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i
(d/dx) and E
-i
(d/dt). The followings are brief sketches to show the essence of the different methods.
,
the wave-length of the wave.
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, which is related to whether p and x can be measured simultaneously(= 0) or not ( 0), and the uncertainty principle p x (see "Schwartz's Inequality"). This qunatization process also linearizes the classical equations with the dependent variable , which allows the superposition of different states creating all kinds of quantum weirdness such as being in 2 places at once (by applying quantum theory to macroscopic scale). |
Figure 12-05a Quantization |
See Figure 12-05a,a for an even shorter introduction. See original derivation in Chapter 9, "Quantum Theory" by D. Bohm, 1951. |
. The scheme is implemented by matrices as shown in Figure 12-05a,b. The replacement of ordinary number by matrix can be interpreted as turning a definite entity into a blurry one, and that has exactly been shown by its relationship with the uncertainty principle
p
x
(see "Schwartz's Inequality").
from which we obtain p
-i
(d/dx), and all occurrences of p in the Hamiltonian H is substituted by such operator. See the wordy justification in 321 pages by P.A.M. Dirac in his 1926 thesis "The Principles of Quantum Mechanics".
(d/dx) can be derived as shown in Figure 12-05a,d (with some hindsights ?). See "Short-cut to the Introduction of Quantum Theory" for more details, and the original book on "Quantum Mechanics" by L. Susskind, 2014.
= 
,
= 2
,
,
E
t
,
i
(d/dt).
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These examples do not exhibits qunatization of E. It occurs only when a potential (energy) V is added to the free particle equation and V has to be something like a well to confine the particle. Such general form is called Schrodinger Equation
| |
Figure 12-05b Traveling Wave [view large image] |
Figure 12-05c Standing Wave |
which has the time dependent part separated out similar to the standing wave. For a given interacting potential V the problem is to find the Energy E and the corresponding wave function .
|
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This form of Schrodinger Equation can be used to find out the structure of the atom or molecule (in steady state and often with approximation). It was very important for finding out the intensity of spectral lines via the transition between energy levels. The basic concepts of superposition, perturbation, transition, and quantum measurement etc. can be explored in a system with an infinite square well potential, see "Mathematical Schrodinger's Cat (QM Basic)" for details. Another good example is the harmonic oscillator with V = kx2/2 (Figure 12-05d). |
Figure 12-05d Energy Quantization |
. Since the atomic nucleus move much slower than the electrons, the Born-Oppenheimer approximation can be adopted to separate the wave function
into
=
electrons
nuclei and the resulting equations are solved separately - the part for the electrons yields the electronic configuration while the vibrational and rotational states (of the nuclei) are obtained from the nuclear part. This method makes the equation more or less solvable but the task is still formidable with increasing number of particles. The Molecular Orbital Theory is used further to alleviate the computational difficulty in calculating the molecular structure (the nuclear part).