MOLECULAR SPECTROSCOPY CHY 6040 Text Book: Colin N Banwell, Elaine M. McCash, Fundamentals of Molecular Spectroscopy, Tata McGraw – Hill Publishing Co. Ltd., 5th Edition, 2013. What is spectroscopy? Studying the properties of matter through its interaction with different frequency components of the electromagnetic spectrum With light, you aren’t looking directly at the molecule—the matter—but its “ghost.” You observe the light’s interaction with different degrees of freedom of the molecule. Each type of spectroscopy—different light frequency—gives a different picture → the spectrum. Goals: • Understand how light interacts with matter and how you can use this to quantitatively understand your sample. • Understand spectroscopy the way you understand other common tools of measurement like the watch or the ruler. • Spectroscopy is a set of tools that you can put together in different ways to understand systems → solve chemical problems. The immediate questions that we want to address are: 1. What does light do to sample? 2. How do you produce a spectrum? 3. What EXACTLY is a spectrum a measurement of ? Molecular Spectroscopy Study of interaction of electromagnetic waves and matter • Nature of electromagnetic radiation • Sort of interactions • Experimental methods ELECTROMAGNETIC RADIATION Also known as radiant heat or radiant energy One of the ways by which energy travels through space Consists of perpendicular electric and magnetic fields that are also perpendicular to direction of propagation Examples heat energy in microwaves light from the sun X-ray radio waves ELECTROMAGNETIC RADIATION Wavelength (m) Gamma X rays Ultrrays violet Visible 10-11 103 Infrared Microwaves Radio frequency FM Shortwave AM Frequency (s-1) 1020 Visible Light: VIBGYOR Violet, Indigo, Blue, Green, Yellow, Orange, Red 400 – 750 nm • White light is a blend of all visible wavelengths • Can be separated using a prism 104 ELECTROMAGNETIC RADIATION λ1 node amplitude ν1 = 4 cycles/second λ2 ν2 = 8 cycles/second peak λ3 ν3 = 16 cycles/second trough one second ELECTROMAGNETIC RADIATION Wavelength (λ) • Distance for a wave to go through a complete cycle • (distance between two consecutive peaks or troughs in a wave) Frequency (ν) • The number of waves (cycles) passing a given point • in space per second Cycle • Crest-to-crest or trough-to-trough Speed (c) • All waves travel at the speed of light in vacuum (3.00 x 108 m/s) ELECTROMAGNETIC RADIATION Plane Polarized Light • Light wave propagating along only one axis (confined to one plane) Monochromatic Light • Light of only one wavelength Polychromatic Light • Consists of more than one wavelength (white light) Visible light • The small portion of electromagnetic radiation to which the human eye responds ELECTROMAGNETIC RADIATION Inverse relationship between wavelength and frequency λ α 1/ν c=λν λ = wavelength (m) ν = frequency (cycles/second = 1/s = s-1 = hertz = Hz) c = speed of light (3.00 x 108 m/s) ELECTROMAGNETIC RADIATION • Light appears to behave as waves and also considered as stream of particles (the dual nature of light) • Is sinusoidal in shape • Light is quantized Photons Particles of light ELECTROMAGNETIC RADIATION hc Energy of one photon (E photon ) hν hc~ν λ ~ν 1 wavenumber (m 1 ) λ h = Planck’s constant (6.626 x 10-34 J.s) ν = frequency of the radiation λ = wavelength of the radiation E is proportional to ν and inversely proportional to λ INTERACTIONS WITH MATTER • Takes place in many ways • Takes place over a wide range of radiant energies • Is not visible to the human eye • Light is absorbed or emitted • Follows well-ordered rules • Can be measured with suitable instruments INTERACTIONS WITH MATTER Molecules Many types of motion are involved - Rotation - Vibration - Translation (move from place to place) These motions are affected when molecules interact with radiant energy Molecules vibrate with greater energy amplitude when they absorb radiant energy INTERACTIONS WITH MATTER Molecules • Bonding electrons move to higher energy levels when molecules interact with visible or UV light • Changes in motion or electron energy levels result in changes in energy of molecules Transition • Change in energy of molecules (vibrational transitions, rotational transitions, electronic transitions) INTERACTIONS WITH MATTER Atoms or Ions • Move between energy levels or in space but cannot rotate or vibrate • The type of interactions of materials with radiant energy are affected by - Physical state - Composition (chemical nature) - Arrangement of atoms or molecules INTERACTIONS WITH MATTER • Light striking a sample of matter may be - Absorbed by the sample - Transmitted through the sample - Reflected off the surface of the sample - Scattered by the sample • Samples can also emit light after absorption (luminescence) • Species (atoms, ions, or molecules) can exist in certain discrete states with specific energies INTERACTIONS WITH MATTER Transmission • Light passes through matter without interaction Absorption • Matter absorbs light energy and moves to a higher energy state Emission • Matter releases energy and moves to a lower energy state Luminescence • Emission following excitation of