50 kA/m), resulting in semi-permanent retention of induced , which serves as a basis for creating semi-permanent magnets but contrasts with the fully reversible nature of soft materials. Electromagnetic induction, governed by Faraday's law, plays a crucial role in generating and modulating the fields that induce magnetism in coils and surrounding materials. Faraday's law states that the induced E\mathcal{E} in a closed loop is E=dΦBdt\mathcal{E} = -\frac{d\Phi_B}{dt}, where ΦB\Phi_B is the through the loop; a changing current in one coil thus produces a varying field that induces currents—and hence fields—in nearby coils or cores. This self- or mutual-induction effect is essential in electromagnets, where ramping the current induces opposing fields (per ) that must be overcome, influencing the design of power supplies for smooth field generation. Unlike permanent magnets, which retain intrinsic magnetism independently, induced magnetism in these systems is entirely dependent on the sustained external field for its existence.

Magnetic Materials and Types

Diamagnetism

Diamagnetism is a fundamental magnetic property exhibited by all materials, characterized by a negative magnetic susceptibility (χ<0\chi < 0), which results in the induction of a weak magnetic field that opposes the applied external magnetic field. This opposition leads to a slight repulsion of the material from magnetic fields, distinguishing diamagnetism as a universal but feeble effect present even in materials that show no permanent magnetism. Unlike paramagnetism, where moments align with the field, diamagnetism always produces an opposing response regardless of temperature or material composition. The underlying mechanism of diamagnetism stems from the application of Lenz's law to the orbital motion of electrons within atoms. When an external magnetic field is applied, it alters the angular velocity of these orbiting electrons, inducing effective current loops that generate a secondary magnetic field directed opposite to the applied field to conserve magnetic flux. This induced opposition arises from the closed-shell electron configurations in atoms, where the orbital precession creates a net diamagnetic moment without requiring unpaired spins. The effect is inherently quantum mechanical but can be understood classically through electromagnetic induction principles. Representative examples of diamagnetic materials include water and graphite, which demonstrate observable effects under strong fields. For instance, small pieces of pyrolytic graphite can levitate stably above powerful permanent magnets due to the repulsive diamagnetic forces, while water droplets can be suspended in high-gradient magnetic fields exceeding 10 T. These phenomena highlight the practical manifestation of diamagnetism despite its weakness. Magnetic susceptibility values for diamagnetic materials typically range from -10^{-5} to -10^{-6} in SI units and remain independent of temperature, reflecting the intrinsic orbital response. Specific cases include water with χ9×106\chi \approx -9 \times 10^{-6} and bismuth with a more pronounced χ1.7×104\chi \approx -1.7 \times 10^{-4}, while graphite exhibits anisotropic values around -4.5 \times 10^{-5}) perpendicular to its layers. Superconductors represent an extreme case of perfect diamagnetism through the Meissner effect, where the material completely expels magnetic fields from its interior upon entering the superconducting state, achieving χ=1\chi = -1. This effect, discovered by Walther Meissner and Robert Ochsenfeld in 1933, arises from the formation of persistent supercurrents on the surface that precisely cancel the internal field, enabling applications like magnetic levitation without energy loss. In type-I superconductors, this expulsion occurs below a critical field strength, underscoring diamagnetism's role in macroscopic quantum phenomena.

Paramagnetism

Paramagnetism refers to the weak attraction of certain materials to an external magnetic field, characterized by a positive magnetic susceptibility χ>0\chi > 0. This susceptibility arises from the alignment of atomic magnetic moments with the applied field, resulting in a that is directly proportional to the field strength HH. The atomic origin of paramagnetism lies in the presence of unpaired electrons, whose spin and orbital angular momenta generate permanent magnetic moments. These moments, typically on the order of Bohr magnetons, can align with the external field but are subject to thermal agitation that randomizes their orientations. In the absence of strong interactions between moments, the net is small and reversible. The in paramagnetic materials follows , expressed as χ=CT,\chi = \frac{C}{T}, where CC is the Curie constant and TT is the absolute temperature (in SI units). The Curie constant CC is determined by the atomic magnetic moments, given by C=μ0Nμ23kBC = \frac{\mu_0 N \mu^2}{3 k_B}, with NN the number of magnetic moments per unit volume, μ\mu the average moment size (related to g2j(j+1)μB2g^2 j(j+1) \mu_B^2, where gg is the , jj the , and μB\mu_B the ), and kBk_B Boltzmann's constant. This law holds for temperatures well above any characteristic scales where thermal energy exceeds the Zeeman splitting energy. Representative examples include aluminum, which exhibits due to its conduction electrons, and oxygen gas (O₂), where the two unpaired electrons per contribute to a measurable susceptibility. For oxygen, the Curie constant reflects the molecular of approximately 2 Bohr magnetons. The susceptibility decreases inversely with temperature, becoming negligible at high temperatures where thermal disorder dominates, though it does not abruptly vanish. Unlike materials with cooperative magnetism, paramagnetic substances show no , as the alignment is purely induced and reversible upon field removal. A related phenomenon is , a temperature-independent contribution arising from second-order perturbation effects in systems with a non-magnetic but nearby excited states admixed by the field, often due to orbital contributions. This effect is smaller than the Curie-type paramagnetism but significant in some ions.

