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Principles of Molecular Principles of Molecular Spectroscopy: Spectroscopy: Electromagnetic Radiation Electromagnetic Radiation and Molecular structure and Molecular structure Nuclear Magnetic Resonance (NMR) Nuclear Magnetic Resonance (NMR)

Principles of Molecular Spectroscopy: Electromagnetic Radiation and Molecular structure

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Principles of Molecular Spectroscopy: Electromagnetic Radiation and Molecular structure. Nuclear Magnetic Resonance (NMR). D E = h n. Electromagnetic radiation is absorbed when the energy of photon corresponds to difference in energy between two states. What Kind of States?. UV-Vis - PowerPoint PPT Presentation

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Page 1: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Principles of Molecular Principles of Molecular Spectroscopy:Spectroscopy:

Electromagnetic Radiation and Electromagnetic Radiation and Molecular structureMolecular structure

Nuclear Magnetic Resonance (NMR)Nuclear Magnetic Resonance (NMR)

Page 2: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Electromagnetic radiation is absorbed when theElectromagnetic radiation is absorbed when theenergy of photon corresponds to difference in energy of photon corresponds to difference in energy between two states.energy between two states.

E = hE = h

Page 3: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

electronicelectronic

vibrationalvibrational

rotationalrotational

nuclear spinnuclear spin

UV-VisUV-Vis

infraredinfrared

microwavemicrowave

radiofrequencyradiofrequency

What Kind of States?What Kind of States?

NMR is concerned with change in the direction of NMR is concerned with change in the direction of spin orientation as the result of the absorption of spin orientation as the result of the absorption of radiofrequency radiation.radiofrequency radiation.

Page 4: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

11H and H and 1313CC

both have spin = ±1/2both have spin = ±1/2

11H is 99% at natural abundanceH is 99% at natural abundance

1313C is 1.1% at natural abundanceC is 1.1% at natural abundance

The two nuclei that are most useful toThe two nuclei that are most useful toorganic chemists are:organic chemists are:

Page 5: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Nuclear SpinNuclear Spin

A spinning charge, such as the nucleus of A spinning charge, such as the nucleus of 11H H or or 1313C, generates a C, generates a magnetic fieldmagnetic field. The . The magnetic field magnetic field generated by a nucleus of spin generated by a nucleus of spin +1/2 is opposite in direction from that +1/2 is opposite in direction from that generated by a nucleus of spin –1/2.generated by a nucleus of spin –1/2.

+ +

Page 6: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

++

+

+

+

The distribution of The distribution of nuclear spins is nuclear spins is random in the random in the absence of an absence of an external magnetic external magnetic field.field.

Page 7: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

++

+

+

+An external magnetic An external magnetic field causes nuclear field causes nuclear magnetic moments to magnetic moments to align parallel and align parallel and antiparallel to applied antiparallel to applied field.field.

HH00

Page 8: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

++

+

+

+There is a slight There is a slight excess of nuclear excess of nuclear magnetic moments magnetic moments aligned parallel to aligned parallel to the applied field.the applied field.

HH00

Page 9: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

no energy difference in absence of magnetic fieldno energy difference in absence of magnetic fieldproportional to strength of external magnetic field proportional to strength of external magnetic field

Energy Differences Between Nuclear Spin StatesEnergy Differences Between Nuclear Spin States

+

+

EE E E ''

increasing field strength, Hincreasing field strength, HZZ

Page 10: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Some important relationships in NMRSome important relationships in NMR

The frequency of absorbedThe frequency of absorbedelectromagnetic radiationelectromagnetic radiationis proportional tois proportional to

the energy difference betweenthe energy difference betweentwo nuclear spin statestwo nuclear spin stateswhich is proportional towhich is proportional to

the applied magnetic fieldthe applied magnetic field

Page 11: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Some important relationships in NMRSome important relationships in NMR

The frequency (The frequency () of absorbed) of absorbedelectromagnetic radiationelectromagnetic radiationis proportional tois proportional to

the energy difference (the energy difference (E) E) betweenbetweentwo nuclear spin statestwo nuclear spin stateswhich is proportional towhich is proportional to

the applied magnetic field (Hthe applied magnetic field (H00))

UnitsUnits

Hz (sHz (s-1-1))

kJ/molkJ/mol(kcal/mol)(kcal/mol)

tesla (T)tesla (T)

Page 12: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Some important relationships in NMRSome important relationships in NMR

The frequency of absorbed electromagneticThe frequency of absorbed electromagneticradiation is different for different elements, radiation is different for different elements, and for different isotopes of the same element.and for different isotopes of the same element.

