Jump to content

英文维基 | 中文维基 | 日文维基 | 草榴社区

Kubo formula

From Wikipedia, the free encyclopedia

The Kubo formula, named for Ryogo Kubo who first presented the formula in 1957,[1][2] is an equation which expresses the linear response of an observable quantity due to a time-dependent perturbation.

Among numerous applications of the Kubo formula, one can calculate the charge and spin susceptibilities of systems of electrons in response to applied electric and magnetic fields. Responses to external mechanical forces and vibrations can be calculated as well.

General Kubo formula

[edit]

Consider a quantum system described by the (time independent) Hamiltonian . The expectation value of a physical quantity at equilibrium temperature , described by the operator , can be evaluated as:

,

where is the thermodynamic beta, is density operator, given by

and is the partition function.

Suppose now that just after some time an external perturbation is applied to the system. The perturbation is described by an additional time dependence in the Hamiltonian:

where is the Heaviside function (1 for positive times, 0 otherwise) and is hermitian and defined for all t, so that has for positive again a complete set of real eigenvalues But these eigenvalues may change with time.

However, one can again find the time evolution of the density matrix rsp. of the partition function to evaluate the expectation value of

The time dependence of the states is governed by the Schrödinger equation

which thus determines everything, corresponding of course to the Schrödinger picture. But since is to be regarded as a small perturbation, it is convenient to now use instead the interaction picture representation, in lowest nontrivial order. The time dependence in this representation is given by where by definition for all t and it is:

To linear order in , we have

.

Thus one obtains the expectation value of up to linear order in the perturbation:

,

thus[3]

Kubo formula (general)


The brackets mean an equilibrium average with respect to the Hamiltonian Therefore, although the result is of first order in the perturbation, it involves only the zeroth-order eigenfunctions, which is usually the case in perturbation theory and moves away all complications which otherwise might arise for .

The above expression is true for any kind of operators. (see also Second quantization)[4]

See also

[edit]

References

[edit]
  1. ^ Kubo, Ryogo (1957). "Statistical-Mechanical Theory of Irreversible Processes. I. General Theory and Simple Applications to Magnetic and Conduction Problems". J. Phys. Soc. Jpn. 12 (6): 570–586. doi:10.1143/JPSJ.12.570.
  2. ^ Kubo, Ryogo; Yokota, Mario; Nakajima, Sadao (1957). "Statistical-Mechanical Theory of Irreversible Processes. II. Response to Thermal Disturbance". J. Phys. Soc. Jpn. 12 (11): 1203–1211. doi:10.1143/JPSJ.12.1203.
  3. ^ Bruus, Henrik; Flensberg, Karsten; Flensberg, ØRsted Laboratory Niels Bohr Institute Karsten (2004-09-02). Many-Body Quantum Theory in Condensed Matter Physics: An Introduction. OUP Oxford. ISBN 978-0-19-856633-5.
  4. ^ Mahan, GD (1981). Many-particle physics. New York: Springer. ISBN 0306463385.