Ferromagnetism

refers to a type of magnetism in which materials exhibit a large positive and in the absence of an external , occurring below a critical known as the . Above the , the material transitions to a paramagnetic state, losing its due to thermal disruption of spin alignments. This phenomenon arises from cooperative interactions among atomic magnetic moments, leading to strong, permanent magnetic behavior in certain metals and alloys. The underlying mechanism of ferromagnetism is the quantum mechanical exchange interaction, which favors parallel alignment of neighboring electron spins, resulting in a net macroscopic magnetization. This interaction is described by the Heisenberg model, a foundational theoretical framework that models the Hamiltonian of spin systems as H=Ji,jSiSjH = -J \sum_{\langle i,j \rangle} \mathbf{S}_i \cdot \mathbf{S}_j, where J>0J > 0 for ferromagnetic coupling promotes aligned . The exchange energy stabilizes domains—regions of uniform spin orientation—contributing to the material's overall magnetic strength. Classic examples of ferromagnetic materials include iron, with a Curie temperature of 1043 K; , at 631 K; and , at 1388 K. In these materials, the process involves , where the lags behind changes in the applied , forming a characteristic loop that demonstrates energy loss during cycling; saturation occurs when the field fully aligns all spins, reaching the maximum value. Modern advancements in ferromagnetic materials include rare-earth alloys such as neodymium-iron-boron (NdFeB) and samarium-cobalt (SmCo), which enhance magnetic performance through higher and for high-field applications like electric motors and MRI machines. These alloys achieve Curie temperatures around 583 K for NdFeB, allowing operation at elevated temperatures while maintaining strong fields exceeding 1.2 tesla.

Antiferromagnetism

Antiferromagnetism is a type of magnetic ordering characterized by the antiparallel alignment of adjacent atomic magnetic moments, leading to complete cancellation and zero net in the ordered state. This phenomenon occurs below a critical temperature known as the Néel temperature, TNT_N, named after Louis Néel who proposed the concept in 1948 to describe materials with such opposing spin arrangements. Above TNT_N, antiferromagnets exhibit paramagnetic behavior, with their magnetic susceptibility obeying the Curie-Weiss law, χ=CTθ\chi = \frac{C}{T - \theta} (in SI units, where the constant incorporates μ0\mu_0), where the Curie-Weiss constant θ\theta is negative, reflecting the dominant antiferromagnetic interactions that favor antiparallel spin alignment. Representative examples include manganese(II) oxide (MnO), which displays antiferromagnetic ordering below TN=116T_N = 116 K, and hematite (α\alpha-Fe₂O₃), an iron oxide mineral that orders antiferromagnetically below approximately 950 K. The antiferromagnetic structure is commonly detected through neutron diffraction, a technique that reveals characteristic reflections arising from the periodic magnetic ordering, as first demonstrated in studies of materials like MnO. In insulating antiferromagnets, the antiparallel coupling often arises via the mechanism, an indirect interaction mediated by non-magnetic anions that bridge magnetic cations, such as the oxygen ions in the Mn-O-Mn pathways of MnO, promoting antiferromagnetic alignment through virtual electron hopping. Certain materials can undergo a transition from to under influences like doping, pressure, or structural distortion; for instance, in the double Sr₂FeOsO₆, lattice distortion drives a shift from a low-temperature antiferromagnetic state to a high-temperature ferrimagnetic one with net .

Ferrimagnetism

arises from the partial cancellation of magnetic moments in materials where atoms form two or more sublattices with opposing spin alignments but unequal magnitudes, yielding a net . This contrasts with , where equal sublattice moments result in complete cancellation and no net effect. The concept was introduced by Louis Néel in 1948 to describe magnetic ordering in complex structures like ferrites, where negative exchange interactions cause antiparallel alignment of sublattices composed of different atomic species, producing a akin to but with reduced saturation value. In these materials, the Néel structure features distinct sublattices—such as tetrahedral and octahedral sites in lattices—with differing numbers or strengths of magnetic ions, leading to the residual moment. Magnetite (Fe₃O₄), the archetypal ferrimagnet and one of the earliest known magnetic minerals, exemplifies this behavior in its inverse structure, where Fe³⁺ ions align ferromagnetically within sublattices but antiparallel between them, resulting in a net moment of approximately 4 μ_B per at low temperatures. Synthetic ferrites, such as nickel-zinc or manganese-zinc variants, extend this to compounds with tailored compositions for practical use. Ferrimagnetic ordering persists below the Curie temperature (T_C), at which point disrupts the alignment, transitioning the material to a paramagnetic state with susceptibility following . For , T_C is about 858 , while engineered ferrites often have lower T_C values suited to device operating ranges. These properties make ferrimagnetic ferrites ideal for high-frequency applications, including cores in transformers and inductors, where their high electrical resistivity (typically >10⁶ Ω·cm) suppresses losses, enabling efficient operation up to frequencies. Synthetic molecular ferrimagnets, constructed via coordination chemistry with metal ions and organic ligands, serve as nanoscale analogs to inorganic ferrites, exhibiting bulk-like ferrimagnetic behavior at low temperatures and holding promise for spintronic and devices.

