EPR Flashcards

1
Q

Types of EPR coordinates

A

Hyperfine: electron and nucleus
Electron Zeeman: electron and magnet
Nuclear Zeeman: nuclear and magnet

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2
Q

Equation for magnetic dipole

A

(-) g factor x bohr magnetion x spin

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3
Q

What is EPR spectroscopy

A

Unpaired electron, using the magnetic field of microwave radiation

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4
Q

Electron Zeeman Equation

A

g value x bohr magneton x magnetic field x spin

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5
Q

KEY: reference sample to determine g value

A

g ref x B ref / B sample

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6
Q

KEY: g value from data

A

planks x frequency / Bohr magneton x B

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7
Q

Nuclear Zeeman equation

A

g(N) x nuclear magneton x magnetic field x spin

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8
Q

Hyperfine interactions equation

A

Spin (e) x Hyperfine x spin (nuc)

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9
Q

How do you predict spectra using trees

A

Largest splitting closest to radical
Branches into next closest atoms (do both even if in same environment)
Ratio gives intensities

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10
Q

KEY: How do you predict spectra using equations

A

Nuclear spin = 1/2
Lines = 2 x number of equiv nuclei x spin + 1
Intensity is Pascal’s triangle

Nuclear spin = 1
Intensity is form of Pascal’s triangle

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11
Q

How to tell if doublet of triplets OR triplet of doublets

A

The one with the biggest splitting is the first word ie that environment is a doublet so it’s a doublet of triplets

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12
Q

Rules for interpreting spectra from STRUCTURE

A

Find number of different nuclear environments
Use 2nI+1 to predict

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13
Q

Rules for interpreting spectra from SPECTRA

A

Work from outside in
Measure separation between first two lines: Hyperfine
Look at intensity
Measure separation distance to next line
If same it’s the same multiplet if not they have overlapped
J value at centre of multiplet

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14
Q

How to find electronic structure

A

Find theoretical Hyperfine values
Find electron spin density
Find radical distribution
Draw orbital structure

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15
Q

Theoretical Hyperfine values

A

Constants calculated and dependent on nuclear and electronic wavefunction

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16
Q

Electron spin density equation: where electron is on nucleus

A

Experimental Hyperfine / theoretical Hyperfine

17
Q

Equation for radical electron distribution

A

Molecule orbital = the sum of atomic orbital coefficient x atomic orbital

18
Q

What is the spin density

A

The probability electron is localised on that atomic orbital
The sum of (atomic orbital coefficients)^2

19
Q

When to use each Hyperfine constant

A

H closest to radical: McConnell coupling
H further away : hyperconjugation

20
Q

Equation for McConnell coupling constant

A

a = - Q x spin density

21
Q

Equation for hyperconjugation constant

A

a = B x spin density x cos^2(dihedral angle)
Geometry effects Hyperfine

22
Q

What is a spin trap

A

Stabilises reactive intermediates so you can analyse them. Use common ones so you can remove them from your data effectively as the nature changes after with radical. Data from databases

23
Q

Equation for spin trap binding

A

Radical (paramagnetic) + ST (diamagnetic) —> STR (paramagnetic)

24
Q

Types of spectral linewidths

A

Homogeneous
Inhomogeneous

25
Q

What is homogeneous broadening

A

Radicals experience magnetic field identically. Lorenzian line shames broad in wings

26
Q

What is inhomogeneous broadening

A

Difference in magnetic field experienced by radicals. Gaussian lineshape: thinner

27
Q

What is anisotropic EPR

A

Sensitive to orientation
Carried out at low temp
Solid or frozen sample

28
Q

Variables to consider for anisotropic EPR

A

Temperature, pressure and light intensity.
Energy is proportional to direction of spin

29
Q

g value and a value of anisotropic EPR

A

Total of values at x/y/z angles to magnetic field, divided by 3