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Page 1: Proton NMR

Nuclear Magnetic Resonance (NMR) Spectroscopy

Part 2

Proton (1H) NMR

Page 2: Proton NMR

Theory of NMR

• The positively charged nuclei of certain elements (e.g., 13C and 1H) behave as tiny magnets.

• In the presence of a strong external magnetic field (Bo), these nuclear magnets align either with ( ) the applied field or opposed to ( ) the applied field.

• The latter (opposed) is slightly higher in energy than aligned with the field.

E is very small

Bo

Energy

Page 3: Proton NMR

Theory of NMR

• The small energy difference between the two alignments of magnetic spin corresponds to the energy of radio waves according to Einstein’s equation E=h.

• Application of just the right radiofrequency (causes the nucleus to “flip” to the higher energy spin state

• Not all nuclei require the same amount of energy for the quantized spin ‘flip’ to take place.

• The exact amount of energy required depends on the chemical identity (H, C, or other element) and the chemical environment of the particular nucleus.

h

Page 4: Proton NMR

Theory of NMR

• Our department’s NMR spectrometer (in Dobo 245) has a superconducting magnet with a field strength of 9.4 Tesla. On this instrument, 1H nuclei absorb (resonate) near a radiofrequency of 400 MHz; 13C nuclei absorb around 100 MHz.

• Nuclei are surrounded by electrons. The strong applied magnetic field (Bo) induces the electrons to circulate around the nucleus (left hand rule).

Bo

e-

(9.4 T)

Page 5: Proton NMR

Theory of NMR

• The induced circulation of electrons sets up a secondary (induced) magnetic field (Bi) that opposes the applied field (Bo) at the nucleus (right hand rule).

• We say that nuclei are shielded from the full applied magnetic field by the surrounding electrons because the secondary field diminishes the field at the nuclei.

Bo

e-

Bi

Page 6: Proton NMR

Theory of NMR

• The electron density surrounding a given nucleus depends on the electronegativity of the attached atoms.

• The more electronegative the attached atoms, the less the electron density around the nucleus in question.

• We say that that nucleus is less shielded, or is deshielded by the electronegative atoms.

• Deshielding effects are generally additive. That is, two highly electronegative atoms (2 Cl atoms, for example) would cause more deshielding than only 1 Cl atom.

C

H

HH

H

C

H

ClH

H

C

H

ClH

Cl

C and H are deshielded C and H are more deshielded

Page 7: Proton NMR

Chemical Shift

• We define the relative position of absorption in the NMR spectrum the chemical shift. It is a unitless number (actually a ratio, in which the units cancel), but we assign ‘units’ of ppm or (Greek letter delta) units.

• For 1H, the usual scale of NMR spectra is 0 to 10 (or 12) ppm (or ).

• The usual 13C scale goes from 0 to about 220 ppm.• The zero point is defined as the position of absorption of

a standard, tetramethylsilane (TMS):• This standard has only one type

of C and only one type of H.Si

CH3

CH3

CH3

CH3

Page 8: Proton NMR

Proton Chemical Shift () vs. Electronegativity

-0.5

0

0.5

1

1.5

2

2.5

3

3.5

4

4.5

5

1.5 2 2.5 3 3.5 4 4.5

Electronegativity

H1

Ch

em

ica

l Sh

ift

Chemical Shifts

CH3 Si

CH3 C

CH3 N

CH3 O

CH3 F

Page 9: Proton NMR

Chemical Shifts

• Both 1H and 13C Chemical shifts are related to three major factors:– The hybridization (of carbon) (lai hóa của cacbon)– Presence of electronegative atoms or electron attracting

groups(sự có mặt của các nguyên tử có độ âm điện cao và nhóm hút điện tử)– The degree of substitution (1º, 2º or 3º). These latter effects

are most important in 13C NMR, and in that context are usually called ‘steric’ effects. (hiệu ứng lập thể)

• Now we’ll turn our attention to 1H NMR spectra (they are more complex, but provide more structural information)

Page 10: Proton NMR

1H Chemical Shifts

0123456789101112

downfield upfield

TMS

CH3

CH2

CH

C CC H

CCH3

O

Ar CH3

C C H

CX

HCO H

C CH

Aromatic HC

H

O

COH

O

1H Chemical shift ()

Page 11: Proton NMR

Classification of Protons

• To interpret or predict NMR spectra, one must first be able to classify proton (or carbon) environments.

