Interpreting pulse-shape effects in pump-probe spectroscopies
The effect of the pulse-shape on pump-probe spectroscopies is examined for the simplest model of noninteracting fermions on an infinite-dimensional hypercubic lattice. The probe-modified density of states follows the time evolution of the pump and displays narrowing and Floquet-like sidebands at th...
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irk-123456789-1574612019-06-21T01:28:21Z Interpreting pulse-shape effects in pump-probe spectroscopies Shvaika, A.M. Matveev, O.P. Devereaux, T.P. Freericks, J.K. The effect of the pulse-shape on pump-probe spectroscopies is examined for the simplest model of noninteracting fermions on an infinite-dimensional hypercubic lattice. The probe-modified density of states follows the time evolution of the pump and displays narrowing and Floquet-like sidebands at the pump maximum, whereas the photoelectron spectra are also strongly affected by the nonequilibrium occupation of the single-particle states due to the excitation from the pump. The nonequilibrium Raman cross section is derived, and the nonresonant one in both the A1g and B1g symmetries contains a number of peaks at the pump maximum, which can be attributed to an interference effect or Brillouin scattering off the time variations of the stress tensor. Both the “measured” occupation of single-particle states and the ratio of Stokes to anti-Stokes peaks are strongly modified by the probe-pulse width, which must be included in the interpretation of experimental results. Дослiджено вплив форми iмпульсу в експериментах з iмпульсами нагнiтання та вимiру для випадку найпростiшої моделi невзаємодiючих фермiонiв на безмежновимiрнiй гiперкубiчнiй ґратцi. Отримано, що модифiкована iмпульсом вимiру густина станiв слiдує часовiй еволюцiї iмпульсу нагнiтання. Коли iмпульс нагнiтання досягає максимуму, пiк на густинi станiв вужчає i з’являються додатковi Флоке-подiбнi боковi зони. Спектри фотоелектронної емiсiї також зазнають значних змiн внаслiдок нерiвноважного заповнення одночастинкових станiв пiд дiєю iмпульсу нагнiтання. Виведено формулу для розрахунку нерiвноважного перерiзу комбiнацiйного розсiяння свiтла та отримано, що нерiвноважна складова перерiзу розсiяння як для A1g, так i для B1g симетрiй має багатопiкову структуру, що може бути пояснено ефектами iнтерференцiї чи брiллюенового розсiяння на часових змiнах оператора тензора напружень. Отримано, що i “вимiряне” заповнення одночастинкових станiв, i вiдношення iнтенсивностi стоксових до антистоксових пiкiв сильно залежать вiд ширини пробного iмпульсу, що необхiдно враховувати при аналiзi результатiв експериментiв. 2018 Article Interpreting pulse-shape effects in pump-probe spectroscopies / A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks // Condensed Matter Physics. — 2018. — Т. 21, № 3. — С. 33707: 1–18. — Бібліогр.: 30 назв. — англ. 1607-324X PACS: 78.47.J-, 79.60.-i, 78.30.-j, 71.10.Fd DOI:10.5488/CMP.21.33707 arXiv:1808.04983 http://dspace.nbuv.gov.ua/handle/123456789/157461 en Condensed Matter Physics Інститут фізики конденсованих систем НАН України |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine |
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DSpace DC |
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English |
description |
The effect of the pulse-shape on pump-probe spectroscopies is examined for the simplest model of noninteracting fermions on an infinite-dimensional hypercubic lattice. The probe-modified density of states follows the time
evolution of the pump and displays narrowing and Floquet-like sidebands at the pump maximum, whereas the
photoelectron spectra are also strongly affected by the nonequilibrium occupation of the single-particle states
due to the excitation from the pump. The nonequilibrium Raman cross section is derived, and the nonresonant one in both the A1g and B1g symmetries contains a number of peaks at the pump maximum, which can
be attributed to an interference effect or Brillouin scattering off the time variations of the stress tensor. Both
the “measured” occupation of single-particle states and the ratio of Stokes to anti-Stokes peaks are strongly
modified by the probe-pulse width, which must be included in the interpretation of experimental results. |
format |
Article |
author |
Shvaika, A.M. Matveev, O.P. Devereaux, T.P. Freericks, J.K. |
spellingShingle |
Shvaika, A.M. Matveev, O.P. Devereaux, T.P. Freericks, J.K. Interpreting pulse-shape effects in pump-probe spectroscopies Condensed Matter Physics |
author_facet |
Shvaika, A.M. Matveev, O.P. Devereaux, T.P. Freericks, J.K. |
author_sort |
Shvaika, A.M. |
title |
Interpreting pulse-shape effects in pump-probe spectroscopies |
title_short |
Interpreting pulse-shape effects in pump-probe spectroscopies |
title_full |
Interpreting pulse-shape effects in pump-probe spectroscopies |
title_fullStr |
Interpreting pulse-shape effects in pump-probe spectroscopies |
title_full_unstemmed |
Interpreting pulse-shape effects in pump-probe spectroscopies |
title_sort |
interpreting pulse-shape effects in pump-probe spectroscopies |
publisher |
Інститут фізики конденсованих систем НАН України |
publishDate |
2018 |
url |
http://dspace.nbuv.gov.ua/handle/123456789/157461 |
citation_txt |
Interpreting pulse-shape effects in pump-probe spectroscopies / A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks // Condensed Matter Physics. — 2018. — Т. 21, № 3. — С. 33707: 1–18. — Бібліогр.: 30 назв. — англ. |
series |
Condensed Matter Physics |
work_keys_str_mv |
AT shvaikaam interpretingpulseshapeeffectsinpumpprobespectroscopies AT matveevop interpretingpulseshapeeffectsinpumpprobespectroscopies AT devereauxtp interpretingpulseshapeeffectsinpumpprobespectroscopies AT freericksjk interpretingpulseshapeeffectsinpumpprobespectroscopies |
first_indexed |
2025-07-14T09:53:19Z |
last_indexed |
2025-07-14T09:53:19Z |
_version_ |
1837615599311650816 |
fulltext |
Condensed Matter Physics, 2018, Vol. 21, No 3, 33707: 1–18
DOI: 10.5488/CMP.21.33707
http://www.icmp.lviv.ua/journal
Interpreting pulse-shape effects in pump-probe
spectroscopies
A.M. Shvaika1, O.P. Matveev1, T.P. Devereaux2,3, J.K. Freericks4
1 Institute for Condensed Matter Physics of the National Academy of Sciences of Ukraine,
1 Svientsitskii St., 79011 Lviv, Ukraine
2 Geballe Laboratory for Advanced Materials, Stanford University, Stanford, CA 94305, USA
3 Stanford Institute for Materials and Energy Sciences (SIMES), SLAC National Accelerator Laboratory,
Menlo Park, CA 94025, USA
4 Department of Physics, Georgetown University, 37th and O Streets, NW, Washington, DC 20057, USA
Received August 15, 2018
The effect of the pulse-shape on pump-probe spectroscopies is examined for the simplest model of noninteract-
ing fermions on an infinite-dimensional hypercubic lattice. The probe-modified density of states follows the time
evolution of the pump and displays narrowing and Floquet-like sidebands at the pump maximum, whereas the
photoelectron spectra are also strongly affected by the nonequilibrium occupation of the single-particle states
due to the excitation from the pump. The nonequilibrium Raman cross section is derived, and the nonreso-
nant one in both the A1g and B1g symmetries contains a number of peaks at the pump maximum, which canbe attributed to an interference effect or Brillouin scattering off the time variations of the stress tensor. Both
the “measured” occupation of single-particle states and the ratio of Stokes to anti-Stokes peaks are strongly
modified by the probe-pulse width, which must be included in the interpretation of experimental results.
