Spectroscopy and Circular Dichroism: Comprehensive Notes

General spectroscopy

  • Spectroscopy deals with the production, measurement, and interpretation of spectra arising from the interaction of electromagnetic radiation with matter.
  • Radiation ranges include ultraviolet (UV), visible, infrared (IR), and radio frequencies used in spectroscopy (e.g., NMR is a radio-frequency technique).
  • Purpose: determine composition, structure, and physical properties of atoms or molecules.
  • Interaction outcomes: absorption, emission, or scattering of radiation.
  • Basic idea: study how matter affects electromagnetic radiation to infer chemical and physical information.

Basic Principles of Spectroscopy

  • Interaction of Radiation with Matter
    • Electromagnetic radiation interacts with matter (atoms or molecules) and can be absorbed, emitted, or scattered.
    • This interaction yields spectral features that encode information about the system.
  • Energy Levels and Transitions
    • Atoms and molecules possess discrete energy levels: electronic, vibrational, and rotational.
    • Absorption: a molecule moves from a lower to a higher energy state (excitation).
    • Emission: a molecule returns from a higher to a lower energy state, releasing energy as radiation.
    • The energy difference ΔE between levels corresponds to the photon frequency ν:
      ΔE=hν.\Delta E = h\nu.
  • Energy level structure in molecules
    • For molecules, energy is a combination: electronic, vibrational, and rotational energies.
    • Internal energy of a molecule:
      E(molecule)=E(electronic)+E(vibrational)+E(rotational).E(\text{molecule}) = E(\text{electronic}) + E(\text{vibrational}) + E(\text{rotational}).
  • Vibrational energy
    • VE is associated with periodic motion of chemical bonds (stretching, bending).
    • IR radiation (2.5–25 μm or 4000–400 cm⁻¹) excites vibrational modes.
  • Internal energy of atoms vs molecules
    • Atom: described by electronic energy levels only (within the simplest picture).
    • Molecule: combines electronic, vibrational, and rotational contributions to energy.

Quantitative and Qualitative Analysis; Regions and Methods

  • Spectroscopic methods solve analytical problems across many species (atomic, molecular) and interactions.
  • Regions of interest include UV, visible, IR, and NMR (radio frequency) ranges.
  • Qualitative Analysis: identifies substances from unique spectral signatures.
  • Quantitative Analysis: measures concentration from spectral intensity, e.g., Beer–Lambert law in UV-Vis.
  • Common spectroscopic families by transitions (types of spectroscopy):
    • UV-Vis: electronic transitions.
    • IR: vibrational transitions.
    • NMR: transitions between nuclear spin states in a magnetic field.
    • Mass Spectrometry: separates ions by mass-to-charge ratio (not based on EM radiation).
  • Note: Mass spectrometry is technically not based on electromagnetic radiation.
  • Optical regions and applications:
    • Absorption/Emission in UV-Vis commonly used for quantitative analysis.
    • IR for vibrational fingerprints of functional groups.
    • NMR for detailed structural information about molecules.
  • Special note on UV-Vis CD:
    • UV-Vis CD investigates charge-transfer transitions in metal–protein complexes.

Types of Spectroscopy (Based on Radiation and Transitions)

  • UV-Vis Spectroscopy: electronic transitions, usually in the UV-Vis range.
  • Infrared (IR) Spectroscopy: vibrational transitions, typically in the IR region.
  • NMR (Nuclear Magnetic Resonance): transitions between nuclear spin states in a magnetic field (radio frequency).
  • Mass Spectrometry: separation of ions by mass-to-charge ratio; not based on electromagnetic radiation in the same sense as the others.

Partial Molecular Energy Levels and Transitions

  • Electronic energy states are depicted with associated vibrational and rotational sublevels.
  • Electronic transition
    • Occurs when an electron changes orbitals, typically upon absorption or emission of a photon with appropriate energy.
    • It is the electron that changes energy level.
  • Rotational energy
    • Quantized energy associated with rotation of the molecule about its center of gravity (center of mass).
  • Relative potential energy
    • The energy difference between the current energy state and the ground state defines the potential energy landscape for the species.

