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Fourier Transforms in NMR, Optical, and Mass Spectrometry. A User's Handbook PDF

449 Pages·1990·12.456 MB·English
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Fourier Transforms in NMR, Optical, and Mass Spectrometry A User's Handbook Alan G. Marshall and Francis R. Verdun Departments of Chemistry and Biochemistry, The Ohio State University, Columbus, OH 43210-1173, U.S.A. Amsterdam — Oxford — New York — Tokyo 1990 ELSEVIER SCIENCE PUBLISHERS B.V. Sara Burgerhartstraat 25 P.O. Box 211, 1000 AE Amsterdam, The Netherlands Distributors for the United States and Canada: ELSEVIER SCIENCE PUBLISHING COMPANY INC. 655, Avenue of the Americas New York, NY 10010, U.S.A. Library of Congress Catalog1ng-1n-Publ1cat1on Data Marshal 1, Alan G., 1944- Fourier transforms 1n NMR, optical, and mass spectrometry : a user's handbook / by Alan G. Marshall and Francis R. Verdun. p. cm. Includes Index. ISBN 0-444-87360-0 1. Fourier transform spectroscopy. 2. Nuclear magnetic resonance spectroscopy. 3. Spectrum analysis. 4. Mass spectrometry. I. Verdun, Francis R. II. Title. QD96.F68M37 1989 543'.0877~dc20 89-1518 CIP ISBN 0-444-87360-0 (hard bound) ISBN 0-444-87412-7 (paperback) © Elsevier Science Publishers B.V., 1990 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system or transmitted in any form or by any means, electronic, mechanical, photocopying, recording or otherwise, without the prior written permission of the publisher, Elsevier Science Publishers B.V./ Physical Sciences & Engineering Division, P.O. Box 330, 1000 AH Amsterdam, The Netherlands. Special regulations for readers in the USA - This publication has been registered with the Copyright Clearance Center Inc. (CCC), Salem, Massachusetts. Information can be obtained from the CCC about conditions under which photocopies of parts of this publication may be made in the USA. All other copyright questions, including photocopying outside of the USA, should be referred to the publisher. No responsibility is assumed by the Publisher for any injury and/or damage to persons or property as a matter of products 'lability, negligence or otherwise, or from any use or operation of any meth­ ods, products, instructions or ideas contained in the material herein. Although all advertising material is expected to conform to ethical (medical) standards, inclusion in this publication does not constitute a guarantee or endorsement of the quality or value of such product or of the claims made of it by its manufacturer. This book is printed on acid-free paper. Printed in The Netherlands Dedicated to Devon W. Meek for helping to bring one of the authors (A.G.M.) to The Ohio State University in 1980, and more generally for his unstinting and selfless efforts on behalf of faculty, staff, and students during his terms as Chairman of the OSU Chemistry Department. XV PREFACE This book is offered as a teaching and reference text for Fourier transform methods as they are applied in spectroscopy. Whereas several other books treat either the mathematics or one type of spectroscopy, or offer a collection of chapters by several authors, the present monograph offers a unified treatment of the three most popular types of FT/spectroscopy, with uniform notation and complete indexing of specialized terms. All mathematics is self-contained, and requires only a knowledge of simple calculus. The main emphasis is on pictures (-200 original illustrations) and physical analogs, with sufficient supporting algebra to enable the reader to enter the literature. Instructive problems offer extensions from the basic treatment. Solutions are given or outlined for all problems. Because the book aims to inform practicing spectroscopists, non-ideal effects are treated in detail: noise (source- and detector-limited); non-linear response; limits to spectrometer performance based on finite detection period, finite data size, mis-phasing, etc. Common puzzles and paradoxes are explained: e.g., use of mathematically complex variables to represent physically real quantities; interpretation of negative-frequency signals; on-resonance vs. off-resonance response; interpolation (when it helps and when it doesn't); ultimate accuracy of discrete representation of an analog signal; differences between linearly- and circularly-polarized radiation; multiplex advantage or disadvantage, etc. Chapter 1 introduces the fundamental line shapes encountered in spectroscopy, from a simple classical mass-on-a-spring model. The Fourier transform relationship between the time-domain response to a sudden impulse and the steady-state frequency-domain response (absorption and dispersion spectra) to a continuous oscillation are established and illustrated. Chapters 2 and 3 summarize the basic mathematics (definitions, formulas, theorems, and examples) for continuous (analog) and discrete (digital) Fourier transforms, and their practical implications. Experimental aspects which are common to the signal (Chapter 4) and noise (Chapter 5) in all forms of Fourier transform spectrometry are followed by separate treatments of those features which are unique to FT/MS (Chapter 7), FT/NMR (Chapter 8), FT/optical (Chapter 9), other types (Chapter 10) of FT/spectrometry. In Chapter 6, non-FT methods (e.g., autoregression, maximum entropy) are presented and critically compared to FT methods. The list of references includes both historical and comprehensive reviews and monographs, along with articles describing several key developments. The Appendices include Fast Fourier and Fast Hartley Transform algorithms in Fortran and Basic, a look-up table of useful integrals (definite and indefinite), and a pictorial atlas of the Fourier transform time/frequency functions most commonly encountered in FT spectroscopy. The comprehensive Index is designed to enable the reader to locate particular key words, including those with more than one name—e.g., foldover (aliasing), throughput (étendue or Jacquinot) advantage; apodization (windowing); Hubert transform (Kramers-Kronig transform. Bode relation), etc. xvi ACKNOWLEDGMENTS The authors acknowledge, with deep appreciation, the inspiration and assistance provided by past and present collaborators, particularly M. B. Comisarow, T. L. Ricca, D. C. Roe, T.