Theory of NMR Nuclear Magnetic Resonance (NMR) Spectroscopy • 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. e- Part 1 Carbon 13 NMR • Nuclei are surrounded by electrons. The strong applied magnetic field (Bo) induces the electrons to circulate around the nucleus (left hand rule). Bo (9.4 T) Theory of NMR Theory of NMR • The positively charged nuclei of certain elements (e.g., 13C and 1H) behave as tiny magnets. • 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). • 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. Bi e- Bo • The latter (opposed) is slightly higher in energy than aligned with the field. Energy ΔE is very small Bo • 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. Theory of 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=hν. • 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 the 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. hν • 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 H C H H H δ H C Cl H C and H are deshielded H δ H C Cl Cl C and H are more deshielded 1 Chemical Shift CMR Spectra • 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 δ (Greek letter delta) units. • For 1H, the usual scale of NMR spectra is 0 to 10 (or 12) ppm (or δ). • 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): CH3 • This standard has only one type CH3 Si CH3 of C and only one type of H. CH3 • Each unique C in a structure gives a single peak in the spectrum; there is rarely any overlap. – The carbon spectrum spans over 200 ppm; chemical shifts only 0.001 ppm apart can be distinguished; this allows for over 2x105 possible chemical shifts for carbon. • The intensity (size) of each peak is NOT directly related to the number of that type of carbon. Other factors contribute to the size of a peak: – Peaks from carbon atoms that have attached hydrogen atoms are bigger than those that don’t have hydrogens attached. • Carbon chemical shifts are usually reported as downfield from the carbon signal of tetramethylsilane (TMS). 13C Chemical Shifts Chemical Shifts C13 Chemical Shift (δ ) vs. Electronegativity CH3 F 90 CH3 CH2 C13 Chemical Shift 80 CH3 O 70 60 CH CH3 N 50 CH3 C 40 C O C C CH3 Si 10 220 200 180 160 0 -10 1.5 2 C N Aromatic C 30 20 C X (halogen) C N 2.5 3 3.5 4 140 13C downfield C O TMS C C 120 100 Chemical shift (δ) 80 60 40 20 0 upfield Electronegativity Chemical Shifts • Both 1H and 13C Chemical shifts are related to three major factors: – The hybridization (of carbon) – Presence of electronegative atoms or electron attracting groups – 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. • First we’ll focus on Carbon NMR spectra (they are simpler) 2 Predicting 13C Spectra • Problem 13.6 Predict the number carbon resonance lines in the 13C spectra of the following: CH3 CH3 CH3 C C C 4 lines C C plane of symmetry CH3 CH3 CH3 CH3 C CH3 O O C c CH3 5 lines O CH3 CH3 C C CH3 5 lines H Predicting 13C Spectra • Predicted the number of carbon resonance lines in the 13C spectra of the products of the following reaction: CH3 CH3 Cl CH2 KOH or ??? ethanol, heat CH3 CH2 CH3 C c C c C C CH2 CH2 C 7 lines C C c C C 5 lines plane of symmetry 1 Predicting 13C Spectra CH3 H3C CH3 H3C CH3 CH3 C C C C 4 lines C C CH3 CH3 CH3 C C CH3 CH3 C C CH3 CH3 2 lines CH3 Symmetry Simplifies Spectra!!! O CH3CCH3 CH3 O C CDCl3 (solvent) 2 OCH3 CH3 O CH3COCH3 CDCl3 (solvent) O C CH3 OCH2 O CH3COCH2CH3 CH3 CDCl3 (solvent) O C 3 CH3 O OCH2 CH3 CH2 CH3CH2COCH2CH3 CDCl3 (solvent) O C O O22COCH2CH3 CH3C CH CH 6H212 ethyl butanoate CDCl3 (solvent) OCH2 CH2 CH3 CH2 CH3 O C 4 O CH2 CH3 CH3CCH2CH3 CH3 CDCl3 (solvent) O C H C H O C C C C C C and C H H CH3 C H CDCl3 (solvent) C C H H O CH3C H H H 5 CH2 CH3 CH2 CH3CH2CH2Br Br CDCl3 (solvent) CH3CH2CH2OH CH2 CH2 CH3 OH CDCl3 (solvent) 6 CH2 CH2 CH3 CH3CH2CH2CH2OH CH2 OH CDCl3 (solvent) CH2 CH2 CH3CH2CH2CH2CH2OH CH2 OH CH2 CH3 CDCl3 (solvent) 7 CH3 C C H C CDCl3 (solvent) C . 2-methyl-1-hexene CH3 and CH2 CDCl3 (solvent) CH2 CH2 CH2 CH3 C CH2 CH3 C CH2CH2CH2CH3 8
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