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Raman scattering
Raman scattering
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In chemistry and physics, Raman scattering or the Raman effect (/ˈrɑːmən/) is the inelastic scattering of photons by matter, meaning that there is both an exchange of energy and a change in the light's direction. Typically this effect involves vibrational energy being gained by a molecule as incident photons from a visible laser are shifted to lower energy. This is called normal Stokes-Raman scattering.

Light has a certain probability of being scattered by a material. When photons are scattered, most of them are elastically scattered (Rayleigh scattering), such that the scattered photons have the same energy (frequency, wavelength, and therefore color) as the incident photons, but different direction. Rayleigh scattering usually has an intensity in the range 0.1% to 0.01% relative to that of a radiation source. An even smaller fraction of the scattered photons (about 1 in a million) can be scattered inelastically, with the scattered photons having an energy different (usually lower) from those of the incident photons—these are Raman scattered photons.[1] Because of conservation of energy, the material either gains or loses energy in the process.

The effect is exploited by chemists and physicists to gain information about materials for a variety of purposes by performing various forms of Raman spectroscopy. Many other variants of Raman spectroscopy allow rotational energy to be examined, if gas samples are used, and electronic energy levels may be examined if an X-ray source is used, in addition to other possibilities. More complex techniques involving pulsed lasers, multiple laser beams and so on are known.

The Raman effect is named after Indian scientist C. V. Raman, who discovered it in 1928 with assistance from his student K. S. Krishnan. Raman was awarded the 1930 Nobel Prize in Physics for his discovery of Raman scattering.

History

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First page to Molecular Diffraction of Light (1922)
First page of Molecular Diffraction of Light (1922)

The elastic light scattering phenomena called Rayleigh scattering, in which light retains its energy, was described in the 19th century. The intensity of Rayleigh scattering is about 10−3 to 10−4 compared to the intensity of the exciting source.[2] In 1908, another form of elastic scattering, called Mie scattering was discovered.

The inelastic scattering of light was predicted by Adolf Smekal in 1923[3] and in older German-language literature it has been referred to as the Smekal-Raman-Effekt.[4] In 1922, Indian physicist C. V. Raman published his work on the "Molecular Diffraction of Light", the first of a series of investigations with his collaborators that ultimately led to his discovery (on 16 February 1928) of the radiation effect that bears his name. The Raman effect was first reported by Raman and his coworker K. S. Krishnan,[5] and independently by Grigory Landsberg and Leonid Mandelstam, in Moscow on 21 February 1928 (5 days after Raman and Krishnan). In the former Soviet Union, Raman's contribution was always disputed; thus in Russian scientific literature the effect is usually referred to as "combination scattering" or "combinatory scattering". Raman received the Nobel Prize in 1930 for his work on the scattering of light.[6]

In 1998 the Raman effect was designated a National Historic Chemical Landmark by the American Chemical Society in recognition of its significance as a tool for analyzing the composition of liquids, gases, and solids.[7]

Instrumentation

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An early Raman spectrum of benzene published by Raman and Krishnan.[8]
Schematic of a dispersive Raman spectroscopy setup in a 180° backscattering arrangement.[9]

Modern Raman spectroscopy nearly always involves the use of lasers as an exciting light source. Because lasers were not available until more than three decades after the discovery of the effect, Raman and Krishnan used a mercury lamp and photographic plates to record spectra.[10] Early spectra took hours or even days to acquire due to weak light sources, poor sensitivity of the detectors and the weak Raman scattering cross-sections of most materials. The most common modern detectors are charge-coupled devices (CCDs). Photodiode arrays and photomultiplier tubes were common prior to the adoption of CCDs.[11]

Theory

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The following focuses on the theory of normal (non-resonant, spontaneous, vibrational) Raman scattering of light by discrete molecules. X-ray Raman spectroscopy is conceptually similar but involves excitation of electronic, rather than vibrational, energy levels.

