8,071 research outputs found
Domain walls in Born-Infeld-dilaton background
We study the dynamics of domain walls in Einstein-Born-Infeld-dilaton theory.
Dilaton is non-trivially coupled with the Born-Infeld electromagnetic field. We
find three different types of solutions consistent with the dynamic domain
walls. For every case, the solutions have singularity. Further more, in these
backgrounds, we study the dynamics of domain walls. We qualitatively plot
various form of the bulk metrics and the potential encountered by the domain
walls. In many cases, depending upon the value of the parameters, the domain
walls show bouncing universe and also undergo inflationary phase followed by
standard decelerated expansion.Comment: 18 pages,6 figures,latex, References added, Some points clarifie
Electronic spectra of linear HCH and cumulene carbene HC
The transition of linear HCH
(A) has been observed in a neon matrix and gas phase. The assignment is based
on mass-selective experiments, extrapolation of previous results of the longer
HCH homologues, and density functional and multi-state CASPT2
theoretical methods. Another band system starting at 303 nm in neon is assigned
as the transition of the cumulene carbene
pentatetraenylidene HC (B).Comment: 7 pages, 4 figures, 5 table
Observable signals in a string inspired axion-dilaton background and Randall-Sundrum scenario
Rotation angle of the plane of polarization of the distant galactic radio
waves has been estimated in a string inspired axion-dilaton background. It is
found that the axion,dual to the field strength of the second rank
antisymmetric massless Kalb-Ramond field in the string spectrum, produces a
wavelength independent optical rotation which is much larger than that produced
by the dilaton. Detection of such rotation has been reported in some recent
cosmological experiments. The observed value has been compared with our
estimated theoretical value following various cosmological constraints. The
effects of warped extra dimensions in a braneworld scenario on such an optical
rotation have been investigated.Comment: 17 Pages, Latex, article revised, To appear in Physical Review
Electrons surf phason waves in moiré bilayers
We investigate the effect of thermal fluctuations on the atomic and electronic structure of a twisted MoSe2/WSe2 heterobilayer using a combination of classical molecular dynamics and ab initio density functional theory calculations. Our calculations reveal that thermally excited phason modes give rise to an almost rigid motion of the moiré lattice. Electrons and holes in low-energy states are localized in specific stacking regions of the moiré unit cell and follow the thermal motion of these regions. In other words, charge carriers surf phason waves that are excited at finite temperatures. We also show that such surfing survives in the presence of a substrate and frozen potential. This effect has potential implications for the design of charge and exciton transport devices based on moiré materials
Bulk Kalb-Ramond field in Randall Sundrum scenario
We have considered the most general gauge invariant five-dimensional action
of a second rank antisymmetric Kalb-Ramond tensor gauge theory, including a
topological term of the form in a
Randall-Sundrum scenario. Such a tensor field (whose rank-3 field
strength tensor is ), which appears in the massless sector of a
heterotic string theory, is assumed to coexist with the gravity in the bulk.
The third rank field strength corresponding to the Kalb-Ramond field has a
well-known geometric interpretation as the spacetime torsion. The only
non-trivial classical solutions corresponding to the effective four-dimensional
action are found to be self-dual or anti-selfdual Kalb-Ramond fields. This
ensures that the four-dimensional effective action on the brane is
parity-conserving. The massive modes for both cases, lying in the TeV range,
are related to the fundamental parameters of the theory. These modes can be
within the kinematic reach of forthcoming TeV scale experiments. However, the
couplings of the massless as well as massive Kalb-Ramond modes with matter on
the visible brane are found to be suppressed vis-a-vis that of the graviton by
the warp factor, whence the conclusion is that both the massless and the
massive torsion modes appear much weaker than curvature to an observer on the
visible brane.Comment: 15 Pages,2 figures,Late
Constraining the Randall-Sundrum modulus in the light of recent PVLAS data
Recent PVLAS data put stringent constraints on the measurement of
birefringence and dichroism of electromagnetic waves travelling in a constant
and homogeneous magnetic field. There have been theoretical predictions in
favour of such phenomena when appropriate axion-electromagnetic coupling is
assumed. Origin of such a coupling can be traced in a low energy string action
from the requirement of quantum consistency. The resulting couplings in such
models are an artifact of the compactification of the extra dimensions present
inevitably in a string scenario. The moduli parameters which encode the compact
manifold therefore play a crucial role in determining the axion-photon
coupling. In this work we examine the possible bounds on the value of compact
modulus that emerge from the experimental limits on the coupling obtained from
the PVLAS data. In particular we focus into the Randall-Sundrum (RS) type of
warped geometry model whose modulus parameter is already restricted from the
requirement of the resolution of gauge hierarchy problem in connection with the
mass of the Higgs. We explore the bound on the modulus for a wide range of the
axion mass for both the birefringence and the dichroism data in PVLAS. We show
that the proposed value of the modulus in the RS scenario can only be
accommodated for axion mass \gsim 0.3 eV.Comment: 26 pages, 1 figure, LaTex; added references, typos corrected. Minor
changes in the text, a comment added in the Conclusio
Correspondence between Electro-Magnetic Field and other Dark Energies in Non-linear Electrodynamics
In this work, we have considered the flat FRW model of the universe filled
with electro-magnetic field. First, the Maxwell's electro-magnetic field in
linear form has been discussed and after that the modified Lagrangian in
non-linear form for accelerated universe has been considered. The corresponding
energy density and pressure for non-linear electro-magnetic field have been
calculated. We have found the condition such that the electro-magnetic field
generates dark energy. The correspondence between the electro-magnetic field
and the other dark energy candidates namely tachyonic field, DBI-essence,
Chaplygin gas, hessence dark energy, k-essenece and dilaton dark energy have
been investigated. We have also reconstructed the potential functions and the
scalar fields in this scenario.Comment: 11 pages, 7 figure
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Is the energy density a reliable parameter for materials synthesis by selective laser melting?
The effective fabrication of materials using selective laser melting depends on the process parameters. Here, we analyse the suitability of the energy density to represent the energy transferred to the powder bed, which is effectively used to melt the particles and to produce the bulk specimens. By properly varying laser power and speed in order to process the powder at constant energy density, we show that the equation currently used to calculate the energy density gives only an approximate estimation and that hatch parameters and material properties should be considered to correctly evaluate the energy density
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