2,913 research outputs found
Spin-Dependent Quantum Emission in Hexagonal Boron Nitride at Room Temperature
Optically addressable spins associated with defects in wide-bandgap
semiconductors are versatile platforms for quantum information processing and
nanoscale sensing, where spin-dependent inter-system crossing (ISC) transitions
facilitate optical spin initialization and readout. Recently, the van der Waals
material hexagonal boron nitride (h-BN) has emerged as a robust host for
quantum emitters (QEs), but spin-related effects have yet to be observed. Here,
we report room-temperature observations of strongly anisotropic
photoluminescence (PL) patterns as a function of applied magnetic field for
select QEs in h-BN. Field-dependent variations in the steady-state PL and
photon emission statistics are consistent with an electronic model featuring a
spin-dependent ISC between triplet and singlet manifolds, indicating that
optically-addressable spin defects are present in h-BN a versatile
two-dimensional material promising efficient photon extraction, atom-scale
engineering, and the realization of spin-based quantum technologies using van
der Waals heterostructures.Comment: 38 pages, 34 figure
Massless Metric Preheating
Can super-Hubble metric perturbations be amplified exponentially during
preheating ? Yes. An analytical existence proof is provided by exploiting the
conformal properties of massless inflationary models. The traditional conserved
quantity \zeta is non-conserved in many regions of parameter space. We include
backreaction through the homogeneous parts of the inflaton and preheating
fields and discuss the role of initial conditions on the post-preheating
power-spectrum. Maximum field variances are strongly underestimated if metric
perturbations are ignored. We illustrate this in the case of strong
self-interaction of the decay products. Without metric perturbations,
preheating in this case is very inefficient. However, metric perturbations
increase the maximum field variances and give alternative channels for the
resonance to proceed. This implies that metric perturbations can have a large
impact on calculations of relic abundances of particles produced during
preheating.Comment: 8 pages, 4 colour figures. Version to appear in Phys. Rev. D.
Contains substantial new analysis of the ranges of parameter space for which
large changes to the inflation-produced power spectrum are expecte
Adiabatic Gravitational Perturbation During Reheating
We study the possibilities of parametric amplification of the gravitational
perturbation during reheating in single-field inflation models. Our result
shows that there is no additional growth of the super-horizon modes beyond the
usual predictions.Comment: Refs added; New version to appear in PR
Chandra Observations of Radio-Loud Quasars at z > 4: X-rays from the Radio Beacons of the Early Universe
We present the results of Chandra observations of six radio-loud quasars
(RLQs) and one optically bright radio-quiet quasar (RQQ) at z = 4.1-4.4. These
observations cover a representative sample of RLQs with moderate radio-loudness
(R ~ 40-400), filling the X-ray observational gap between optically selected
RQQs and the five known blazars at z > 4 (R ~ 800-27000). We study the
relationship between X-ray luminosity and radio-loudness for quasars at high
redshift and constrain RLQ X-ray continuum emission and absorption. From a
joint spectral fit of nine moderate-R RLQs observed by Chandra, we find
tentative evidence for absorption above the Galactic N_H, with a best-fit
neutral intrinsic column density of N_H = 2.4^{+2.0}_{-1.8} x 10^{22} cm^{-2},
consistent with earlier claims of increased absorption toward high-redshift
RLQs. We also search for evidence of an enhanced jet-linked component in the
X-ray emission due to the increased energy density of the cosmic microwave
background (CMB) at high redshift, but we find neither spatial detections of
X-ray jets nor a significant enhancement in the X-ray emission relative to
comparable RLQs at low-to-moderate redshifts. Overall, the z ~ 4-5 RLQs have
basic X-ray properties consistent with comparable RLQs in the local universe,
suggesting that the accretion/jet mechanisms of these objects are similar as
well.Comment: 12 pages, The Astronomical Journal, in pres
Testing for double inflation with WMAP
With the WMAP data we can now begin to test realistic models of inflation
involving multiple scalar fields. These naturally lead to correlated adiabatic
and isocurvature (entropy) perturbations with a running spectral index. We
present the first full (9 parameter) likelihood analysis of double inflation
with WMAP data and find that despite the extra freedom, supersymmetric hybrid
potentials are strongly constrained with less than 7% correlated isocurvature
component allowed when standard priors are imposed on the cosomological
parameters. As a result we also find that Akaike & Bayesian model selection
criteria rather strongly prefer single-field inflation, just as equivalent
analysis prefers a cosmological constant over dynamical dark energy in the late
universe. It appears that simplicity is the best guide to our universe.Comment: 7 pages, 6 figure
Are Kaluza-Klein modes enhanced by parametric resonance?
We study parametric amplification of Kaluza-Klein (KK) modes in a higher
-dimensional generalized Kaluza-Klein theory, which was originally
considered by Mukohyama in the narrow resonance case. It was suggested that KK
modes can be enhanced by an oscillation of a scale of compactification by the
-dimensional sphere and by the direct product . We extend this past work to the more general case where
initial values of the scale of compactification and the quantum number of the
angular momentum of KK modes are not small. We perform analytic approaches
based on the Mathieu equation as well as numerical calculations, and find that
the expansion of the universe rapidly makes the KK field deviate from
instability bands. As a result, KK modes are not enhanced sufficiently in an
expanding universe in these two classes of models.Comment: 15 pages, 5 figure
Preheating of the nonminimally coupled inflaton field
We investigate preheating of an inflaton field coupled nonminimally to
a spacetime curvature. In the case of a self-coupling inflaton potential
, the dynamics of preheating changes by the effect of
the negative . We find that the nonminimal coupling works in two ways.
First, since the initial value of inflaton field for reheating becomes
smaller with the increase of , the evolution of the inflaton quanta is
delayed for fixed . Second, the oscillation of the inflaton field is
modified and the nonadiabatic change around occurs significantly. That
makes the resonant band of the fluctuation field wider. Especially for strong
coupling regimes , the growth of the inflaton flutuation is
dominated by the resonance due to the nonminimal coupling, which leads to the
significant enhancement of low momentum modes. Although the final variance of
the inflaton fluctuation does notchange significantly compared with the
minimally coupled case, we have found that the energy transfer from the
homogeneous inflaton to created particles efficiently occurs for .Comment: 13pages, 11figure
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