Molecular vibrations

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Raman scattering generally gives information about vibrations within a molecule. In the case of gases, information about rotational energy can also be gleaned.[12] For solids, phonon modes may also be observed.[13] The basics of infrared absorption regarding molecular vibrations apply to Raman scattering although the selection rules are different.

Degrees of freedom

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For any given molecule, there are a total of 3N degrees of freedom, where N is the number of atoms. This number arises from the ability of each atom in a molecule to move in three dimensions.[14] When dealing with molecules, it is more common to consider the movement of the molecule as a whole. Consequently, the 3N degrees of freedom are partitioned into molecular translational, rotational, and vibrational motion. Three of the degrees of freedom correspond to translational motion of the molecule as a whole (along each of the three spatial dimensions). Similarly, three degrees of freedom correspond to rotations of the molecule about the , , and -axes. Linear molecules only have two rotations because rotations along the bond axis do not change the positions of the atoms in the molecule. The remaining degrees of freedom correspond to molecular vibrational modes. These modes include stretching and bending motions of the chemical bonds of the molecule. For a linear molecule, the number of vibrational modes is 3N-5, whereas for a non-linear molecule the number of vibrational modes is 3N-6.[14]

Vibrational energy

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Molecular vibrational energy is known to be quantized and can be modeled using the quantum harmonic oscillator (QHO) approximation or a Dunham expansion when anharmonicity is important. The vibrational energy levels according to the QHO are

,

where n is a quantum number. Since the selection rules for Raman and infrared absorption generally dictate that only fundamental vibrations are observed, infrared excitation or Stokes Raman excitation results in an energy change of

The energy range for vibrations is in the range of approximately 5 to 3500 cm−1. The fraction of molecules occupying a given vibrational mode at a given temperature follows a Boltzmann distribution. A molecule can be excited to a higher vibrational mode through the direct absorption of a photon of the appropriate energy, which falls in the terahertz or infrared range. This forms the basis of infrared spectroscopy. Alternatively, the same vibrational excitation can be produced by an inelastic scattering process. This is called Stokes Raman scattering, by analogy with the Stokes shift in fluorescence discovered by George Stokes in 1852, with light emission at longer wavelength (now known to correspond to lower energy) than the absorbed incident light. Conceptually similar effects can be caused by neutrons or electrons rather than light.[15] An increase in photon energy which leaves the molecule in a lower vibrational energy state is called anti-Stokes scattering.

Raman scattering

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Raman scattering is conceptualized as involving a virtual electronic energy level which corresponds to the energy of the exciting laser photons. Absorption of a photon excites the molecule to the imaginary state and re-emission leads to Raman or Rayleigh scattering. In all three cases the final state has the same electronic energy as the initial state but is higher in vibrational energy in the case of Stokes Raman scattering, lower in the case of anti-Stokes Raman scattering or the same in the case of Rayleigh scattering. Normally this is thought of in terms of wavenumbers, where is the wavenumber of the laser and is the wavenumber of the vibrational transition. Thus Stokes scattering gives a wavenumber of while is given for anti-Stokes. When the exciting laser energy corresponds to an actual electronic excitation of the molecule then the resonance Raman effect occurs.

A classical physics based model is able to account for Raman scattering and predicts an increase in the intensity which scales with the fourth-power of the light frequency. Light scattering by a molecule is associated with oscillations of an induced electric dipole. The oscillating electric field component of electromagnetic radiation may bring about an induced dipole in a molecule which follows the alternating electric field which is modulated by the molecular vibrations. Oscillations at the external field frequency are therefore observed along with beat frequencies resulting from the external field and normal mode vibrations.[10][2]

The different possibilities of light scattering: Rayleigh scattering (no exchange of energy: incident and scattered photons have the same energy), Stokes Raman scattering (atom or molecule absorbs energy: scattered photon has less energy than the incident photon) and anti-Stokes Raman scattering (atom or molecule loses energy: scattered photon has more energy than the incident photon)