Other Exotic Types

Superparamagnetism arises in ferromagnetic nanoparticles when their size is reduced to the nanoscale, typically below 10-20 nm for materials like , where overcome the energy barrier, causing the to fluctuate rapidly and exhibit no or , thus behaving like a paramagnet despite the ferromagnetic core. This phenomenon, first modeled by William F. Brown in , leads to a blocking below which the particles retain , as seen in superparamagnetic nanoparticles (SPIONs) used in biomedical applications such as contrast agents. The superparamagnetic limit depends on particle volume, constant, and , with kBTk_B T competing against the energy barrier KVK V, where KK is the anisotropy constant and VV the particle volume. Nagaoka magnetism refers to a theoretical prediction of in the infinite-U at half-filling with one hole, where strong on-site repulsion favors a fully polarized ferromagnetic to minimize loss. Proposed by Yosuke Nagaoka in 1966, this exact solution applies to narrow-band systems with nearest-neighbor hopping, demonstrating that can emerge from purely kinetic exchange in strongly correlated systems. Although realized experimentally in quantum simulators and certain lattices, it remains a benchmark for understanding itinerant in the beyond mean-field approximations. Spin ice describes geometrically frustrated magnetic systems in pyrochlore lattices, such as Dy₂Ti₂O₇ or Ho₂Ti₂O₇, where rare-earth ions' Ising-like spins obey "ice rules" analogous to water ice, leading to a degenerate manifold of configurations with zero net magnetization. Discovered in the early 2000s, these systems exhibit emergent monopolar excitations as defects in the ice-rule background, behaving as magnetic charges that interact via a Coulomb-like potential and can be observed through neutron scattering or muon spin relaxation. The monopole dynamics in spin ice, confirmed experimentally around 2009, reveal diffusive transport and string-like correlations, providing a playground for studying fractionalized excitations in condensed matter. Multiferroics are materials exhibiting simultaneous and , with coupled orders enabling magnetoelectric effects where an induces or vice versa, often through mechanisms like inverse Dzyaloshinskii-Moriya interactions or in type-II systems. intensified post-2000 with discoveries in compounds like TbMnO₃ and BiFeO₃, where spiral magnetic orders break inversion to induce polarization, achieving coefficients up to 10⁴ times larger than in linear magnetoelectrics. Ongoing efforts focus on thin films and heterostructures for device applications, such as sensors and memory, though challenges persist in achieving room-temperature operation and strong in single-phase materials. As of 2025, advances include functioning up to 160°C, such as Tb₂(MoO₄)₃, and theoretical frameworks for permanent electric control of magnetism, enhancing prospects for practical devices. Magnetic skyrmions are topologically stable, particle-like spin textures in non-centrosymmetric magnets, characterized by a swirling that winds around a core, protected by a nonzero topological charge Q=m(xm×ym)dxdy=1Q = \int \mathbf{m} \cdot (\partial_x \mathbf{m} \times \partial_y \mathbf{m}) \, dx dy = 1, enabling robust configurations against perturbations. First observed experimentally in 2009 via in chiral magnets like MnSi under magnetic fields, skyrmions form lattices with sizes of 10-100 nm and promise applications in due to their low-energy drive by spin currents and high density. Subsequent real-space in 2010 confirmed their vortex-like , spurring into room-temperature skyrmions in thin films for next-generation . Recent 2025 has advanced skyrmion control and stability, including gradient-induced methods and laser-induced skyrmion bags, alongside studies of quantum effects.

Magnetic Interactions

Magnetic Force

The magnetic force on moving in is described by the law, which states that the force F\mathbf{F} experienced by a particle of charge qq moving with v\mathbf{v} in B\mathbf{B} is given by F=q(v×B)\mathbf{F} = q (\mathbf{v} \times \mathbf{B}). This vector cross product ensures that the force is always perpendicular to both the velocity and the magnetic field vectors. A key property of this force is that it performs no work on the particle, as the dot product Fv=q(v×B)v=0\mathbf{F} \cdot \mathbf{v} = q (\mathbf{v} \times \mathbf{B}) \cdot \mathbf{v} = 0, since the cross product v×B\mathbf{v} \times \mathbf{B} is orthogonal to v\mathbf{v}. Consequently, the magnetic force cannot change the kinetic energy or speed of the particle, only its direction. In a uniform magnetic field, this perpendicular force causes charged particles to follow circular paths, with the centripetal force provided by the magnetic force: mv2r=qvBsinθ\frac{m v^2}{r} = q v B \sin \theta, where θ\theta is the angle between v\mathbf{v} and B\mathbf{B}. For perpendicular motion (θ=90\theta = 90^\circ), the radius of the circular path, known as the cyclotron radius, is r=mvqBr = \frac{m v}{q B}. The law extends to current-carrying conductors, where a wire of length L\mathbf{L} carrying current II in a experiences a force F=I(L×B)\mathbf{F} = I (\mathbf{L} \times \mathbf{B}). This arises from the collective effect of the on the individual moving charges within the wire. One observable consequence is the , discovered by Edwin Hall in 1879, in which a transverse voltage develops across a current-carrying conductor placed in a due to the deflection of charges by the . This voltage, known as the Hall voltage, is proportional to the strength, current, and properties, enabling measurements of material characteristics. For macroscopic magnets, approximated as magnetic dipoles with moments m1m_1 and m2m_2, the force between them along the axial direction (aligned end-to-end) is approximately F3μ0m1m22πr4r^\mathbf{F} \approx \frac{3 \mu_0 m_1 m_2}{2 \pi r^4} \hat{r}, where μ0\mu_0 is the permeability of free space, rr is the separation distance, and r^\hat{r} is the unit vector along the axis; the depends on the relative orientation of the dipoles. This interaction falls off rapidly with distance, as expected from the 1/r41/r^4 dependence. These principles find practical applications in devices such as mass spectrometers, where charged particles are accelerated and deflected by into paths with radii dependent on their , allowing separation and identification of isotopes. Similarly, in particle accelerators like cyclotrons, the magnetic force confines beams of charged particles to circular orbits, enabling repeated acceleration to high energies for collision experiments.

