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in the time-independent case.  We will also find that the Schrödinger equation respects [[Conservation of Probability|conservation of probability]], as expected.
in the time-independent case.  We will also find that the Schrödinger equation respects [[Conservation of Probability|conservation of probability]], as expected.


<b>Chapter Contents</b>
== Chapter Contents ==


* [[Original Idea of Schrödinger Equation]]
* [[Original Idea of Schrödinger Equation]]

Revision as of 12:18, 6 March 2013

Quantum Mechanics A
SchrodEq.png
Schrödinger Equation
The most fundamental equation of quantum mechanics; given a Hamiltonian , it describes how a state evolves in time.
Basic Concepts and Theory of Motion
UV Catastrophe (Black-Body Radiation)
Photoelectric Effect
Stability of Matter
Double Slit Experiment
Stern-Gerlach Experiment
The Principle of Complementarity
The Correspondence Principle
The Philosophy of Quantum Theory
Brief Derivation of Schrödinger Equation
Relation Between the Wave Function and Probability Density
Stationary States
Heisenberg Uncertainty Principle
Some Consequences of the Uncertainty Principle
Linear Vector Spaces and Operators
Commutation Relations and Simultaneous Eigenvalues
The Schrödinger Equation in Dirac Notation
Transformations of Operators and Symmetry
Time Evolution of Expectation Values and Ehrenfest's Theorem
One-Dimensional Bound States
Oscillation Theorem
The Dirac Delta Function Potential
Scattering States, Transmission and Reflection
Motion in a Periodic Potential
Summary of One-Dimensional Systems
Harmonic Oscillator Spectrum and Eigenstates
Analytical Method for Solving the Simple Harmonic Oscillator
Coherent States
Charged Particles in an Electromagnetic Field
WKB Approximation
The Heisenberg Picture: Equations of Motion for Operators
The Interaction Picture
The Virial Theorem
Commutation Relations
Angular Momentum as a Generator of Rotations in 3D
Spherical Coordinates
Eigenvalue Quantization
Orbital Angular Momentum Eigenfunctions
General Formalism
Free Particle in Spherical Coordinates
Spherical Well
Isotropic Harmonic Oscillator
Hydrogen Atom
WKB in Spherical Coordinates
Feynman Path Integrals
The Free-Particle Propagator
Propagator for the Harmonic Oscillator
Differential Cross Section and the Green's Function Formulation of Scattering
Central Potential Scattering and Phase Shifts
Coulomb Potential Scattering

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