2,371 research outputs found
Tuning of heat and charge transport by Majorana fermions
We investigate theoretically thermal and electrical conductances for the
system consisting of a quantum dot (QD) connected both to a pair of Majorana
fermions residing the edges of a Kitaev wire and two metallic leads. We
demonstrate that both quantities reveal pronounced resonances, whose positions
can be controlled by tuning of an asymmetry of the couplings of the QD and a
pair of MFs. Similar behavior is revealed for the thermopower, Wiedemann-Franz
law and dimensionless thermoelectric figure of merit. The considered geometry
can thus be used as a tuner of heat and charge transport assisted by MFs
Can stellar activity make a planet seem misaligned?
Several studies have shown that the occultation of stellar active regions by
the transiting planet can generate anomalies in the high-precision transit
light curves, and these anomalies may lead to an inaccurate estimate of the
planetary parameters (e.g., the planet radius). Since the physics and geometry
behind the transit light curve and the Rossiter- McLaughlin effect
(spectroscopic transit) are the same, the Rossiter-McLaughlin observations are
expected to be affected by the occultation of stellar active regions in a
similar way. In this paper we perform a fundamental test on the spin-orbit
angles as derived by Rossiter-McLaughlin measurements, and we examine the
impact of the occultation of stellar active regions by the transiting planet on
the spin-orbit angle estimations. Our results show that the inaccurate
estimation on the spin-orbit angle due to stellar activity can be quite
significant (up to 30 degrees), particularly for the edge-on, aligned, and
small transiting planets. Therefore, our results suggest that the aligned
transiting planets are the ones that can be easily misinterpreted as misaligned
owing to the stellar activity. In other words, the biases introduced by
ignoring stellar activity are unlikely to be the culprit for the highly
misaligned systems.Comment: 8 pages, 8 figures, accepted for publication in Astronomy &
Astrophysic
Existence criteria for stabilization from the scaling behaviour of ionization probabilities
We provide a systematic derivation of the scaling behaviour of various
quantities and establish in particular the scale invariance of the ionization
probability. We discuss the gauge invariance of the scaling properties and the
manner in which they can be exploited as consistency check in explicit
analytical expressions, in perturbation theory, in the Kramers-Henneberger and
Floquet approximation, in upper and lower bound estimates and fully numerical
solutions of the time dependent Schroedinger equation. The scaling invariance
leads to a differential equation which has to be satisfied by the ionization
probability and which yields an alternative criterium for the existence of
atomic bound state stabilization.Comment: 12 pages of Latex, one figur
Coulomb-corrected quantum interference in above-threshold ionization: Working towards multi-trajectory electron holography
Using the recently developed Coulomb Quantum Orbit Strong-Field Approximation
(CQSFA), we perform a systematic analysis of several features encountered in
above-threshold ionization (ATI) photoelectron angle-resolved distributions
(PADs), such as side lobes, and intra- and intercycle interference patterns.
The latter include not only the well-known intra-cycle rings and the
near-threshold fan-shaped structure, but also previously overlooked patterns.
We provide a direct account of how the Coulomb potential distorts different
types of interfering trajectories and changes the corresponding phase
differences, and show that these patterns may be viewed as generalized
holographic structures formed by up to three types of trajectories. We also
derive analytical interference conditions and estimates valid in the presence
or absence of the residual potential, and assess the range of validity of
Coulomb-corrected interference conditions provided in the literature.Comment: 17 pages, 11 figures. Some figures have been compressed in order to
comply with the arXiv requirement
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