Hubbry Logo
Energy gapEnergy gapMain
Open search
Energy gap
Community hub
Energy gap
logo
7 pages, 0 posts
0 subscribers
Be the first to start a discussion here.
Be the first to start a discussion here.
Energy gap
Energy gap
from Wikipedia

In solid-state physics, an energy gap or band gap is an energy range in a solid where no electron states exist, i.e. an energy range where the density of states vanishes.

Especially in condensed matter physics, an energy gap is often known more abstractly as a spectral gap, a term which need not be specific to electrons or solids.

Band gap

[edit]

If an energy gap exists in the band structure of a material, it is called band gap. The physical properties of semiconductors are to a large extent determined by their band gaps, but also for insulators and metals the band structure—and thus any possible band gaps—govern their electronic properties.[1][2]

Superconductors

[edit]

For superconductors the energy gap is a region of suppressed density of states around the Fermi energy, with the size of the energy gap much smaller than the energy scale of the band structure. The superconducting energy gap is a key aspect in the theoretical description of superconductivity and thus features prominently in BCS theory. Here, the size of the energy gap indicates the energy gain for two electrons upon formation of a Cooper pair.[1][2][3] If a conventional superconducting material is cooled from its metallic state (at higher temperatures) into the superconducting state, then the superconducting energy gap is absent above the critical temperature , it starts to open upon entering the superconducting state at , and it grows upon further cooling. BCS theory predicts that the size of the superconducting energy gap for conventional superconductors at zero temperature scales with their critical temperature :[3] (with Boltzmann constant ).

Pseudogap

[edit]

If the density of states is suppressed near the Fermi energy but does not fully vanish, then this suppression is called pseudogap. Pseudogaps are experimentally observed in a variety of material classes; a prominent example are the cuprate high-temperature superconductors.[4]

Hard gap vs. soft gap

[edit]

If the density of states vanishes over an extended energy range, then this is called a hard gap. If instead the density of states exactly vanishes only for a single energy value (while being suppressed, but not vanishing for nearby energy values), then this is called a soft gap. A prototypical example of a soft gap is the Coulomb gap that exists in localized electron states with Coulomb interaction.[5]

References

[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
In condensed matter physics, an energy gap is a range of energies in which no electronic or quasiparticle states can exist, often referred to more abstractly as a spectral gap. While most commonly referring to the electronic band gap in solids—the minimum energy difference between the top of the valence band and the bottom of the conduction band, representing a forbidden energy range where no electron states exist—the term also applies to other phenomena such as the superconducting energy gap and pseudogaps, discussed in subsequent sections. This band gap fundamentally determines the material's electrical and optical properties, classifying solids as metals (overlapping bands, no gap), semiconductors (band gaps typically ~0.1–4 eV, including wide-bandgap types up to ~6 eV), or insulators (gaps typically >4 eV). In semiconductors, the band gap governs conductivity by controlling the thermal excitation of electrons from the valence band to the conduction band, with smaller gaps enabling higher carrier concentrations and thus greater electrical response, especially as temperature increases. Optically, the band gap dictates light absorption and emission wavelengths, as photons with energy matching or exceeding the gap can excite electrons, influencing material color—for instance, silicon (1.1 eV gap) appears dark due to visible light absorption, while wider-gap materials like gallium nitride (3.4 eV) transmit visible light and emit in the ultraviolet. Band gaps are categorized as direct (valence band maximum and conduction band minimum at the same momentum, enabling efficient photon interactions) or indirect (requiring phonon assistance for momentum conservation, reducing optical efficiency), with direct-gap materials like gallium arsenide (1.42 eV) excelling in light-emitting applications. The significance of the energy gap extends to diverse technologies, including where it enables devices such as LEDs, lasers, and solar cells by tuning emission or absorption spectra, and where wide-bandgap semiconductors like (3.2 eV) support high-voltage operation with low losses. Bandgap —through alloying, strain, or nanostructuring—allows precise control over these properties, as seen in III-V compounds for detectors or emitters.

