1,678 research outputs found
Influence of the Coulomb potential on above-threshold ionization: a quantum-orbit analysis beyond the strong-field approximation
We perform a detailed analysis of how the interplay between the residual
binding potential and a strong laser field influences above-threshold
ionization (ATI), employing a semi-analytical, Coulomb-corrected strong-field
approximation (SFA) in which the Coulomb potential is incorporated in the
electron propagation in the continuum. We find that the Coulomb interaction
lifts the degeneracy of some SFA trajectories, and we identify a set of orbits
which, for high enough photoelectron energies, may be associated with
rescattering. Furthermore, by performing a direct comparison with the standard
SFA, we show that several features in the ATI spectra can be traced back to the
influence of the Coulomb potential on different electron trajectories. These
features include a decrease in the contrast, a shift towards lower energies in
the interference substructure, and an overall increase in the photoelectron
yield. All features encountered exhibit a very good agreement with the \emph{ab
initio} solution of the time-dependent Schr\"odinger equation.Comment: 12 pages, 10 figure
Time evolution of non-Hermitian Hamiltonian systems
We provide time-evolution operators, gauge transformations and a perturbative
treatment for non-Hermitian Hamiltonian systems, which are explicitly
time-dependent. We determine various new equivalence pairs for Hermitian and
non-Hermitian Hamiltonians, which are therefore pseudo-Hermitian and in
addition in some cases also invariant under PT-symmetry. In particular, for the
harmonic oscillator perturbed by a cubic non-Hermitian term, we evaluate
explicitly various transition amplitudes, for the situation when these systems
are exposed to a monochromatic linearly polarized electric field.Comment: 25 pages Latex, 1 eps figure, references adde
Understanding stellar activity-induced radial velocity jitter using simultaneous K2 photometry and HARPS RV measurements
One of the best ways to improve our understanding of the stellar
activity-induced signal in radial velocity (RV) measurements is through
simultaneous high-precision photometric and RV observations. This is of prime
importance to mitigate the RV signal induced by stellar activity and therefore
unveil the presence of low-mass exoplanets. The K2 Campaign 7 and 8
field-of-views were located in the southern hemisphere, and provided a unique
opportunity to gather unprecedented simultaneous high precision photometric
observation with K2 and high-precision RV measurements with the HARPS
spectrograph to study the relationship between photometric variability and RV
jitter. We observed nine stars with different levels of activity; from quiet to
very active. We probe the presence of any meaningful relation between measured
RV jitter and the simultaneous photometric variation, and also other activity
indicators (e.g. BIS, FWHM, , and F8), by evaluating the strength
and significance of the correlation between RVs and each indicator. We found
that for the case of very active stars, strong and significant correlations
exist between almost all the observables and measured RVs; however, for lower
activity levels the correlations become random. Except for the F8 which its
strong correlation with RV jitter persists over a wide range of stellar
activity level, and thus our result suggests that F8 might be a powerful proxy
for activity induced RV jitter. Moreover, we examine the capability of two
state-of-the-art modeling techniques, namely the FF' method and SOAP2.0, in
accurately predicting the RV jitter amplitude using the simultaneous
photometric observation. We found that for the very active stars both
techniques can reasonably well predict the amplitude of the RV jitter, however,
at lower activity levels the FF' method underpredicts the RV jitter amplitude.Comment: 13 pages, 7 figures, 2 tables, accepted for publication in A&
Holographic detection of parity in atomic and molecular orbitals
We introduce a concise methodology to detect the parity of atomic and molecular orbitals based on photoelectron holography, which is more general than the existing schemes. It fully accounts for the Coulomb distortions of electron trajectories, does not require sculpted fields to retrieve phase information and, in principle, is applicable to a broad range of electron momenta. By comparatively measuring the differential photoelectron spectra from strong-field ionization of
N
2
molecules and their companion atoms of Ar, some photoelectron holography patterns are found to be dephased for both targets. This is well reproduced by the full-dimensional time-dependent Schrödinger equation and the Coulomb quantum-orbit strong-field approximation (CQSFA) simulation. Using the CQSFA, we trace back our observations to different parities of the
3
p
orbital of Ar and the highest-occupied molecular orbital of
N
2
via interfering Coulomb-distorted quantum orbits carrying different initial phases. This method could in principle be used to extract bound-state phases from any holographic structure, with a wide range of potential applications in recollision physics and spectroscopy
Fermion localization on asymmetric two-field thick branes
In this paper we investigate the localization of fermions on asymmetric thick
branes generated by two scalars and . In order to trap fermions on
the asymmetric branes with kink-like warp factors, the couplings with the
background scalars are introduced, where
is a function of and . We find that the coupling
do not support the localization of 4-dimensional
fermions on the branes. While, for the case
, which is the kink-fermion
coupling corresponding to one-scalar-generated brane scenarios, the zero mode
of left-handed fermions could be trapped on the branes under some conditions.Comment: v2: 11 pages, 4 figures, accepted by CQ
The HARPS search for southern extra-solar planets XXXV. The interesting case of HD41248: stellar activity, no planets?