Key words: pump-probe spectroscopy, photoelectron spectroscopy, electronic Raman scattering,
nonequilibrium Green’s function
PACS: 78.47.J-, 79.60.-i, 78.30.-j, 71.10.Fd
1. Introduction
Time-resolved spectroscopy is a powerful tool to investigate the dynamical properties of quantum
materials at their inherent time-scales [1–6]. In most cases, it is employed in a pump-probe setup— first a
pump excites the system into a nonequilibrium state and then the probe measures the property of interest.
Using pulsed lasers in different spectral regions for the pump, one can select particular excitation modes
to be resonantly driven by tuning the driving frequency to the excitation energy. There are many different
probes that can be employed depending onwhether one ismeasuring scattered electrons via photoemission
spectroscopy (PES) or angle-resolved photoemission spectroscopy (ARPES) or is measuring scattered
photons in infrared (IR) spectroscopy, or X-ray absorption spectroscopy (XAS), or many others. We want
to highlight one recent study on the time-resolved phononic Raman scattering [7], which was combined
with time-resolved ARPES to separately determine electronic and phononic temperatures in graphite.
This is an example, which is becoming increasingly common, of an experiment that combines multiple
probes on the same material in order to learn more about its nonequilibrium relaxation dynamics.
There is a fair amount of theoretical work on these problems — we have considered time-resolved
PES [8–10] and nonresonant electronic Raman scattering [11] for the Falicov-Kimball model [12], which
is the simplest strongly correlated electronic model that has an exact solution within dynamical mean-
field theory (DMFT) [13]. Obviously, whenever one performs a pump-probe experiment, there arises a
question: to what extent does the shape of the pump or probe pulse affect the results of the experiment,
This work is licensed under a Creative Commons Attribution 4.0 International License . Further distribution
of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.
33707-1
https://doi.org/10.5488/CMP.21.33707
http://www.icmp.lviv.ua/journal
http://creativecommons.org/licenses/by/4.0/
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
and how can we best compensate for these effects if we want to understand the behaviour of the system
unmodified by artifacts of the experimental measurement process? Themost obvious issue arises from the
width of the pulses, because frequency and time are related via a Fourier transformation and hence they
obey energy-time uncertainty relations [14]. However, there are also effects due to the pulse amplitude
(which can even create inverted populations [15]) and the shape of the envelope. A related question is:
how do the probes affect the ability to extract effective temperatures for the excited system? A number of
experiments have employed different methods to determine these effective temperatures [7, 16–18].
In order to determine the effect of the pulse shape on experimental results, we consider the case of
noninteracting fermions on a D-dimensional hypercubic lattice. We take the DMFT limit of D → ∞,
which, on the one hand, allows for a comparison with the previous DMFT results and, on the other hand,
makes it sometimes possible to obtain analytic results. The organization of the paper is as follows: In
section 2, we present our model. Section 3 considers the single-particle properties, i.e., the density of
states (DOS) and the time-resolved PES signal, while section 4 considers nonresonant electronic Raman
scattering, which measures two-particle (collective bosonic) excitations. We conclude in section 5.
2. Hamiltonian
We consider noninteracting spinless fermions on a D-dimensional hypercubic lattice. The interaction
with an electromagnetic field is included through the Peierls substitution [19–21]
H(t) = −
∑
i j
ti je
−i
∫Ri
R j
dr′ ·A(r′,t)
c†i cj . (2.1)
The hopping is between nearest neighbours only with a hopping integral given by t = t∗/2
√
D, and t∗ is
used as the energy unit. The pump is described by a homogeneous electric field directed along the unit
cell diagonal of a D-dimensional lattice E(t) = (E(t), E(t), E(t), . . .), where
E(t) = E0 cos (ωpt) e
− t2
σ2
p . (2.2)
Here, ωp is the pump pulse frequency and σp is the pump probe width; the pump is always centered at
t = 0. The total vector potential A(t) = (A(t), A(t), A(t), . . .) contains two contributions — one from the
pump pulse and the other one from the probe pulse,
A(t) = Apump(t) + Aprobe(t), Apump(t) = −
t∫
−∞
E(t ′)dt ′. (2.3)
We describe the probe pulse later; it is small, so it will be treated in perturbation theory via the Kubo
response methodology.
We can also write the Hamiltonian in momentum space via
H(t) =
∑
k
ε(k − A(t))c†kck , ck =
1
√
N
N∑
j=1
cj e
ik·R j , (2.4)
where ε(k − A(t)) = −
∑
j ti j exp{i[k − A(t)] · Ri j} is the band energy. The sum is over all neighbours j
of site i and Ri j = Ri −Rj . Note that this form of the Hamiltonian allows us to immediately see that the
Hamiltonian commutes with itself at different times [H(t),H(t ′)] = 0. This result makes determining
many time-dependent quantities much easier than for systems where the Hamiltonian does not commute
with itself at two different times.
3. DOS, PES, and occupation of the single-particle states
Now, we proceed to the calculations of the DOS and the time-resolved PESmeasured in a pump-probe
experiment. Such quantities are defined through the single-particle Green’s function and it is convenient
33707-2
Interpreting pulse-shape effects in pump-probe spectroscopies
to apply the Kadanoff-Baym-Keldysh formalism [22, 23] in this case. The single-particle Green’s function
on the Schwinger-Keldysh contour is defined by
Gc
k(t, t
′) = −i
〈
Tcck(t)c
†
k(t
′)
〉
(3.1)
and in the case of noninteracting electrons (2.4), it takes the form [21, 24]
Gc
k(t, t
′) = i [ f (ε(k) − µ) − Θc(t, t ′)] exp
−i
t∫
t′
dt̄ ε(k − A(t̄))
, (3.2)
where
f (ω − µ) =
1
e β(ω−µ) + 1
(3.3)
is the Fermi-Dirac distribution function, which arises from the initial equilibrium occupation of the
single-particle states before the pump, and Θc(t, t ′) is the Heaviside step function on the Schwinger-
Keldysh contour which equals 1 when t is ahead of t ′, 0 when t is behind of t ′, and 1/2 when t coincides
with t ′ on the contour.
