The Schrödinger Equation in Dirac Notation: Difference between revisions

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where <math> c_n </math> is a complex number.  
where <math> c_n </math> is a complex number.  


By projecting the state vector <math>|\psi\rangle</math> onto different bases, we can obtain the wave functions of the system in different bases. For example, if we project <math>|\psi\rangle</math> onto the position basis <math>\langle \textbf{r}|,</math> we would get <math>\langle\textbf{r}|\psi\rangle \equiv  \psi(\textbf{r}),</math> while projecting onto the momentum basis <math>\langle \textbf{p}|</math> gives us <math>\langle\textbf{p}|\psi\rangle \equiv  \phi(\textbf{p}).</math>  We interpret <math>|\psi( \textbf{r} )|^{2}</math> as the probability density of finding the system at position <math>\textbf{r},</math> and <math>|\phi( \textbf{p} )|^{2}</math> as the probability density of finding the system with momentum <math>\textbf{p}</math>.


By projecting the state vector <math>|\psi\rangle</math> onto different bases, we can obtain the wave functions of the system in different bases. For example, if we project <math>|\psi\rangle</math> onto the position basis <math>\langle \textbf{r}|,</math> we would get <math>\langle\textbf{r}|\psi\rangle \equiv  \psi(\textbf{r}),</math> while projecting onto the momentum basis <math>\langle \textbf{p}|</math> gives us <math>\langle\textbf{p}|\psi\rangle \equiv  \psi(\textbf{p}).</math>  We interpret <math>|\psi( \textbf{r} )|^{2}</math> as the probability density of finding the system at position <math>\textbf{r},</math> and <math>|\psi( \textbf{p} )|^{2}</math> as the probability density of finding the system with momentum <math>\textbf{p}</math>.


In Dirac notation, the scalar product of two state vectors <math>|\phi\rangle</math> and <math>|\psi\rangle</math> is denoted by a “bracket” <math>\langle\phi|\psi\rangle </math>.  In the position-space representation, the scalar product is given by


In Dirac notation, the scalar product of two state vectors (<math> \phi\ </math>, <math> \psi\ </math>) is denoted by a “bra-ket” <math>\langle\phi|\psi\rangle </math>. In coordinate representation the scalar product is given by:
<math>\langle\phi|\psi\rangle = \int \phi^{\ast}(\mathbf{r},t)\psi(\mathbf{r},t)\,d^3\mathbf{r},</math>


<math>\langle\phi|\psi\rangle = \int \phi^*(r,t)\psi(r,t)d^3r </math>
and thus the normalization condition may now be written as


And so, the normalization condition may now be written:
<math>\langle\psi_m|\psi_n\rangle = \delta_{mn}.</math>


<math>\langle\psi_m|\psi_n\rangle = \delta_{mn} </math>
This additionally shows that any wave function is determined to within a phase factor, <math> e^{i\gamma}</math>, where <math>\gamma</math> is some real number.
 
Which additionally shows that any wavevector is determined to within a phase factor, <math> e^{i\gamma}</math>, where <math>\gamma</math> is some real number.


The vectors in this space also obey some useful rules following from the fact that the Hilbert space is linear and complete:  
The vectors in this space also obey some useful rules following from the fact that the Hilbert space is linear and complete:  


<math> \langle\phi|c\psi\rangle = c\langle\phi|\psi\rangle </math>
<math> \langle\phi|c\psi\rangle = c\langle\phi|\psi\rangle </math>


<math> \langle c\phi|\psi\rangle = c^*\langle\phi|\psi\rangle </math> where c is some c-number.  
<math> \langle c\phi|\psi\rangle = c^*\langle\phi|\psi\rangle </math> where <math>c</math> is a complex number.  


<math> \langle\phi|\psi_1 + \psi_2\rangle = \langle\phi|\psi_1\rangle + \langle\phi|\psi_2\rangle </math>
<math> \langle\phi|\psi_1 + \psi_2\rangle = \langle\phi|\psi_1\rangle + \langle\phi|\psi_2\rangle </math>


In Dirac notation, the [[Schrödinger Equation|Schrödinger equation]] is written as


In Dirac's notation, [[Schrödinger Equation|Schrödinger's equation]] is written as
<math>i\hbar \frac{d}{dt}|\psi(t)\rangle=\mathcal{H}|\psi(t)\rangle </math>  
 
