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NESSi
v1.0.2
The NonEquilibrium Systems Simulation Library
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| void cntr::dyson_start | ( | herm_matrix< T > & | G, |
| T | mu, | ||
| function< T > & | H, | ||
| herm_matrix< T > & | Sigma, | ||
| T | beta, | ||
| T | h, | ||
| const int | SolveOrder | ||
| ) |
Start-up procedure for solving the Dyson equation of the integral-differential form for a Green's function \(G\)
One solves the Dyson equation of the following form: \( [ id/dt + \mu - H(t) ] G(t,t^\prime) - [\Sigma*G](t,t^\prime) = \delta(t,t^\prime)\) for a hermitian matrix \(G(t, t^\prime)\) for the first k timesteps (given by the integrator class 'I'). One assumes that the Matsubara component of \(G\) and \(\Sigma(t,t^\prime)\) for \(t,t^\prime\)<=k are given.
| &G |
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| mu |
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| &H |
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| &Sigma |
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| beta |
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| h |
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| SolveOrder |
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Definition at line 1502 of file cntr_dyson_impl.hpp.
References cntr::herm_matrix< T >::nt(), cntr::herm_matrix< T >::ntau(), cntr::function< T >::ptr(), and cntr::herm_matrix< T >::size1().
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