Fundamentals

Definition

In quantum mechanics, an energy gap, also referred to as a spectral gap, denotes a range of energies within a system's spectrum where no quantum states are available, thereby prohibiting electron or other particle transitions across that interval. This absence of states arises from the discrete nature of quantum energy levels, distinguishing it from classical continuous spectra and influencing properties such as stability and excitation thresholds in physical systems. Mathematically, the energy gap ΔE\Delta E is quantified as the difference between the energy of the lowest unoccupied quantum state and the highest occupied state; for instance, in molecular systems, it is expressed as ΔE=ELUMOEHOMO\Delta E = E_{\text{LUMO}} - E_{\text{HOMO}}, where ELUMOE_{\text{LUMO}} is the energy of the lowest unoccupied molecular orbital and EHOMOE_{\text{HOMO}} is that of the highest occupied molecular orbital. This representation captures the minimal energy required to promote an electron from a filled to an empty state, a fundamental concept underlying optical and electrical responses in various materials. The notion of an energy gap is most prominently applied in to describe forbidden energy regions in electronic structures. It also extends to atomic, molecular, and , where discrete energy levels similarly produce gaps between allowed states, though the scales and mechanisms differ across these domains. In solid-state contexts, a specific manifestation is the band gap, representing the separation between in materials like semiconductors.

Historical Development

The concept of the energy gap in originated in the late 1920s amid efforts to apply to electron behavior in . , in his 1928 doctoral thesis, developed the periodic potential model, demonstrating how in a crystal lattice form extended wavefunctions that result in allowed energy bands separated by forbidden gaps, a result encapsulated in . This foundational work shifted understanding from free-electron models to periodic structures, laying the groundwork for band theory. In the early 1930s, Alan Wilson advanced Bloch's ideas by applying band theory to classify materials as metals, insulators, or semiconductors based on the positioning of the relative to these energy gaps. Wilson's 1931 paper introduced the notion that a significant in insulators prevents to conduction bands at typical temperatures, while narrower gaps in semiconductors allow thermal activation, thus explaining diverse electrical conductivities. These influential contributions by Bloch and Wilson established the energy gap as a central parameter in , influencing subsequent theoretical developments. Following , the 1950s saw intensified experimental and theoretical focus on semiconductors, where researchers like connected band gaps directly to device performance. Bardeen's work at Bell Laboratories and later at the University of Illinois explored and impurity effects on band gaps, elucidating how controlled doping modulates the gap to enable operation, a breakthrough recognized in the 1956 . This era bridged abstract band theory with practical electronics, highlighting the energy gap's role in conductivity control. The energy gap concept expanded into superconductivity in 1957 through the Bardeen-Cooper-Schrieffer (BCS) theory, which described a pairing mechanism opening an excitation gap in the superconducting state below the critical temperature. Decades later, in the late 1980s, the discovery of high-temperature cuprate superconductors revealed pseudogap features—partial gaps in the normal state—first evidenced by nuclear magnetic resonance studies showing suppressed density of states. These milestones underscored the energy gap's versatility across condensed matter phases.

Band Gap in Solids

Characteristics in Semiconductors and Insulators

In solids, the energy gap, denoted as EgE_g, represents the energy difference between the maximum of the valence band (EvE_v) and the minimum of the conduction band (EcE_c), expressed as Eg=EcEvE_g = E_c - E_v. This gap determines the material's ability to conduct by separating filled states from empty ones. Materials are classified based on the magnitude of EgE_g: metals exhibit Eg0E_g \approx 0 eV with overlapping , enabling free electron movement; semiconductors have EgE_g ranging from approximately 0.1 to 4 eV, allowing partial thermal excitation of electrons across the gap for moderate conductivity; and insulators possess Eg>4E_g > 4 eV, preventing conduction at due to insufficient to bridge the gap. In semiconductors, this intermediate gap facilitates tunable electrical properties through doping or temperature changes, while in insulators, the large gap ensures high resistivity. The band gap in semiconductors and insulators exhibits temperature dependence, generally decreasing with increasing primarily due to lattice expansion from anharmonic vibrations, which alters interatomic distances and band overlaps. This behavior is empirically modeled using relations like the Varshni equation, which fits experimental data for various materials. interactions also contribute to this reduction, enhancing electron-phonon coupling at higher temperatures. Representative examples illustrate these characteristics: , a quintessential , has Eg1.1E_g \approx 1.1 eV at , enabling its widespread use in . In contrast, serves as a classic insulator with Eg5.5E_g \approx 5.5 eV, reflecting its exceptional and stability but poor electrical conductivity.