Vibrational Energy and Molecular Energy Decomposition

  • Vibrational energy (VE)
    • Quantized energy associated with the periodic motion of chemical bonds (stretching, angle bending).
  • IR excitation range for VE
    • 2.5–25 μm or 4000–400 cm⁻¹.
  • Energy accounting for a molecule
    • E(atom) = E(electronic)
    • E(molecule) = E(electronic) + E(vibrational) + E(rotational)

Energy Level Transitions in Spectroscopy: Absorption and Emission

  • Absorption of Radiation
    • Process: a photon transfers energy to the absorbing species, moving it from a lower to a higher energy state.
    • Most absorbers begin in the ground state before absorption.
    • The photon energy must exactly match the energy difference ΔE for the specific transition: ΔE=hν.\Delta E = h\nu. (selection rule and energy matching)
  • Emission of Radiation
    • Reverse process of absorption: energy from an excited molecule is released as a photon.
    • Excited state lifetimes are typically short; energy often dissipates as kinetic energy (heat) via internal conversion, not affecting the system measurably under normal conditions.
    • Fluorescence or phosphorescence may accompany emission when de-excitation occurs via photon emission.
  • Non-radiative pathways
    • Internal conversion and vibrational relaxation commonly convert excess energy to heat before photon emission occurs in many systems.

Circular Dichroism (CD) and ORD: Principles and Instrumentation

  • Circular Dichroism (CD)
    • Differential absorption of left- and right-circularly polarized light by chiral molecules.
    • Widely used to study molecular structures, especially proteins and nucleic acids.
    • A CD instrument is often called a spectropolarimeter.
  • Basic observables
    • Absorbance difference: ΔA=A<em>LA</em>R\Delta A = A<em>L - A</em>R where AL and AR are absorbances for left- and right-circularly polarized light.
    • Ellipticity: θ\theta (in degrees) is related to the ellipse formed by the transmitted polarization.
    • There is a simple numerical relation between delta A and ellipticity: θ=32.98ΔA.\theta = 32.98\,\Delta A.
    • The CD spectrum is typically plotted as ellipticity vs wavelength (a CD spectrum).
  • Instrumentation (general outline)
    • Light is linearly polarized and passed through a monochromator to select a wavelength.
    • A modulating device (often a photoelastic modulator, PEM) converts linear to circular polarization and alternates between left- and right-handed circular polarization.
    • The sample is alternately exposed to LCP and RCP, and the differential absorption is measured to obtain CD.
    • The measured differential molar absorptivity (and derived quantities) provide the CD signal.
  • Circular Dichroism vs ORD
    • CD measures differential absorption of circular polarizations; ORD (optical rotatory dispersion) relates to rotation of the plane of polarization due to chiral media.

Applications and Interpretations of Circular Dichroism

  • General utilities of CD spectroscopy
    • Assess protein folding status and characterize secondary structure (secondary, tertiary, and structural family).
    • Compare protein structures across species or expression systems; compare mutants.
    • Evaluate conformational stability under stress, buffer changes, or additives (stabilizers/excipients).
    • Identify solvent conditions that increase melting temperature or reversibility of thermal unfolding (informing shelf life).
    • Detect whether protein–protein or protein–ligand interactions alter conformation.
    • If conformational changes occur, the CD spectrum will deviate from the sum of individual components; small conformational changes can occur upon complex formation.
  • Instrumentation note
    • Most commercial CD instruments employ modulation techniques (e.g., Grosjean and Legrand approach).

Determination of Protein Secondary Structure by CD

  • Far-UV CD (190–250 nm) is used to determine secondary structure because the chromophore is the peptide bond when located in a regular, folded environment.
  • Characteristic secondary structures and their CD signatures:
    • Alpha-helix:
    • Dominant motif in many globular proteins; can be over one-third of residues.
    • CD spectrum features: two negative peaks near 222 nm and 208 nm, and a larger positive peak near 192 nm.
    • The magnitude and relative intensities provide information on helix content.
    • The relative magnitudes of the 222-nm and 208-nm bands depend on hydrophobic environment, membrane association, or oligomerization (e.g., dimerization) which can increase the 222-nm signal.
    • A 222/208 intensity ratio of about 0.8 has been proposed for a single-stranded α-helix; a ratio of about 1.0 is associated with a two-stranded coiled-coil of α-helices. Actual ratio depends on hydrogen bonding and environment.
    • Beta-sheet:
    • Can be parallel or antiparallel; variable lengths and widths; extended β-sheets often show a twist rather than perfect planarity.
    • CD signature: a negative band between 215–219 nm and a larger positive band between 195–202 nm.
    • Random coil (disordered):
    • Strong negative signal near ~200 nm; may have a small positive band near ~218 nm; possible very weak negative band near 235 nm.

