Owen's material Flashcards
Electromagnetic radiation (EMR)
EMR consists of two perpendicular components (oscillating electric (E) and magnetic (B) fields). Interaction with matter requires a molecular response in E or B. The molecular response is in phase with the oscillation. Creates diffraction patterns (constructive and destructive interference) when monochromatic planar waves are passed through slits.
Wavenumber
The distance between two successive crests (m)
Frequency
The number of waves passing a point over a unit time (Hz or /s)
Wavenumber
Number of wavelengths in a unit distance (/m). Inverse of wavelength.
Photoelectric effect
When light hits as object, it immediately releases a photocurrent. The max Ek of the electrons released depends on the frequency of the wave (not intensity).
The threshold frequency is the frequency for a material below which no electrons will be released.
E=hc/λ - shorter wavelength = higher frequency and energy (gamma rays - UV)
Quantisation of Energy
Discrete values
Only electrons bound by nuclei have discrete energies. Unbound electrons are free to have any values of energy.
Hydrogen emission spectrum - all electrons in their lowest state gives the ground state. If in higher E orbitals they are excited.
E = -hcR/n^2, where n=prinicpal qn
Single photon transitions
Transitions result from interactions of E or B dipoles of the molecule with the electric or magnetic field of radiation.
Electrons can jump from one orbital to another, which requires E(photon)=difference in E levels.
The electronic energy in an atom can increase/decrease resulting in absorption/emission of a photon of suitable energy.
UV-Vis Spectrophotometer - single beam
Light source - emits white light (all wavelengths)
Monochromator - separates the light into separate wavelengths and passes each wavelength in turn through the sample
Sample - absorbs radiation of certain wavelengths
Light detector - measures intensity of light at each wavelength after passing through the sample
Signal processing - computer to generate spectrum
Monochromator
Separates light into different wavelengths, and passes each wavelength in turn through the sample.
Slit - 1) white light passes through and 2) allow a narrow range of wavelength out
Concave focussing mirror - 1) directs light to dispersing elements and 2) directs one wavelength out the slit
Dispersing element - diffracting grating and prism separate white light into different wavelengths
Photomultiplier tube (detector)
Photon enters through a transparent window into a sealed and evacuated tube. A photocathode (negative high voltage) causes the photoelectric effect. Dynodes (increasing voltage towards anode) cause electron cascade. Strong signal (lots of electrons) by the anode. Current-voltage amplifier.
UV-Vis Spectrophotometer - double beam
Source of EM radiation -> monochromator -> beam splitter (2 identical beams) -> one beam sent through sample the other sent through a reference -> detector -> computer (compares the 2 signals, eliminating background absorption)
Absorption spectroscopy
Incident radiation (I0) Transmitted radiation (IT) - reduced in intensity due to absorption Transmittance: T=IT/I0 Absorbance: A=log(I0/IT)=-log(T) - if 90% of light is absorbed, 10% is transmitted (0.1)
Beer-Lambert Law
A=log(I0/IT)=εcl
-ε = molar absorptivity coefficient = measure of how strongly the sample absorbs (depends on wavelength)
Transition intensities
Depend on c and l
The transition probability - the intrinsic probability that a molecule in the appropriate state can interact with the radiation to undergoing a transition to the final state.
P(fi)=0 - forbidden state
P(fi)>0 - allowed transition
-determined by selection rules
Boltzmann distribution - determines the number of molecules in the initial state
Selection rules
Transitions result from interactions between B or E dipoles of the molecule with the E or B field of the radiation
Gross selection rules
Physical properties that a system must have to be able to undergo any such transitions.
- rotational - permanent dipole moment
- vibrational - magnitude of electric dipole moment must change during vibration
- NMR - non-zero magnetic dipole moment
Specific selection rules
Determine the particular states between which transitions are allowed.
-photons carry one unit of angular moment. So atomic spectroscopy angular qn = +/-1
(sp not sd)
Boltzmann distribution
Determines the number of molecules in the initial state
For a small energy difference (high T), molecular state are evenly distributed
For a large energy difference (low T), molecules are in lower states
(ni/nj) = (gi/gj)e^(-E/kBT)
-ni = number of molecules in state i
-gi = degeneracy of state i
-Eij=Ei-Ej
For nmr, the upper and lower state populations are almost equal
For electronic, the upper-state can usually be ignored
Atomic spectra
Atomic transitions give sharp lines in the UV, visible or near IR.
The hotter the flame, the stronger the emission.
ni/nj=0 - no transition
ni/nj=1 - strong transition
Atomic Emission Spectroscopy (AES)
Quantify the amount of an element by measuring its emission intensity in a hot flame, atomising any compounds and thermally exciting atoms.
Requires careful control of flow rates, flame T and geometry.
Sample -> mixing chamber -> burner head and flame -photons-> monochromator -> detector -> recorder
Inductively coupled plasma - optical emission spectroscopy (ICP-OES)
Atomisation and excitation by RF induction in argon to create an extremely hot plasma
Plasma much hotter and steadier than flame (stronger intensity)
Sample -> plasma torch with RF coils -photon-> monochromator -> detector -> recorder
Atomic absorption spectroscopy (AAS)
In a flame, the vast majority of atoms are in the ground state, so absorption is much stronger than emission.
Sample -> mixing chamber -> hallow-cathode lamp emitting photon to a burner head with a flame -photon-> monochromator -> detector -> recorder
Hallow-cathode lamp is filled with low P inert buffer gas and made of an alloy containing the desired elemental analyte.
Molecular dynamics
Quantised:
Electronic energy - larger E gap
Vibrational energy - each vibrational mode has a rotational mode. Produced when electrons are excited. Linearly spaced
Rotational energy - microwave region (low E), spacings get further apart
Not quantised:
Translational energy
Rotational motion
I = moment of inertia (rotational inertia) P(rot) = rotational angular momentum J=rotational quantum number (0,1,2...) h-bar = h/2pi g = degeneracy = 2J+1