Owen's material Flashcards

1
Q

Electromagnetic radiation (EMR)

A

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.

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2
Q

Wavenumber

A

The distance between two successive crests (m)

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3
Q

Frequency

A

The number of waves passing a point over a unit time (Hz or /s)

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4
Q

Wavenumber

A

Number of wavelengths in a unit distance (/m). Inverse of wavelength.

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5
Q

Photoelectric effect

A

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)

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6
Q

Quantisation of Energy

A

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

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7
Q

Single photon transitions

A

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.

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8
Q

UV-Vis Spectrophotometer - single beam

A

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

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9
Q

Monochromator

A

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

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10
Q

Photomultiplier tube (detector)

A

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.

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11
Q

UV-Vis Spectrophotometer - double beam

A

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)

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12
Q

Absorption spectroscopy

A
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)
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13
Q

Beer-Lambert Law

A

A=log(I0/IT)=εcl

-ε = molar absorptivity coefficient = measure of how strongly the sample absorbs (depends on wavelength)

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14
Q

Transition intensities

A

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

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15
Q

Selection rules

A

Transitions result from interactions between B or E dipoles of the molecule with the E or B field of the radiation

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16
Q

Gross selection rules

A

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
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17
Q

Specific selection rules

A

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)

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18
Q

Boltzmann distribution

A

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

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19
Q

Atomic spectra

A

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

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20
Q

Atomic Emission Spectroscopy (AES)

A

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

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21
Q

Inductively coupled plasma - optical emission spectroscopy (ICP-OES)

A

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

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22
Q

Atomic absorption spectroscopy (AAS)

A

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.