Determination of Nucleic Acids by Vibrational CD (VCD)

  • Two spectral regions probe nucleic acid structure by VCD:
    • 1700–1600 cm⁻¹: C=O, C=N, and C=C stretching modes of nucleic acid bases; higher-frequency bands (above ~1650 cm⁻¹) relate to C=O stretch; lower-frequency bands (below ~1650 cm⁻¹) relate to C=C and some C=N contributions. Base composition affects VCD due to differences in C=O content among bases (e.g., cytosine, inosine, guanosine have C=O groups; adenosine has none).
    • 1250–1000 cm⁻¹: symmetric and antisymmetric stretching modes of the PO2⁻ group and sugar moieties; if not coupled to base-originating modes, VCD in this region may be independent of base composition.
  • Base composition influences the VCD signature via base-specific vibrational modes; incident environmental coupling can also modulate the spectra.

References (contextual)

  • Several foundational and review sources discuss vibrational circular dichroism (VCD), protein CD in the far-UV, and methodological considerations for analyzing biomolecules via CD/VCD. Examples include work by Polavarapu & Zhao, Kelly et al., and related encyclopedia/handbook entries.

Summary of Key Formulas and Concepts

  • Energy differences and transitions
    • Electronic transitions occur when absorbing photons of energy matching ΔE between electronic states: ΔE=hν.\Delta E = h\nu.
  • Molecular energy decomposition
    • For a molecule: E(molecule)=E(electronic)+E(vibrational)+E(rotational).E(\text{molecule}) = E(\text{electronic}) + E(\text{vibrational}) + E(\text{rotational}).
  • Vibrational spectroscopy range
    • IR activity typically involves vibrations excited by radiation in the range 2.525μm2.5\text{–}25\,\mu\text{m} or 4000400cm1.4000\text{–}400\,\text{cm}^{-1}.
  • Beer–Lambert law (context for quantitative UV-Vis spectroscopy)
    • Absorbance: A=εcl,A = \varepsilon c l, where (\varepsilon) is the molar extinction coefficient, (c) is the concentration, and (l) is the path length.
    • Transmittance: T=II0=10A.T = \frac{I}{I_0} = 10^{-A}.
  • Circular Dichroism observables
    • Ellipticity: θ=tan1(ba)\theta = \tan^{-1}\left(\frac{b}{a}\right) where (a) and (b) are the major and minor axes of the polarization ellipse.
    • Relationship between ellipticity and absorbance difference: θ=32.98ΔA,\theta = 32.98\,\Delta A, with ΔA=A<em>LA</em>R.\Delta A = A<em>L - A</em>R.
  • CD instrumentation outline
    • Light path: linearly polarized light → monochromator → modulator (e.g., PEM) → circularly polarized light → sample → detector; switching between LCP and RCP allows measurement of differential absorption.

Practical takeaways for exams

  • CD is a powerful tool for probing protein secondary structure in the far-UV (190–250 nm) and for assessing structural changes due to environment or ligand binding.
  • Alpha-helices give characteristic double minimum at 208 and 222 nm and a maximum around 190 nm; the 222/208 ratio provides insight into helicity and coiled-coil formation.
  • Beta-sheets show a negative minimum near 217–219 nm and a positive band around 195–202 nm.
  • Random coils show a strong negative band near 200 nm.
  • Nucleic acid VCD adds complementary information about base composition and backbone conformations, with distinct regions around 1700–1600 cm⁻¹ and 1250–1000 cm⁻¹.
  • The presence and magnitude of CD signals rely on chirality and structural asymmetry; achiral or highly symmetric systems exhibit little to no CD signal.