molecules or atoms by absorption of electromagnetic radiation INTERACTIONS WITH MATTER Ground State: The lowest energy state Excited state: higher energy state (usually short-lived) Energy Excited state Absorption Emission Ground state INTERACTIONS WITH MATTER Change in state requires the absorption or emission of energy Change in energy ( E) hν hc λ Matter can only absorb specific wavelengths or frequencies These correspond to the exact differences in energy between the two states involved Absorption: Energy of species increases (ΔE is positive) Emission: Energy of species decreases (ΔE is negative) INTERACTIONS WITH MATTER Frequencies and the extent of absorption or emission of species are unique Specific atoms or molecules absorb or emit specific frequencies This is the basis of identification of species by spectroscopy Relative energy of transition in a molecule Rotational < vibrational < electronic The are many associated rotational and vibrational sublevels for any electronic state (absorption occurs in closely spaced range of wavelenghts) INTERACTIONS WITH MATTER Absorption Spectrum A graph of intensity of light absorbed versus frequency or wavelength Emission spectrum is obtained when molecules emit energy by returning to the ground state after excitation Excitation may include - Absorption of radiant energy - Transfer of energy due to collisions between atoms or molecules - Addition of thermal energy - Addition of energy from electrical charges Spectroscopy is a general methodology It can be adapted in many ways to extract the information you need (energies of electronic, vibrational, rotational states, structure and symmetry of molecules, dynamic information). ATOMS AND ATOMIC SPECTROSCOPY MOLECULES AND MOLECULAR SPECTROSCOPY ATOMS AND ATOMIC SPECTROSCOPY The electronic state of atoms are quantized Elements have unique atomic numbers (numbers of protons and electrons) Electrons in orbitals are associated with various energy levels An atom absorbs energy of specific magnitude and a valence electron moves to the excited state The electron returns spontaneously to the ground state and emits energy ATOMS AND ATOMIC SPECTROSCOPY Emitted energy is equivalent to the absorbed energy (ΔE) Each atom has a unique set of permitted electronic energy levels (due to unique electronic structure) The wavelength of light absorbed or emitted are characteristic of a specific element The absorption wavelength range is narrow due to the absence of rotational and vibrational energies The wavelength range falls within the ultraviolet and visible regions of the spectrum (UV-VIS) ATOMS AND ATOMIC SPECTROSCOPY Wavelengths of absorption or emission are used for qualitative identification of elements in a sample The intensity of light absorbed or emitted at a given wavelength is used for the quantitative analysis Atomic Spectroscopy Methods Absortion spectroscopy Emission spectroscopy Fluorescence spectroscopy X-ray spectroscopy (makes use of core electrons) MOLECULES AND MOLECULAR SPECTROSCOPY Molecular Processes Occurring in Each Region 103 Gamma UltrX rays rays violet 1020 Visible 10-11 Infrared Microwaves Radio frequency FM Shortwave AM rotation vibration Electronic excitation Bond breaking and ionization 104 The entire electromagnetic spectrum is used by chemists Frequency, n in Hz ~1019 ~1017 ~1015 ~1013 ~1010 ~105 0.01 cm 100 m ~10-4 ~10-6 Wavelength, l ~.0001 nm ~0.01 nm 10 nm 1000 nm Energy (kcal/mol) > 300 g-rays nuclear excitation (PET) X-rays core electron excitation (X-ray cryst.) 300-30 300-30 UV electronic excitation (p to p*) IR molecular vibration Visible Microwave Radio molecular rotation Nuclear Magnetic Resonance NMR (MRI) MOLECULES AND MOLECULAR SPECTROSCOPY Energy states are quantized Rotational Transitions Molecules rotate in space and rotational energy is associated Absorption of the correct energy causes transition to a higher energy rotational state Molecules rotate faster in a higher energy rotational state Rotational spectra are usually complex MOLECULES AND MOLECULAR SPECTROSCOPY Rotational Transitions Rotational energy of a molecule depends on shape, angular velocity, and weight distribution Shape and weight distribution change with bond angle Molecules with more than two atoms have many possible shapes Change in shape is therefore restricted to diatomic molecules Associated energies are in the radio and microwave regions MOLECULES AND MOLECULAR SPECTROSCOPY Vibrational Transitions Atoms in a molecule can vibrate toward or away from each other at different angles to each other Each vibration has characteristic energy associated with it Vibrational energy is associated with absorption in the infrared (IR region) Increase in rotational energy usually accompanies increase in vibrational energy MOLECULES AND MOLECULAR SPECTROSCOPY Vibrational Transitions IR absorption corresponds to changes in both rotational and vibrational energies in molecules IR absorption spectroscopy is used to deduce the structure of molecules Used for both qualitative and quantitative analysis MOLECULES AND MOLECULAR SPECTROSCOPY Electronic Transitions Molecular orbitals are formed when atomic orbitals combine to