Magnetic Dipoles

A consists of a pair of equal and opposite magnetic poles separated by a small , or equivalently, a with m=IA\mathbf{m} = I \mathbf{A}, where II is the current and A\mathbf{A} is the of the loop. For a loop with NN turns, the moment is m=NIA\mathbf{m} = N I \mathbf{A}. In a uniform magnetic field B\mathbf{B}, a magnetic dipole experiences a torque τ=m×B\mathbf{\tau} = \mathbf{m} \times \mathbf{B} that tends to align the dipole moment with the field. The magnitude of this torque is τ=mBsinθ\tau = m B \sin \theta, where θ\theta is the angle between m\mathbf{m} and B\mathbf{B}, and it is zero when the dipole is aligned (θ=0\theta = 0^\circ or 180180^\circ). The potential energy of the dipole in the field is given by U=mB=mBcosθU = -\mathbf{m} \cdot \mathbf{B} = -m B \cos \theta, which is minimized when the dipole aligns parallel to the field. This torque causes observable alignment effects, such as a needle, which acts as a , rotating to point along the local lines, with its toward Earth's magnetic south pole. At the atomic scale, magnetic moments from electron orbits or in atoms partially align with an external field, contributing to the material's response. The magnetic field produced by a dipole at large distances rr (where rr \gg dipole size) approximates that of a point , with the field strength falling off as B1/r3B \propto 1/r^3. For a dipole moment m\mathbf{m} along the z-axis, the field components in spherical coordinates are: Br=2μ0mcosθ4πr3,Bθ=μ0msinθ4πr3,B_r = \frac{2 \mu_0 m \cos \theta}{4 \pi r^3}, \quad B_\theta = \frac{\mu_0 m \sin \theta}{4 \pi r^3}, where μ0\mu_0 is the permeability of free space; this approximation is useful for modeling interactions between at separations much larger than their size. The concept of magnetic arises from the absence of isolated magnetic monopoles in nature, as every magnet has both north and south poles. Theoretical isolated north or south magnetic poles, or monopoles, would simplify by introducing a magnetic charge, but none have been observed experimentally. In 1931, showed that the existence of even one monopole would imply charge quantization in , via the Dirac quantization condition eg=2πnceg = 2\pi n \hbar c (where ee is , gg magnetic charge, nn an integer, \hbar reduced Planck's constant, and cc ). Searches for monopoles continue in , such as the MoEDAL experiment at the LHC, which has set limits on monopole production in high-energy collisions but found no evidence. Grand unified theories (GUTs), which unify the strong, weak, and electromagnetic forces, predict magnetic monopoles as topological defects formed during in the early . These monopoles would have masses around 101610^{16} GeV, far beyond current accelerators, motivating ongoing hunts in cosmic rays and accelerator experiments.

Fields in Materials

Magnetization and Susceptibility

In magnetic materials, the M\mathbf{M} represents the moment per unit volume, quantifying the of aligned atomic or molecular magnetic moments within the material. This arises from the collective response of the material's microscopic magnetic dipoles to an applied . The relationship between the magnetic induction B\mathbf{B}, the magnetic field strength H\mathbf{H}, and the magnetization M\mathbf{M} is given by the equation B=μ0(H+M),\mathbf{B} = \mu_0 (\mathbf{H} + \mathbf{M}), where μ0\mu_0 is the permeability of free space. This expression accounts for the total magnetic field inside the material as the sum of the applied field contribution (via H\mathbf{H}) and the field's modification due to the material's magnetization. In vacuum, M=0\mathbf{M} = 0, reducing to B=μ0H\mathbf{B} = \mu_0 \mathbf{H}. The magnetic susceptibility χm\chi_m measures the material's tendency to develop magnetization in response to an applied H\mathbf{H} field and is defined as the dimensionless ratio χm=MH,\chi_m = \frac{M}{H}, assuming a linear relationship M=χmH\mathbf{M} = \chi_m \mathbf{H}. The magnetic permeability μ\mu then follows as μ=μ0(1+χm),\mu = \mu_0 (1 + \chi_m), which describes how the material amplifies or attenuates the magnetic field compared to vacuum; materials with χm>0\chi_m > 0 enhance the field, while those with χm<0\chi_m < 0 weaken it. Demagnetizing fields arise from the magnetization itself and act to oppose the applied H\mathbf{H} field, reducing the net internal field within the material. These fields are shape-dependent, with ellipsoidal shapes yielding uniform internal demagnetizing fields characterized by a demagnetizing factor NN (where 0N10 \leq N \leq 1), such that the internal H\mathbf{H} is Hint=HappNM\mathbf{H}_\text{int} = \mathbf{H}_\text{app} - N \mathbf{M}. For non-ellipsoidal shapes, the fields are nonuniform and more complex to compute, influencing the overall magnetic behavior based on geometry. In diamagnetic and paramagnetic materials, the response is typically linear, where M\mathbf{M} is directly proportional to H\mathbf{H} over a wide range, allowing the use of constant χm\chi_m values. Ferromagnetic materials, however, exhibit nonlinear behavior, with M\mathbf{M} saturating at high fields and showing hysteresis, requiring more advanced models beyond simple proportionality. At interfaces between magnetic materials or between a material and vacuum, boundary conditions ensure continuity of the fields. The normal component of B\mathbf{B} is continuous across the boundary, reflecting the absence of magnetic monopoles. The tangential component of H\mathbf{H} exhibits a discontinuity equal to the surface current density K\mathbf{K} at the interface, given by n^×(H2H1)=K\mathbf{\hat{n}} \times (\mathbf{H}_2 - \mathbf{H}_1) = \mathbf{K}, where n^\mathbf{\hat{n}} is the unit normal. These conditions are essential for solving problems involving magnetic materials with varying properties.