For a field strength of HFor a field strength of H00 = 4.7 T: = 4.7 T:11H absorbs radiation having a frequencyH absorbs radiation having a frequencyof 200 MHz (200 x 10of 200 MHz (200 x 1066 s s-1-1))1313C absorbs radiation having a frequencyC absorbs radiation having a frequencyof 50.4 MHz (50.4 x 10of 50.4 MHz (50.4 x 1066 s s-1-1))

Compare to 10Compare to 101515 s s-1-1 for electrons; 10 for electrons; 101313 s s-1-1 for vibrations for vibrations

Page 13: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Some important relationships in NMRSome important relationships in NMR

The frequency of absorbed electromagneticThe frequency of absorbed electromagneticradiation for a particular nucleus (such as radiation for a particular nucleus (such as 11H or H or 1313C) C) depends on the depends on the molecularmolecular environment of the environment of the nucleus (the electronic environment). nucleus (the electronic environment).

This is why NMR is such a useful toolThis is why NMR is such a useful toolfor structure determination. The signals of different for structure determination. The signals of different protons and carbon atoms in a molecule show protons and carbon atoms in a molecule show different signals, just like different functional groups different signals, just like different functional groups show different signals in the IR.show different signals in the IR.

Page 14: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Nuclear Shieldingand

1H Chemical Shifts

What do we mean by "shielding?"What do we mean by "shielding?"What do we mean by "chemical shift?"What do we mean by "chemical shift?"

Page 15: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

ShieldingShielding

An external magnetic field An external magnetic field affects the motion of the affects the motion of the electrons in a molecule, electrons in a molecule, inducing a magnetic field inducing a magnetic field within the molecule.within the molecule. CC HH

HH 00

Page 16: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

ShieldingShielding

An external magnetic field An external magnetic field affects the motion of the affects the motion of the electrons in a molecule, electrons in a molecule, inducing a magnetic field inducing a magnetic field within the molecule.within the molecule.

The direction of the The direction of the induced magnetic field is induced magnetic field is opposite to that of the opposite to that of the applied field.applied field.

CC HH

HH 00

Page 17: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

ShieldingShielding

The induced field shields The induced field shields the nuclei (in this case, the nuclei (in this case, 1313C C and and 11H) from the applied H) from the applied field.field.

A stronger external field is A stronger external field is needed in order for energy needed in order for energy difference between spin difference between spin states to match energy of states to match energy of rf radiation.rf radiation.

CC HH

HH 00

Page 18: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Chemical ShiftChemical Shift

Chemical shift is a Chemical shift is a measure of the degree to measure of the degree to which a nucleus in a which a nucleus in a molecule is shielded.molecule is shielded.

Protons in different Protons in different environments are shielded environments are shielded to greater or lesser to greater or lesser degrees; they have degrees; they have different chemical shifts.different chemical shifts.

CC HH

HH 00

Page 19: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

01.02.03.04.05.06.07.08.09.010.0

Chemical shift (Chemical shift (, ppm), ppm)measured relative to TMSmeasured relative to TMS

UpfieldUpfieldIncreased shieldingIncreased shielding

DownfieldDownfieldDecreased shieldingDecreased shielding

(CH(CH33))44Si (TMS)Si (TMS)

HH00

Page 20: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

01.02.03.04.05.06.07.08.09.010.0

Chemical shift (Chemical shift (, ppm), ppm)

7.28 ppm7.28 ppm

HH CC

ClCl

ClCl

ClCl

HH00

Page 21: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Effects of Molecular Structureon

1H Chemical Shifts

protons in different environments experience different degrees of shielding and have

different chemical shifts

Page 22: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Electronegative substituents decreaseElectronegative substituents decreasethe shielding of methyl groupsthe shielding of methyl groups

