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The Kubo formula, named for Ryogo Kubo who first presented the formula in 1957, 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

Consider a quantum system described by the (time independent) Hamiltonian H_0. The expectation value of a physical quantity, described by the operator \hat, can be evaluated as: : \begin \left\langle\hat\right\rangle &= \operatorname\,\left hat\hat\right= \sum_n \left\langle n \left, \hat \ n \right\rangle e^ \\ \hat &= e^ = \sum_n , n \rangle\langle n , e^ \end where Z_0 = \operatorname\,\left hat\rho_0\right/math> is the partition function. Suppose now that just above some time t = t_0 an external perturbation is applied to the system. The perturbation is described by an additional time dependence in the Hamiltonian: \hat(t) = \hat_0 + \hat(t) \theta (t - t_0), where \theta (t) is the Heaviside function (1 for positive times, 0 otherwise) and \hat V(t) is hermitian and defined for all ''t'', so that \hat H(t) has for positive t - t_0 again a complete set of real eigenvalues E_n(t). But these eigenvalues may change with time. However, one can again find the time evolution of the
density matrix In quantum mechanics, a density matrix (or density operator) is a matrix that describes the quantum state of a physical system. It allows for the calculation of the probabilities of the outcomes of any measurement performed upon this system, usin ...
\hat(t) rsp. of the partition function Z(t) = \operatorname\, \left hat\rho (t)\right to evaluate the expectation value of \left\langle\hat A\right\rangle = \operatorname\,\left rho (t)\,\hat A\right\operatorname\,\left hat\rho (t)\right The time dependence of the states , n(t) \rangle is governed by the
Schrödinger equation The Schrödinger equation is a linear partial differential equation that governs the wave function of a quantum-mechanical system. It is a key result in quantum mechanics, and its discovery was a significant landmark in the development of th ...
i\partial_t , n(t) \rangle = \hat(t), n(t) \rangle , which thus determines everything, corresponding of course to the Schrödinger picture. But since \hat(t) is to be regarded as a small perturbation, it is convenient to now use instead the
interaction picture In quantum mechanics, the interaction picture (also known as the Dirac picture after Paul Dirac) is an intermediate representation between the Schrödinger picture and the Heisenberg picture. Whereas in the other two pictures either the state ...
representation, \left, \hat n(t) \right\rangle , in lowest nontrivial order. The time dependence in this representation is given by , n(t) \rangle = e^ \left, \hat(t) \right\rangle = e^\hat(t, t_0) \left, \hat(t_0) \right\rangle , where by definition for all t and t_0 it is: \left, \hat(t_0) \right\rangle = e^ , n(t_0) \rangle To linear order in \hat(t), we have \hat(t, t_0) = 1 - i\int_^t dt' \hat\mathord\left(t'\right). Thus one obtains the expectation value of \hat(t) up to linear order in the perturbation. ::\begin \left\langle\hat(t)\right\rangle &= \left\langle \hat \right\rangle_0 - i\int_^t dt' \sum_n e^ \left\langle n (t_0) \left, \hat(t) \hat\mathord\left(t'\right) - \hat\mathord\left(t'\right)\hat(t) \ n(t_0) \right\rangle \\ &= \left\langle \hat \right\rangle_0 - i\int_^t dt' \left\langle \left hat(t), \hat\mathord\left(t'\right)\rightright\rangle_0 \end The brackets \langle \rangle_0 mean an equilibrium average with respect to the Hamiltonian H_0 . 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 t > t_0. The above expression is true for any kind of operators. (see also
Second quantization Second quantization, also referred to as occupation number representation, is a formalism used to describe and analyze quantum many-body systems. In quantum field theory, it is known as canonical quantization, in which the fields (typically as ...
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See also

* Green–Kubo relations


References

{{Reflist, 2 Quantum mechanics