Domains and Hysteresis

In ferromagnetic materials, magnetic domains are microscopic regions where the atomic magnetic moments are aligned in a uniform direction, forming to minimize the total magnetic energy by reducing stray fields outside the material while allowing internal alignment without requiring a strong external field. This concept was introduced by Pierre Weiss in 1907, who proposed that ferromagnets consist of such domains to explain their high saturation magnetization observed even in the absence of external fields. Within each domain, the magnetization is nearly uniform, but the overall material magnetization is the vector sum of these domain contributions, which can be reoriented by external fields. The boundaries between adjacent domains, known as domain walls, are narrow transition zones—typically tens to hundreds of nanometers thick—over which the magnetization direction rotates continuously to connect the orientations of neighboring domains, balancing exchange energy and magnetostatic costs. There are two primary types of domain walls: Bloch walls, where the magnetization rotates perpendicular to the wall plane, first theoretically described by in 1932, and Néel walls, where the rotation occurs in the plane of the wall, particularly favored in thin films to minimize stray fields, as proposed by Louis Néel in the 1950s. Under an applied magnetic field, domain walls move, expanding domains aligned with the field and shrinking those opposed, which drives the net magnetization change. The dynamic response of domains to cyclic variation of the external magnetic field H\mathbf{H} is characterized by magnetic hysteresis, where the magnetic induction B\mathbf{B} does not follow the same path during increasing and decreasing fields, forming a closed loop in the B-H plane. Key features of the hysteresis loop include remanence, the residual B\mathbf{B} when H=0\mathbf{H} = 0 after saturation, and coercivity, the reverse H\mathbf{H} required to reduce B\mathbf{B} to zero, both arising from the energy barriers to domain wall motion due to pinning at defects. The area enclosed by the loop represents the energy dissipated per cycle as heat, quantified by the integral HdB\oint \mathbf{H} \cdot d\mathbf{B}, which accounts for irreversible work during domain reconfiguration. A manifestation of the discontinuous nature of domain wall motion is the Barkhausen effect, observed as discrete jumps in magnetization when the field changes, producing audible noise or voltage pulses in detection coils due to sudden unpinning and rapid wall displacement over microscopic avalanches. This phenomenon was first reported by Heinrich Barkhausen in 1919 during experiments on ferromagnetic hysteresis. As temperature increases toward the Curie point, thermal agitation disrupts domain stability, causing walls to become more mobile and domains to grow larger to further minimize energy, until at the the ordered domain structure collapses entirely, transitioning the material to paramagnetism.

Electromagnetism Connections

Electromagnets

An electromagnet is a device that generates a magnetic field through the application of electric current to a coil of wire, typically wound around a ferromagnetic core to enhance the field strength. The basic construction involves wrapping insulated copper or aluminum wire into multiple turns, or a coil, around a core made of soft iron or another high-permeability material, which concentrates the magnetic flux lines and amplifies the field. This amplification occurs because the magnetic flux density BB inside the core is proportional to the relative permeability μr\mu_r of the material, where B=μ0μrHB = \mu_0 \mu_r H and μ0\mu_0 is the permeability of free space, allowing fields much stronger than those produced by air-core coils alone. For practical designs, solenoids and toroids are common geometries that produce controllable magnetic fields. A solenoid consists of a helical coil, often with an iron core, where the magnetic field inside is uniform and given by B=μnIB = \mu n I, with μ=μ0μr\mu = \mu_0 \mu_r, nn the number of turns per unit length, and II the current. Toroids, formed by bending a solenoid into a closed loop, provide even more uniform fields within their core, approximating the same formula B=μnIB = \mu n I for thin windings, and are used to minimize external fringing fields. These configurations allow precise control of the field strength by varying the current, enabling the magnetism to be turned on and off instantly./University_Physics_II_-Thermodynamics_Electricity_and_Magnetism(OpenStax)/12%3A_Sources_of_Magnetic_Fields/12.07%3A_Solenoids_and_Toroids) Electromagnets find widespread use in applications requiring switchable magnetism, such as lifting magnets in industrial settings and electrical relays. Lifting electromagnets, often large solenoids with iron cores, are employed to hoist scrap metal in recycling yards by energizing the coil to create a strong attractive field, which is released by cutting the current. Relays utilize smaller electromagnets to control circuits, where the coil's activation moves an armature to open or close contacts, functioning as an electrically operated switch for on/off operation in devices like starters and sensors. Advanced electromagnets employ superconducting materials to achieve exceptionally high fields without resistance losses. Superconducting electromagnets use coils of materials like niobium-titanium, cooled to cryogenic temperatures (near 4 K), enabling persistent currents that generate fields up to several teslas with zero electrical resistance. In medical imaging, such as MRI scanners, these produce homogeneous fields of 1 to 7 T for detailed anatomical visualization. Despite their versatility, electromagnets have inherent limitations, including core saturation and thermal heating. Ferromagnetic cores saturate when the magnetic flux density reaches a material-specific maximum (typically 1.5–2 T for soft iron), beyond which further current increases yield diminishing returns in field strength. Additionally, resistive losses in the coil windings cause Joule heating (P=I2RP = I^2 R), which can overheat the device and limit continuous operation unless mitigated by cooling systems.

Relativity and Unified View

In special relativity, magnetic fields arise as a relativistic correction to electric fields when observed from different inertial frames. For an observer at rest relative to a stationary electric charge, only an electric field is present, but for an observer moving relative to that charge, the transformed electromagnetic field includes a magnetic component due to the Lorentz transformation of the fields. This effect ensures that the laws of electromagnetism remain consistent across frames, with the magnetic field emerging from the velocity-dependent aspects of the electric field. A key example illustrates this: consider a positive test charge moving parallel to a stationary line of positive charges, which produce a radial electric field. In the rest frame of the test charge, the line charges appear contracted due to length contraction, altering the electric field and resulting in an attractive force; however, in the lab frame, this attraction manifests as the Lorentz force F=qv×BF = q \mathbf{v} \times \mathbf{B}, where the magnetic field B\mathbf{B} is generated by the effective current from the transformed charge distribution. This demonstrates that the magnetic force on the moving charge derives directly from the relativistic transformation of the original electric field, without invoking magnetism as a separate entity. The full unification of electric and magnetic fields occurs in Maxwell's equations, which are invariant under Lorentz transformations when expressed in covariant form using the electromagnetic field tensor. This invariance resolves apparent asymmetries in classical electromagnetism for moving bodies, showing that electric and magnetic phenomena are intertwined aspects of a single electromagnetic field. Albert Einstein's 1905 paper "On the Electrodynamics of Moving Bodies" highlighted this connection, proposing that the distinction between electric and magnetic fields depends on the observer's motion, thereby linking electromagnetism to the principles of relativity. From a modern perspective, electromagnetism constitutes a unified fundamental force, with magnetism not being an independent phenomenon but rather a velocity-dependent manifestation of electric interactions under relativistic effects. This view extends in quantum electrodynamics, where the framework is quantized but the relativistic unification remains foundational.