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23
Q

Molecular dynamics

A

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

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24
Q

Rotational motion

A
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
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25
Rotational selection rules - diatomic molecule
Single-photon rotational spectroscopy involves an electric dipole mechanism. The magnitude or orientation of the electric dipole must be changed by the transition. GS rule - the molecule must have a permanent electric dipole moment (heteronuclear diatoms_ SP rule - photons carry one unit of angular moment, so angular momentum qns must change by +/-1. ΔJ=+/-1 (+absorption-emission) Measurements done in gas phase where molecules can freely rotate (nJ/nO)=(2J+1)e^(-EJ/kBT)
26
Absorbance vs wavenumber graph
Increases from 0-20 /cm - increasing degeneracy of initial state Decreasing from 20 /cm - higher E so lower Boltzmann population
27
Rotational spectroscopy - polyatomic molecules
3 orthogonal rotational axes; 3 moments of inertia. GSR - have to have a permanent electric dipole moment. Applications - determine molecular geometries by microwave absorption, detection of atmospheric molecules by microwave emission.
28
Vibrations of Hooke's Law - diatomic molecule
Vibrations between atoms similar to spring. F=-kx V=1/2kx^2 - parabolic potential Force constant (k) - proportional to bond strength (stiffer bond has larger k - steeper parabola). v(vib) is proportional to k and 1/reduced mass. -more confined motions (stiffer bond = larger k) lead to greater separation (larger hvvib) -heavier particles have less separation of quantum levels Gaps separated by wavenumber (one vibrational frequency) Zero point energy - E=(v+0.5)hvvib, so a molecule can never have zero vibrational energy.
29
Vibrational selection rules - diatomic molecule
Electric-dipole mechanism. GSR - the electric dipole moment of the molecule must change during the vibration, so it must have a permanent electric dipole moment (heteronuclear diatoms) SPR - for a harmonic oscillator Δv=+/-1 Most molecules will be in the zero-point level
30
Vibration states of anharmonic oscillators
Anharmonic bands are commonly described by Morse potential. - a bond gets weaker as it is stretched (decreasing k). Ep decreases so the E gap decreases at higher vibrational modes. Eventually bond will snap (E goes to 0 - bond dissociation). The effects of anharmonicity are more prevalent at higher E and at larger displacements from r0. Vibrational energy levels are closer together at higher E. Transitions with ΔV=>1 (overtones) are weakly allowed.
31
Vibrations - polyatomic molecules
Normal modes - combinations of localised vibrations (stretches, bends and torsions) Linear - 2 degenerate bending modes < symmetric stretch < asymmetric stretch (E and ṽ). 3N-5 -same E but differ in direction they bend Non-linear - bending < symmetric stretch < asymmetric stretch. 3N-6 GSR - vibrations must involve a change in dipole to appear in IR spectrum (does not need a permanent electric dipole) -larger dipole = stronger intensity. Fine structures in IR bands due to rotational energy levels. H2O - permanent electric dipole, so direction of dipole changes -> all IR active CO2 - no permanent dipole, symmetric stretch is IR inactive, but all others are IR active. SSR - Δv=+/-1 (fundamental is stongest), +/-2... (overtunes due to anharmonicity - weak)
32
Isotropic substitution
Bond strength similar, but reduced mass can change significantly, reducing the vibrational energy, leading to a smaller wavenumber.
33
Fingerprint region
Region in IR spectra where skeletal vibrations can be observed (unique to each molecule).
34
Characteristic group frequencies
A group of atoms have very different vibration frequencies, it will absorb a narrow frequency range that is characteristic of the group. Higher v require large k (multiple bonds) or smaller reduced mass (H).
35
IR regions
Near IR - overtones, combination bands Mid IR - fundamental vibrations and fingerprint region Far IR - fundamental vibrations of bonds with heavy atoms or weak bonds.
36
IR spectra collection
Nujol mull - ground up sample is suspended in oil and held between KBr plates KBr pellet - ground up sample with crystalline KBr then compressed into a disk Reflectance - ground up pure sample or diluted with ground up KBr Solution - held between KBr plates Gas cell - IR invisible windows
37
Molecular electronic spectroscopy