For the D-dimensional hypercubic lattice with a nearest-neighbour hopping, we have
ε(k − A(t)) = lim
D→∞
{
−
t∗
√
D
D∑
α=1
cos[kα − A(t)]
}
= ε(k) cos A(t) + ε̄(k) sin A(t), (3.4)
where
ε(k) = lim
D→∞
(
−
t∗
√
D
D∑
α=1
cos kα
)
, ε̄(k) = lim
D→∞
(
−
t∗
√
D
D∑
α=1
sin kα
)
. (3.5)
Since the Green’s function depends on the momentum only through the band energy ε and the
projection of the electron velocity onto the electric field direction ε̄, we will replace a summation over
wavevector by an integration over a joint DOS
1
N
∑
k
−→
∫
dε
∫
dε̄ ρ(ε, ε̄). (3.6)
Furthermore, the momentum-dependent Green’s function can be written as
Gc
ε,ε̄(t, t
′) = i [ f (ε − µ) − Θc(t, t ′)] exp
−i
t∫
t′
dt̄ [ε cos A(t̄) + ε̄ sin A(t̄)]
. (3.7)
While the expressions in (3.2)–(3.5) are exact for any lattice with nearest-neighbour hopping, we consider
only the DMFT limit D→∞, with t∗ = 1. In this case, the joint DOS becomes Gaussian [21]
ρ(ε, ε̄) =
1
N
∑
k
δ(ε − ε(k)) δ(ε̄ − ε̄(k)) = e−ε2
√
π
e−ε̄2
√
π
, (3.8)
which simplifies calculations and allows us to obtain many analytic results.
Now, with all these preliminaries done, we are ready to consider the effect of the probe pulse width
on the single-particle quantities.
3.1. Equilibrium case
In equilibrium, with no pump pulse (Apump(t) = 0), the retarded Green’s function is given by
Gr
k(t − t ′) = −iΘ(t − t ′) exp [−iε(k)(t − t ′)] (3.9)
33707-3
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
and if we employ a monochromatic probe beam of infinite width, the Fourier transform of the Green’s
function is
Gr
k(ω) =
1
ω − ε(k) + i0+
. (3.10)
This yields the local DOS via
Ad(ω) =
1
N
∑
k
δ(ω − ε(k)) = e−ω2
√
π
. (3.11)
In the same situation, the lesser Green’s function is given by
G<
k (t − t ′) = i f (ε(k) − µ) exp [−iε(k)(t − t ′)] , (3.12)
which Fourier transforms to
P(ω) = f (ω − µ)Ad(ω). (3.13)
This result, which is the product of the distribution function times the local DOS, also yields the PES
signal (if we neglect matrix-element effects).
In a pump/probe experiment with probe pulses, we always have to make tradeoffs. The pulses should
be narrow enough to achieve good temporal selectivity but not too narrow, otherwise they lose all spectral
features in frequency space. This is called energy-time uncertainty [14]. We analyze this behaviour now.
If we express the probe-pulse vector potential as
A0eiωt s(t; t0) (3.14)
with A0 being the probe vector potential amplitude, and s(t; t0)—the probe envelope function; we assume
A0 is small, and it will not enter any of the perturbative results we calculate below. For Gaussian probe
pulses, with an envelope function centered at t0 and with width σb, we have
s(t; t0) =
1
σb
√
π
e
−
(t−t0)
2
σ2
b . (3.15)
The Fourier transformation from time to frequency is then modified by additional factors of s(t; t0) and
s(t ′; t0). For example, the DOS will be changed to a probe-modified DOS which equals
Ad(ω;σb) = Im
∫
dt
∫
dt ′ s(t; t0)s(t ′; t0)eiω(t−t′) 1
N
∑
k
Gr
k(t − t ′)
=
∫
dt
∫
dt ′ s(t; 0)s(t ′; 0)eiω(t−t′)
∫
dε
e−ε2
√
π
e−iε(t−t′)
=
1√
σ2
b
2 + 1
exp ©«− ω2
1 + 2
σ2
b
ª®¬ . (3.16)
Note that the final result is independent of t0. This is because the rest of the integrand is just a function of
t − t ′, so one can remove t0 by the following shifts in the integration variables: t → t + t0 and t ′→ t ′+ t0.
Due to the final width of the probe pulses, this probe-modified DOS is not normalized. One can see that
the initial Gaussian DOS (3.11) remains Gaussian, but with a wider bandwidth given by
√
1 + 2
σ2
b
instead
of 1. Note that this pulse-modified DOS is not easily measured, so we examine more experimentally
relevant quantities below.
Similarly, when we calculate the spectral density or probe-modified PES, we obtain [25]
P(ω;σb) =
∫
dt
∫
dt ′ s(t; t0)s(t ′; t0) eiω(t−t′) 1
N
∑
k
G<
k (t − t ′)
33707-4
Interpreting pulse-shape effects in pump-probe spectroscopies
=
∫
dε f (ε − µ)
e−ε2
√
π
e−σ
2
b (ω−ε)
2/2. (3.17)
For a monochromatic probe beam (σb →∞), the Gaussian factor that depends onω becomes a δ-function
and one recovers the result in equation (3.13). On the other hand, for narrow probe pulses σb → 0, the
spectral density or PES becomes its average value, averaged over all frequencies. Since the Fermi-Dirac
distribution function approaches a unit step function at zero temperature (β → ∞), the integral can be
evaluated and we find an expression similar to equation (3.13) for the pulse-modified PES
P(ω;σb) = f (ω, µ;σb)Ad(ω;σb), (3.18)
where Ad(ω;σb) is defined by (3.16) and instead of the step-like Fermi-Dirac distribution function, we
find a smoothed function given by
f (ω, µ;σb) =
1
2
+
1
2
erf
σ2
b√
4 + 2σ2
b
[(
1 +
2
σ2
b
)
µ − ω
] . (3.19)
At zero temperature, the probe-modified PES has a smoothed step-like feature that is located at a shifted
Fermi level! Such a smoothed function looks similar to the Fermi-Dirac distribution but at a higher
temperature. From the slope of f (ω, µ;σb) at the Fermi level (1 + 2/σ2
b )µ, we can estimate this effective
inverse temperature (introduced from the finite width of the probe pulse) via β = 4σ2
b /
(√
π
√
4 + 2σ2
b
)
.