Quantum and Modern Perspectives

Quantum Origin

The quantum mechanical origin of magnetism in atoms arises from the intrinsic angular momenta of electrons, specifically their orbital angular momentum L\mathbf{L} and spin angular momentum S\mathbf{S}. The orbital contribution generates a magnetic moment through the electron's circulation around the nucleus, analogous to a current loop, while the spin contribution stems from the electron's intrinsic rotation, a purely quantum phenomenon without classical counterpart. The total atomic magnetic moment operator is μ=μB(L+2S)\boldsymbol{\mu} = -\frac{\mu_B}{\hbar} (\mathbf{L} + 2\mathbf{S}), where μB=e/(2me)\mu_B = e \hbar / (2 m_e) is the , ee and mem_e are the electron charge and mass. In the coupled basis, where the total angular momentum is J=L+S\mathbf{J} = \mathbf{L} + \mathbf{S}, the expectation value of the magnetic moment is gμBJ/-g \mu_B \mathbf{J}/\hbar, with gg the Landé g-factor that accounts for the coupling between L\mathbf{L} and S\mathbf{S}. This vector model of the atom yields g=1g = 1 for pure orbital motion and g=2g = 2 for pure spin. In materials with free conduction electrons, such as metals, paramagnetism emerges from the partial alignment of electron spins in an external magnetic field, constrained by the Pauli exclusion principle. This Pauli paramagnetism arises because the field shifts the energy levels of spin-up and spin-down electrons, leading to a net magnetization proportional to the at the Fermi level, but without the exponential suppression seen in classical Curie paramagnetism at low temperatures. The susceptibility is χ=μ0μB2g(EF)\chi = \mu_0 \mu_B^2 g(E_F), where g(EF)g(E_F) is the density of states, remaining temperature-independent for degenerate electron gases. Ferromagnetism in solids originates from quantum exchange interactions, where the Pauli exclusion principle and for electrons with parallel spins compared to antiparallel configurations, particularly in partially filled d- or f-shells. This exchange energy, arising from the overlap of wavefunctions and the antisymmetry of the fermionic wavefunction, favors ferromagnetic alignment when the gain exceeds kinetic energy costs. For itinerant electrons in metals, the Stoner criterion quantifies this instability of the paramagnetic state toward ferromagnetism: IN(EF)>1I N(E_F) > 1, where II is the exchange integral and N(EF)N(E_F) the density of states at the Fermi energy; satisfaction of this condition, as in iron and , leads to band splitting and . A key distinction in quantum magnetism lies between itinerant and localized electron behaviors. Localized electrons, confined to atomic-like orbitals in insulators or Mott systems, retain well-defined atomic moments that interact via , producing ordered states like . In contrast, itinerant electrons in metallic bands delocalize, enabling collective band magnetism where manifests as a shift in the and spin polarization across the material, as observed in transition metals; this band model unifies weak itinerant ferromagnets like manganese alloys with strong localized ones like rare-earth compounds. Relativistically, the Dirac equation for electrons incorporates spin naturally and predicts a g-factor of exactly 2 for the spin magnetic moment, unifying the orbital and spin contributions without ad hoc assumptions. This arises from the equation's structure, iψt=cαpψ+βmc2ψi \hbar \frac{\partial \psi}{\partial t} = c \boldsymbol{\alpha} \cdot \mathbf{p} \psi + \beta m c^2 \psi, where the Dirac matrices α\boldsymbol{\alpha} and β\beta encode the electron's intrinsic magnetism. However, quantum electrodynamic corrections introduce anomalies, with the observed g-factor deviating as g/21α/(2π)0.00116g/2 - 1 \approx \alpha / (2\pi) \approx 0.00116, where α\alpha is the , arising from interactions.

