Block 2 - Spectroscopy Flashcards

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

A

200nm

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
Q

Nuclei magnetic field - irradiation

A

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
Q

NMR absorptions

A

Known as chemical shifts
Measured in 𝛿 (delta) units (ppm)
TMS = 0 –> ignore

27
Q

0𝛿 - close and far

A

Closer to 0: shielded (C-H or C-C)

Further from 0: de-shielded (bonded to more electronegative atoms)

28
Q

What Cs or Hs give rise to different signals

A

Each unique C or H will give rise to different signals

29
Q

Chemical range for 13C NMR

A

Generally 𝛿0 - 210
𝛿0 - 90: sp3 carbon
𝛿100 - 210 (or sometimes higher): sp2 carbon

30
Q

13C NMR: intensity of signal

A

Generally not an indication of the number of Cs giving rise to a signal

31
Q

Interpreting 1H NMR - absorption signals

A

Number of absorption signals
Position of absorption signals
Relative areas under absorption signals
Splitting pattern for absorption signals

32
Q

Chemical shift range for 1H NMR

A

Generally 𝛿0 - 15, with most signals observed in 𝛿0 - 10

33
Q

NMR: signals for H bonded to sp2 carbon

A

Signals are at higher 𝛿 values

34
Q

NMR: C and H link to deshielding

A

If C experiences less electron density around it, then the H bonded to the C will also experience less –> more de-shielded

35
Q

Splitting pattern for absorption signals (H)

A

Splitting of an H absorption signal occurs when there are vicinal Hs for said H

36
Q

Vicinal Hs

A

Neighbouring Hs

Signal for one H is split by vicinal Hs and vice versa

37
Q

Number of H signals

A

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