<math>i\hbar \frac{\partial}{\partial t}|\psi(t)\rangle=\mathcal{H}|\psi(t)\rangle </math>  
 
By projecting the equation in position space, we can obtain the previous form of Schrödinger's equation:


<math> i\hbar\frac{\partial \psi(\textbf{r},t)}{\partial t} = \left[ -\frac{\hbar^2}{2m}\nabla^2 + V(\textbf{r})\right]\psi(\textbf{r},t)</math>
By projecting the equation in position space, we can obtain the previous form of the Schrödinger equation,


On the other hand, we can also project the Schrödinger's equation in other space like momentum space and obtain:
<math> i\hbar\frac{\partial \psi(\textbf{r},t)}{\partial t} = \left[ -\frac{\hbar^2}{2m}\nabla^2 + V(\textbf{r})\right]\psi(\textbf{r},t).</math>


<math> i\hbar\frac{\partial \psi(\textbf{p},t)}{\partial t} = \left[ \frac{\textbf {p}^{2}}{2m} + V\left ( i\hbar \frac{\partial}{\partial \textbf{p}}\right)\right]\psi(\textbf{p},t)</math>
On the other hand, we can also project it into momentum space and obtain


where <math>\psi(\textbf{p},t)</math> and <math>\psi(\textbf{r},t)</math> are related through Fourier transform as described in the [[Heisenberg Uncertainty Principle|next section]]<nowiki />.
<math> i\hbar\frac{\partial \phi(\textbf{p},t)}{\partial t} = \left[ \frac{\textbf {p}^{2}}{2m} + V\left ( i\hbar \frac{\partial}{\partial \textbf{p}}\right)\right]\phi(\textbf{p},t),</math>


where <math>\phi(\textbf{p},t)</math> and <math>\psi(\textbf{r},t)</math> are related through Fourier transform as described in the [[Heisenberg Uncertainty Principle|next section]]<nowiki />.


For time-independent Hamiltonians, Schrödinger's equation separates and we can seek the solution in the form of stationary states.
For time-independent Hamiltonians, the wave function may be separated into a position-dependent part and a time-dependent part,


<math>|\psi_n(t)\rangle=e^{-iE_n t/\hbar}|\psi_n\rangle</math>.
<math>|\psi_n(t)\rangle=e^{-iE_n t/\hbar}|\psi_n\rangle</math>.


The equation for stationary states in the Dirac notation is then
as described [[Stationary States|previously]], thus yielding the equation for stationary states in Dirac notation:


<math>E_n|\psi_n\rangle=\mathcal{H}|\psi_n\rangle.</math>
<math>E_n|\psi_n\rangle=\mathcal{H}|\psi_n\rangle.</math>


The eigenfunctions (now also referred to as eigenvectors) are replaced by eigenkets.  Use of this notation makes solution of the Schrödinger equation much simpler for some problems, where the Hamiltonian can be re-written in the form of matrix operators having some algebra (defined set of operations on the basis vectors) over the Hilbert space of the eigenvectors of that Hamiltonian. (See the section on Operators.)
The eigenfunctions (now also referred to as eigenvectors) are replaced by eigenkets.  Use of this notation makes solution of the Schrödinger equation much simpler for some problems, where the Hamiltonian can be re-written in the form of matrix operators having some algebra (defined set of operations on the basis vectors) over the Hilbert space of the eigenvectors of that Hamiltonian. (See the section on [[Operators, Eigenfunctions, Symmetry, and Time Evolution|operators]].)


If we prepare an arbitrary state <math>|\phi\rangle </math> at t=0, how does it evolve in time? <math>|\phi\rangle </math> can be expressed as the linear superposition of the energy eignstates:
We now ask how an arbitrary state <math>|\phi\rangle </math> evolves in time? The initial state <math>|\phi\rangle </math> can be expressed as the linear superposition of the energy eignstates:


<math> | \phi \rangle=\sum_{n}c_n| \psi_n \rangle </math>
<math> | \phi \rangle=\sum_{n}c_n| \psi_n \rangle </math>


Then, we can get:
We can then solve the time-dependent Schrödinger equation, we obtain, for a time-independent Hamiltonian,