The spectrum of the scattered photons is termed the Raman spectrum. It shows the intensity of the scattered light as a function of its frequency difference Δν to the incident photons, more commonly called a Raman shift. The locations of corresponding Stokes and anti-Stokes peaks form a symmetric pattern around the RayleighΔν=0 line. The frequency shifts are symmetric because they correspond to the energy difference between the same upper and lower resonant states. The intensities of the pairs of features will typically differ, though. They depend on the populations of the initial states of the material, which in turn depend on the temperature. In thermodynamic equilibrium, the lower state will be more populated than the upper state. Therefore, the rate of transitions from the more populated lower state to the upper state (Stokes transitions) will be higher than in the opposite direction (anti-Stokes transitions). Correspondingly, Stokes scattering peaks are stronger than anti-Stokes scattering peaks. Their ratio depends on the temperature, and can therefore be exploited to measure it:

Selection rules

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In contrast to IR spectroscopy, where there is a requirement for a change in dipole moment for vibrational excitation to take place, Raman scattering requires a change in polarizability. A Raman transition from one state to another is allowed only if the molecular polarizability of those states is different. For a vibration, this means that the derivative of the polarizability with respect to the normal coordinate associated to the vibration is non-zero: . In general, a normal mode is Raman active if it transforms with the same symmetry of the quadratic forms , which can be verified from the character table of the molecule's point group. As with IR spectroscopy, only fundamental excitations () are allowed according to the QHO. There are however many cases where overtones are observed. The rule of mutual exclusion, which states that vibrational modes cannot be both IR and Raman active, applies to certain molecules.

The specific selection rules state that the allowed rotational transitions are , where is the rotational state. This generally is only relevant to molecules in the gas phase where the Raman linewidths are small enough for rotational transitions to be resolved.

A selection rule relevant only to ordered solid materials states that only phonons with zero phase angle can be observed by IR and Raman, except when phonon confinement is manifest.[13]

Symmetry and polarization

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Monitoring the polarization of the scattered photons is useful for understanding the connections between molecular symmetry and Raman activity which may assist in assigning peaks in Raman spectra.[16] Light polarized in a single direction only gives access to some Raman–active modes, but rotating the polarization gives access to other modes. Each mode is separated according to its symmetry.[17]

The symmetry of a vibrational mode is deduced from the depolarization ratio ρ, which is the ratio of the Raman scattering with polarization orthogonal to the incident laser and the Raman scattering with the same polarization as the incident laser: Here is the intensity of Raman scattering when the analyzer is rotated 90 degrees with respect to the incident light's polarization axis, and the intensity of Raman scattering when the analyzer is aligned with the polarization of the incident laser.[18] When polarized light interacts with a molecule, it distorts the molecule which induces an equal and opposite effect in the plane-wave, causing it to be rotated by the difference between the orientation of the molecule and the angle of polarization of the light wave. If , then the vibrations at that frequency are depolarized; meaning they are not totally symmetric.[19][18]

Stimulated Raman scattering and Raman amplification

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The Raman-scattering process as described above takes place spontaneously; i.e., in random time intervals, one of the many incoming photons is scattered by the material. This process is thus called spontaneous Raman scattering.

On the other hand, stimulated Raman scattering can take place when some Stokes photons have previously been generated by spontaneous Raman scattering (and somehow forced to remain in the material), or when deliberately injecting Stokes photons ("signal light") together with the original light ("pump light"). In that case, the total Raman-scattering rate is increased beyond that of spontaneous Raman scattering: pump photons are converted more rapidly into additional Stokes photons. The more Stokes photons that are already present, the faster more of them are added. Effectively, this amplifies the Stokes light in the presence of the pump light, which is exploited in Raman amplifiers and Raman lasers.

Stimulated Raman scattering is a nonlinear optical effect.

Requirement for space-coherence

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Suppose that the distance between two points A and B of an exciting beam is x. Generally, as the exciting frequency is not equal to the scattered Raman frequency, the corresponding relative wavelengths λ and λ' are not equal. Thus, a phase-shift Θ = 2πx(1/λ − 1/λ') appears. For Θ = π, the scattered amplitudes are opposite, so that the Raman scattered beam remains weak.

  • A crossing of the beams may limit the path x.