Direct and Indirect Band Gaps

In , the nature of the band gap in semiconductors is classified as direct or indirect depending on the momentum-space alignment of the valence band maximum (VBM) and conduction band minimum (CBM) within the . A direct band gap arises when the VBM and CBM occur at the same wavevector , permitting vertical electronic transitions that inherently conserve as dictated by the selection rules for optical processes. This configuration allows electrons to move between bands solely through interaction with photons, without requiring additional momentum exchange. In contrast, an indirect band gap features the VBM and CBM at distinct points, such that a pure electronic transition across the gap would violate conservation. To enable such transitions, electrons must couple with lattice vibrations, or , to bridge the momentum mismatch, typically denoted as Δ**** ≈ _phonon. This phonon-mediated involvement introduces non-radiative pathways and reduces the overall transition probability, distinguishing indirect gaps from their direct counterparts. The distinction profoundly influences optical absorption and emission efficiencies in these materials. Direct semiconductors facilitate strong light-matter coupling, enabling efficient absorption above the energy Eg and radiative recombination, which is ideal for optoelectronic devices like LEDs and lasers. For instance, (GaAs) possesses a direct of approximately 1.43 eV, allowing for high-efficiency light emission in the near-infrared spectrum. Indirect band gap materials, however, exhibit weaker optical responses because assistance is required for both absorption and emission, often leading to predominant non-radiative decay and lower quantum yields. (Si) and (Ge) serve as representative examples, with indirect band gaps of about 1.1 eV and 0.67 eV, respectively, which contribute to their limited direct optical activity despite widespread use in . Phonon-assisted processes in indirect band gaps typically involve either the absorption of a phonon (for upward transitions) or its emission (for downward ones), with the phonon energy matching the difference in k-space. These second-order perturbations, described within Fermi's golden rule framework, result in transition rates that are suppressed by factors of 103 to 105 relative to direct processes due to the need for virtual intermediate states. Consequently, indirect semiconductors like Si and Ge rely on indirect optical absorption edges that tail into lower energies, but with significantly reduced coefficients compared to direct materials.

Superconducting Energy Gap

BCS Theory and Gap Formation

In the Bardeen-Cooper-Schrieffer () theory, the superconducting energy gap arises from the attractive interaction between electrons mediated by lattice vibrations, or phonons, which overcomes the repulsive forces at low temperatures. This interaction leads to the formation of Cooper pairs—bound states of two electrons with opposite momenta and spins near the EFE_F—resulting in a collective condensation that lowers the ground-state energy of the system. The pairing opens an energy gap of magnitude 2Δ2\Delta in the electronic around EFE_F, prohibiting low-energy single-particle excitations and enabling zero-resistance current flow. The magnitude of the superconducting gap Δ\Delta is determined self-consistently through the BCS gap equation, which balances the pairing potential against the at the . At zero , for a weak-coupling superconductor with phonon-mediated attraction limited by the Debye frequency ωD\omega_D, the gap is given by Δ(0)2ωDexp(1N(0)V),\Delta(0) \approx 2 \hbar \omega_D \exp\left(-\frac{1}{N(0) V}\right), where N(0)N(0) is the single-spin at EFE_F and VV is the effective pairing interaction strength. This exponential dependence highlights the sensitivity of the gap to the pairing mechanism, with typical values of Δ\Delta on the order of millielectronvolts for conventional superconductors. In the superconducting state, the elementary excitations are Bogoliubov quasiparticles rather than free electrons, with a dispersion relation that reflects the paired nature of the ground state: E(k)=ε(k)2+Δ2,E(\mathbf{k}) = \sqrt{\varepsilon(\mathbf{k})^2 + \Delta^2},
Add your contribution
Related Hubs
User Avatar
No comments yet.