The search for planets orbiting metal-poor stars is of uttermost importance
for our understanding of the planet formation models. However, no dedicated
searches have been conducted so far for very low mass planets orbiting such
objects. Only a few cases of low mass planets orbiting metal-poor stars are
thus known. Amongst these, HD41248 is a metal-poor, solar-type star on which a
resonant pair of super-Earth like planets has In the present paper we present a
new planet search program that is using the HARPS spectrograph to search for
Neptunes and Super-Earths orbiting a sample of metal-poor FGK dwarfs. We then
present a detailed analysis of an additional 162 radial velocity measurements
of HD41248, obtained within this program, with the goal of confirming the
existence of the proposed planetary system. We analyzed the precise radial
velocities, obtained with the HARPS spectrograph, together with several stellar
activity diagnostics and line profile indicators. A careful analysis shows no
evidence for the planetary system previously announced. One of the signals,
with a period of about 25 days, is shown to be related to the rotational period
of the star, and is clearly seen in some of the activity proxies. The remaining
signal (P~18 days) could not be convincingly retrieved in the new data set. We
discuss possible causes for the complex (evolving) signals observed in the data
of HD41248, proposing that they may be explained by the appearance and
disappearance of active regions on the surface of a star with strong
differential rotation, or by a combination of the sparse data sampling and
active region evolution.Comment: Accepted for publication in A&
Oral tolerance to cancer can be abrogated by T regulatory cell inhibition
Oral administration of tumour cells induces an immune hypo-responsiveness known as oral tolerance. We have previously shown that oral tolerance to a cancer is tumour antigen specific, non-cross-reactive and confers a tumour growth advantage. We investigated the utilisation of regulatory T cell (Treg) depletion on oral tolerance to a cancer and its ability to control tumour growth. Balb/C mice were gavage fed homogenised tumour tissue – JBS fibrosarcoma (to induce oral tolerance to a cancer), or PBS as control. Growth of subcutaneous JBS tumours were measured; splenic tissue excised and flow cytometry used to quantify and compare systemic Tregs and T effector (Teff) cell populations. Prior to and/or following tumour feeding, mice were intraperitoneally administered anti-CD25, to inactivate systemic Tregs, or given isotype antibody as a control. Mice which were orally tolerised prior to subcutaneous tumour induction, displayed significantly higher systemic Treg levels (14% vs 6%) and faster tumour growth rates than controls (p<0.05). Complete regression of tumours were only seen after Treg inactivation and occurred in all groups - this was not inhibited by tumour feeding. The cure rates for Treg inactivation were 60% during tolerisation, 75% during tumour growth and 100% during inactivation for both tolerisation and tumour growth. Depletion of Tregs gave rise to an increased number of Teff cells. Treg depletion post-tolerisation and post-tumour induction led to the complete regression of all tumours on tumour bearing mice. Oral administration of tumour tissue, confers a tumour growth advantage and is accompanied by an increase in systemic Treg levels. The administration of anti-CD25 Ab decreased Treg numbers and caused an increase in Teffs. Most notably Treg cell inhibition overcame established oral tolerance with consequent tumor regression, especially relevant to foregut cancers where oral tolerance is likely to be induced by the shedding of tumour tissue into the gut
Pushed traveling fronts in monostable equations with monotone delayed reaction
We study the existence and uniqueness of wavefronts to the scalar
reaction-diffusion equations with monotone delayed reaction term and . We are mostly interested in the situation when the graph of is not
dominated by its tangent line at zero, i.e. when the condition , is not satisfied. It is well known that, in such a case, a
special type of rapidly decreasing wavefronts (pushed fronts) can appear in
non-delayed equations (i.e. with ). One of our main goals here is to
establish a similar result for . We prove the existence of the minimal
speed of propagation, the uniqueness of wavefronts (up to a translation) and
describe their asymptotics at . We also present a new uniqueness
result for a class of nonlocal lattice equations.Comment: 17 pages, submitte
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