This implies that the presence of a probe pulse mimics the behaviour of thermal excitations when we
examine a PES signal at T = 0.
We can also evaluate the probe-modified PES in the limit of infinite temperature (β → 0). Here,
the Fermi-Dirac distribution function is replaced by a constant equal to the filling, because every state is
occupied with the same probability. Then, the PES signal is simply equal to the filling multiplied by the
probe-modified DOS. In this case, while the probe affects the DOS, it has no effect on the distribution
function. From these results, we conjecture that the effect of the probe on the distribution function is the
greatest at low temperatures and disappears as we go to higher temperatures.
Surely these behaviours will play a role when we try to extract effective temperatures for nonequilib-
rium cases too. We examine this point next.
3.2. Nonequilibrium case
In the nonequilibrium case, the Peierls’ substitution shifts themomentum label of the different energies
in the bandstructure as a function of time. Note that the complete set of energy eigenvalues is unchanged,
meaning if we diagonalized the instantaneous Hamiltonian at any given moment, the set of eigenvalues
would not change. But the labels do. Since the degeneracy structure of the bands in momentum space
influences the DOS, we expect the DOS to change as a function of time due to this relabelling. However,
since the DOS is defined via the Green’s function, the DOS is also affected by the time dependence of
the wavefunctions, which enter the equation of motion for the Green’s functions. This means that we
should not interpret the transient nonequilibrium DOS as simply being the DOS of the instantaneous
Hamiltonian. It is a more complex object. In addition, the driving fields can change the distribution of
electrons amongst these states. Fortunately, all of these effects can be treated exactly in a noninteracting
system.
In the presence of a pump, the time-dependent DOS is normally defined through the retarded Green’s
function. When we make a Fourier transform to express it as a function of frequency and some time (due
to the fact that it changes with time), we have a number of different choices we can make. One of the
most common choices is to perform a Wigner transformation to average and relative times and perform
the Fourier transform with respect to relative time. This has the advantage of a clearly defined “time” at
which we have constructed the DOS, but the noncausal nature of this time can make the interpretation of
this DOS confusing. For example, even for an average time before the pump, we will have some relative
times where one of the original times t or t ′ will be after the pump. If these times contribute significantly
33707-5
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
to the Fourier transform, one will see an effect of the pump on the DOS at an average time before the
pump is applied. In addition, there is no guarantee that the DOS defined in this fashion is nonnegative.
There are alternatives one can make as well. One can instead fix t ′ and set t = t ′ + ∆t and perform the
Fourier transform with respect to ∆t. This produces a causal structure to the system, since only times
after t ′ are involved in the result. However, this DOS is not guaranteed to be nonnegative either. It is also
unclear what time we should associate with this DOS. Here, we instead define a probe-modified DOS in
analogy to the probe-modified DOS and PES we worked with above. It is
Ad(ω; t0) =
∫
dt
∫
dt ′ s(t; t0)s(t ′; t0) eiω(t−t′)e−
1
4φ
2(t,t′)e−
1
4ψ
2(t,t′), (3.20)
where the pump field enters through the quantities
φ(t, t ′) =
t∫
t′
dt̄ cos A(t̄) and ψ(t, t ′) =
t∫
t′
dt̄ sin A(t̄). (3.21)
One can see that the probe-modified DOS does not depend on temperature (as is expected for non-
interacting fermions). More importantly, one can immediately verify that the probe-modified DOS is
nonnegative. It is also clearly associated with the time t0, although this is still a bit fuzzy due to the finite
probe widths and the energy-time uncertainty relations. Similarly, the spectral density or PES signal is
equal to [25]
P(ω; t0) =
∫
dt
∫
dt ′ s(t; t0)s(t ′; t0) eiω(t−t′)
∫
dε
∫
dε̄ ρ(ε, ε̄) G<
ε,ε̄(t, t
′)
=
∫
dt
∫
dt ′ s(t; t0)s(t ′; t0) eiω(t−t′)e−
1
4ψ
2(t,t′)
∫
dε
e−ε2
√
π
f (ε − µ)e−iεφ(t,t′), (3.22)
which is also manifestly nonnegative. The time delay between the pump and probe pulses is set by t0,
since the pump is centered at the origin in time.
In equilibrium, we employed the ratio of the PES to the DOS to determine the distribution function
in equation (3.13). We generalized this result to take into account the probe in equation (3.18). Motivated
by these results, we define the probe-modified nonequilibrium occupation of single-particle states to be
the ratio of the probe-modified nonequilibrium PES to the probe-modified nonequilibrium DOS [16, 17]
nd(ω; t0) =
P(ω; t0)
Ad(ω; t0)
. (3.23)
One can estimate an effective temperature at t0 either from the slope of nd(ω, t0) at the chemical potential
or from a least squares (LSQ) interpolation of nd(ω; t0) with the Fermi-Dirac distribution function (there
are other definitions one could use for the effective temperature, but these two are the simplest ones to
use, and we examine them thoroughly in this paper).
In figures 1 and 2, we plot results for the DOS, PES, and occupation of the single-particle states
nd(ω; t0) for different pump amplitudes and widths. For the large pump amplitude E0 = 30 (figure 1), the
DOS, which does not depend on temperature, has the same Gaussian profile far before and far after the
pump, but becomes narrowed and sharper near the pump maximum. It also has some small Floquet-like
peaks caused by both the pump driving frequency and by the Bloch oscillations of the band energy
ε(k − A(t)).
The behaviour for the PES is different. The PES first displays an equilibrium profile at t0 = −30. As
we approach the pumpmaximum at t0 = 0, the peak becomes narrow and shifts toward zero frequency. At
large times, the peak spreads again, but remains in the vicinity ofω = 0. The difference in the PES spectra
before and after the pump is determined by the change in the occupation of the single-particle states. The
initial occupation follows the probe-modified Fermi-Dirac distribution. As the pump amplitude increases,
the distribution function becomes more flat and exhibits oscillations. After the pump, a step-like shape of
the Fermi-Dirac distribution function is almost restored. For frequencies in the vicinity of the chemical
33707-6
Interpreting pulse-shape effects in pump-probe spectroscopies
D
O
S
0
0.2
0.4
0.6
0.8
1
1.2
frequency
−4 −2 0 2 4
D
O
S
0
0.2
0.4
0.6
0.8
1
frequency
−4 −2 0 2 4
P
E
S
0
0.2
0.4
0.6
frequency
−4 −2 0 2 4
P
E
S
0
0.1
0.2
0.3
0.4
0.5
frequency
−4 −2 0 2 4
Figure 1. (Colour online) Waterfall images of the time-resolved DOS and PES data, plotted for different
delay times t0 ∈ [−30, 30] and offset for clarity, and occupation of single-particle states nd(ω; t0) for
E0 = 30 and σb = 7 (left) and σb = 12 (right).