CHCH33FF 4.3 ppm 4.3 ppm

CHCH33OOCHCH33 3.2 ppm 3.2 ppm

CHCH33NN(CH(CH33))22 2.2 ppm 2.2 ppm

CHCH33CHCH33 0.9 ppm 0.9 ppm

CHCH33SiSi(CH(CH33))33 0.0 ppm 0.0 ppm

012345678910

CHCH33SiSi(CH(CH33))33

CHCH33CHCH33

CHCH33NN(CH(CH33))22CHCH33FF

CHCH33OOCHCH33

Page 23: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Effect is cumulativeEffect is cumulative

012345678910

CHCHClCl33 7.3 ppm 7.3 ppm

CHCH22ClCl22 5.3 ppm 5.3 ppm

CHCH33ClCl 3.1 ppm 3.1 ppm

CHCH33ClCl

CHCH22ClCl22

CHCHClCl33

Page 24: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Protons attached to spProtons attached to sp22 hybridized carbon hybridized carbonare less shielded than those attachedare less shielded than those attached

to spto sp33 hybridized carbon hybridized carbon

012345678910

HH HH

HHHHHH

HH

7.3 ppm7.3 ppm

CC CCHHHH

HH HH

5.3 ppm5.3 ppm

CHCH33CHCH33

0.9 ppm0.9 ppm

Page 25: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

1. number of signals1. number of signals

2. their intensity (as measured by area 2. their intensity (as measured by area under peak)under peak)

3. splitting pattern (multiplicity)3. splitting pattern (multiplicity)

Information contained in an NMRInformation contained in an NMRspectrum includes:spectrum includes:

We shall not consider spin-spin splittingWe shall not consider spin-spin splitting

Page 26: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

01.02.03.04.05.06.07.08.09.010.0

Chemical shift (Chemical shift (, ppm), ppm)

CCCCHH22OCOCHH33NN

OCOCHH33

NCCNCCHH22OO

Number of SignalsNumber of Signals

protons that have different protons that have different

chemical shifts are chemically chemical shifts are chemically

nonequivalent and exist in nonequivalent and exist in

chemically different molecular chemically different molecular

environmentsenvironments

HH00

Page 27: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

11H and H and 1313C NMR compared:C NMR compared:

both give us information about the environment of the both give us information about the environment of the nuclei (hybridization state, attached atoms, etc.)nuclei (hybridization state, attached atoms, etc.)

both give us information about the number of both give us information about the number of chemically nonequivalent nuclei (nonequivalent chemically nonequivalent nuclei (nonequivalent hydrogens or nonequivalent carbons)hydrogens or nonequivalent carbons)

Page 28: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

ClClCCHH22CHCH22CHCH22CHCH22CCHH33

CCHH33ClClCCHH22

Chemical shift (Chemical shift (, ppm), ppm)

01.02.03.04.05.06.07.08.09.010.0

11HH HH00

??

1H NMR cannot 1H NMR cannot distinguish two of the CHdistinguish two of the CH22 groups (Cgroups (C22 and C and C44))

Page 29: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

Chemical shift (Chemical shift (, ppm), ppm)

ClClCHCH22CHCH22CHCH22CHCH22CHCH33

020406080100120140160180200

1313CC

CDClCDCl33

a separate, distinct peak appears for each of the 5 carbons

SolventSolvent

HH00

Page 30: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

1313C Chemical shifts are most affected by:C Chemical shifts are most affected by:

• hybridization state of carbonhybridization state of carbon• electronegativity of groups attached to carbonelectronegativity of groups attached to carbon

020406080100120140160180200220

Increasing electronegativityIncreasing electronegativity

HH00

Page 31: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

020406080100120140160180200220

OOHH6161

2323

138138

spsp22 hybridized carbon is at lower field than hybridized carbon is at lower field than spsp33

As the atom attached to a carbon becomes more As the atom attached to a carbon becomes more electronegative, the carbon atom signal is observed electronegative, the carbon atom signal is observed at lower fieldat lower field

2323

OO202202

HH00

Page 32: Principles of Molecular  Spectroscopy: Electromagnetic Radiation and  Molecular structure

020406080100120140160180200220