form molecules Absorption of the correct radiant energy causes an outer electron to move to an excited state Excited electron spontaneously returns to the ground state (relax) emitting UV or visible energy Excitation in molecules causes changes in the rotational and vibrational energies MOLECULES AND MOLECULAR SPECTROSCOPY Electronic Transitions The total energy is the sum of all rotational, vibrational, and electronic energy changes Associated with wide range of wavelengths (called absorption band) UV-VIS absorption bands are simpler than IR spectra MOLECULES AND MOLECULAR SPECTROSCOPY Molecular Spectroscopy Methods Molecular absorption spectroscopy Molecular emission spectroscopy Nuclear Magnetic Resonance (NMR) UV-VIS IR MS Molecular Fluorescence Spectroscopy Regions of spectrum Change of orientation ESR Microwave Change of configuration Infrared Change of electron distribution Change of nuclear configuration Visible and UV X-rays Gamma rays Increasing energy Change of spin NMR 10 m 100 cm 1 cm 100 µm 1 µm 10 nm 100 pm What variables do we need to characterize a molecule? Nuclear and electronic configurations: What is the structure of the molecule? What are the bond lengths? How strong or stiff are the bonds? What is the symmetry? Where is the electron density? Molecular Behavior: How much do the nuclei move (vibration/rotation)? How do the structural variables change with time? Dynamics Different spectroscopies will tell us about different variables Rotational spectroscopy: will tell us where re is. Vibrational spectroscopy: will tell us how stiff the bond is and about the curvature of potential. Electronic spectroscopy: will tell us about where electronic states lie → potential energy curves, barriers, dissociation energies Molecular coordinates For any free particle (nucleus or electron): Kinetic and potential energy associated with the motion of a particle Translation along x, y, z → n particles → 3n degrees of freedom (d.o.f). In a molecule the positions of these particles is not independent To solve problems in molecular structure and motion, chose a molecular frame of reference: • Coordinates along symmetry axes • Origin (often) at the center of mass To simplify problem, treat nuclear and electronic motion separately Electrons are much lighter than nuclei. Therefore, we expect that the electrons will occupy a fixed distribution in space about a nuclear configuration. Separate different types of motion based on time-scale or energy of motion. The basis for drawing potential energy curves is the BornOppenheimer Approximation: Motion of electron is much faster than nuclei Doesn’t depend on nuclear kinetic energy Electrons: The spatial extent motion is described by atomic or molecular orbitals. Nuclei: Three types of motion for nuclei with respect to the C.O.M. of the molecule Consider a diatomic (with 6 d.o.f). Displacement of atoms relative to one another / C.O.M. fixed Motion about C.O.M. / C.O.M. fixed move C.O.M. How are these motions related to the structure of the molecule? A classical description allows you to say a lot about spectroscopy, but it doesn’t explain experiments very well! We need quantum mechanics! Classically: Position and motion of particles with arbitrary accuracy No restriction on energy of system or spatial configuration Quantum: Energy levels are quantized Fixed energy and spatial configuration Probabilistic description of particle position and motion We represent the state of the system through quantum numbers—usually integers. The energy is related to these numbers. “Ground State” : configuration of electrons, nuclei, … (a set of quantum numbers) that represent the lowest energy state of the system. Electronic States: atomic + molecular orbitals: which represent discrete energy states that electrons can occupy through discrete quantum numbers, i.e. for atom: n, l, m, ms n: principle quantum number/Size & energy l: orb. ang. mom./Shapes m: degeneracy/orientation ms: spin Electronic states have definite energy and electron density distribution (spatial dimension). There is no way for an electron to occupy an intermediate energy between quantized values. The energy to move an electron from the ground (lowest energy) state to another state: Typically 20,000-100,000 cm-1 = 10-50 kJ/mol. This corresponds to UV and visible light, λ~100-500nm For polyatomic molecules, we can use linear combinations of atomic orbitals. Quantization of nuclear degrees of freedom: The vibration, rotation, and translation of the 3n nuclear d.o.f. of a molecule are also quantized. Vibrations: Classically vibra onal mo on → moves energy levels to higher displacement Quantum mechanics there are discrete vibrational energy levels corresponding to specific vibrational states (wave functions) The simplest quantum mechanical model for Vibration: Quantum mechanical harmonic oscillator Rotation: Rotational angular momentum is quantized – Rigid Rotor/non-Rigid Rotor Translation: (motion of center of mass) Energy levels given by particle-in-a-box Quantum mechanical energies are summed over all degrees of freedom: specify energy through a set of quantum numbers, and characteristic vib./rot./etc. constants