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10.3 Applications of Spectroscopy in Inorganic Chemistry

10.3 Applications of Spectroscopy in Inorganic Chemistry

Written by the Fiveable Content Team • Last updated August 2025
Written by the Fiveable Content Team • Last updated August 2025
🧶Inorganic Chemistry I
Unit & Topic Study Guides

Electronic Spectroscopy

UV-Visible Spectroscopy and Charge Transfer

UV-Vis spectroscopy is one of the most routine tools for characterizing coordination compounds. It measures how a complex absorbs light in the ultraviolet and visible regions, which directly tells you about the electronic transitions happening within the molecule.

When a complex absorbs a photon of the right energy, an electron gets promoted from a lower-energy state to a higher-energy one. The wavelengths absorbed (and therefore the colors you see) depend on the energy gap between those states.

Charge transfer (CT) transitions are especially prominent in UV-Vis spectra of coordination compounds. These involve the transfer of electron density between the metal and its ligands:

  • MLCT (metal-to-ligand charge transfer): An electron moves from a metal-centered orbital to a ligand-centered orbital. Common when the metal is electron-rich and the ligand has low-lying empty orbitals (e.g., π\pi^* orbitals on CO or bipyridine).
  • LMCT (ligand-to-metal charge transfer): An electron moves from a ligand-centered orbital to a metal-centered orbital. Common with highly oxidized metals and electron-rich ligands (e.g., MnO4\text{MnO}_4^-, where the intense purple color comes from LMCT).

CT bands are typically very intense (high molar absorptivity, often ε>1000L mol1cm1\varepsilon > 1000 \, \text{L mol}^{-1}\text{cm}^{-1}) because they are Laporte-allowed transitions.

Quantitative analysis relies on the Beer-Lambert law:

A=εbcA = \varepsilon b c

where AA is absorbance (unitless), ε\varepsilon is the molar absorptivity (L mol1cm1\text{L mol}^{-1}\text{cm}^{-1}), bb is the path length (cm), and cc is the concentration (mol L1\text{mol L}^{-1}). This relationship is linear at low concentrations and lets you determine unknown concentrations from measured absorbance.

d-d Transitions and Selection Rules

The d-d transitions are the other major category of electronic transitions in coordination compounds. These occur when an electron is excited from one d orbital to another within the same metal center, and they're responsible for the characteristic colors of many transition metal complexes.

Two selection rules govern whether a transition is "allowed" or "forbidden":

  1. Laporte selection rule: Transitions between states of the same parity (symmetry with respect to inversion) are forbidden. In a centrosymmetric complex (like a perfect octahedron), d orbitals are all gerade (g), so d-d transitions are formally Laporte-forbidden. They still occur, though, because molecular vibrations temporarily break the center of symmetry. This mechanism is called vibronic coupling, and it's why d-d bands are weak but not absent.
  2. Spin selection rule: Transitions that require a change in total spin multiplicity are forbidden. For example, going from a triplet state to a singlet state is spin-forbidden and will be extremely weak.

Because d-d transitions violate at least the Laporte rule, they tend to have low molar absorptivities (typically ε150L mol1cm1\varepsilon \approx 1\text{–}50 \, \text{L mol}^{-1}\text{cm}^{-1}), much weaker than CT bands.

The energy of d-d transitions depends on the ligand field splitting (Δ\Delta):

  • Strong-field ligands (e.g., CN^-, CO) produce large Δ\Delta values, shifting d-d absorptions to higher energy (shorter wavelength).
  • Weak-field ligands (e.g., I\text{I}^-, Br\text{Br}^-) produce small Δ\Delta values, shifting absorptions to lower energy (longer wavelength).

Note that geometry also matters. Tetrahedral complexes lack a center of inversion, so the Laporte rule is relaxed, and their d-d bands are often more intense than those of octahedral complexes (though Δtet\Delta_{\text{tet}} is smaller than Δoct\Delta_{\text{oct}}, roughly 49Δoct\frac{4}{9}\Delta_{\text{oct}}).

Vibrational Spectroscopy

Infrared (IR) Spectroscopy

IR spectroscopy probes the vibrational modes of molecules by measuring which infrared frequencies a sample absorbs. For a vibration to be IR-active, it must cause a change in the molecule's dipole moment.

Vibrational modes include symmetric and asymmetric stretching, bending, rocking, wagging, and twisting. Each type of bond vibrates at a characteristic frequency range, so you can use group frequencies to identify functional groups. For coordination chemistry, particularly useful absorptions include:

  • Metal-carbonyl stretches (νCO\nu_{\text{CO}}): Typically 1850–2125 cm1^{-1}. The exact position tells you about the degree of back-bonding from the metal to CO. More back-bonding weakens the C–O bond and lowers νCO\nu_{\text{CO}}.
  • Metal-halide and metal-nitrogen stretches: Found at lower frequencies (200–600 cm1^{-1}), often requiring far-IR measurements.
  • Coordinated vs. free ligand shifts: Comparing the IR spectrum of a free ligand to its coordinated form reveals which donor atoms are bound to the metal.

