46,201 research outputs found
Losses for microwave transmission in metamaterials for producing left-handed materials: The strip wires
This paper shows that the effective dielectric permitivity for the
metamaterials used so far to obtain left-handed materials, with strip wires
0.003cm thick, is dominated by the imaginary part at 10.6- 11.5 GHz
frequencies, where the band pass filter is, and therefore there is not
propagation and the wave is inhomogeneous inside the medium. This is shown from
finite-differences time-domain calculations using the real permitivity values
for the Cu wires. For thicker wires the losses are reduced and the negative
part of the permitivity dominates. As the thickness of the wires is critical
for the realization of a good transparent left- handed material we propose that
the strip wires should have thickness of 0.07-0.1cm and the split ring
resonators 0.015-0.03c
A skyrmion-based spin-torque nano-oscillator
A model for a spin-torque nano-oscillator based on the self-sustained
oscillation of a magnetic skyrmion is presented. The system involves a circular
nanopillar geometry comprising an ultrathin film free magnetic layer with a
strong Dzyaloshinkii-Moriya interaction and a polariser layer with a
vortex-like spin configuration. It is shown that spin-transfer torques due to
current flow perpendicular to the film plane leads to skyrmion gyration that
arises from a competition between geometric confinement due to boundary edges
and the vortex-like polarisation of the spin torques. A phenomenology for such
oscillations is developed and quantitative analysis using micromagnetics
simulations is presented. It is also shown that weak disorder due to random
anisotropy variations does not influence the main characteristics of the
steady-state gyration.Comment: 15 pages, 6 figure
Evolving wormhole geometries within nonlinear electrodynamics
In this work, we explore the possibility of evolving (2+1) and
(3+1)-dimensional wormhole spacetimes, conformally related to the respective
static geometries, within the context of nonlinear electrodynamics. For the
(3+1)-dimensional spacetime, it is found that the Einstein field equation
imposes a contracting wormhole solution and the obedience of the weak energy
condition. Nevertheless, in the presence of an electric field, the latter
presents a singularity at the throat, however, for a pure magnetic field the
solution is regular. For the (2+1)-dimensional case, it is also found that the
physical fields are singular at the throat. Thus, taking into account the
principle of finiteness, which states that a satisfactory theory should avoid
physical quantities becoming infinite, one may rule out evolving
(3+1)-dimensional wormhole solutions, in the presence of an electric field, and
the (2+1)-dimensional case coupled to nonlinear electrodynamics.Comment: 17 pages, 1 figure; to appear in Classical and Quantum Gravity. V2:
minor corrections, including a referenc
Lambda-inflation and CMB anisotropy
We explore a broad class of three-parameter inflationary models, called the
-inflation, and its observational predictions: high abundance of
cosmic gravitational waves consistent with the Harrison-Zel'dovich spectrum of
primordial cosmological perturbations, the non-power-law wing-like spectrum of
matter density perturbations, high efficiency of these models to meet current
observational tests, and others. We show that a parity contribution of the
gravitational waves and adiabatic density perturbations into the large-scale
temperature anisotropy, T/S , is a common feature of
-inflation; the maximum values of T/S (basically not larger than 10)
are reached in models where (i) the local spectrum shape of density
perturbations is flat or slightly red (), and (ii) the residual
potential energy of the inflaton is near the GUT scale (). The conditions to find large T/S in the paradigm of cosmic
inflation and the relationship of T/S to the ratio of the power spectra, ,
and to the inflationary and Hubble parameters, are discussed. We argue
that a simple estimate, T/S, is true for most known inflationary solutions and allows
to relate straightforwardly the important parameters of observational and
physical cosmology.Comment: 29 pages, 3 figures include
Vlasov scaling for the Glauber dynamics in continuum
We consider Vlasov-type scaling for the Glauber dynamics in continuum with a
positive integrable potential, and construct rescaled and limiting evolutions
of correlation functions. Convergence to the limiting evolution for the
positive density system in infinite volume is shown. Chaos preservation
property of this evolution gives a possibility to derive a non-linear
Vlasov-type equation for the particle density of the limiting system.Comment: 32 page
Supernova 1996cr: SN 1987A's Wild Cousin?
We report on new VLT optical spectroscopic and multi-wavelength archival
observations of SN1996cr, a previously identified ULX known as Circinus Galaxy
X-2. Our optical spectrum confirms SN1996cr as a bona fide type IIn SN, while
archival imaging isolates its explosion date to between 1995-02-28 and
1996-03-16. SN1996cr is one of the closest SNe (~3.8 Mpc) in the last several
decades and in terms of flux ranks among the brightest radio and X-ray SNe ever
detected. The wealth of optical, X-ray, and radio observations that exist for
this source provide relatively detailed constraints on its post-explosion
expansion and progenitor history, including an preliminary angular size
constaint from VLBI. The archival X-ray and radio data imply that the
progenitor of SN1996cr evacuated a large cavity just prior to exploding: the
blast wave likely expanded for ~1-2 yrs before eventually striking the dense
circumstellar material which surrounds SN1996cr. The X-ray and radio emission,
which trace the progenitor mass-loss rate, have respectively risen by a factor
of ~2 and remained roughly constant over the past 7 yr. This behavior is
reminiscent of the late rise of SN1987A, but 1000 times more luminous and much
more rapid to onset. Complex Oxygen line emission in the optical spectrum
further hints at a possible concentric shell or ring-like structure. The
discovery of SN1996cr suggests that a substantial fraction of the closest SNe
observed in the last several decades have occurred in wind-blown bubbles. An
Interplanetary Network position allows us to reject a tentative GRB association
with BATSE 4B960202. [Abridged]Comment: 25 pages with tables, 12 figures (color), accepted to ApJ, comments
welcome; v2 - updated to reflect the subsequent rejection of our tentative
GRB association based on a revised error region from the Interplanetary
Network (thanks to Kevin Hurley) and include a few additional references; v3
- corrected some errors in Tables 7 and
- …