Electronic transitions typically occur in UV and visible. Transitions in the visible result in pigments, in UV they are colourless - ligand-field transition of transition metals (weak) - charge-transfer transitions between ligands and metal ions (strong) - molecular orbitals π->π* transition in conjugated organic molecules like dyes (strong)
38
π->π* transitions
Conjugations arises in organic molecules with alternating double-single bonds, allowing the π electrons to "spread-out" over larger distances, increasing the size of the bound potential. This causes the energy levels to become closer together. Thus, the energy required to excite an electron from the HOMO to LUMO is less, moving the necessary wavelength from far-UV to near-UV.
39
Vibrational progressions
Transitions can occur from ground-state to a number of vibrational levels in the electronic excited state. Bond is longer in π* (k smaller), thus E levels have smaller gap. Franck-Cordon principle - electronic transitions occur on much shorter time scales than vibrational motions. Bands are usually broad due to vibrational modes.
40
NMR
Involves a magnetic-dipole mechanism (weaker than electric), thus a nucleus must have a non-zero spin (uneven #protons and/or #neutrons). 1H, 13C, 19F etc are commonly used. GSR - must have a non-zero magnetic dipole moment SSR - Δm(I)=+/-1 Larmor frequency (v) in MHz (xE6) Very nearly equally populations and intrinsic weaknesses of magnetic dipole mechanism makes NMR absorption spectroscopy extremely insensitive.
41
Nuclear spin of a proton
Described by quantum numbers I (nuclear spin qn) and M(I) (nuclear magnetic qn). I=1/2 m(I)=+/-1/2
42
Zeeman effect for a proton
In the absence of an applied magnetic field, the spins have no orientation and equal E. In the presence of an applied magnetic field of strength B, they can adopt 2I+1 orientations, corresponding to different values of m(I), with E: E(MI)(B) = -m(I)γ(N)ℏB -γ(N)=gyromagnetic ratio of a proton (constant) -ℏ = h/2π 1H (I=1/2) can adopt 2 orientations corresponding to m(I)=+/-1/2 (+aligned with field), with E separated by E(p) =γ(p)ℏB. -m(I)=-1/2 so E(-1/2)=+γ(p)ℏB/2
43
NMR spectrometer
A compound in between a strong magnet. A strong pulse of RF from the input oscillator (coil) excites nuclei to higher-energy level, creating a non-equilibrium population. Population relaxes back to eqm by emitting RF radiation at Larmor frequency. Emitted radiation detected by output receiver (coil). Signal frequencies sorted by Fourier transform. Stronger field -> greater population difference -> stronger signal
44
1H NMR spectrum
Reference signal at 0ppm - TMS Number of resonance sets - number of H environments (if there is a chiral C, then each C will have separate H environments) Integral - number of H associated with C Chemical shift - nature of chemical environment multiplicity - number of H on adjacent C (within 3 bonds)
45
Timescale
NMR is a slow technique, so for planar molecules electronic transitions and vibrations are much faster, leading to an average spin for 2 methyl groups.
46
Chemical shift
A magnetic field (B) induces electrons to circulate around a nuclei (diamagnetic current). This induces a secondary magnetic field that is proportional, but opposed to B. The net field at the nucleus is weaker than the applied field due to electrons shielding the nucleus and the resonant frequency (chemical shift) is reduced. This caused an upfield shift. Nearby electron-withdrawing groups reduce electron density, deshielding the atom and increasing the resonance frequency. Aromatic rings - diamagnetic ring currents augment the field experienced by in-plane nuclei (effectively deshielding the ring) - same for multiple bonds. CH, OH and NH signals - CH give sharp lines and multiples at distinct chemical shifts. NH and OH subect to H-bonding and exchange with solvent. Highly purified in very pure solvents give broad singlets (no splitting).
47
Multiplicity (spin-spin coupling)
``` Spin-spin coupling arises from interactions between magnetic dipoles associated with spins and cause spin-spin splitting. Intensities follow pascal's triangle. Singlet - no adj H, 1 Doublet - one adj H, 1:1 -spin up and spin down Triplet - 2 adj H, 1:2:1 Quartet - 3 adj H, 1:3:3:1 ```
48
Heteronuclear NMR spectroscopy
A nucleus with a spin of 1/2 is the best: 19F, 31 P etc. Coupling to quadrupolar nuclei (spin >1/2) gives multiple lines. 2H nuclear spin =1, splitting the signal into 3 peaks at -1,0,1. 2H solvents lock the spectrometer frequency (C-D seen in CNMR). Sensitivity of nuclei in NMR depends on gyromagnetic ratio and natural abundance (1H most sensitive).
49
Mass spectrometry
