39,890 research outputs found
Artificial Life in an Exciton-Polariton Lattice
We show theoretically that a lattice of exciton-polaritons can behave as a
life-like cellular automaton when simultaneously excited by a continuous wave
coherent field and a time-periodic sequence of non-resonant pulses. This
provides a mechanism of realizing a range of highly sought spatiotemporal
structures under the same conditions, including: discrete solitons, oscillating
solitons, rotating solitons, breathers, soliton trains, guns, and choatic
behaviour. These structures can survive in the system indefinitely, despite the
presence of dissipation, and allow universal computation.Comment: 14 pages, 14 figure
Global monopole in scalar tensor theory
The well known monopole solution of Barriola and Vilenkin (BV) resulting from
the breaking of a global SO(3) symmetry is extended in general relativity along
with a zero mass scalar field and also in Brans-Dicke(BD) theory of gravity.In
the case of BD theory, the behaviour of spacetime and other variables such as
BD scalar field and the monopole energy density have been studied
numerically.For monopole along with a zero mass scalar field, exact solutions
are obtained and depending upon the choice of arbitary parameters, the
solutions either reduce to the BV case or to a pure scalar field solution as
special cases.It is interesting to note that unlike the BV case the global
monopole in the BD theory does exert gravitational pull on a test particle
moving in its spacetime.Comment: 12 pages LaTex, 3 postscript figures, Communicated to
Class.Quant.Gra
Quantum Tunneling, Blackbody Spectrum and Non-Logarithmic Entropy Correction for Lovelock Black Holes
We show, using the tunneling method, that Lovelock black holes Hawking
radiate with a perfect blackbody spectrum. This is a new result. Within the
semiclassical (WKB) approximation the temperature of the spectrum is given by
the semiclassical Hawking temperature. Beyond the semiclassical approximation
the thermal nature of the spectrum does not change but the temperature
undergoes some higher order corrections. This is true for both black hole
(event) and cosmological horizons. Using the first law of thermodynamics the
black hole entropy is calculated. Specifically the -dimensional static,
chargeless black hole solutions which are spherically symmetric and
asymptotically flat, AdS or dS are considered. The interesting property of
these black holes is that their semiclassical entropy does not obey the
Bekenstein-Hawking area law. It is found that the leading correction to the
semiclassical entropy for these black holes is not logarithmic and next to
leading correction is also not inverse of horizon area. This is in contrast to
the black holes in Einstein gravity. The modified result is due to the presence
of Gauss-Bonnet term in the Lovelock Lagrangian. For the limit where the
coupling constant of the Gauss-Bonnet term vanishes one recovers the known
correctional terms as expected in Einstein gravity. Finally we relate the
coefficient of the leading (non-logarithmic) correction with the trace anomaly
of the stress tensor.Comment: minor modifications, two new references added, LaTeX, JHEP style, 34
pages, no figures, to appear in JHE
Two-step melting of the vortex solid in layered superconductors with random columnar pins
We consider the melting of the vortex solid in highly anisotropic layered
superconductors with a small concentration of random columnar pinning centers.
