Schrödinger Equation: Difference between revisions
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<math> -\frac{\hbar^2}{2m}\nabla^2\psi+V(\textbf{r},t)\psi=E\psi. </math> | <math> -\frac{\hbar^2}{2m}\nabla^2\psi+V(\textbf{r},t)\psi=E\psi. </math> | ||
As stated before, the wave function is a measure of the probability that a particle is in a given state; in fact, the probability density of finding a particle at a position <math>\textbf{r}</math> at a given time <math>t</math> is <math>|\Psi(\textbf{r},t)|^2</math>, or <math>|\psi(\textbf{r})|^2</math> for the time-independent case. Because of this, the wave function must be normalized such that | |||
<math>\int d^3\textbf{r}\,|\Psi(\textbf{r},t)|^2 = 1,</math> | |||
or | |||
<math>\int d^3\textbf{r}\,|\psi(\textbf{r})|^2 = 1</math> | |||
in the time-independent case. We will also find that the Schrödinger equation respects conservation of probability, as expected. | |||
<b>Chapter Contents</b> | <b>Chapter Contents</b> |
Revision as of 12:17, 6 March 2013
In this chapter, we introduce the Schrödinger equation, the most fundamental equation in quantum mechanics. Given a Hamiltonian , this equation describes how the wave function evolves in time. In Dirac bra-ket notation, the (time-dependent) Schrödinger equation is
If the Hamiltonian does not depend on time, then the wave function can be written as
and we obtain the time-independent Schrödinger equation,
For a single particle in a potential , the Schrödinger equation becomes, when projected onto position space,
If the potential does not depend on time, then we obtain the time-independent form of the equation,
As stated before, the wave function is a measure of the probability that a particle is in a given state; in fact, the probability density of finding a particle at a position at a given time is , or for the time-independent case. Because of this, the wave function must be normalized such that
or
in the time-independent case. We will also find that the Schrödinger equation respects conservation of probability, as expected.
Chapter Contents