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The Kubo formula, named for
Ryogo Kubo was a Japanese mathematical physicist, best known for his works in statistical physics and non-equilibrium statistical mechanics. Work In the early 1950s, Kubo transformed research into the linear response properties of near-equilibrium conden ...
who first presented the formula in 1957, is an equation which expresses the
linear response A linear response function describes the input-output relationship of a signal transducer such as a radio turning electromagnetic waves into music or a neuron turning synaptic input into a response. Because of its many applications in information ...
of an observable quantity due to a time-dependent
perturbation Perturbation or perturb may refer to: * Perturbation theory, mathematical methods that give approximate solutions to problems that cannot be solved exactly * Perturbation (geology), changes in the nature of alluvial deposits over time * Perturbatio ...
. 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 The Heaviside step function, or the unit step function, usually denoted by or (but sometimes , or ), is a step function, named after Oliver Heaviside (1850–1925), the value of which is zero for negative arguments and one for positive argume ...
(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, using ...
\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 the ...
i\partial_t , n(t) \rangle = \hat(t), n(t) \rangle , which thus determines everything, corresponding of course to the
Schrödinger picture In physics, the Schrödinger picture is a formulation of quantum mechanics in which the state vectors evolve in time, but the operators (observables and others) are mostly constant with respect to time (an exception is the Hamiltonian which may ...
. But since \hat(t) is to be regarded as a small perturbation, it is convenient to now use instead the interaction picture 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 t ...
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See also

*
Green–Kubo relations The Green–Kubo relations ( Melville S. Green 1954, Ryogo Kubo 1957) give the exact mathematical expression for transport coefficients \gamma in terms of integrals of time correlation functions: :\gamma = \int_0^\infty \left\langle \dot(t) \dot( ...


References

{{Reflist, 2 Quantum mechanics