• Easiest to classify are those that are unrelated, or different. Replacement of each of those one at a time with some group (G) in separate models creates constitutional isomers.

These protons have different chemical shifts. This classification is usually the most obvious.

CH3CH2CH2CH3: CH3CH2CHCH3

G

CH3CH2CH2CH2

G

Page 12: Proton NMR

Classification of Protons

• Homotopic hydrogens are those that upon replacement one at a time with some group (G) in separate models creates identical structures.

Homotopic protons have the same chemical shifts. We sometimes call them identical. Methyl hydrogens will always be in this category (because of free rotation around the bond to the methyl carbon). Molecular symmetry can also make protons homotopic.

CH3CH2CH2CH3 CH3CH2CH2C

G

HH

CH3CH2CH2C

H

GH

CH3CH2CH2C

H

HG

:

Page 13: Proton NMR

Classification of Protons

• If replacement of one hydrogen at a time in separate models creates enantiomers, the hydrogens are enantiotopic.

Enantiotopic protons have the same chemical shifts.

CH3CH2CH2CH3: C

CH3CH3CH2

HG

C

CH3CH3CH2

GH

Page 14: Proton NMR

Classification of Protons

• If replacement of hydrogens in separate models creates diastereomers, the hydrogens are diastereotopic.

Diastereotopic protons have different chemical shifts. Usually, in order to have diastereotopic protons, there has to be a stereocenter somewhere in the molecule. However, cis-trans alkene stereoisomers may also have diastereotopic protons.

CCH3

G H

CCH3

H Br

CCH3

H G

CCH3

H Br

CCH3

H H

CCH3

H Br:

Page 15: Proton NMR

1H NMR Problems

• How many unique proton environments are there in:

CH3CH2Br CH3CH2Br

CH3OCH2CH2CHCH3

CH3

CH3OCH2CH2CHCH3

CH3

CH3

C

CC

C

CC

CH3

H

H

H

H

H

CH3

2 environments

5 environments

4 environments

Page 16: Proton NMR

1H NMR Problems

C CCH3

H

CH3

CH3

C CCH3

H

CH3

CH3

C CCH2CH3

H

CH3CH2

HC C

CH2CH3

H

CH3CH2

H

4 environments

3 environments

Symmetry Simplifies Spectra!!!

Page 17: Proton NMR

CH3CCH3

O

Page 18: Proton NMR

CH3COCH3

O

CH3OCH3

Page 19: Proton NMR

Spin-spin splitting (Coupling)

• Proton NMR spectra are not typically as simple as CMR (13C NMR) spectra, which usually give a single peak for each different carbon atom in the structure.

• Proton NMR spectra are often much more complex.• Because of its nuclear spin, each proton exerts a slight

effect on the localized magnetic field experienced by its neighboring proton(s).

• The spin state ( or ) of any one proton is independent of any other proton.

• The energies of protons of different spin states are so nearly equal that there is close to a 50:50 chance for each proton to be up (or down).

Page 20: Proton NMR

Spin-spin splitting (Coupling)

• The spin states of the neighboring protons (those on the adjacent carbon) exert a small influence on the magnetic field, and therefore on the chemical shift of a given proton.

• The result is that proton signals in the NMR spectrum are typically split into multiplets. This phenomenon is called coupling; the consequence is signal splitting.

• The type of multiplet (doublet, triplet, quartet, etc.) depends on the number of protons on the next carbon.

Page 21: Proton NMR

The n+1 rule

• The multiplicity of a proton or a group of protons is given by the n+1 rule, where n = the number of protons on the adjacent (adjoining) carbon atom (or atoms)

n n+1 multiplet name (abbrev) intensity pattern

1 2 doublet (d) 1 : 1

2 3 triplet (t) 1 : 2 : 1

3 4 quartet (q) 1 : 3 : 3 : 1

4 5 quintet/pentet - 1 : 4 : 6 : 4 : 1

5 6 sextet - 1 : 5 : 10 : 10 : 5 : 1

6 7 septet/heptet - 1 : 6 : 15 : 20 :15 : 6 : 1

Page 22: Proton NMR

Multiplets

• Consider the ethyl group in chloroethane CH3CH2Cl.