-C. L. Wang, L. Chen, A. T. Hsu, C. E. Cottrell, J. E. Meier, C. P. Williams, M. Wang, P. B. Grosshans, Z. Liang, G. M. Alber, E. C. Craig, J. Skilling, and S. Goodman. We also thank several individuals for their critical and helpful comments about the manuscript: M. B. Comisarow, P. K. Dutta, T. Gäumann, P. R. Griffiths, T. L. Gustafson, J. A. de Haseth, M. Wang, G. M. Alber, P. B. Grosshans, N. M. M. Nibbering, and E. Williams. We thank G. M. Alber, E. J. Behrman, R. B. Cody, C. E. Cottrell, R. Doskotch, W. G. Fateley, B. S. Freiser, T. Gäumann, G. Horlick, D. Horton, D. Hunt, F. W. McLafferty, M. D. Morris, P. Schmalbrock, M. Wang, and J. Wu for providing illustrations. F.R.V. especially thanks T. Gäumann for his help and indulgence during the preparation of the manuscript. Finally, A.G.M. wishes to thank his family for their patience and support. 1 CHAPTER 1 Spectral line shape derived from the motion of a damped mass on a spring 1.1 Terminology Virtually everything we need to know about line shapes in Fourier transform spectra can be understood from the simple physical model of a mass on a spring. It is easy to see why. In general, if the (time-independent) force, F, acting on a particle of mass, m, varies with distance, x, we can express Newton's second law as a Taylor series in x, in which x is measured from some arbitrary origin (e.g., the center of an atom). d2x Net force = m -jr^ =ao + aix + a2 x2 + ··· (1.1) However, the representation of even a relatively simple force, such as the Coulomb force, m d2x/dt2 = q2/x2, between two particles each of charge, q, may require an infinite number of terms in Eq. 1.1. Fortunately, two simplifications render the problem tractable and useful. First, we can dispense with the constant term, ao, simply by choosing a suitable "reference" frame. For example, we can neglect the (constant) force of gravity in most problems. Second, if the force is so weak that the observed displacement, x, is very small (i.e., x » x2 » x3 ...), then we may conveniently neglect all of the higher order terms, leaving d2x Net force = m ,, = a l x (1.2) 2 If we then rename the constant, a i, as a new constant, -Jc, then Eq. 1.2 becomes identical to the equation for the (restoring) force for a weight (of mass, m) on a spring of force constant, k. d2 x Net force = m ^+2 = - k x (1.3) For example, even though we know that the force binding an electron to an atom or molecule is a Coulomb force, we may still treat the electron as if it were bound by springs, provided that whatever forces we apply do not displace the electron very far from its equilibrium position. Thus, because the electric and magnetic forces from electromagnetic waves (light, x-rays, radiofrequencies, microwaves, infrared, etc.) on atoms and molecules are indeed weak, we can successfully describe many effects of electromagnetic radiation on ions, atoms, and molecules using the same mathematics that describe the response of a simple mechanical weight on a spring to some externally applied "jiggling". Before we discuss the motion of a "jiggled" spring, it is useful to review the vocabulary of wave motion, since electromagnetic radiation can be described by the same language as that for ordinary water waves. 2 A transverse wave is a disturbance whose displacement oscillates in a direction perpendicular to the direction of propagation of the wave. For example, a Cork floating on water moves up and down vertically as the water wave moves along horizontally, as shown in Figure 1.1. Amplitude E Figure 1.1 Transverse monochromatic waves. Top: water wave, viewed according either to its displacement as a function of distance at a given time instant (left), or to its displacement as a function of time at a particular point in space. Bottom: electromagnetic wave (plane-polarized for simplest display). Both waves are generated continuously at the left of the figure, so that propagation is from left to right. See text for definitions of terms. 3 The amplitude of the wave is the maximum displacement from the equilibrium position. The wavelength, X, for a monochromatic (see below) wave is the distance (along the direction of propagation) between two successive points of maximal displacement at a given instant in time. The velocity, c, of a monochromatic wave is defined as the distance a given wave crest moves per unit time. The frequency, v (in cycles per second, or Hz), of a monochromatic wave is the number of times per second that the wave displacement at a given point in space passes through its maximum value. The period, T, is the time (in seconds) required to complete one cycle of the oscillation of a monochromatic wave. Finally, the phase (or "phase angle"), <p, of a wave at a given time instant, t, can be defined as the number of radians of oscillation accumulated since time zero (there are 2π radians per oscillation cycle). Beginning at an (arbitrary) zero