Mass spectrometry vaporises a sample, then ionises it (charge often +1). During this process, the sample may undergo chemical reactions. Sorts according to m/z ratio. Ionisation processes depend on analyte volatility and the desired degree of subsequent reactions Hard ionisation (extensive fragmentation with volatile analytes) - electron impact (EI) Soft ionisation (minimal fragementation) -chemical ionisation (CI) -fast-atom bombardment (FAB) -Matrix-assisted laser desorption ionisation (MALDI) -Electrospray ionisation (ESI)
50
EI ionisation
Ionisation by collision with high-energy electrons. M -electon impact -> M+. + e- M+. is molecular/parent ion (must be charged to be seen in spectra) m/s=M electron usually lost from weakly bonded/non-bonding orbitals (lp). Excess energy of ionising electrons breaks bonds (fragmentation). Fragments can provide information about isomers. M+. -> R+ + R. R+ - fragmented ion R. - neutral radical fragment (not detected) Gas phase -> high vacuum -> e- source -> extractor plates and ion lenses -> m/z analyser
51
CI
Soft ionisation by reaction with reagent ions (NH4+ and CH3+), no significant excess E (minimal fragmentation). M + NH4+ -> [MH]+ + NH3 m/z: (M+1) MH + CH3+ -> M+ + CH4 m/z: (M-1) gas phase -> low vacuum -> reagent ion source -> extractor plates -> m/z analyser
52
FAB
Ionisation from a matrix by collision with fast atoms (Ar/Xe). Matrix absorbs the extra E so fragmentation is weak. M + Ar -> M+ + e- + Ar If the matrix contain acids/salts, adduct ions are produced: [MH]+ (M+1) or [MK]+ (M+39) - matrix influences peaks Fast atom source -> matrix -> extractor plates -> m/z analyser
53
MALDI
Ionisation from a matrix by ablation with a pulsed laser. Matrix absorbs excess E. M + hv -> M+ + e- If the matrix contains salts/acids, adduct ions can be produced Pulsed laser -> matrix -> extractor plates -> m/z analyser
54
ES-MS
Ionisation from a liquid by evaporation and Coulomb fission. Produces unfragmented adduct ions. [MHn]n+ so m/z: (M+n)/n Cone voltage of the spray nozzle can be increased to increase fragmentation (good for non-volatile ions). Spray nozzle (in solution) -> charged droplet (spray solution through shared nozzle into vacuum) -> solvent evaporation (droplet evaporates and charge concentrates) -> coulomb fission (coloumb explosion - smaller droplets until you have a single +) -> extractor plates -> m/z analyser.
55
m/z analysis methods
Time-of-flight mass analyser (TOF-MA) | Magnetic-sector mass analyser
56
TOF-MA
Pulsed ionisation unite -> accerlating voltage (15kV) -< ion pulse -> drifts through tube of length d -> detector (smaller are faster and heavier are slower). m/z ration = K(TOF)t^2 -K(TOF)=2eV/d^2 For given v and d, t depends on m/z Resolution can be improved by increasing d (longer drift tube), which requires a physically larger analyser.
57
Magnetic-sector mass analyser
Ionisation unit -> accelerating voltage -> magnetic field (centrifugal force up and Lorentz force down) -> detector (smaller m/z closer to ionisation unit) Lorentz force = f(L)=Bzev Centrifugal force = f(c)mv^2/r The radius of curvature of the ion trajectory is constant when f(c)=f(L) ->mv^2/r = Bzev -> r=mv^2/Bzev ->m/z=K(mag)B^2 -K(mag)=er^2/2V For given V and r, B depends on m/z (vary B) Resolution can be improved by increasing V, requires physically larger analyser or stronger B.
58
Mass spectra
M+1 peak due to isotopes (C13) Base peak - most intense, assigned 100% (most stable ion) (M-15) peak is methyl m/z=15 peak is methyl radical M->M.+ -> R. + R+ Alkanes - form stable carbocations -> 2/3 C=O groups - form R-CO+ Ethers, amines and alcohols - form oxonium (O) and iminium (N) cations
59
Isotope patterns
``` Major isotope: 1-p(x) Minor isotope: p(x) If P(x)<<1 (C13 or less), then N(x)~(p1/p0)/px For small organic molecules, peaks due to 2H will be weak since px=0.02% ```
60
Halogen isotope peaks
``` The minor isotopes of Cl and Br have very substantial abundances and are two mass units heavier than the major isotopes. 35Cl:37Cl is 3:1 79Br:81Br is ~1:1 p1/p0=(Nxpx)/(1-px) Cl - 31.9% for 1 atom Br - 97.2% for 1 atom Multiple halogen isotope peaks: 2 Cl: 35Cl/35Cl - 100 35Cl/37Cl or 37Cl/35Cl - 63.8 37Cl/37Cl - 10.2 (M+4) 2Br: Br follows pascal's triangle 1:2:1 Isotope patterns for heavier elements can be very complex ```
61
Different charges
For cations that form chargers such as +2 or +3, the m/z will not equate to the atomic mass. Divide molecular mass by 1/2 or 1/3.
62
High-resolution mass spectra
Some ion masses conincide at low resolution, but are different under high resolution. Not a proof of purity (elemental analysis) instead proof of composition.