• The methyl protons experience a magnetic field that is somewhat influenced by the chlorine on the adjacent carbon, but is also affected slightly by the nuclear spin states of the adjacent methylene (CH2) protons.

• The two CH2 protons can have the following possible combination of spins: magnetic field

two spin up (1 way)

one up and one down (2)

two spin down (1)

1 : 2 : 1 .• This results in a 1:2:1 triplet for the methyl group

Page 23: Proton NMR

Multiplets

• The magnetic field experienced by the CH2 protons in chloroethane (CH3CH2Cl) is mainly influenced by the electronegative chlorine.

• However, it is slightly perturbed by the spin states of the three methyl (CH3) protons on the adjoining carbon

• They have four possible combinations of spins: Three spin up (1 way)

Two up and one down (3)

Two down and one up (3)

Three spin down (1)

1 : 3 : 3 : 1

• As a result, the CH2 group appears as a 1:3:3:1 quartet.

Page 24: Proton NMR

Spectrum of chloroethane

• Putting the multiplets together gives the predicted spectrum.

• The pattern of a downfield quartet and an upfield triplet is typical of the presence of an ethyl group in the molecular structure.

• Note that the triplet is larger than the quartet. That is because there are 3 protons giving rise to the triplet, and only 2 protons giving rise to the quartet.

• The integrated signal areas are in a 3:2 ratio.

TMS

4 3 2 1 0

CH3CH2Cl

CH3

CH2

Page 25: Proton NMR

1H NMR Problems

• Predict the splitting patterns (multiplets) for each proton environment in the following:

CH3CHBr2

CH3OCH2CH2Br

ClCH2CH2CH2Cl

CH3CH2COCHCH3

CH3O

triplet

triplet

singlet

singlet

doublet

doublet

triplet

triplet

quartet

quartet

quintet

septet

triplet

triplet

triplet

quartet

Page 26: Proton NMR

The Integral

• Integration is performed to determine the relative number of protons in a given environment.

• The number is set at 1, 2 or 3 for a given peak, then the areas of the other signals are reported relative to that one.

• The integral should be rounded to the nearest whole number; after all, there is either 1, or 2, or 3 protons in a certain environment, never a decimal fraction.

• Our spectrometer prints the integral below the spectrum written sideways and in red.

Page 27: Proton NMR

CH3COCH2CH3

O

OCH2

OCH2

CH3

CH3

CH3

CH3

(2H) (3H) (3H)

Page 28: Proton NMR

CH3CH2COCH2CH3

O

CH3CH3

CH3CH3

CH3

CH3

OCH2OCH2

OCH2OCH2 CH2

CH2

Page 29: Proton NMR

C6H12O2ethyl butanoate

.

CH3CH2CH2COCH2CH3

O CH3CH3

OCH2OCH2

CH2

CH2

Page 30: Proton NMR

CH3CCH2CH3

O

CH3

CH3

CH2

CH2

CH3

CH3

Page 31: Proton NMR

CH3C

OHH

H

HH

CH3

CH3

CC

C

CC

C

H

H

H

H

HH

H

H

H

H

H

Page 32: Proton NMR

CH3

CH3

CH2

CH2

CH2 O

CH2 O

OH

OH

CH3CH2CH2OH

Page 33: Proton NMR

CH3CH2CH2CH2OH

CH3

CH3

CH2

CH2

CH2

CH2

CH2 O

CH2 O

OH

OH

Page 34: Proton NMR

CH3CH2CH2CH2CH2OH

OH

OH

CH2 O

CH2 O

CH2

CH2

CH2

CH2

and

and

CH2

CH2

CH3

CH3

Page 35: Proton NMR

CH3

HH

H

H

H

CH3

CH3

H

H

H

H

H

H

other Hs

other Hs

Page 36: Proton NMR

CH3CH2CH2Br

CH3

CH3

CH2

CH2

CH2

CH2

Page 37: Proton NMR

2-methyl-1-hexene

CH2

CCH3 CH2CH2CH2CH3

CH3

CH2CH2

CH2

CH2

CH3

Page 38: Proton NMR

C8H16CH2 CHCH2CH2CH2CH2CH2CH3

CH3

CH2CH2CH2CH2

HH

H

1-octene

Page 39: Proton NMR

C10H14 (sec-butylbenzene)

CHCH2CH3

CH3

H

HH

H

Aromatic Hs


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