Chemistry 125: Lecture 60 March 24, 2010 NMR Spectroscopy Isotropic J and Dynamics This For copyright notice see final page of this file.

Slides:



Advertisements
Similar presentations
1 The world leader in serving science A Practical Introduction to Nuclear Magnetic Resonance Spectroscopy Basic Theory.
Advertisements

1 Signals from coupled protons that are close together (in Hz) can show distorted patterns. When ν >> J, the spectra is said to be first-order. Non-first-order.
NMR Spectroscopy.
Chemistry 125: Lecture 60 March 23, 2011 NMR Spectroscopy Chemical Shift and Diamagnetic Anisotropy, Spin-Spin Coupling This For copyright notice see final.
1 Nuclear Magnetic Resonance Spectroscopy III Advanced Concepts: ORGANIC I LABORATORY W. J. Kelly.
NMR Spectroscopy Part II. Signals of NMR. Free Induction Decay (FID) FID represents the time-domain response of the spin system following application.
After applying the united-atom “plum-pudding” view of molecular orbitals, introduced in the previous lecture, to more complex molecules, this lecture introduces.
Chemistry 125: Lecture 48 February 8, 2010 Addition to Alkenes a Physical-Organic MO Perspective This For copyright notice see final page of this file.
Chemistry 125: Lecture 16 October 9, 2009 Reaction Analogies and Carbonyl Reactivity Comparing the low LUMOs that make both HF and CH 3 F acidic underlines.
Chemistry 125: Lecture 64 April 7, 2010 Carbonyl Compounds Preliminary This For copyright notice see final page of this file.
Chemistry 125: Lecture 55 February 24, 2010 (4n+2) Aromaticity Cycloaddition Electrocyclic Reactions This For copyright notice see final page of this file.
Chemistry 125: Lecture 61 March 26, 2010 NMR Spectroscopy Through-Space Coupling, Decoupling & Correlation This For copyright notice see final page of.
Chemistry 125: Lecture 43 January 25, 2010 Solvation, Ionophores and Brønsted Acidity This For copyright notice see final page of this file.
Chemistry 125: Lecture 66 April 9, 2010 Oxidizing/Reducing Reagents Bookeeping & Mechanism This For copyright notice see final page of this file.
After applying the united-atom “plum-pudding” view of molecular orbitals, introduced in the previous lecture, to a more complex molecule, this lecture.
After discussion of how increased nuclear charge affects the energies of one-electron atoms and discussion of hybridization, this lecture finally addresses.
Case Western Reserve University
Chemistry 125: Lecture 47 February 5, 2010 Addition to Alkenes a Synthetic Perspective guest lecture by Prof. Jay S. Siegel Universit ä t Zurich This For.
Chemistry 125: Lecture 71 April 21, 2010  -H Reactivity (Ch. 19) A Few Topics in Carbohydrate Chemistry (Ch. 22) Preliminary This For copyright notice.
Chemistry 125: Lecture 40 January 15, 2010 Predicting Rate Constants, and Reactivity - Selectivity Relation. Rates of Chain Reactions. This For copyright.
Chemistry 125: Lecture 64 April 2, 2010 Carbonyl Compounds Overview This For copyright notice see final page of this file.
Chemistry 125: Lecture 65 April 7, 2010 Addition to C=O Mechanism & Equilibrium Protecting Groups Oxidation/Reduction & Electron Transfer This For copyright.
Chemistry 125: Lecture 17 Reaction Analogies and Carbonyl Reactivity In molecular orbital terms there is a close analogy among seemingly disparate organic.
Chemistry 125: Lecture 57 March 3, 2010 Normal Modes: Mixing and Independence in Infrared Spectroscopy This For copyright notice see final page of this.
Chemistry 125: Lecture 69 April 16, 2010 Decarboxylation (Ch. 17) and Acyl Compounds (Ch. 18) This For copyright notice see final page of this file.
Chemistry 125: Lecture 54 February 22, 2010 Linear and Cyclic Conjugation Allylic Intermediates (4n+2) Aromaticity This For copyright notice see final.
After discussion of how increased nuclear charge affects the energies of one-electron atoms and discussion of hybridization, this lecture finally addresses.
Chemistry 125: Lecture 71 April 21, 2010  -H Reactivity (Ch. 19) A Few Topics in Carbohydrate Chemistry (Ch. 22) Preliminary This For copyright notice.