Several tricks may be used to get a larger amplitude:

  • In an optically anisotropic crystal, a light ray may have two modes of propagation with different polarizations and different indices of refraction. If energy may be transferred between these modes by a quadrupolar (Raman) resonance, phases remain coherent along the whole path, transfer of energy may be large. It is an Optical parametric generation.[citation needed]
  • Light may be pulsed, so that beats do not appear. In Impulsive Stimulated Raman Scattering (ISRS),[20][21][22][23] the length of the pulses must be shorter than all relevant time constants.[24] Interference of Raman and incident lights is too short to allow beats, so that it produces a frequency shift roughly, in best conditions, inversely proportional to the cube of the pulse length.

In labs, femtosecond laser pulses must be used because the ISRS becomes very weak if the pulses are too long. Thus ISRS cannot be observed using nanosecond pulses making ordinary time-incoherent light.[citation needed]

Inverse Raman effect

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The inverse Raman effect is a form of Raman scattering first noted by W. J. Jones and Boris P. Stoicheff. In some circumstances, Stokes scattering can exceed anti-Stokes scattering; in these cases the continuum (on leaving the material) is observed to have an absorption line (a dip in intensity) at νLM. This phenomenon is referred to as the inverse Raman effect; the application of the phenomenon is referred to as inverse Raman spectroscopy, and a record of the continuum is referred to as an inverse Raman spectrum.

In the original description of the inverse Raman effect,[25] the authors discuss both absorption from a continuum of higher frequencies and absorption from a continuum of lower frequencies. They note that absorption from a continuum of lower frequencies will not be observed if the Raman frequency of the material is vibrational in origin and if the material is in thermal equilibrium.

Supercontinuum generation

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For high-intensity continuous wave (CW) lasers, stimulated Raman scattering can be used to produce a broad bandwidth supercontinuum. This process can also be seen as a special case of four-wave mixing, in which the frequencies of the two incident photons are equal and the emitted spectra are found in two bands separated from the incident light by the phonon energies. The initial Raman spectrum is built up with spontaneous emission and is amplified later on. At high pumping levels in long fibers, higher-order Raman spectra can be generated by using the Raman spectrum as a new starting point, thereby building a chain of new spectra with decreasing amplitude. The disadvantage of intrinsic noise due to the initial spontaneous process can be overcome by seeding a spectrum at the beginning, or even using a feedback loop as in a resonator to stabilize the process. Since this technology easily fits into the fast evolving fiber laser field and there is demand for transversal coherent high-intensity light sources (i.e., broadband telecommunication, imaging applications), Raman amplification and spectrum generation might be widely used in the near-future.[citation needed]

Applications

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Raman spectroscopy employs the Raman effect for substances analysis. The spectrum of the Raman-scattered light depends on the molecular constituents present and their state, allowing the spectrum to be used for material identification and analysis. Raman spectroscopy is used to analyze a wide range of materials, including gases, liquids, and solids. Highly complex materials such as biological organisms and human tissue[26] can also be analyzed by Raman spectroscopy.

For solid materials, Raman scattering is used as a tool to detect high-frequency phonon and magnon excitations.

Raman lidar is used in atmospheric physics to measure the atmospheric extinction coefficient and the water vapour vertical distribution.

Due to its velocity-selective nature, the stimulated Raman transition is useful for cooling atoms.[27] It also enables the construction of atom interferometer by providing a well-defined momentum kick.[28] Stimulated Raman transitions are also widely used for manipulating a trapped ion's energy levels, and thus basis qubit states.

Raman spectroscopy can be used to determine the force constant and bond length for molecules that do not have an infrared absorption spectrum.

Raman amplification is used in optical amplifiers.

The Raman effect is also involved in producing the appearance of the blue sky (see Rayleigh Scattering: 'Rayleigh scattering of molecular nitrogen and oxygen in the atmosphere includes elastic scattering as well as the inelastic contribution from rotational Raman scattering in air').