time, phase angle accumulates at an "angular" velocity (or "angular" frequency), ω = 2πν radians per second, for a wave of frequency, v oscillations/second. The relations between the previous definitions are given by the following equations: c = Xv meter/second = (meter/cycle)«(cycles/second) (1.4) T = — seconds/cycle (1.5) v φ = φο + ω t radians accumulated since time zero (1.6) ω = 2 π v radians/second = (radians/cycle)-(cycles/second) (1.7) The principle of superposition states that when two waves travel through the same region of space, their displacements add, as, for example, when two light waves of different frequency (color) travel together. The ways (coherent, incoherent) in which two or more waves combine (interference, diffraction) will be discussed in Chapter 9.2.1. A wave is said to be monochromatic if all of its components have the same frequency (and thus the same wavelength). The intensity (joule m~2 s_1) of a wave is the energy flow per unit time across unit area perpendicular to the direction of propagation. Radiation power (Watts) is the product of intensity and cross-sectional area across which the wave passes. Intensity is proportional to the square of the wave amplitude, as may be seen by analogy to the water wave. If the amplitude of a water wave doubles, then the water molecules must travel twice as far in a given length of time, and therefore have on the average twice as much velocity. Since kinetic energy is proportional to the square of velocity, intensity must be proportional to the square of wave amplitude. Intensity ~ (amplitude)2 (1.8) Returning to Eq. 1.3, we recall that the equation of motion of a mass, m, attached to a spring of stiffness (spring constant), k, in the absence of any damping or driving force is d2x m^T2-+fcx=0 (1.3) The reader can quickly verify by substitution that Eq. 1.9 is a solution of Eq. 1.3 for the undamped, undriven mass on a spring. x= xo cos ω t (1.9) 0 4 in which ω» °° == VVm rn == natura^ angular frequency for mass on a spring (1.10) for a maximum initial displacement, x = x o at time, t = 0. Since there is no frictional "damping", the displacement (position) of the mass continues to oscillate sinusoidally indefinitely at the natural frequency, νο=ωο/2π Hz. Eq. 1.9 also shows why angular frequency is almost always used in the mathematical description of spring motion, since the wave frequency, v o, appears in the equa­ tions in the form, ω o = 2πν o · Armed with the necessary vocabulary, we are now prepared to discuss the motion of a mass on a spring in the presence of additional driving and damping forces. There are two ways to discover the natural frequency of a weight on a spring. One could simply strike the weight to displace it suddenly from its equilibrium position, and then count the oscillations per unit time as the mass moves up and down. Alternatively, one could jiggle the spring steadily at each of various "driving" frequencies and wait until the system settles into a steady-state motion; when the jiggling frequency matches the natural frequency, the system will oscillate with maximal amplitude (Just as a tuning fork is set into motion by sound applied at its natural frequency). These two approaches are shown schematically in Figure 1.2. If the driven spring were completely free to move, then when the driving frequency is set equal to (in "resonance" with) the natural spring frequency, vo, we would expect the spring to absorb energy continuously and execute larger and larger amplitude motion without limit. However, any real spring (including an electron bound to a molecule) is hindered in its motion by frictional resistance, or drag, expressed by a "damping" force (characterized by frictional coefficient, /) proportional to the velocity of the moving mass. dx Damping force = - / -JT (1.11) In the spectroscopic examples to be discussed later, the natural frequencies of various springs correspond to the frequencies of power absorption (peaks) in the spectrum and the damping constant of a given spring is related to the width of a spectral line. The practical interest in these parameters is that the natural frequencies indicate the strength of the spring of interest, and are related to color, chemical bond strength or type, optical activity, and ionic mass-to-charge ratio; spectral line widths reflect rates of molecular collisions, chemical reactions and molecular motions. 1.2 Transient response to a sudden impulse: relaxation The transient experiment consists of monitoring the displacement as a function of time for a damped mass on a spring (damped harmonic oscillator), just after the mass has been displaced by an initial distance, xo ♦ and then released. Mathematically, the equation of motion becomes d ^ x dx Net force = m ~^T =~kx ~ f ~di (112) Transient Dispersion Absorption ι ρ τ Hilbert Figure 1.2 Interrelations between various scattering, spectroscopy, and transient experiments, by analogy to the motion of either a sinusoidally driven or a suddenly displaced damped weight on a spring. The weight has mass, m , bound to a spring of force constant, k , immersed in a medium whose effect is represented by frictional coefficient, / , and is subjected either to a sinusoidally time-varying continuous force, F[t) = F cos ω t (steady-state response, left), or to a sudden 0 displacement (transient response, right) The massless limit corresponds to scattering (steady-state) or relaxation (transient) experiments. The various results are related by Fourier and Hubert transforms as shown.

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