By J. Michael Hollas
ISBN-10: 0470844159
ISBN-13: 9780470844151
ISBN-10: 0470844167
ISBN-13: 9780470844168
The most recent variation of this hugely acclaimed identify introduces the reader to quite a lot of spectroscopies, and contains either the history thought and purposes to constitution choice and chemical analysis. It covers rotational, vibrational, digital, photoelectron and Auger spectroscopy, in addition to EXAFs and the speculation of lasers and laser spectroscopy.
- A revised and up to date version of a winning, sincerely written e-book
- Includes the newest advancements in smooth laser options, resembling hollow space ring-down spectroscopy and femtosecond lasers
- Provides a variety of labored examples, calculations and questions on the finish of chapters
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Extra resources for Modern Spectroscopy
Sample text
28). For the quantum mechanical results that we require we shall be concerned only with stationary states, known sometimes as eigenstates. The wave functions for these states may be referred to as eigenfunctions and the associated energies E as the eigenvalues. The details of the methods of solving the Schro¨dinger equation for c and E for various systems do not concern us here but may be found in books listed in the bibliography. We require only the results, some of which will now be discussed.
1 illustrates one photon of such radiation travelling along the x axis. The electric component of the radiation is in the form of an oscillating electric field of strength E and the magnetic component is in the form of an oscillating magnetic field of strength H. These oscillating fields are at right angles to each other, as shown, and, if the directions of the vectors E and H are y and z respectively, then Ey ¼ A sinð2pnt À kxÞ Hz ¼ A sinð2pnt À kxÞ ) ð2:1Þ where A is the amplitude. Therefore, the fields oscillate sinusoidally with a frequency of 2pn and, because k is the same for each component, they are in-phase.
In the wave picture the circumference 2pr of an orbit of radius r must contain an integral number of wavelengths nl ¼ 2pr ð1:14Þ where n ¼ 1; 2; 3; . . ; 1, for a standing wave to be set up. 3(b) shows how a travelling wave results when n is not an integer: the wave interferes with itself and is destroyed. The picture of the electron in an orbit as a standing wave does, however, pose the important question of where the electron, regarded as a particle, is. We shall consider the answer to this for the case of an electron travelling with constant velocity in a direction x.
Modern Spectroscopy by J. Michael Hollas
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