Raman spectroscopy has been used to chemically image small molecules, such as nucleic acids, in biological systems by a vibrational tag.[29]

See also

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References

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Further reading

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Raman scattering, also known as the Raman effect, is the of photons by atoms or molecules in a , resulting in a shift of the scattered light's relative to the incident light due to exchange with vibrational, rotational, or other low-energy excitations. This phenomenon contrasts with elastic , where the remains unchanged, and only a tiny fraction (approximately 1 in 10^6 to 10^7 photons) of the scattered light exhibits the Raman shift, which provides a spectroscopic fingerprint of the 's molecular structure. The effect was discovered in 1928 by Indian physicist Sir Chandrasekhara Venkata Raman and his student during experiments on the scattering of monochromatic light in liquids such as and , where they observed modified wavelengths in the scattered spectrum. Independently, Soviet physicists Grigory Landsberg and Leonid Mandelstam reported similar observations in crystals that same year. For this groundbreaking work on light scattering, Raman was awarded the 1930 , becoming the first Asian recipient in the sciences. Raman scattering forms the basis of , a non-destructive analytical technique that probes , phase, polymorphism, and stress in solids, liquids, and gases without requiring . The technique excels in identifying symmetric molecular vibrations inaccessible to and has applications in fields ranging from and pharmaceuticals to forensics and biomedical imaging, often enhanced by lasers for greater sensitivity since the . Quantum mechanically, it is described by the Kramers-Heisenberg-Dirac dispersion formula, involving virtual energy states and changes in the scatterer.

Introduction and History

Definition and Phenomenon

Raman scattering is the inelastic scattering of photons by molecules, in which the scattered light experiences a shift in frequency due to the exchange of energy with the molecular vibrational or rotational modes. This process occurs when an incident photon interacts with a molecule, temporarily exciting it to a virtual intermediate state before the molecule returns to a different vibrational or rotational energy level, resulting in the emission of a scattered photon with altered energy. Unlike elastic , where the scattered retains the same frequency as the incident light with no net transfer, Raman scattering involves a measurable energy exchange, leading to either Stokes scattering (lower frequency, longer wavelength) or anti-Stokes scattering (higher frequency, shorter wavelength). In Stokes Raman scattering, the gains from the , transitioning to a higher vibrational or rotational state, while in anti-Stokes scattering, the loses to the , starting from an already excited state. The basic process can be schematically described as follows: an incident is absorbed by the , promoting it to a short-lived virtual that does not correspond to a real electronic ; from this state, the emits a scattered while relaxing to a different vibrational or rotational level in the ground electronic state. This mediation distinguishes Raman scattering from resonant absorption-emission processes, as the intermediate state exists only transiently during the scattering event. Raman signals are inherently weak, typically on the order of 10^{-6} to 10^{-7} of the incident light intensity, due to the low probability of inelastic scattering events compared to elastic ones. The intensity depends on factors such as the laser excitation wavelength—shorter wavelengths generally enhance scattering cross-sections—and the sample's molecular polarizability and concentration. For example, in gaseous samples, rotational Raman scattering is often prominent due to well-defined molecular orientations, whereas in liquids or solids, vibrational modes dominate the spectra because of denser intermolecular interactions and broader rotational broadening.