Chemistry 125: Lecture 14 Checking Hybridization Theory with XH 3 Synchronize when the speaker finishes saying “…whether what we have done is realistic.
Nuclear Magnetic Resonance (NMR) Spectroscopy
Chemistry 125: Lecture 65 April 4, 2011 Addition to C=O Mechanism & Equilibrium Protecting Groups Imines This For copyright notice see final page of this.
Chapter 13 Nuclear Magnetic Resonance Spectroscopy
1 Nuclear Magnetic Resonance Spectroscopy Renee Y. Becker Valencia Community College CHM 2011C.
NMR = Nuclear Magnetic Resonance Some (but not all) nuclei, such as 1 H, 13 C, 19 F, 31 P have nuclear spin. A spinning charge creates a magnetic moment,
Chapter 10 NMR in Practice I.Chemical Equivalence A.Using Molecular Symmetry 1)Chemically equivalent protons have identical chemical shifts 2)It is not.
13.6 Interpreting Proton NMR Spectra. 1. number of signals 2. their intensity (as measured by area under peak) 3. splitting pattern (multiplicity) Information.
Proton NMR Spectroscopy. The NMR Phenomenon Most nuclei possess an intrinsic angular momentum, P. Any spinning charged particle generates a magnetic field.
13. Structure Determination: Nuclear Magnetic Resonance Spectroscopy Based on McMurry’s Organic Chemistry, 7 th edition.
Chemistry 125: Lecture 59 March 22, 2010 NMR Spectroscopy Chemical Shift and Spin-Spin Coupling This For copyright notice see final page of this file.
Nuclear Magnetic Resonance Spectroscopy. The Use of NMR Spectroscopy Used to map carbon-hydrogen framework of molecules Most helpful spectroscopic technique.
Nuclear Magnetic Resonance Spectroscopy
Nuclear Magnetic Resonance
NMR-Part Chemical Shifts in NMR The nuclei not only interact with the magnetic field but also with the surronding nuclei and their electrons. The.
Nuclear Magnetic Resonance Spectroscopy Dr. Sheppard Chemistry 2412L.
13. Structure Determination: Nuclear Magnetic Resonance Spectroscopy Based on McMurry’s Organic Chemistry, 6 th edition.
1 Chapter 13 Nuclear Magnetic Resonance Spectroscopy Leroy Wade.
Nuclear Magnetic Resonance Spectroscopy. 2 Introduction NMR is the most powerful tool available for organic structure determination. It is used to study.
Nuclear Magnetic Resonance Spectroscopy
Chapter 14 NMR Spectroscopy Organic Chemistry 6th Edition Dr. Halligan
Learning Objectives Use high resolution n.m.r spectrum of simple molecules (carbon, hydrogen & oxygen) to predict The different types of proton present.
NMR Spectroscopy A proton NMR spectrum. Information from peaks: Size (integration), position and multiplicity.
All atoms, except those that have an even atomic number and an even mass number, have a property called spin.
Nuclear Magnetic Resonance Information Gained: Different chemical environments of nuclei being analyzed ( 1 H nuclei): chemical shift The number of nuclei.
Chapter 13 Structure Determination: Nuclear Magnetic Resonance Spectroscopy.
NMR Spectroscopy. NMR NMR uses energy in the radio frequency range. NMR uses energy in the radio frequency range. This energy is too low to cause changes.
The Number of Absorptions Protons have different chemical shifts when they are in different chemical environments Types of protons: – Homotopic Protons.
Nuclear Magnetic Resonance Spectroscopy A proton NMR spectrum. Information from peaks: magnitude (integration), position and multiplicity.
NUCLEAR MAGNETIC RESONANCE SPECTROSCOPY … or NMR for short.
Chemistry 125: Lecture 48 February 7, 2011 Alkenes: Stability and Addition Mechanisms Electrophilic Addition This For copyright notice see final page of.
Nuclear Magnetic Resonance Spectroscopy
Structure Elucidation Method
13.6 Interpreting 1H NMR Spectra
MOLECULAR STRUCTURE ANALYSIS NMR Spectroscopy VCE Chemistry Unit 3: Chemical Pathways Area of Study 2 – Organic Chemistry.
Nuclear magnetic resonance Spectroscopy Basic Concept.
11.1 Nuclear Magnetic Resonance Spectroscopy
NMR spectroscopy – key principles
The Use of NMR Spectroscopy
Structure Determination: Nuclear Magnetic Resonance Spectroscopy
1H NMR spectrum of: All signals in spectrum are due to a proton
Diamagnetic Anisotropy, Spin-Spin Coupling
Presentation transcript:

Chemistry 125: Lecture 60 March 24, 2010 NMR Spectroscopy Isotropic J and Dynamics This For copyright notice see final page of this file

ZERO! average over sphere Electrons Orbiting Other Nuclei B applied

Isotropic J H-H is mediated by bonding electrons (the anisotropic through-space part is averaged to zero by tumbling)

15.44.jpg Not spatial proximity! 3.07 Å 1.85 Å 2.38 Å Might overlap be greater for anti C-H bonds ?? HOMO-3 When the “up” electron of this MO is on Nucleus A only its “down” electron is available to be on Nucleus B In tumbling molecules, nuclear spins communicate not through space, but through paired electrons on the nuclei. Through-space interaction of dipoles averages to zero on tumbling.

15.44.jpg good p  -p  good s-s bad p  -p  bad s-s 2 bad s-p  good s-p  ; good p  -s s-p  > s-s and p   p  (lecture 13 frame 2) Better Overlap! ++  ++

H No “handle” if same chem shift (see Frame 11 below) 2-13 Hz, depends on conformation (overlap) 13 Hz2 Hz H gauche ~7 Hz 11 Hz (approximate way to measure torsional angle!)

J C-H 13 Amplify 30x 126 Hz Coupling electron must be on the C 13 nucleus. 99% of sample is C 12 (instrumental artifact)

Hybridization and J coupling sp 3 sp 2 sp

Units for  and J ppmHz

Energy Scale Same Frequency (Hz) Scale (relative to TMS) Same ppm (  ) Scale 0 Hz300 Hz

Two unsymmetrical Doublets  a b

Lose the “handle” as  becomes smaller than J   By increasing  (Hz) big magnet reduces asymmetry and gives “ideal” pattern. Note:  is measured in Hz (not ppm) between the weighted average positions of the lines in the two doublets

Slope up toward splitting partner quartet * * * * doublets of * * * * Cf. Fig , p. 738

Dynamics (the NMR Time Scale / Decoupling) Sec pp Sec. 15.6e p. 739

ROH chemical shift? CH 3 CH 2 OH spin-spin splitting? average of many H-bond structures (dependent on concentration & temperature) average for exchange among many molecules (H + / solvent) Three OH peaks from three different kinds of molecules (with different neighboring CH 2 proton spins) Fig p

Form A Why doesn’t IR show OH averaging? 110 x Hz102 x Hz Difference ~ Hz (This particular sample is a solid, but no averaging is observed in solution spectra either.)

How long does it take to measure frequency precisely? 1 second 20 Hz 22 Hz 21 Hz But a 1 sec pulse samples full range of phases. 0.5 sec (1/  ) is long enough to sample the full range, favorable and unfavorable. Match with a short pulse of 20 Hz light is nearly as good. No net interaction with light. 1 sec light pulse distinguishes 20 Hz from 21 Hz. light field

What if protons are “exchanging” faster than 1/  ? 1 second 20 Hz 22 Hz 21 Hz 22 Hz 20 Hz 22 Hz20 Hz Very good match with the 21Hz average frequency  single, sharp peak.

When do Peaks Average? When atoms don’t stay put long enough to tell the difference in frequency. e.g. If two peaks differ by 100 Hz, you must count for ~0.01 sec to tell them apart. These IR peaks differ by Hz. Exchange of position is not that fast.

One average chemical shift (no splitting observed) equatorial axial 15.58

Compared to What? The NMR Time Scale p Hz Coalescence at ~30 flips per second axial equatorial d 11 to avoid complications from spin-spin splitting.

a Probably no splitting (broad singlet) because of rapid OH proton exchange among different molecules 1:1 doublet from single H on neighboring carbon (J about 7 Hz) Almost anyplace (  1-6) depending on concentration and temperature (averaged H-bonding) Slightly deshielded by two oxygen atoms on neighboring carbon  1-2 (a real analogue is at  1.3) b c Deshielded by two oxygen atoms on the same carbon  4-5 (a real analogue is at  4.7) 1:3:3:1 quartet from three H atoms on neighboring carbon (J about 7 Hz)

d 1:1 doublet from single H on neighboring C (J about 7 Hz) Seven line multiplet from 6 H atoms on neighboring carbons (J about 7 Hz) Slightly deshielded by oxygen atom on neighboring carbon  1 (a real analogue is at  1.1) Deshielded by oxygen atom on the same carbon (but less than c)  4 (a real analogue is at  3.8) e f Slightly deshielded by oxygen atom on neighboring carbon.  1 (a real analogue is at  1.1) 1:1 doublet from single H on neighboring carbon (J about 7 Hz) different from d (diastereotopic)

End of Lecture 60 March 24, 2010 Copyright © J. M. McBride Some rights reserved. Except for cited third-party materials, and those used by visiting speakers, all content is licensed under a Creative Commons License (Attribution-NonCommercial-ShareAlike 3.0).Creative Commons License (Attribution-NonCommercial-ShareAlike 3.0) Use of this content constitutes your acceptance of the noted license and the terms and conditions of use. Materials from Wikimedia Commons are denoted by the symbol. Third party materials may be subject to additional intellectual property notices, information, or restrictions. The following attribution may be used when reusing material that is not identified as third-party content: J. M. McBride, Chem 125. License: Creative Commons BY-NC-SA 3.0