potential, one can estimate an effective temperature from the slope of the measured distribution function
at ω = 0 or by using LSQ interpolation (see figure 3). The initial fitted temperature is close to the actual
33707-7
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
D
O
S
0
0.2
0.4
0.6
0.8
1
frequency
−4 −2 0 2 4
D
O
S
0
0.2
0.4
0.6
0.8
1
frequency
−4 −2 0 2 4
P
E
S
0
0.1
0.2
0.3
0.4
0.5
frequency
−4 −2 0 2 4
P
E
S
0
0.1
0.2
0.3
0.4
0.5
frequency
−4 −2 0 2 4
Figure 2. (Colour online) Waterfall images of the time-resolved DOS and PES data, plotted for different
delay times t0 ∈ [−30, 30] and offset for clarity, and occupation of single-particle states nd(ω; t0) for
E0 = 1 and σb = 7 (left) and σb = 12 (right).
initial temperature β = 10 (T = 0.1); the differences arise from our use of a Fermi-Dirac distribution
function instead of a probe-modified distribution function for the fits. During and after the pump, the
effective temperature increases and its “measured” value is sensitive to the probe-function width σb.
33707-8
Interpreting pulse-shape effects in pump-probe spectroscopies
be
ta
0
2
4
6
8
10
12
time
−30 −20 −10 0 10 20 30
σb = 7
σb = 7 (LSQ)
σb = 12
σb = 12 (LSQ)
be
ta
0
5
10
time
−30 −20 −10 0 10 20 30
σb = 7
σb = 7 (LSQ)
σb = 12
σb = 12 (LSQ)
Figure 3. (Colour online) Effective inverse temperatures β = 1/T determined from the slope of the probe-
modified nonequilibrium distribution function at the Fermi level (dashed lines) and by LSQ interpolation
(solid lines) for E0 = 30 (left) and E0 = 1 (right).
For small amplitudes of the pump, such as E0 = 1 (see figure 2), the DOS is weakly modified
by the pump while the PES shows a much faster evolution during the pump than it occurs for larger
pump amplitudes. Even more strange is the occupation of single-particle states which eventually display
population inversion resulting in a negative effective temperature, as seen in figure 3. This population
inversion remains after the pump because there are no interactions or other mechanisms for relaxation
and thermalization.
We explain this odd behaviour for small field amplitudes in the following way: The PES is sensitive
to the final value of the vector potential because a nonzero value means that the system will remain in
a current carrying state (recall that noninteracting metals are perfect conductors). The final value of the
pump vector potential is equal to
A(+∞) = −
√
πE0σp exp
(
−
ω2
pσ
2
p
4
)
. (3.24)
The induced electric current as a function of the pump vector potential is
j(t) = −i
∫
dε
∫
dε̄ρ(ε, ε̄)
[
−ε sin Apump(t) + ε̄ cos Apump(t)
]
G<
ε,ε̄(t, t) = j0 sin Apump(t) (3.25)
with
j0 = −
∫
dε
e−ε2
√
π
f (ε − µ)ε =
1
2
∫
dε
e−ε2
√
π
[
−
d f (ε − µ)
dε
]
. (3.26)
In figure 4, we present the results for three different pump-field amplitudes which give final vector
potential values equal to A(+∞) = −2π, −3π/2, and −π, respectively. For A(+∞) = 2nπ, which does not
change the final band energy ε(k − A(+∞)) = ε(k), there is no net current j(+∞) = 0 and the final PES
(as well as the final occupation of the single-particle states) after the pump is the same as the initial one.
Whereas, for A(+∞) = (2n+1)π, which changes the sign of the final band energy ε(k−A(+∞)) = −ε(k)
(band flip), we find that the final PES and final occupation of the single-particle states are both inverted
even though the net current is still zero j(+∞) = 0. The case of A(+∞) = π2 + nπ makes the band energy
antisymmetric (cosine is replaced by sine) so that the net current reaches its maximum allowed value
j(+∞) = ± j0 and the final PES is half of the DOS with an uniform occupation of the single-particle states
nd(ω) = 1
2 . This appears odd because the PES looks like an infinite-temperature result, while the current
is nonzero. But what is happening is we are fully occupying the electrons that move in the direction of
the field with no electrons moving opposite. This then saturates the current at its maximum value while
making the PES appear to be an infinite-temperature PES because the band degeneracy says for every
state moving in the direction of the field that there is a degenerate state moving opposite to the field. The
corresponding changes of the effective inverse temperatures are shown in figure 5. The cases shown in
figure 3 correspond to both large E0 = 30 and small E0 = 1 field amplitudes, with final vector potential
values given by A(+∞) = −17.74π and A(+∞) = −0.59π, respectively. The DOS displays a simple
behaviour. It has a monotonous change with increasing pump amplitude E0. It has the same equilibrium
profiles at long times while it becomes enhanced and narrowed near the pump maximum.
33707-9
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
D
O
S
0
0.2
0.4
0.6
0.8
1
frequency
−4 −2 0 2 4
D
O
S
0
0.2
0.4
0.6
0.8
1
frequency
−4 −2 0 2 4
D
O
S
0
0.2
0.4
0.6
0.8
1
frequency
−4 −2 0 2 4
P
E
S
0
0.1
0.2
0.3
0.4
0.5
0.6
frequency
−4 −2 0 2 4
P
E
S
0
0.1
0.2
0.3
0.4
0.5
frequency
−4 −2 0 2 4
P
E
S
0
0.1
0.2
0.3
0.4
0.5
0.6
frequency
−4 −2 0 2 4
Figure 4. (Colour online) Waterfall images of the time-resolved DOS and PES data, plotted for different
delay times t0 ∈ [−30, 30] and offset for clarity, and occupation of the single particle states nd(ω) for
A(+∞) = −2π (left), −3π/2 (center) and −π (E0 = 1.69118088, right) for σp = 5 and ωp = 0.5.
be
ta
−10
−5
0
5
10
time
−30 −20 −10 0 10 20 30
2π
2π (LSQ)
3π/2
3π/2 (LSQ)
π
π (LSQ)
Figure 5. (Color online) Effective inverse temperatures β = 1/T for A(+∞) = −2π, −3π/2, and −π.
33707-10
Interpreting pulse-shape effects in pump-probe spectroscopies
4. Nonresonant Raman scattering
Now, we proceed to examine electronic inelastic light (Raman) scattering, which measures the two-
particle excitations. Since a time-varying Hamiltonian does not have well-defined energy eigenstates, we
cannot directly apply the Kramers-Heisenberg formula as is often done in the linear-response regime.