Discovery and Early Development

The Raman effect was discovered in 1928 by Indian physicist Chandrasekhara Venkata Raman and his student at the Indian Association for the Cultivation of Science in Calcutta. The phenomenon had been theoretically predicted in 1923 by Austrian physicist Adolf Smekal. They observed the inelastic scattering of light while passing through various liquids, such as , , and , using a spectrograph to detect frequency shifts in the scattered light relative to the incident beam. These shifts, later identified as corresponding to molecular vibrational and rotational transitions, were reported in their seminal paper published on 16 February 1928. For this groundbreaking work on light scattering, Raman was awarded the in 1930, becoming the first Asian recipient in the sciences. Independently, Soviet physicists Grigory Landsberg and Leonid Mandelstam observed the same phenomenon just days later, on 21 February 1928, at . Their experiment involved illuminating a quartz with a mercury and recording the scattered at a 90-degree angle using a spectrograph, which revealed modified spectral lines distinct from . This confirmation was published in July 1928, highlighting the effect's occurrence in solids as well as liquids. Early theoretical interpretations of the Raman effect emerged in the late 1920s and 1930s, building on the Kramers-Heisenberg-Dirac dispersion formula. Developed initially by Hendrik Kramers and in 1925 and refined by in 1927, the formula provided a quantum mechanical framework for light scattering by atoms and molecules, treating the process as occurring through virtual intermediate states rather than real electronic transitions. This approach explained the inelastic nature of the scattering without requiring in the intermediate steps, aligning with the observed frequency shifts. In the pre-laser era, experimental challenges dominated Raman studies due to the inherently weak intensity of scattered signals, which were typically a million times fainter than . Long exposure times—often several hours—were required on photographic plates to capture spectra, limiting observations to highly samples like liquids and crystals under intense illumination from mercury arcs. Despite these hurdles, the 1930s saw the development of dedicated Raman spectrometers, such as those pioneered by George Placzek, incorporating and improved spectrographs for better resolution. These advancements enabled initial applications in chemistry, where Raman spectra were used to identify molecular structures and vibrational modes in organic compounds, complementing for structural elucidation in the 1930s and 1940s.

Molecular and Quantum Foundations

Vibrational and Rotational Modes

Molecules possess three degrees of freedom per atom, corresponding to translation along the x, y, and z axes, resulting in a total of 3N degrees of freedom for a molecule with N atoms. Three of these are translational degrees of freedom for the molecule as a whole, and for non-linear molecules, there are three rotational degrees of freedom, leaving 3N-6 vibrational degrees of freedom; for linear molecules, there are only two rotational degrees of freedom, yielding 3N-5 vibrational degrees of freedom. These vibrational modes represent the internal oscillations of atoms relative to one another, which are crucial for Raman scattering as they correspond to the energy changes observed in scattered light. Vibrational motion in molecules is often approximated using the quantum harmonic oscillator model, where the potential energy is given by V=12k(xx0)2V = \frac{1}{2} k (x - x_0)^2, with kk as the force constant and x0x_0 as the equilibrium position. In this model, the energy levels are quantized as Ev=ω(v+12)E_v = \hbar \omega (v + \frac{1}{2}), where vv is the vibrational quantum number (an integer starting from 0), \hbar is the reduced Planck's constant, and ω\omega is the angular vibrational frequency. This approximation assumes a parabolic potential, leading to equally spaced energy levels separated by ω\hbar \omega, which provides a foundational understanding of the discrete energy transitions involved in Raman processes. Rotational motion is described by the approximation, treating the molecule as a fixed structure rotating about its . The rotational energy levels are given by EJ=BJ(J+1)E_J = B J(J+1), where JJ is the rotational (a non-negative integer), and B=22IB = \frac{\hbar^2}{2I} is the rotational constant, with \hbar as the reduced Planck's constant and II as the . Each level JJ has a degeneracy of 2J+12J+1, reflecting the possible projections of along a quantization axis, and the energy spacing increases quadratically with JJ, influencing the in Raman spectra. In polyatomic molecules, the vibrational manifest as normal modes, which are collective oscillations where all atoms move in phase with the same frequency. These modes are classified into stretching vibrations, such as symmetric stretches (where bond lengths change in unison) and asymmetric stretches (where bonds alternately lengthen and shorten), as well as bending modes including scissoring, rocking, wagging, and twisting. The specific forms of these normal modes are determined by the molecule's symmetry, often analyzed using point groups like C2vC_{2v} for or D3hD_{3h} for , which dictate the irreducible representations and degeneracies of the modes. For example, in (a linear molecule), the three normal modes consist of one symmetric stretch (inactive in but Raman-active), one asymmetric stretch, and one degenerate bending mode. Real molecular vibrations deviate slightly from the ideal harmonic model due to , arising from the asymmetric shape of the actual , which allows for higher-order terms beyond the quadratic approximation. This leads to effects such as , where transitions to higher vibrational states (Δv>1\Delta v > 1) occur at frequencies lower than integer multiples of the fundamental, and enables weak interactions between modes that would otherwise be forbidden. While these deviations are small for low-energy vibrations, they become more pronounced in excited states and provide subtle corrections to the energy levels relevant for detailed Raman analysis.

