Keldysh.jl provides a set of tools for working with non-equilibrium Keldysh Green's functions.
It contains types to represent contours, grids defined on these contours, and two-time Green's functions defined on these grids.
Additionally, it provides functions for generating Green's functions, performing integration on a contour and hdf5 serialization.
Credit to Andrey Antipov and Igor Krivenko for designing a first version of the abstractions implemented here.
The following code constructs a Green's function object from a spectral density and plots the Matsubara, retarded, and lesser Keldysh components.
using Keldysh, PyPlot
# first define a contour
tmax = 5.0
β = 10.0
c = FullContour(; tmax, β)
# now define a grid which represents a discretization of the contour
nt = 51
ntau = 101
grid = FullTimeGrid(c, nt, ntau)
# construct a spectral density
dos = flat_dos(; D=5.0, ν=10.0)
# construct a Green's function from a spectral density
G = FullTimeGF(dos, grid)
fig, axes = plt.subplots(nrows=2, ncols=2)
make_plot = (ax, xlabel, ylabel, t, f...) -> begin
map(fi -> ax.plot(t, fi), f)
ax.set_xlabel(xlabel); ax.set_ylabel(ylabel)
end
ω = range(-10.0, 10.0, length=1001)
t = realtimes(grid)
τ = imagtimes(grid)
make_plot(axes[1], L"ω", L"Γ(ω)/π", ω, dos.(ω))
make_plot(axes[2], L"τ", L"G^M(τ)", τ, G[:matsubara])
make_plot(axes[3], L"t", L"G^<(t, 0)", t, real(G[:lesser][:,1]), imag(G[:lesser][:,1]))
make_plot(axes[4], L"t", L"G^R(t, 0)", t, real(G[:retarded][:,1]), imag(G[:retarded][:,1]))
fig.tight_layout()
fig.savefig("keldysh_components.jpg", dpi=200)This produces the following output:
See also anderson_nca.jl which implements a NCA solver for the anderson impurity model using Keldysh.jl.
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