979 research outputs found
The Crooks relation in optical spectra - universality in work distributions for weak local quenches
We show that work distributions and non-equilibrium work fluctuation theorems
can be measured in optical spectra for a wide class of quantum systems. We
consider systems where the absorption or emission of a photon corresponds to
the sudden switch on or off of a local perturbation. For the particular case of
a weak local perturbation, the Crooks relation establishes a universal relation
in absorption as well as in emission spectra. Due to a direct relation between
the spectra and work distribution functions this is equivalent to universal
relations in work distributions for weak local quenches. As two concrete
examples we treat the X-ray edge problem and the Kondo exciton.Comment: 4+ pages, 1 figure; version as publishe
Describing many-body localized systems in thermal environments
In this work we formulate an efficient method for the description of fully many-body localized systems in weak contact with thermal environments at temperature T. The key idea is to exploit the representation of the system in terms of quasi-local integrals of motion (l-bits) to efficiently derive the generator for the quantum master equation in Born-Markov approximation. We, moreover, show how to compute the steady state of this equation efficiently by using quantum-jump Monte-Carlo techniques as well as by deriving approximate kinetic equations of motion. As an example, we consider a one-dimensional disordered extended Hubbard model for spinless fermions, for which we derive the l-bit representation approximately by employing a recently proposed method valid in the limit of strong disorder and weak interactions. Coupling the system to a global thermal bath, we study the transport between two leads with different chemical potentials at both of its ends. We find that the temperature-dependent current is captured by an interaction-dependent version of Mott's law for variable range hopping, where transport is enhanced/lowered depending on whether the interactions are attractive or repulsive, respectively. We interpret these results in terms of spatio-energetic correlations between the l-bits
Polarization Evolution in Strong Magnetic Fields
Extremely strong magnetic fields change the vacuum index of refraction.
Although this polarization dependent effect is small for typical neutron stars,
it is large enough to decouple the polarization states of photons traveling
within the field. The photon states evolve adiabatically and follow the
changing magnetic field direction. The combination of a rotating magnetosphere
and a frequency dependent state decoupling predicts polarization phase lags
between different wave bands, if the emission process takes place well within
the light cylinder. This QED effect may allow observations to distinguish
between different pulsar emission mechanisms and to reconstruct the structure
of the magnetosphere.Comment: 22 pages, 10 figures, accepted for publication in MNRA
How Common Are Magnetars? The Consequences of Magnetic-Field Decay
Ultramagnetized neutron stars or magnetars have been invoked to explain
several astrophysical phenomena. We examine how the magnetic field of a
magnetar will decay over time and how this decay affects the cooling of the
object. We find that for sufficiently strong nascent fields, field decay alters
the cooling evolution significantly relative to similarly magnetized neutron
stars with constant fields. As a result, old magnetars can be expected to be
bright in the soft X-ray band. The soft X-ray source RXJ~0720.43125 may well
be the nearest such old magnetar.Comment: 7 pages, 1 figure, accepted for publication in Ap. J. Letter
Dynamical Quantum Phase Transitions in the Transverse Field Ising Model
A phase transition indicates a sudden change in the properties of a large
system. For temperature-driven phase transitions this is related to
non-analytic behavior of the free energy density at the critical temperature:
The knowledge of the free energy density in one phase is insufficient to
predict the properties of the other phase. In this paper we show that a close
analogue of this behavior can occur in the real time evolution of quantum
systems, namely non-analytic behavior at a critical time. We denote such
behavior a dynamical phase transition and explore its properties in the
transverse field Ising model. Specifically, we show that the equilibrium
quantum phase transition and the dynamical phase transition in this model are
intimately related.Comment: 4+4 pages, 4 figures, Appendix adde
Magnetar giant flare high-energy emission
High energy ( keV) emission has been detected persisting for several
tens of seconds after the initial spike of magnetar giant flares. It has been
conjectured that this emission might arise via inverse Compton scattering in a
highly extended corona generated by super-Eddington outflows high up in the
magnetosphere. In this paper we undertake a detailed examination of this model.
We investigate the properties of the required scatterers, and whether the
mechanism is consistent with the degree of pulsed emission observed in the tail
of the giant flare. We conclude that the mechanism is consistent with current
data, although the origin of the scattering population remains an open
question. We propose an alternative picture in which the emission is closer to
that star and is dominated by synchrotron radiation. The observations
of the December 2004 flare modestly favor this latter picture. We assess the
prospects for the Fermi Gamma-Ray Space Telescope to detect and characterize a
similar high energy component in a future giant flare. Such a detection should
help to resolve some of the outstanding issues.Comment: 20 pages, 14 figure
Handling and analysis of ices in cryostats and glove boxes in view of cometary samples
Comet nucleus sample return mission and other return missions from planets and satellites need equipment for handling and analysis of icy samples at low temperatures under vacuum or protective gas. Two methods are reported which were developed for analysis of small icy samples and which are modified for larger samples in cometary matter simulation experiments (KOSI). A conventional optical cryostat system was modified to allow for transport of samples at 5 K, ion beam irradiation, and measurement in an off-line optical spectrophotometer. The new system consists of a removable window plug containing nozzles for condensation of water and volatiles onto a cold finger. This plug can be removed in a vacuum system, changed against another plug (e.g., with other windows (IR, VIS, VUV) or other nozzles). While open, the samples can be treated under vacuum with cooling by manipulators (cut, removal, sample taking, irradiation with light, photons, or ions). After bringing the plug back, the samples can be moved to another site of analysis. For handling the 30 cm diameter mineral-ice samples from the KOSI experiments an 80x80x80 cm glove box made out of plexiglass was used. The samples were kept in a liquid nitrogen bath, which was filled from the outside. A stream a dry N2 and evaporating gas from the bath purified the glove box from impurity gases and, in particular, H2O, which otherwise would condense onto the samples
1RXS J214303.7+065419/RBS 1774: A New Isolated Neutron Star Candidate
We report on the identification of a new possible Isolated Neutron Star
candidate in archival ROSAT observations. The source 1RXS J214303.7+065419,
listed in the ROSAT Bright Survey as RBS 1774, is very soft, exhibits a thermal
spectrum well fitted by a blackbody at eV and has a low column
density, . Catalogue searches revealed
no known sources in other energy bands close to the X-ray position of RBS 1774.
Follow-up optical observations with NTT showed no peculiar object within the
X-ray error circle. The absence of any plausible optical counterpart down to
results in an X-ray to optical flux ratio in excess of 1000.Comment: LaTeX (A&A style files), 5 pages, 3 figures. Accepted for publication
in Astronomy and Astrophysics Letters. Minor correction
The oxygen-II luminosity density of the Universe
Equivalent widths of [OII] 3727 A lines are measured in 375 faint galaxy
spectra taken as part of the Caltech Faint Galaxy Redshift Survey centered on
the Hubble Deep Field. The sensitivity of the survey spectra to the [OII] line
is computed as a function of magnitude, color and redshift. The luminosity
function of galaxies in the [OII] line and the integrated luminosity density of
the Universe in the [OII] line are computed as a function of redshift. It is
found that the luminosity density in the [OII] line was a factor of ~10 higher
at redshifts z~1 than it is at the present day. The simplest interpretation is
that the star formation rate density of the Universe has declined dramatically
since z~1.Comment: accepted for publication in Ap
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