Instead, we have to derive the scattering cross-section from scratch using the Nozières and Abrahams
approach [26] for inelastic light scattering.
We start by analyzing the evolution of the initial electronic state plus one initial probe photon that
has momentum ki, polarization ei, and frequency ωi = c |ki |. Expanding the full evolution operator to
include up to the second-order terms in the probe field, we find
|ψ(t)〉 = U(t,−∞)|n〉 ⊗ a†ki,ei |0〉 = Tt exp
[
−i
t∫
−∞
dt̃ H(t̃)
]
|n〉 ⊗ a†ki,ei |0〉
≈
1
2
t∫
−∞
dt̃ U0(+∞, t̃)Aαprobe(t̃)γαβ(t̃)A
β
probe(t̃)U0(t̃,−∞) |n〉 ⊗ a†ki,ei |0〉
+
t∫
−∞
dt̃
t̃∫
−∞
dt̃ ′ U0(+∞, t̃) jα(t̃)Aαprobe(t̃)U0(t̃, t̃ ′) jβ(t̃ ′)A
β
probe(t̃
′)U0(t̃,−∞) |n〉 ⊗ a†ki,ei |0〉, (4.1)
where
γαβ(t) =
∑
k
∂2ε(k − Apump(t))
∂kα∂kβ
c†kck (4.2)
is the nonequilibrium generalization of the stress tensor and
jα(t) =
∑
k
∂ε(k − Apump(t))
∂kα
c†kck (4.3)
is the nonequilibrium generalization of the current operator. Note that the time-evolution operator acts
on both terms in the tensor product depending on whether it is an electron or photon operator and the
operators are in the interaction representation with respect to the photon operator, because the evolution
with respect to the electronic and electron-photon coupling terms is included explicitly via the U0 factors
(which only include the pump vector potential). In equation (4.1), the first term describes nonresonant
scattering and the second term describes resonant scattering of the probe photons (within a time envelope)
Aαprobe(t) = s(t; t0)
∑
k,e
(
2π
ωk
)1/2
eα
(
eiωkta†k,e + e−iωktak,e
)
. (4.4)
The scattering cross-section is defined by the probability to find a scattered probe photon with momen-
tum kf, polarization ef, and frequency ωf = c |kf | in the final state. It becomes
R =
∑
ψ
e−βEψ
Z
〈ψ(t → +∞)|a†kf,efakf,ef |ψ(t → +∞)〉,
whereH(t → −∞)|ψ(t → −∞)〉 = Eψ |ψ(t → −∞)〉.
After tracing over the photon operators, we find that the nonresonant contribution to the electronic
Raman scattering (with frequency loss Ω = ωi − ωf) becomes
RN (Ω; t0) = i
∫
dt
∫
dt ′ s2(t; t0)s2(t ′; t0)eiΩ(t−t′)RN (t, t ′). (4.5)
This result arises from the greater Green’s function
RN (t, t ′) = R>(t, t ′) = R−+(t, t ′) = −i 〈γ̃(t)γ̃(t ′)〉 , (4.6)
33707-11
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
where (+,−) denote the upper and lower branches of the Keldysh contour and
γ̃(t) = eiαγαβ(t)efβ (4.7)
is the contraction of the stress tensor with the polarization vectors of the initial (i) and scattered (f)
photons.
4.1. Ratio of Stokes and anti-Stokes peaks and the probe pulse shape
Let us first consider the influence of the probe pulse shape on the ratio of the Stokes and anti-Stokes
peaks [27] for the “equilibrium” linear-response case. This ratio is often used for the estimation of
local temperatures [28] and can be applied in the pump-probe experiments too [7], but the conventional
derivation holds only for the equilibrium case with continuous probes. In equilibrium, the greater Green’s
function depends only on the time difference of its arguments
R>(t, t ′) = R>eq(t − t ′), (4.8)
hence, the Fourier transform becomes
Req
N (Ω) = i
+∞∫
−∞
d(t − t ′) eiΩ(t−t′)R>eq(t − t ′). (4.9)
From the spectral properties of the greater Green’s function it follows that the ratio of amplitudes of the
Stokes and anti-Stokes lines for the nonresonant Raman scattering of a monochromatic beam is equal to
Req
N (Ω)
Req
N (−Ω)
= exp(βΩ). (4.10)
Now, let us check how this ratio is distorted by finite-width probe pulse envelope functions. From
equation (4.5), we obtain (after introducing the inverse Fourier transform for RN )
RN (Ω) =
+∞∫
−∞
dt
+∞∫
−∞
dt ′R>eq(t − t ′)s2(t; t0)s2(t ′; t0)eiΩ(t−t′)
=
1
2π
+∞∫
−∞
dΩ′Req
N (Ω
′)
+∞∫
−∞
dt
+∞∫
−∞
dt ′s2(t)s2(t ′)ei(Ω−Ω′)(t−t′), (4.11)
where the dependence on the probe pulse time t0 vanishes just like it did for PES because the remainder of
the integrand is just a function of relative time. After substituting in the Gaussian form for the probe-pulse
envelope function, we find
RN (Ω) =
1
2π
+∞∫
−∞
dΩ′Req
N (Ω
′)
1
σ4
bπ
2
+∞∫
−∞
dte−2t2/σ2
b+i(Ω−Ω′)t
+∞∫
−∞
dt ′e−2t′2/σ2
b−i(Ω−Ω′)t′
=
1
2π
+∞∫
−∞
dΩ′Req
N (Ω
′)e−σ
2
b (Ω−Ω
′)2/4 1
2πσ2
b
. (4.12)
Evaluating equation (4.12) for negative frequencies gives
RN (−Ω) =
1
4π2σ2
b
+∞∫
−∞
dΩ′Req
N (−Ω
′)e−σ
2
b (Ω−Ω
′)2/4 =
1
4π2σ2
b
+∞∫
−∞
dΩ′Req
N (Ω
′)e−βΩ
′
e−σ
2
b (Ω−Ω
′)2/4
33707-12
Interpreting pulse-shape effects in pump-probe spectroscopies
=
1
4π2σ2
b
e−βΩ+β
2/σ2
b
+∞∫
−∞
dΩ′Req
N (Ω
′)e−σ
2
b (Ω−Ω
′−2β/σ2
b )
2/4
= e
−β
(
Ω−
β
σ2
b
)
RN
(
Ω −
2β
σ2
b
)
, (4.13)
after using the equilibrium relation for the ratio inside the integrand. We now introduce the shifted
frequency Ω̃ = Ω − β
σ2
b
and finally conclude that the Stokes-anti-Stokes ratio changes to
RN
(
Ω̃ −
β
σ2
b
)
RN
(
−Ω̃ −
β
σ2
b
) = exp(βΩ̃), (4.14)
when the probe-pulse has a finite width. Note that this shift vanishes at high temperatures, but can be
significant at a low temperature.