Magnetic Monopoles

Magnetic monopoles are hypothetical particles that would carry a single magnetic charge, either north or south, in contrast to the observed paired north-south poles in all known magnets. Their existence would restore between and magnetism, as electric monopoles (isolated charges) are fundamental in . In , treat electric and magnetic fields asymmetrically, with B=0\nabla \cdot \mathbf{B} = 0 implying no magnetic charges, while E=ρe/ϵ0\nabla \cdot \mathbf{E} = \rho_e / \epsilon_0 allows density ρe\rho_e. The introduction of magnetic monopoles would extend these equations to include magnetic charge density ρm\rho_m and current Jm\mathbf{J}_m, yielding B=μ0ρm\nabla \cdot \mathbf{B} = \mu_0 \rho_m and ×E=Btμ0Jm\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t} - \mu_0 \mathbf{J}_m, alongside the symmetric magnetic counterparts to Ampère's and Faraday's laws. This symmetrization motivates theoretical pursuits, as monopoles would unify the treatment of electric and magnetic phenomena. In 1931, Paul Dirac proposed a quantum mechanical description of point-like magnetic monopoles to explain the observed quantization of electric charge. Dirac showed that the wave function of an electrically charged particle in the field of a monopole acquires a phase factor upon encircling the monopole, leading to the quantization condition eg=2πnceg = 2\pi n \hbar c, where ee is the electric charge, gg the magnetic charge, nn an integer, \hbar the reduced Planck's constant, and cc the speed of light. This condition implies that electric charge must be quantized in units compatible with the monopole's existence, providing an explanation for why all observed charges are integer multiples of the elementary charge. Within grand unified theories (GUTs) developed in the 1970s, monopoles emerge as stable topological solitons. In 1974, and Alexander Polyakov independently demonstrated that non-Abelian gauge theories, such as those in GUTs, admit monopole solutions where the magnetic field configuration is characterized by a , with the Higgs field pointing radially outward. These 't Hooft-Polyakov monopoles would have masses on the order of the GUT scale, around 101610^{16} GeV, and could have been produced copiously in the early shortly after the , serving as relics that dilute through cosmic expansion. Despite extensive searches, no magnetic monopoles have been confirmed experimentally. In cosmic rays, detectors like the Pierre Auger Observatory and IceCube have set stringent upper limits on monopole fluxes, such as below 101910^{-19} cm2^{-2} s1^{-1} sr1^{-1} for relativistic monopoles, ruling out significant populations from GUT relics without invoking mechanisms like to suppress their abundance. Candidate events, such as a 1982 signal at the Stanford accelerator interpreted as a monopole-induced , remain unverified and attributed to instrumental artifacts. In condensed matter systems, emergent monopole-like quasiparticles have been observed in spin ice materials, such as dysprosium titanate, where frustrated magnetic interactions lead to excitations behaving as free magnetic charges. Neutron scattering experiments in 2009 provided evidence for these monopoles, with dynamics matching theoretical predictions, and further studies in 2014 demonstrated their trapping and manipulation at low temperatures, confirming fractionalized spin configurations analogous to monopole pairs. More recently, in 2023, emergent monopoles were observed in hematite, an antiferromagnet, using quantum diamond magnetometry, revealing a rich tapestry of monopolar, dipolar, and quadrupolar magnetic charges. Recent theoretical models explore monopole analogs in two-dimensional systems through anyons, quasiparticles with fractional statistics intermediate between bosons and fermions. In fractional quantum Hall fluids, anyons exhibit braiding phases that mimic the Aharonov-Bohm effect of monopoles, enabling effective quantization and potential realizations of monopole-like defects in topological phases. These constructs, proposed since the and advanced in modern contexts, highlight monopoles' role in exotic statistics without requiring fundamental particles.

Units and Measurement

SI Units

The (SI) provides a coherent framework for measuring magnetic quantities, with units derived from seven base units fixed by fundamental constants since the 2019 redefinition. This ensures stability and universality in magnetism-related measurements, linking them to electrical and mechanical standards without reliance on artifacts. The magnetic flux density, denoted as B, is measured in teslas (T), where 1 T equals 1 weber per square meter (Wb/m²) or equivalently 1 newton per ampere-meter (N/(A·m)). The weber (Wb) itself is the unit of , defined as 1 volt-second (V·s), tying magnetic measurements to voltage and time standards. Electric currents driving magnetic fields are quantified in amperes (A), the SI base unit for current, now defined exactly by fixing the elementary charge at e=1.602176634×1019e = 1.602176634 \times 10^{-19} C, where 1 C = 1 A·s. , which relates to current in coils, uses the henry (H), with 1 H = 1 Wb/A or 1 V·s/A. The moment is expressed in ampere-square meters (A·m²), a derived unit reflecting the product of current and loop area in simple models. , a dimensionless measure of a material's response to an applied field (χ = M/H, where M is and H is the strength), requires no units in SI, emphasizing its role as a indicator minus one. For historical context, 1 T ≈ 10,000 gauss (G), bridging SI to older CGS systems, though SI prioritizes coherence over such legacy scales. Post-2019 SI redefinition, magnetic metrology relies on force (via newton, = kg·m/s²) or voltage standards for realization, with the permeability of vacuum (μ₀) now an experimentally determined constant at approximately 4π×1074\pi \times 10^{-7} , carrying a relative of 1.6 × 10^{-10} (CODATA 2022). This shift enhances precision in calibrating instruments like Hall probes or SQUIDs, ensuring magnetic units align with quantum electrical effects such as the Josephson junction for voltage.

CGS and Other Systems

The Gaussian variant of the centimeter-gram-second (CGS) system, also known as the electromagnetic unit (emu) system, has been widely used in magnetism, particularly in legacy on magnetostatics. In this system, the magnetic flux density [B](/page/Listofpunkrapartists)[B](/page/List_of_punk_rap_artists) is measured in gauss (G), the magnetic field strength HH in (Oe), and the magnetic moment in electromagnetic units (emu). These units treat [B](/page/Listofpunkrapartists)[B](/page/List_of_punk_rap_artists) and HH as having the same dimensions in , simplifying expressions where the permeability is unity. Key conversions between Gaussian CGS and the (SI) include 11 tesla (T) =104= 10^4 G for magnetic flux density and 11 per meter (A/m) =4π×103= 4\pi \times 10^{-3} Oe for magnetic field strength. The μ\mu in is given by μ=1+4πχ\mu = 1 + 4\pi \chi, where χ\chi is the , contrasting with the SI form that incorporates the permeability of free space μ0\mu_0. For magnetic moments, 1 corresponds to 10310^{-3} A·m² in SI units. Other unit systems include the Heaviside-Lorentz system, a rationalized form of favored in and for eliminating factors of 4π4\pi in field equations. , derived from Gaussian conventions, set fundamental constants like the to unity and equate the dimensions of magnetic induction BB and EE, aiding theoretical calculations in quantum magnetism. The CGS Gaussian system offers simplicity in vacuum calculations, where μ=1\mu = 1 avoids explicit constants like μ0\mu_0, making it preferable for and early literature. However, the SI system is advantageous for applications due to its unified electrical and magnetic units and practical scalability with larger base quantities. Despite SI's dominance, CGS persists in specialized fields like for compatibility with historical data.

