DeBroglie's matter waves weighing heavy upon his mind, Erwin Schrodinger
wanted time to ponder, time to consider all the implications. Schrodinger,
an Austrian physicist noted for his work on the physics of strings, took
flight to a villa in the Swiss Alps in 1925, leaving his wife behind and
gathering a former Viennese girlfriend. What would come of this (presumably)
quiet period of reflection and thought would forever change the landscape
of physics. Indeed, it would change the way we as a species reckons
the universe we live in.
A sort of microscopic solar system, with electrons orbiting about the nucleus like planets to stars -- the Bohr atomic model was proving to be of limited utility. For hydrogen atoms, the agreement between predicted and observed behavior was sterling. However, for atoms with more than one electron -- even helium with only two electrons -- predicted and observed behavior radically diverged. Schrodinger desired to develop a model that agreed with the experimental evidence. What came of that illicit vacation to the Swiss Alps was a model that was not derived from any other, a model that can be called an intuitive guess, a leap of imagination, a model that is astonishingly accurate.
In these pages, we will, for the sake of both
brevity and simplicity, only consider the time-independent Schrodinger
wave equation in one dimension. We will not consider the full
equation in all of its gruesome splendor. The time-independent Schrodinger
Wave Equation, which could validly be called Schrodinger's law, is given
by the differential equation
where j (x) is
the is the wave function, m is mass,
is Planck's constant divided by 2p,
E is the total energy of the particle, and U(x) is the potential
energy function of the particle. As when one ingests something disagreeable
and the natural reaction is nausea, so too is the natural reaction to this
equation. However, comfort may be taken if we consider that acceleration
is the second derivative of the position function and, therefore, could
be written
As surely as acceleration simplifies to something more palatable, The Schrodinger wave equation must simplify (a little, at least).
To find general solutions to this equation,
boundary conditions must be established. The principle conditions
that it must adhere to are
| 1. |
| 2. |
| 3. j (x) is a continuos function |
| 4. j (x) is a normalized function |
energy function has two states:
| 1. U(x)=0 for |
| 2. U(x)= |
Since it is physically impossible for the particle to be outside of
the box, it is the first state that is of interest. Indeed, this
simplifies the wave equation considerably, with the term U(x) dropping
out. Therefore, the wave equation corresponding to the particle in
the box is given by
Therefore, the wave equation becomes
It becomes clear, a trigonometric function like sine or cosine
would be a good candidate for j
(x). Therefore, our guess for the solutions to the
wave equations is
By the first above boundary condition, it is known that
Therefore,
where n=1,2,3,... When the smoke clears, we have that
where A is the function's amplitude. To determine the amplitude,
recall the fourth boundary condition, j
(x) is a normalized function. Mathematically, this
means
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In words, this states that the probability of finding the particle somewhere
on the x-axis is one or 100%. Waving hands a bit to omit the gory
details, this gives
Gasping for breath, we at last have unearthed the solution to the wave
equation for the particle of the nth quantum state in the rigid
box.