Quantum Theory of Inelastic Scattering

The quantum mechanical description of Raman scattering emerges from time-dependent applied to the interaction between and , treating the process as a second-order transition where an incident excites the system to a virtual intermediate state before a scattered is emitted with a shift corresponding to a vibrational or difference. In this framework, the scattering is because the final state of the differs from the initial state by a small energy quantum, typically on the order of vibrational energies (\hbar \omega_{vib} ~ 100-4000 cm⁻¹), while the intermediate state is a non-resonant electronic excitation that does not satisfy for a real transition, ensuring the process remains virtual and coherent. This virtual excitation arises from the interaction Hamiltonian, where the of the incident couples the ground electronic state to an excited electronic manifold, followed by a second coupling to the scattered field, leading to no net change in electronic state but a shift in . The is rigorously captured by the Kramers-Heisenberg-Dirac (KHD) dispersion formula, derived using the correspondence principle and later formalized in , which expresses the induced tensor α as αfie[fμ^eeμ^iEeEiω+iΓ+fμ^eeμ^iEeEf+ω+iΓ],\alpha_{fi} \propto \sum_e \left[ \frac{\langle f | \hat{\mu} | e \rangle \langle e | \hat{\mu} | i \rangle}{E_e - E_i - \hbar \omega + i \Gamma} + \frac{\langle f | \hat{\mu} | e \rangle \langle e | \hat{\mu} | i \rangle}{E_e - E_f + \hbar \omega + i \Gamma} \right], where |i⟩ and |f⟩ are the initial and final molecular states (typically vibrational levels in the electronic ground state), |e⟩ sums over virtual electronic excited states, μ^\hat{\mu} is the electric operator, ω is the incident , E denotes energies, and Γ accounts for the finite lifetime of the intermediate state. The first term in the sum dominates for non-resonant , reflecting absorption to the followed by , while the complex denominator ensures unitarity and causality, with the imaginary part preventing divergences. This formula unifies Rayleigh (elastic) and Raman (inelastic) under a single quantum mechanical umbrella, with the energy shift ΔE = E_f - E_i determining the scattered ω_s = ω - ΔE/ℏ. In Raman spectra, two primary inelastic processes occur: Stokes scattering, where the molecule gains vibrational energy (ΔE = +ℏ ω_{vib}, ω_s < ω) from the photon, populating an excited vibrational state |v'⟩ from initial |v⟩, and anti-Stokes scattering, where the molecule loses energy (ΔE = -ℏ ω_{vib}, ω_s > ω), requiring thermal population of |v'⟩ beforehand. The intensity ratio of anti-Stokes to Stokes lines follows the , I_{anti-Stokes}/I_{Stokes} = (N_{v'}/N_v) = e^{-\hbar \omega_{vib}/kT}, where at (kT ~ 200 cm⁻¹), this factor suppresses anti-Stokes signals for modes above ~500 cm⁻¹ since higher vibrational levels are sparsely populated. This thermal dependence allows to probe temperature via the Stokes-anti-Stokes ratio without assuming beyond the quantum amplitudes. The differential scattering cross-section, quantifying the probability per unit solid angle per scatterer, is given by dσ/dΩ ∝ |α|^2, where |α|^2 averages over the polarizability tensor components, incorporating orientational and tensorial factors for isotropic samples. The scattered intensity is then I_s ∝ I_0 (dσ/dΩ), with I_0 the incident intensity. This expression, derived from the squared KHD amplitude, scales the weak Raman signal (typically 10^{-6} to 10^{-3} of elastic scattering) and highlights the role of molecular polarizability in determining observable intensities. When the incident frequency ω approaches an electronic transition (resonance condition, |E_e - E_i - ℏω| ≲ Γ), the denominator in the KHD formula shrinks, enhancing the cross-section by factors of 10² to 10⁶ through partial of real electronic states, as formalized in Albrecht's vibronic coupling theory where the A-term (Franck-Condon overlap) dominates for allowed transitions. This resonance Raman effect selectively amplifies coupled to the electronic mode, providing enhanced sensitivity for studying chromophores while the virtual non-resonant mechanism remains for off-resonance cases.