Biological and Applied Aspects

Magnetism in Living Organisms

Magnetism plays a significant role in various biological processes, enabling organisms to sense and respond to the Earth's geomagnetic field for , orientation, and other functions. This , known as or , has been observed across diverse taxa, from prokaryotes to vertebrates. Mechanisms include the use of biogenic crystals and light-dependent chemical reactions involving radical pairs in cryptochromes, which allow detection of weak magnetic on the order of 50 microtesla, comparable to the Earth's field. One of the earliest discovered examples of biological magnetism is in , which synthesize intracellular chains of (Fe₃O₄) nanocrystals called . These structures act as miniature compasses, aligning the bacteria along geomagnetic field lines to orient toward optimal oxygen levels in aquatic sediments. The phenomenon was first reported in 1975 by Richard Blakemore, who observed these microbes in mud samples from a New England pond, noting their consistent swimming direction relative to a bar magnet. are membrane-bound organelles, typically 35-120 nanometers in size, produced via processes that ensure uniform crystal shape and alignment for maximal . In higher animals, magnetoreception facilitates long-distance migration. Migratory birds, such as European robins ( rubecula), use a light-dependent magnetic mediated by proteins in their retinas, where photoexcitation generates radical pairs whose spin states are influenced by the geomagnetic field, enabling directional sensing. This quantum-based mechanism, involving electron spin entanglement, allows birds to detect field inclination and polarity during nocturnal flights. Similarly, sea turtles like loggerhead hatchlings (Caretta caretta) imprint on the magnetic signatures of their natal beaches, using variations in field intensity and inclination as a "magnetic map" for homing across oceans; experiments shifting magnetic fields have redirected their swimming orientation accordingly. Evolutionary evidence suggests these abilities arose independently in birds and reptiles, possibly as adaptations to geomagnetic gradients aiding dispersal and resource location. In humans, magnetic fields are detectable through (), a technique that measures the weak biomagnetic signals produced by neuronal currents in the , typically in the range of 100–1000 femtotesla (fT, 10^{-15} T). These fields arise from synchronized synaptic activity and provide non-invasive insights into function, with applications in diagnosing and mapping cognition. The existence of human magnetoreception remains controversial; while some studies report subconscious responses, such as alpha-wave desynchronization, to rotating Earth-strength fields, others find no consistent behavioral effects, attributing signals to artifacts or non-specific arousal. Proposed mechanisms, potentially involving cryptochromes in the retina or in tissues, lack definitive validation, highlighting ongoing debates in the field.

Technological Applications

One of the most transformative applications of magnetism in data storage is the use of giant magnetoresistance (GMR) in hard disk drives (HDDs). Discovered independently in 1988 by Albert Fert and Peter Grünberg, GMR involves multilayer structures where the electrical resistance changes dramatically in response to an applied magnetic field, enabling the detection of tiny magnetic domains on disk platters. This effect, which earned Fert and Grünberg the 2007 Nobel Prize in Physics, revolutionized HDD read heads by increasing storage density from gigabits to terabits per square inch, allowing modern drives to store petabytes of data efficiently. GMR-based sensors remain integral to HDD technology, supporting the massive data demands of cloud computing and big data analytics. In electric motors and generators, the —arising from the interaction between a current-carrying conductor and a —drives the conversion of to mechanical work and vice versa. This principle underpins brushless permanent magnet motors in electric vehicles (EVs), where rotor magnets interact with stator currents to produce , enabling efficient propulsion with energy densities exceeding 5 kW/kg in advanced designs. For instance, EVs like those from major manufacturers achieve ranges over 500 km per charge partly due to optimized utilization in traction motors. In wind turbines, synchronous generators employ similar Lorentz interactions to convert blade rotation into electrical power, with direct-drive permanent magnet systems eliminating gearboxes for higher reliability in multi-megawatt offshore installations. Magnetic resonance imaging (MRI) leverages strong static s to align nuclear spins, primarily of atoms in molecules, for non-invasive medical diagnostics. Developed in the 1970s, with Paul Lauterbur's 1973 demonstration of spatial encoding via gradients marking a pivotal advance, MRI uses radiofrequency pulses to perturb these spins and detect relaxation signals for image reconstruction. Clinical MRI systems, operating at 1.5–3 Tesla fields, provide high-resolution images of soft tissues without , revolutionizing diagnostics for conditions like tumors and neurological disorders since FDA approval in 1984. The technique's sensitivity to variations enables functional MRI (fMRI) to map activity, aiding research and patient care. Magnetic (maglev) trains utilize superconducting magnets for repulsion-based suspension, achieving frictionless high-speed travel. In systems like Japan's , onboard niobium-titanium superconductors cooled to 4 K generate persistent currents that expel magnetic fields from guideway coils via the , creating repulsive forces for at speeds over 500 km/h. This technology, pioneered in concepts from the 1960s and operational in Shanghai's line since 2004, reduces energy consumption by 30% compared to wheeled and minimizes wear, supporting sustainable urban transport. Emerging applications in exploit electron spin alongside charge for next-generation devices, particularly in via spin valves—structures where spin-dependent transport controls current flow. Advances in the 2020s include graphene-based spin valves demonstrating high room-temperature spin injection efficiencies, enabling compact manipulation for scalable quantum processors. Researchers have also developed spin liquid states in , where entangled resist ordering to serve as robust qubits, potentially reducing decoherence in fault-tolerant quantum computers—as demonstrated in 2025 studies on materials like sodium-cobalt-antimony under . These innovations promise energy-efficient logic gates and memory with densities surpassing limits, with prototypes integrating spin valves into hybrid quantum-classical systems.

References

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