21,013 research outputs found
Cosmic age, Statefinder and diagnostics in the decaying vacuum cosmology
As an extension of CDM, the decaying vacuum model (DV) describes the
dark energy as a varying vacuum whose energy density decays linearly with the
Hubble parameter in the late-times, , and
produces the matter component. We examine the high- cosmic age problem in
the DV model, and compare it with CDM and the Yang-Mills condensate
(YMC) dark energy model. Without employing a dynamical scalar field for dark
energy, these three models share a similar behavior of late-time evolution. It
is found that the DV model, like YMC, can accommodate the high- quasar APM
08279+5255, thus greatly alleviates the high- cosmic age problem. We also
calculate the Statefinder and the {\it Om} diagnostics in the model. It
is found that the evolutionary trajectories of and in the DV
model are similar to those in the kinessence model, but are distinguished from
those in CDM and YMC. The in DV has a negative slope and
its height depends on the matter fraction, while YMC has a rather flat , whose magnitude depends sensitively on the coupling.Comment: 12 pages, 4 figures, with some correction
Life assessment of combustor liner using unified constitutive models
Hot section components of gas turbine engines are subject to severe thermomechanical loads during each mission cycle. Inelastic deformation can be induced in localized regions leading to eventual fatigue cracking. Assessment of durability requires reasonably accurate calculation of the structural response at the critical location for crack initiation. In recent years nonlinear finite element computer codes have become available for calculating inelastic structural response under cyclic loading. NASA-Lewis sponsored the development of unified constitutive material models and their implementation in nonlinear finite element computer codes for the structural analysis of hot section components. These unified models were evaluated with regard to their effect on the life prediction of a hot section component. The component considered was a gas turbine engine combustor liner. A typical engine mission cycle was used for the thermal and structural analyses. The analyses were performed on a CRAY computer using the MARC finite element code. The results were compared with laboratory test results, in terms of crack initiation lives
The optical/UV excess of isolated neutron stars in the RCS model
The X-ray dim isolated neutron stars (XDINSs) are peculiar pulsar-like
objects, characterized by their very well Planck-like spectrum. In studying
their spectral energy distributions, the optical/UV excess is a long standing
problem. Recently, Kaplan et al. (2011) have measured the optical/UV excess for
all seven sources, which is understandable in the resonant cyclotron scattering
(RCS) model previously addressed. The RCS model calculations show that the RCS
process can account for the observed optical/UV excess for most sources . The
flat spectrum of RX J2143.0+0654 may due to contribution from bremsstrahlung
emission of the electron system in addition to the RCS process.Comment: 6 pages, 2 figures, 1 table, accepted for publication in Research in
Astronomy and Astrophysic
AXPs and SGRs in the outer gap model: confronting Fermi observations
Anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are
magnetar candidates, i.e., neutron stars powered by strong magnetic field. If
they are indeed magnetars, they will emit high-energy gamma-rays which are
detectable by Fermi-LAT according to the outer gap model. However, no
significant detection is reported in recent Fermi-LAT observations of all known
AXPs and SGRs. Considering the discrepancy between theory and observations, we
calculate the theoretical spectra for all AXPs and SGRs with sufficient
observational parameters. Our results show that most AXPs and SGRs are
high-energy gamma-ray emitters if they are really magnetars. The four AXPs 1E
1547.0-5408, XTE J1810-197, 1E 1048.1-5937, and 4U 0142+61 should have been
detected by Fermi-LAT. Then there is conflict between out gap model in the case
of magnetars and Fermi observations. Possible explanations in the magnetar
model are discussed. On the other hand, if AXPs and SGRs are fallback disk
systems, i.e., accretion-powered for the persistent emissions, most of them are
not high-energy gamma-ray emitters. Future deep Fermi-LAT observations of AXPs
and SGRs will help us make clear whether they are magnetars or fallback disk
systems.Comment: 15 pages, 3 figures, 1 table, accepted for publication in The
Astrophysical Journa
Non-adiabatic holonomic quantum computation
We develop a non-adiabatic generalization of holonomic quantum computation in
which high-speed universal quantum gates can be realized by using non-Abelian
geometric phases. We show how a set of non-adiabatic holonomic one- and
two-qubit gates can be implemented by utilizing optical transitions in a
generic three-level configuration. Our scheme opens up for universal
holonomic quantum computation on qubits characterized by short coherence times.Comment: Some changes, journal reference adde
The quantitative condition is necessary in guaranteeing the validity of the adiabatic approximation
The usual quantitative condition has been widely used in the practical
applications of the adiabatic theorem. However, it had never been proved to be
sufficient or necessary before. It was only recently found that the
quantitative condition is insufficient, but whether it is necessary remains
unresolved. In this letter, we prove that the quantitative condition is
necessary in guaranteeing the validity of the adiabatic approximation.Comment: 4 pages,1 figue
- …