<math> | \phi(t) \rangle=e^{-i\mathcal{H} t/\hbar}| \phi \rangle=e^{-i\mathcal{H} t/\hbar}\sum_{n}c_n| \psi_n \rangle=\sum_{n}c_ne^{-iE_n t/\hbar}|\psi_n\rangle </math>.
<math> | \phi(t) \rangle=e^{-i\mathcal{H} t/\hbar}| \phi \rangle=e^{-i\mathcal{H} t/\hbar}\sum_{n}c_n| \psi_n \rangle=\sum_{n}c_ne^{-iE_n t/\hbar}|\psi_n\rangle.</math>

Revision as of 11:06, 17 April 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

The physical state of a system is represented by a set of probability amplitudes (wave functions), which form a linear vector space. This linear vector space is a particular type of space called a Hilbert Space. Another way to think about the Hilbert space is as an infinite-dimensional space of square normalizable functions. This is analogous to a three-dimensional space, where the basis is in a generalized coordinate system. In the Hilbert space, the basis is formed by an infinite set of complex functions. The basis for a Hilbert space is written like , where each is a complex vector function.

We denote a state vector in Hilbert space with Dirac notation as a “ket” , and its complex conjugate (or dual vector) is denoted by a “bra” .

Therefore, in the space of wavefunctions that belong to the Hilbert space, any wave function can be written as a linear combination of the basis functions:

where is a complex number.

By projecting the state vector onto different bases, we can obtain the wave functions of the system in different bases. For example, if we project onto the position basis we would get while projecting onto the momentum basis gives us We interpret as the probability density of finding the system at position and as the probability density of finding the system with momentum .


In Dirac notation, the scalar product of two state vectors and is denoted by a “bracket” . In the position-space representation, the scalar product is given by

and thus the normalization condition may now be written as

This additionally shows that any wave function is determined to within a phase factor, , where Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \gamma} is some real number.

The vectors in this space also obey some useful rules following from the fact that the Hilbert space is linear and complete:

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \langle\phi|c\psi\rangle = c\langle\phi|\psi\rangle }

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \langle c\phi|\psi\rangle = c^*\langle\phi|\psi\rangle } where Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle c} is a complex number.

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \langle\phi|\psi_1 + \psi_2\rangle = \langle\phi|\psi_1\rangle + \langle\phi|\psi_2\rangle }

In Dirac notation, the Schrödinger equation is written as

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle i\hbar \frac{d}{dt}|\psi(t)\rangle=\mathcal{H}|\psi(t)\rangle }

By projecting the equation in position space, we can obtain the previous form of the Schrödinger equation,

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle i\hbar\frac{\partial \psi(\textbf{r},t)}{\partial t} = \left[ -\frac{\hbar^2}{2m}\nabla^2 + V(\textbf{r})\right]\psi(\textbf{r},t).}

On the other hand, we can also project it into momentum space and obtain

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle i\hbar\frac{\partial \phi(\textbf{p},t)}{\partial t} = \left[ \frac{\textbf {p}^{2}}{2m} + V\left ( i\hbar \frac{\partial}{\partial \textbf{p}}\right)\right]\phi(\textbf{p},t),}

where Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \phi(\textbf{p},t)} and Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \psi(\textbf{r},t)} are related through Fourier transform as described in the next section.

For time-independent Hamiltonians, the wave function may be separated into a position-dependent part and a time-dependent part,

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle |\psi_n(t)\rangle=e^{-iE_n t/\hbar}|\psi_n\rangle} .

as described previously, thus yielding the equation for stationary states in Dirac notation:

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle E_n|\psi_n\rangle=\mathcal{H}|\psi_n\rangle.}

The eigenfunctions (now also referred to as eigenvectors) are replaced by eigenkets. Use of this notation makes solution of the Schrödinger equation much simpler for some problems, where the Hamiltonian can be re-written in the form of matrix operators having some algebra (defined set of operations on the basis vectors) over the Hilbert space of the eigenvectors of that Hamiltonian. (See the section on operators.)

We now ask how an arbitrary state Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle |\phi\rangle } evolves in time? The initial state Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle |\phi\rangle } can be expressed as the linear superposition of the energy eignstates:

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle | \phi \rangle=\sum_{n}c_n| \psi_n \rangle }

We can then solve the time-dependent Schrödinger equation, we obtain, for a time-independent Hamiltonian,

Failed to parse (SVG (MathML can be enabled via browser plugin): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle | \phi(t) \rangle=e^{-i\mathcal{H} t/\hbar}| \phi \rangle=e^{-i\mathcal{H} t/\hbar}\sum_{n}c_n| \psi_n \rangle=\sum_{n}c_ne^{-iE_n t/\hbar}|\psi_n\rangle.}