Using large-scale numerical minimization of a free-energy functional, we find
that melting of the low-temperature, nearly crystalline vortex solid (Bragg
glass) into a vortex liquid occurs in two steps as the temperature increases:
the Bragg glass and liquid phases are separated by an intermediate Bose glass
phase. A suitably defined local melting temperature exhibits spatial variation
similar to that observed in experiments.Comment: To appear in Phys. Rev. Let
Quantification of Entanglement of Teleportation in Arbitrary Dimensions
We study bipartite entangled states in arbitrary dimensions and obtain
different bounds for the entanglement measures in terms of teleportation
fidelity. We find that there is a simple relation between negativity and
teleportation fidelity for pure states but for mixed states, an upper bound is
obtained for negativity in terms of teleportation fidelity using convex-roof
extension negativity (CREN). However, with this it is not clear how to
distinguish betweeen states useful for teleportation and positive partial
transpose (PPT) entangled states. Further, there exists a strong conjecture in
the literature that all PPT entangled states, in 3 \times 3 systems, have
Schmidt rank two. This motivates us to develop measures capable of identifying
states useful for teleportation and dependent on the Schmidt number. We thus
establish various relations between teleportation fidelity and entanglement
measures depending upon Schmidt rank of the states. These relations and bounds
help us to determine the amount of entanglement required for teleportation,
which we call the ``Entanglement of Teleportation''. These bounds are used to
determine the teleportation fidelity as well as the entanglement required for
teleportation of states modeled by a two qutrit mixed system, as well as two
qubit open quantum systems.Comment: 10 pages, 17 figure
Tunnel Spin Polarization Versus Energy for Clean and Doped Al2O3 Barriers
The variation of the tunnel spin-polarization (TSP) with energy is determined using a magnetic tunnel transistor, allowing quantification of the energy dependent TSP separately for both ferromagnet/insulator interfaces and direct correlation with the tunnel magnetoresistance (TMR) measured in the same device. The intrinsic TSP is reduced below the Fermi level, and more strongly so for tunneling into empty states above the Fermi level. For artificially doped barriers, the low bias TMR decreases due to defect-assisted tunneling. Yet, this mechanism becomes ineffective at large bias, where instead inelastic spin scattering causes a strong TMR decay
Forward Modelling of Standing Slow Modes in Flaring Coronal Loops
Standing slow mode waves in hot flaring loops are exclusively observed in
spectrometers and are used to diagnose the magnetic field strength and
temperature of the loop structure. Due to the lack of spatial information, the
longitudinal mode cannot be effectively identified. In this study, we simulate
standing slow mode waves in flaring loops and compare the synthesized line
emission properties with SUMER spectrographic and SDO/AIA imaging observations.
We find that the emission intensity and line width oscillations are a quarter
period out of phase with Doppler shift velocity both in time and spatial
domain, which can be used to identify a standing slow mode wave from
spectroscopic observations. However, the longitudinal overtones could be only
measured with the assistance of imagers. We find emission intensity asymmetry
in the positive and negative modulations, this is because the contribution
function pertaining to the atomic emission process responds differently to
positive and negative temperature variations. One may detect \textbf{half}
periodicity close to the loop apex, where emission intensity modulation is
relatively small. The line-of-sight projection affects the observation of
Doppler shift significantly. A more accurate estimate of the amplitude of
velocity perturbation is obtained by de-projecting the Doppler shift by a
factor of rather than the traditionally used .
\textbf{If a loop is heated to the hotter wing, the intensity modulation could
be overwhelmed by background emission, while the Doppler shift velocity could
still be detected to a certain extent.Comment: 18 pages, 10 figures, Astrophysics Journa
Measuring Long-Run Exchange Rate Pass-Through.
The paper discusses the issue of estimating short- and long-run exchange rate pass-through to import prices in euro area countries and reviews some problems with the measures recently proposed in the literature. Theoretical considerations suggest a long-run Engle and Granger cointegrating relationship (between import unit values, the exchange rate and foreign prices), which is typically ignored in existing empirical studies. We use time series and up-to-date panel data techniques to test for cointegration with the possibility of structural breaks and show how the long-run may be restored in the estimation. The main finding is that allowing for possible breaks around the formation of EMU and the appreciation of the euro starting in 2001 helps restore a long run cointegration relationship, where over the sample period the fixed component of the pass-through decreased while the variable component tended to increase.Exchange rates ; Pass-through ; Import prices ; Panel cointegration ; Structural break.
Spin injection and perpendicular spin transport in graphite nanostructures
Organic and carbon-based materials are attractive for spintronics because
their small spin-orbit coupling and low hyperfine interaction is expected to
give rise to large spin-relaxation times. However, the corresponding
spin-relaxation length is not necessarily large when transport is via weakly
interacting molecular orbitals. Here we use graphite as a model system and
study spin transport in the direction perpendicular to the weakly bonded
graphene sheets. We achieve injection of highly (75%) spin-polarized electrons
into graphite nanostructures of 300-500 nm across and up to 17 nm thick, and
observe transport without any measurable loss of spin information. Direct
visualization of local spin transport in graphite-based spin-valve sandwiches
also shows spatially uniform and near-unity transmission for electrons at 1.8
eV above the Fermi level
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