Block 2 - Spectroscopy Flashcards

(37 cards)

1
Q

Types of spectroscopy

A

Mass spectroscopy (MS)
Infrared spectroscopy (IR)
Ultraviolet-visible spectroscopy (UV-VIS)
Nuclear magnetic resonance spectroscopy (NMR)

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2
Q

Molecular spectroscopy

A

IR, UV-Vis and NMR are forms of spectroscopy collectively known as molecular spectroscopy
Depend on interaction of molecules with radiation of specific energy

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3
Q

Energy, frequency, and wavelength relationship

A

Energy directly proportional to frequency

Energy inversely proportional to wavelength

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4
Q

Mass spectrometry allows…

A

The determination of the mass of individual ions derived from compounds in the gas phase

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5
Q

Mass spectrometry - how to read the molar mass

A

The highest m/z (where z = 1, so m) value on the graph is the molar mass

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6
Q

Mass spectrometry - limitation(s)

A

Unable to distinguish between compounds with same molecular formula
Unable to distinguish between different molecular formulae that have same integer mass

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7
Q

IR spectroscopy - units

A

1/cm

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8
Q

UV radiation is of…

A

Appropriate energy to raise electrons in some molecules (generally those with pi e-) from lower energy bonding (or non-bonding (lone pairs)) molecular orbitals to higher energy anti-bonding molecular orbitals

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9
Q

UV-VIS radiation causes…

A

The transition of an e- from a lower energy (ground state) to a higher energy (excited state) level

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10
Q

Conjugation

A

Pi electron systems (double bonds) that are linked together

Double bonds are only conjugated when there is only ONE single bond between the double bonds, i.e. double-single-double

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11
Q

Conjugated vs non-conjugated systems

A

Exhibit different UV-VIS absorbance
ΔE for electron excitement is smaller in conjugated systems, so absorption is observed at longer wavelengths than for non-conjugated systems

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12
Q

Bonding molecular orbital

A

When 2 atoms share 2e- (one molecular orbit between 2 atoms)

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13
Q

UV-VIS - sigma bonds

A

Compounds containing only sigma bonds are generally transparent to UV-VIS light - won’t see an absorption

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14
Q

UV-VIS - number of double bonds?

A

Can’t tell how many C=C or C=O bonds there are; only one absorption seen

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15
Q

UV-VIS: non-conjugated C=C bond

A

Shows an absorption at ~170nm due to π-π* electron transition

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16
Q

UV-VIS: non-conjugated C=O bond

A

Shows an extra absorption (weak) at 280nm due to a n-π* electron transition
i.e. has absorption at 170nm and 280nm

17
Q

Conjugated double bond - minimum absorption

18
Q

The greater the number of double bonds in conjugation…

A

The smaller the ΔE and the larger the max wavelength

19
Q

For a particular compound at a specified wavelength…

A

Absorbance is directly proportional to concentration and path length

20
Q

Beer’s Law

A
A = ɛ b c
Where
A = absorbance (no unit)
ɛ = molar absorptivity (L mol-1 cm-1)
b = path length (cm)
c = concentration (mol L-1)
21
Q

Effectiveness of molecule absorbing light and absorbance

A

The more ‘effective’ a molecule is at absorbing light at a wavelength, the greater the absorbance

22
Q

Bonding vs non-bonding orbitals - energy

A

Bonding orbitals lower in energy than anti-bonding orbitals

23
Q

UV-VIS - least to most energy bonds

A

C=C: σ < π < π* < σ*

C=O: σ < π < n(on-bonding) < π* < σ*

24
Q

What happens when nuclei with spin are placed in a magnetic field

A

They align themselves with (parallel to) or against (anti-parallel to) the external magnetic field
Nuclei aligned with the magnetic field have slightly lower energy than those aligned against the field

25
Nuclei magnetic field - irradiation
On irradiation with radio frequency of appropriate energy, energy is absorbed and the nuclear spin flips from the lower energy state to the higher energy state
26
NMR absorptions
Known as chemical shifts Measured in 𝛿 (delta) units (ppm) TMS = 0 --> ignore
27
0𝛿 - close and far
Closer to 0: shielded (C-H or C-C) | Further from 0: de-shielded (bonded to more electronegative atoms)
28
What Cs or Hs give rise to different signals
Each unique C or H will give rise to different signals
29
Chemical range for 13C NMR
Generally 𝛿0 - 210 𝛿0 - 90: sp3 carbon 𝛿100 - 210 (or sometimes higher): sp2 carbon
30
13C NMR: intensity of signal
Generally not an indication of the number of Cs giving rise to a signal
31
Interpreting 1H NMR - absorption signals
Number of absorption signals Position of absorption signals Relative areas under absorption signals Splitting pattern for absorption signals
32
Chemical shift range for 1H NMR
Generally 𝛿0 - 15, with most signals observed in 𝛿0 - 10
33
NMR: signals for H bonded to sp2 carbon
Signals are at higher 𝛿 values
34
NMR: C and H link to deshielding
If C experiences less electron density around it, then the H bonded to the C will also experience less --> more de-shielded
35
Splitting pattern for absorption signals (H)
Splitting of an H absorption signal occurs when there are vicinal Hs for said H
36
Vicinal Hs
Neighbouring Hs | Signal for one H is split by vicinal Hs and vice versa
37
Number of H signals
In general, an absorption signal is split into N+1 lines, where N is the number of vicinal Hs The line intensities within the split signal accord with Pascal's triangle