4.2. Nonresonant Raman scattering off noninteracting electrons
We now examine the nonequilibrium case for nonresonant electronic Raman scattering. For nonin-
teracting fermions, we have only the bare bubble contribution in equation (4.6), which becomes
R>(t, t ′) =
i
N
∑
k
γ(k − Apump(t))γ(k − Apump(t ′))G>
k (t, t
′)G<
k (t
′, t)
=
i
N
∑
k
γ(k − Apump(t))γ(k − Apump(t ′))G−+k (t, t
′)G+−k (t
′, t), (4.15)
where
γ(k − Apump(t)) =
∑
α,β
eiα
∂2ε(k − Apump(t))
∂kα∂kβ
efβ (4.16)
is the contraction of the stress tensor amplitude with the polarization vector components of the incident
(scattered) photons.
For an A1g symmetry, with ei = ef = (1, 1, 1, . . .), we have γ(k−Apump(t)) = −ε(k−Apump(t)), which
gives
R>A1g
(t, t ′) = i
∫
dε
∫
dε̄ ρ(ε, ε̄)
[
ε cos Apump(t) + ε̄ sin Apump(t)
] [
ε cos Apump(t ′) + ε̄ sin Apump(t ′)
]
× G−+ε,ε̄(t, t
′)G+−ε,ε̄(t
′, t). (4.17)
For a B1g symmetry,with ei = (1, 1, 1, 1, . . .) and ef = (1,−1, 1,−1, . . .) (and for nearest-neighbour hopping
only), we have γ(k − Apump(t)) = − t∗√
D
∑D
α=1(−1)α cos[kα − Apump(t)] and the nonzero contributions in
the D→∞ limit become
γ(k − Apump(t))γ(k − Apump(t ′)) →
t∗2
D
D∑
α=1
cos[kα − Apump(t)] cos[kα − Apump(t ′)]
=
t∗2
2
{
cos[Apump(t) − Apump(t ′)] +
1
D
D∑
α=1
cos[2kα − Apump(t) − Apump(t ′)]
}
→
t∗2
2
cos[Apump(t) − Apump(t ′)], (4.18)
33707-13
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
which we can use to rewrite (4.15) as
R>B1g
(t, t ′) = i
t∗2
2
cos[Apump(t) − Apump(t ′)]
∫
dε
∫
dε̄ ρ(ε, ε̄)G−+ε,ε̄(t, t
′)G+−ε,ε̄(t
′, t). (4.19)
Remarkably, for noninteracting electrons, the product of the lesser and greater Green’s functions (3.7)
is equal to just the products of Fermi factors
G−+ε,ε̄(t, t
′)G+−ε,ε̄(t
′, t) = f (ε − µ)[1 − f (ε − µ)] (4.20)
and does not depend on the time variables. As a result, an equilibriumRaman cross-section (Apump(t) = 0)
for a monochromatic beam is proportional to a δ-function, RN (Ω) ∼ δ(Ω) (no inelastic light scattering),
whereas in a pump/probe experiment, we find
RN
A1g
(Ω) =
∫
dε
∫
dε̄ ρ(ε, ε̄) f (ε − µ)[1 − f (ε − µ)]
∫
dt
∫
dt ′ s2(t)s2(t ′)eiΩ(t−t′)
×
[
ε cos Apump(t) + ε̄ sin Apump(t)
] [
ε cos Apump(t ′) + ε̄ sin Apump(t ′)
]
=
∫
dε
e−ε2
√
π
f (ε − µ)[1 − f (ε − µ)]ε2
����∫ dt s2(t)eiΩt cos Apump(t)
����2
+
1
2
T N(µ)
����∫ dt s2(t)eiΩt sin Apump(t)
����2 (4.21)
and
RN
B1g
(Ω) = T N(µ) ·
t∗2
2
∫
dt
∫
dt ′ s2(t)s2(t ′)eiΩ(t−t′) cos
[
Apump(t) − Apump(t ′)
]
= T N(µ) ·
t∗2
2
[����∫ dt s2(t)eiΩt cos Apump(t)
����2 + ����∫ dt s2(t)eiΩt sin Apump(t)
����2] . (4.22)
Here, the prefactor N(µ) does not depend on the pump and only gives the occupation of the Fermi level
at T = 0
N(µ) = β
∫
dε
e−ε2
√
π
f (ε − µ) [1 − f (ε − µ)] =
∫
dε
e−ε2
√
π
[
−
d f (ε − µ)
dε
]
= 2 j0. (4.23)
In equilibrium, as well as far before or far after a pump (where Apump(t) = Aeq), we obtain Gaussian
profiles for both symmetry channels:
RN
A1g
(Ω) =
{∫
dε
e−ε2
√
π
f (ε − µ)[1 − f (ε − µ)]ε2 cos2 Aeq +
1
2
T N(µ) sin2 Aeq
}
2
σ2
bπ
e−σ
2
bΩ
2/4
≈
1
2
T N(µ)
2
σ2
bπ
e−σ
2
bΩ
2/4 sin2 Aeq for T → 0 (4.24)
and
RN
B1g
(Ω) = T N(µ) ·
t∗2
2
2
σ2
bπ
e−σ
2
bΩ
2/4. (4.25)
This corresponds to the spreading of the δ-peaks by the finite-width probe pulses. One can see that
the final A1g scattering amplitude does depend on the final value of the vector potential, while the B1g
scattering is independent of the final vector potential value.
If we instead examine the Raman response function
χN (Ω) = RN (Ω)
(
e βΩ − 1
)
(4.26)
33707-14
Interpreting pulse-shape effects in pump-probe spectroscopies
Figure 6. (Colour online) A1g and B1g Raman cross sections for E0 = 1 and σb = 7 (left) and σb = 12
(right).
defined by the retarded Green’s function
Rr(t, t ′) = −iΘ(t − t ′) 〈[γ̃(t), γ̃(t ′)]〉 , (4.27)
we find it is exactly zero
χN (Ω) ≡ 0. (4.28)
This is obviously true for monochromatic beams, where it follows from the identity δ(Ω)(e βΩ − 1) = 0,
whereas for the finite-width probe pulses, “the Raman response” defined by (4.26) is only nonzero due
to the spreading of the δ-peak.
In equilibrium, the Raman cross-section is the product of some prefactor and δ(Ω). In figures 6 and
7, we observe a spreading of the δ-function due to both the finite width of the probe envelope functions
and due to the cosine factor (which originated from the stress tensor as modified by pump), which
describes the inelastic scattering of light by the temporal variations of the driven stress tensor, due to
Bloch oscillations.