Selection Rules and Symmetry

Polarizability and Transition Rules

Raman scattering occurs when the polarizability of a molecule changes during a vibrational or rotational transition, allowing for inelastic light scattering. Specifically, a vibrational mode is Raman-active if the polarizability tensor α\alpha varies with the normal coordinate QQ of the vibration, such that αQ0\frac{\partial \alpha}{\partial Q} \neq 0. This contrasts with infrared (IR) absorption, where activity requires a change in the dipole moment μ\mu, i.e., μQ0\frac{\partial \mu}{\partial Q} \neq 0. As a result, Raman spectroscopy complements IR by probing modes that do not involve dipole changes, such as symmetric stretches in homonuclear diatomic molecules like N2_2 or O2_2. In centrosymmetric molecules, the rule dictates that vibrational modes active in Raman scattering are inactive in IR absorption, and vice versa. This arises from considerations: under inversion through the center of symmetry, the polarizability tensor (a second-rank tensor) remains unchanged, while the dipole moment (a vector) reverses sign. Thus, vibrations that alter the (IR-active) cannot change the (Raman-inactive) in such molecules, as exemplified by CO2_2, where the symmetric stretch is Raman-active but IR-inactive. For pure rotational Raman scattering in linear molecules, the selection rule is ΔJ=0,±2\Delta J = 0, \pm 2, where JJ is the rotational . This leads to spectral branches: the O branch for ΔJ=2\Delta J = -2, the Q branch for ΔJ=0\Delta J = 0 (absent in linear molecules due to zero intensity), and the S branch for ΔJ=+2\Delta J = +2. These branches appear as lines spaced by approximately 4B4B (where BB is the rotational constant), providing information on the molecular . Isotopic substitution affects Raman spectra by shifting vibrational frequencies due to changes in , which alter the in the vibrational potential. Heavier isotopes lower the frequency of modes involving those atoms, enabling identification of atomic contributions to specific . For instance, replacing 12^{12}C with 13^{13}C in organic molecules shifts C-H stretches, aiding structural elucidation in Raman . The depolarization ρ=II\rho = \frac{I_\perp}{I_\parallel}, where II_\perp and II_\parallel are the intensities of Raman-scattered perpendicular and parallel to the incident polarization, respectively, reveals mode . Totally symmetric modes yield ρ0\rho \approx 0 (polarized scattering), while non-totally symmetric or asymmetric modes give ρ34\rho \approx \frac{3}{4} (depolarized), as the of the tensor randomizes the scattered polarization.

Polarization Effects

In Raman scattering, the polarization of the incident and scattered light provides critical insights into the symmetry properties of molecular vibrations. Vibrational modes are classified according to the irreducible representations of the molecule's symmetry, which dictate the allowed components of the Raman tensor. For instance, in molecules belonging to the C3vC_{3v} , such as (NH₃), modes transform as A1A_1, EE, or other representations, determining which tensor elements contribute to the scattering intensity for specific polarization configurations. This classification arises from , where the Raman activity requires the derivative to belong to the same as the quadratic forms of the Cartesian coordinates. The Raman tensor, denoted as αij\alpha_{ij}, represents the change in molecular with respect to and transforms as a second-rank under the point group operations. It can be expressed as: α=(αxxαxyαxzαyxαyyαyzαzxαzyαzz)\alpha = \begin{pmatrix} \alpha_{xx} & \alpha_{xy} & \alpha_{xz} \\ \alpha_{yx} & \alpha_{yy} & \alpha_{yz} \\ \alpha_{zx} & \alpha_{zy} & \alpha_{zz} \end{pmatrix}
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