FTIR (Fourier transform IR) is the standard modern technique, offering better resolution and signal-to-noise than older dispersive instruments. ATR (attenuated total reflectance) accessories simplify sample preparation since you can press a solid or drop a liquid directly onto the crystal without making KBr pellets.

UV-Visible Spectroscopy and Charge Transfer, Understanding charge transfer, defects and surface states at hematite photoanodes - Sustainable ...

Raman Spectroscopy

Raman spectroscopy measures the inelastic scattering of monochromatic light (usually from a laser). When a photon interacts with a molecule, most photons scatter elastically (Rayleigh scattering, same frequency). A small fraction scatter inelastically:

  • Stokes scattering: The scattered photon has lower energy than the incident photon (molecule gains vibrational energy). This is the more commonly measured signal.
  • Anti-Stokes scattering: The scattered photon has higher energy (molecule loses vibrational energy). Weaker at room temperature because fewer molecules start in excited vibrational states.

For a vibration to be Raman-active, it must cause a change in the molecule's polarizability (how easily the electron cloud is distorted).

This is where the rule of mutual exclusion becomes useful: for molecules with a center of symmetry, vibrations that are IR-active are Raman-inactive, and vice versa. This means IR and Raman are complementary techniques. Together, they give you a more complete picture of a molecule's vibrational modes and can help confirm whether a complex is centrosymmetric.

  • Resonance Raman spectroscopy uses an excitation wavelength that coincides with an electronic absorption band, dramatically enhancing the Raman signal for vibrations coupled to that electronic transition. This is great for selectively probing metal-ligand bonds in colored complexes.
  • SERS (surface-enhanced Raman spectroscopy) amplifies signals by factors of 10610^6 or more using roughened metal surfaces (typically Au or Ag), enabling detection of very low concentrations.

Magnetic Resonance Spectroscopy

Nuclear Magnetic Resonance (NMR) Spectroscopy

NMR spectroscopy detects transitions between nuclear spin states in an applied magnetic field. Only nuclei with a nonzero spin quantum number (I0I \neq 0) are NMR-active.

The chemical shift (δ\delta, in ppm) reports how shielded or deshielded a nucleus is by its surrounding electron density. Different electronic environments produce different chemical shifts, making NMR a powerful structural probe.

Spin-spin coupling (J-coupling) between neighboring NMR-active nuclei splits signals into multiplets. The splitting pattern and coupling constant (JJ, in Hz) reveal connectivity and bond angles.

For inorganic and organometallic chemistry, NMR goes well beyond 1H^1\text{H} and 13C^{13}\text{C}:

  • 31P^{31}\text{P} NMR: Extremely useful for phosphine-containing complexes. 100% natural abundance and good sensitivity.
  • 19F^{19}\text{F} NMR: Useful for fluoride ligands and fluorinated ligands. Also 100% abundant and highly sensitive.
  • 15N^{15}\text{N} NMR: Low natural abundance (0.37%), but valuable for nitrogen-donor ligands when enriched samples are available.

2D NMR techniques (COSY, HSQC, HMBC) map out correlations between nuclei and are essential for assigning complex spectra. Solid-state NMR (using magic angle spinning) extends the technique to insoluble compounds, polymers, and heterogeneous catalysts that can't be dissolved for solution-phase measurements.

One important caveat: paramagnetic metal centers cause severe line broadening and large, unpredictable chemical shifts in NMR spectra. For strongly paramagnetic complexes, NMR may be impractical, and EPR becomes the better choice.

Electron Paramagnetic Resonance (EPR) Spectroscopy

EPR (also called ESR) spectroscopy is specifically designed for species with unpaired electrons. It works on the same basic principle as NMR but detects electron spin transitions rather than nuclear spin transitions.

Key parameters from an EPR spectrum:

  • g-factor: Analogous to chemical shift in NMR. Deviations from the free-electron value (ge=2.0023g_e = 2.0023) reflect spin-orbit coupling and the symmetry of the electronic environment. Anisotropic g-values (gxgygzg_x \neq g_y \neq g_z) reveal the symmetry at the metal center.
  • Hyperfine coupling: Splitting of EPR lines due to interaction of the unpaired electron with nearby magnetic nuclei. This tells you which nuclei the unpaired electron "sees" and how strongly.
  • Zero-field splitting: In systems with more than one unpaired electron (S>12S > \frac{1}{2}), electron-electron interactions split energy levels even without an external magnetic field.