Since the Raman response is equal to zero and all of the temperature dependence, as well as the band
contributions of the Raman cross-section reside in the factors like T N(µ), there can be no separation
Figure 7. (Colour online) A1g and B1g Raman cross sections for E0 = 30 and σb = 7 (left) and σb = 12
(right).
33707-15
A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
of Stokes and anti-Stokes lines, and the profiles are symmetric. One can see the suppression of the
scattering amplitude as well as the appearance of additional sideband oscillations when we are at the
pump maximum. These are more prominent for large pump field amplitudes, but the oscillations are
more likely an interference effect or Brillouin scattering off the time variations of the stress tensor than
Floquet sidebands. It is the oscillations observed in the single-particle DOS and the “occupations” at the
pump maximum that can be primarily attributed to the Floquet bands [29].
5. Conclusions
In this article, we have investigated the effect of pulse shapes on pump-probe spectroscopies, on the
probe modified nonequilibrium DOS, and PES as well as on electronic Raman scattering. We considered
noninteracting fermions on a D = ∞ hypercubic lattice with a Gaussian unperturbed DOS, which allows
one to obtain some analytic results.
The nonequilibrium DOS Ad(ω; t0) immediately follows the pump pulse. It is completely restored
after the pump (to its equilibrium result) and displays both a band narrowing and side-band peaks of
Floquet-like sidebands near the pumpmaximum. For wider probe pulses, more details of the fine structure
of the DOS are observed, whereas for narrow probes, the DOS is more smooth; nevertheless, the main
peaks are all still visible.
The time evolution of the nonequilibrium PES P(ω; t0) is different. After the pump, the PES strongly
deviates from the initial one and such a behaviour can be attributed to the nonequilibrium redistribution
of the occupations of the single-particle states
nd(ω; t0) =
P(ω; t0)
Ad(ω; t0)
. (5.1)
From the slope of the occupation of single-particle states nd(ω; t0), one can estimate an effective temper-
ature of the single-particle excitations, which is increasing with the pump, and its value depends on the
probe width, which modifies the Fermi-Dirac distribution function. For some pump profiles, an inverse
occupation of the single-particle states is observed leading to negative effective temperatures.
We have also developed the general approach for obtaining the nonequilibrium Raman cross section
and derived an expression for the nonresonant case. We find that even in equilibrium, without a pump,
the ratio of Stokes to anti-Stokes peaks is strongly modified by the probe pulse width, and the deviation
becomes large at low temperatures and for narrow probe pulses. The Raman response is zero for non-
interacting fermions; nevertheless, the Raman cross section is nonzero and displays an interesting time
evolution. For the early and late time values, before and after the pump, the Gaussian central peak, more
prominent for the B1g symmetry, is observed at zero frequency, which is a probe-modified δ-function.
With an increasing pump, the central peak is suppressed and splits into a series of peaks whose frequency
distribution depends on the pump parameters, the field amplitude E0 and the driving frequency ωp.
We suppose that these peaks are more likely an interference effect or Brillouin scattering off the time
variations of the stress tensor due to Bloch oscillations.
Acknowledgements
It is our pleasure to dedicate this paper to the 80th birthday of Professor I.V. Stasyuk, a prominent
scientist and lecturer, who has made valuable contributions in many fields of quantum statistical physics
and solid state theory and taught one of us (A.M.S.) the enjoyment of the Green’s functions [30].
This work was supported by the Department of Energy, Office of Basic Energy Sciences, Division of
Materials Sciences and Engineering under Contract Nos. DE-AC02-76SF00515 (Stanford/SIMES) and
DE-FG02-08ER46542 (Georgetown). J.K.F. was also supported by the McDevitt bequest at Georgetown.
33707-16
Interpreting pulse-shape effects in pump-probe spectroscopies
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https://doi.org/10.1103/PhysRevB.93.245403
http://arxiv.org/abs/1804.01403
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A.M. Shvaika, O.P. Matveev, T.P. Devereaux, J.K. Freericks
Iнтерпретацiя впливу форми iмпульсiв у спектроскопiї
нагнiтання-вимiр
А.М.Швайка1, О.П.Матвєєв1, Т.П. Деверо2,3, Дж.К. Фрiрiкс4
1 Iнститут фiзики конденсованих систем НАН України, вул. I. Свєнцiцького, 1, 79011 Львiв, Україна
2 Ґебаллiвська лабораторiя передових матерiалiв, Стенфордський унiверситет,
Стенфорд, Калiфорнiя 94305, США
3 Стенфордський iнститут матерiалiв та наук про енергетику (SIMES), Нацiональна прискорювальна
лабораторiя SLAC,Мелно Парк, Калiфорнiя 94025, США
4 Фiзичний факультет, Джорджтаунський унiверситет,
вул. 37 & О NW, Вашинґтон, округ Колумбiя 20057, США
Дослiджено вплив форми iмпульсу в експериментах з iмпульсами нагнiтання та вимiру для випадку най-
простiшої моделi невзаємодiючих фермiонiв на безмежновимiрнiй гiперкубiчнiй ґратцi. Отримано, що
модифiкована iмпульсом вимiру густина станiв слiдує часовiй еволюцiї iмпульсу нагнiтання. Коли iмпульс
нагнiтання досягає максимуму, пiк на густинi станiв вужчає i з’являються додатковi Флоке-подiбнi боковi
зони. Спектри фотоелектронної емiсiї також зазнають значних змiн внаслiдок нерiвноважного заповне-
ння одночастинкових станiв пiд дiєю iмпульсу нагнiтання. Виведено формулу для розрахунку нерiвнова-
жного перерiзу комбiнацiйного розсiяння свiтла та отримано, що нерiвноважна складова перерiзу роз-
сiяння як для A1g, так i для B1g симетрiй має багатопiкову структуру, що може бути пояснено ефектами
iнтерференцiї чи брiллюенового розсiяння на часових змiнах оператора тензора напружень. Отримано,
що i “вимiряне” заповнення одночастинкових станiв, i вiдношення iнтенсивностi стоксових до антисто-
ксових пiкiв сильно залежать вiд ширини пробного iмпульсу, що необхiдно враховувати при аналiзi ре-
зультатiв експериментiв.
Ключовi слова: спектроскопiя нагнiтання-вимiр, фотоелектронна емiсiя, комбiнацiйне розсiяння свiтла,
нерiвноважна функцiя Ґрiна
33707-18
Introduction
Hamiltonian
DOS, PES, and occupation of the single-particle states
Equilibrium case
Nonequilibrium case
Nonresonant Raman scattering
Ratio of Stokes and anti-Stokes peaks and the probe pulse shape
Nonresonant Raman scattering off noninteracting electrons
Conclusions
|