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@ARTICLE{Nghiem:874513,
author = {Nghiem, H. T. M. and Dang, H. T. and Costi, T. A.},
title = {{T}ime-dependent spectral functions of the {A}nderson
impurity model in response to a quench with application to
time-resolved photoemission spectroscopy},
journal = {Physical review / B},
volume = {101},
number = {11},
issn = {2469-9950},
address = {Woodbury, NY},
publisher = {Inst.},
reportid = {FZJ-2020-01487},
pages = {115117},
year = {2020},
abstract = {We investigate several definitions of the time-dependent
spectral function A(ω,t) of the Anderson impurity model
following a quench and within the time-dependent numerical
renormalization group (TDNRG) method. In terms of the
single-particle two-time retarded Green function Gr(t1,t2),
the definitions we consider differ in the choice of the time
variable t with respect to t1 and/or t2 (which we refer to
as the time reference). In a previous study [H. T. M. Nghiem
et al., Phys. Rev. Lett. 119, 156601 (2017)], we
investigated the spectral function A(ω,t), obtained from
the Fourier transform of Im[Gr(t1,t2)] with respect to the
time difference t′=t1−t2, with time reference t=t2.
Here, we complement this work by deriving expressions for
the retarded Green function for the choices t=t1 and the
average, or Wigner, time t=(t1+t2)/2, within the TDNRG
approach. We compare and contrast the resulting A(ω,t) for
the different choices of time reference. While the choice
t=t1 results in a spectral function with no time dependence
before the quench (t<0) (being identical to the equilibrium
initial-state spectral function for t<0), the choices
t=(t1+t2)/2 and t=t2 exhibit nontrivial time evolution both
before and after the quench. Expressions for the lesser,
greater, and advanced Green functions are also derived
within TDNRG for all choices of time reference. The
average-time lesser Green function G<(ω,t) is particularly
interesting, as it determines the time-dependent occupied
density of states N(ω,t)=G<(ω,t)/(2πi), a quantity that
determines the photoemission current in the context of
time-resolved pump-probe photoemission spectroscopy. We
present calculations for N(ω,t) for the Anderson model
following a quench, and discuss the resulting time evolution
of the spectral features, such as the Kondo resonance and
high-energy satellite peaks. We also discuss the issue of
thermalization at long times for N(ω,t). Finally, we use
the results for N(ω,t) to calculate the time-resolved
photoemission current for the Anderson model following a
quench (acting as the pump) and study the different
behaviors that can be observed for different resolution
times of a Gaussian probe pulse.},
cin = {IAS-3},
ddc = {530},
cid = {I:(DE-Juel1)IAS-3-20090406},
pnm = {142 - Controlling Spin-Based Phenomena (POF3-142)},
pid = {G:(DE-HGF)POF3-142},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000518950200002},
doi = {10.1103/PhysRevB.101.115117},
url = {https://juser.fz-juelich.de/record/874513},
}