EPR is widely applied to paramagnetic transition metal complexes (e.g., Cu(II), Mn(II), Fe(III)), organic radicals, and defect sites in solids. It's also valuable for studying reaction mechanisms that involve radical intermediates.

Advanced pulsed EPR techniques like ENDOR (electron-nuclear double resonance) and ESEEM (electron spin echo envelope modulation) provide much higher resolution for hyperfine interactions than continuous-wave EPR.

UV-Visible Spectroscopy and Charge Transfer, Charge-transfer band - Wikipedia

Mössbauer Spectroscopy

Mössbauer spectroscopy exploits the recoil-free emission and absorption of gamma rays by nuclei in a solid lattice (the Mössbauer effect). It's a niche but incredibly informative technique, most commonly applied to 57Fe^{57}\text{Fe}, which makes it invaluable for iron chemistry and biochemistry.

Three parameters are extracted from a Mössbauer spectrum:

  1. Isomer shift (δ\delta): Reflects the s-electron density at the nucleus. Different oxidation states and spin states produce different isomer shifts. For example, high-spin Fe(III) and low-spin Fe(II) have distinct δ\delta values.
  2. Quadrupole splitting (ΔEQ\Delta E_Q): Arises from an asymmetric electric field gradient at the nucleus. This is sensitive to the symmetry of the coordination environment and the d-electron configuration.
  3. Magnetic hyperfine splitting: In the presence of a magnetic field (external or internal, as in magnetically ordered materials), the nuclear levels split further, producing a six-line pattern for 57Fe^{57}\text{Fe}.

Because Mössbauer spectroscopy requires the sample to be a solid (to achieve recoil-free conditions), it's particularly suited for studying solid-state materials, minerals, catalysts, and frozen biological samples.

X-ray and Mass Spectrometry

X-ray diffraction (XRD) is the gold standard for determining the three-dimensional structure of crystalline inorganic compounds. When X-rays hit a crystal, they scatter off the electron density in a regular pattern governed by Bragg's law:

nλ=2dsinθn\lambda = 2d\sin\theta

where nn is an integer (the order of diffraction), λ\lambda is the X-ray wavelength, dd is the spacing between crystal planes, and θ\theta is the angle of incidence.

  • Single-crystal XRD gives you precise bond lengths, bond angles, and the full 3D arrangement of atoms. This is the definitive structural characterization method when suitable crystals can be grown.
  • Powder XRD is used when single crystals aren't available. It's excellent for phase identification (matching patterns to a database) and can also be used for unit cell determination and Rietveld refinement.

X-ray absorption spectroscopy (XAS) doesn't require crystalline samples, which is a major advantage. It probes the local environment around a specific element:

  • XANES (X-ray absorption near-edge structure): The region near the absorption edge is sensitive to oxidation state and coordination geometry.
  • EXAFS (extended X-ray absorption fine structure): The oscillations beyond the edge encode information about the number, type, and distance of neighboring atoms. Useful for amorphous materials, solutions, and biological samples.

XPS (X-ray photoelectron spectroscopy) measures the binding energies of core electrons ejected from a surface. Shifts in binding energy reveal oxidation states and chemical bonding at the surface, making it a key technique for catalysis and materials science.

Mass Spectrometry in Inorganic Analysis

Mass spectrometry (MS) separates and detects ions based on their mass-to-charge ratio (m/zm/z). It confirms molecular formulas, reveals fragmentation patterns, and can detect trace elements at extremely low concentrations.

Common ionization methods for inorganic compounds:

  • Electrospray ionization (ESI): Gentle technique that keeps intact ions in solution (good for charged coordination complexes).
  • MALDI: Uses a matrix to assist ionization; useful for large clusters and polymeric species.
  • Electron impact (EI): Harsher ionization that produces more fragmentation; less common for sensitive coordination compounds.

Mass analyzers (TOF, quadrupole, ion trap) separate the ions, and the resulting spectrum shows peaks at characteristic m/zm/z values. Isotope patterns are particularly useful in inorganic MS because many metals have distinctive isotope distributions that serve as fingerprints for identifying metal-containing fragments.

  • ICP-MS (inductively coupled plasma MS) is the standard for trace elemental analysis, with detection limits often in the parts-per-trillion range.
  • Isotope ratio MS precisely measures relative isotope abundances for geochemistry and environmental studies.
  • Tandem MS (MS/MS) fragments selected ions a second time, providing detailed structural information about how a complex breaks apart.

Coupling MS with chromatographic separation (GC-MS, LC-MS) allows you to analyze complex mixtures by separating components before they enter the mass spectrometer.