1,764 research outputs found
Synchronization of micromasers
We investigate synchronization effects in quantum self-sustained oscillators theoretically using the micromaser as a model system. We use the probability distribution for the relative phase as a tool for quantifying the emergence of preferred phases when two micromasers are coupled together. Using perturbation theory, we show that the behavior of the phase distribution is strongly dependent on exactly how the oscillators are coupled. In the quantum regime where photon occupation numbers are low we find that although synchronization effects are rather weak, they are nevertheless significantly stronger than expected from a semiclassical description of the phase dynamics. We also compare the behavior of the phase distribution with the mutual information of the two oscillators and show that they can behave in rather different ways
Supercurvaton
We discuss observational consequences of the curvaton scenario, which
naturally appears in the context of the simplest model of chaotic inflation in
supergravity. The non-gaussianity parameter f_NL in this scenario can take
values in the observationally interesting range from O(10) to O(100). These
values may be different in different parts of the universe. The regions where
f_NL is particularly large form a curvaton web resembling a net of thick domain
walls, strings, or global monopoles.Comment: 17 pages, 1 figure. Non-perturbative effects related to
non-gaussianity in the curvaton scenario are discussed, some references are
added. This is the version accepted in JCA
From the Big Bang Theory to the Theory of a Stationary Universe
We consider chaotic inflation in the theories with the effective potentials
phi^n and e^{\alpha\phi}. In such theories inflationary domains containing
sufficiently large and homogeneous scalar field \phi permanently produce new
inflationary domains of a similar type. We show that under certain conditions
this process of the self-reproduction of the Universe can be described by a
stationary distribution of probability, which means that the fraction of the
physical volume of the Universe in a state with given properties (with given
values of fields, with a given density of matter, etc.) does not depend on
time, both at the stage of inflation and after it. This represents a strong
deviation of inflationary cosmology from the standard Big Bang paradigm. We
compare our approach with other approaches to quantum cosmology, and illustrate
some of the general conclusions mentioned above with the results of a computer
simulation of stochastic processes in the inflationary Universe.Comment: No changes to the file, but original figures are included. They
substantially help to understand this paper, as well as eternal inflation in
general, and what is now called the "multiverse" and the "string theory
landscape." High quality figures can be found at
http://www.stanford.edu/~alinde/LLMbigfigs
Operator-Algebraic Approach to the Yrast Spectrum of Weakly Interacting Trapped Bosons
We present an operator-algebraic approach to deriving the low-lying
quasi-degenerate spectrum of weakly interacting trapped N bosons with total
angular momentum \hbar L for the case of small L/N, demonstrating that the
lowest-lying excitation spectrum is given by 27 g n_3(n_3-1)/34, where g is the
strength of the repulsive contact interaction and n_3 the number of excited
octupole quanta. Our method provides constraints for these quasi-degenerate
many-body states and gives higher excitation energies that depend linearly on
N.Comment: 7 pages, one figur
Inflation driven by scalar field with non-minimal kinetic coupling with Higgs and quadratic potentials
We study a scalar field with non-minimal kinetic coupling to itself and to
the curvature. The slow rolling conditions allowing an inflationary background
have been found. The quadratic and Higgs type potentials have been considered,
and the corresponding values for the scalar fields at the end of inflation
allows to recover the connection with particle physics.Comment: 16 pages, to appear in JCA
Non-equilibrium Goldstone phenomenon in tachyonic preheating
The dominance of the direct production of elementary Goldstone waves is
demonstrated in tachyonic preheating by numerically determining the evolution
of the dispersion relation, the equation of state and the kinetic power spectra
for the angular degree of freedom of the complex matter field. The importance
of the domain structure in the order parameter distribution for the
quantitative understanding of the excitation mechanism is emphasized. Evidence
is presented for the very early decoupling of the low-momentum Goldstone modes.Comment: 14 LaTeX pages, 5 figures, version published in Phys. Rev.
First performance studies of a prototype for the CASTOR forward calorimeter at the CMS experiment
We present results on the performance of the first prototype of the CASTOR quartz-tungsten sampling calorimeter, to be installed in the very forward region of the CMS experiment at the LHC. This study includes GEANT Monte Carlo simulations of the Cherenkov light transmission efficiency of different types of air-core light guides, as well as analysis of the calorimeter linearity and resolution as a function of energy and impact-point, obtained with 20-200 GeV electron beams from CERN/SPS tests in 2003. Several configurations of the calorimeter have been tested and compared, including different combinations of (i) structures for the active material of the calorimeter (quartz plates and fibres), (ii) various light-guide reflecting materials (glass and foil reflectors) and (iii) photodetector devices (photomultipliers and avalanche photodiodes)
Moving persistence assessments into the 21st century: A role for weight-of-evidence and overall persistence
An improved cosmological bound on the tau-neutrino mass
We consider the influence of non-equilibrium electronic neutrinos (and
anti-neutrinos) on the neutron-to-proton ratio. These neutrinos would come from
massive annihilations . For sufficiently large masses this new effect would strongly
enhance the (n/p)-ratio, leading to a very stringent bound on the
mass, even adopting a rather weak upper bound on the effective number on
neutrino species during nucleosynthesis.Comment: 10 pages, LaTex file + 1 figure compressed using uufile
A Supersymmetric SO(10) Model with Inflation and Cosmic Strings
We have built a supersymmetric SO(10) model consistent with cosmological
observations. The model gives rise to a false vacuum hybrid inflationary
scenario which solves the monopole problem. We argue that this type of
inflationary scenario is generic in supersymmetric SO(10) model, and arises
naturally from the theory. Neither any external field nor any external symmetry
has to be added. It can just be a consequence of the theory. In our specific
model, at the end of inflation, cosmic strings form. The properties of the
strings are presented. The cosmic background radiation anisotropies induced by
the inflationary perturbations and the cosmic strings are estimated. The model
produces a stable lightest superparticle and a very light left-handed neutrino
which may serve as the cold and hot dark matter. The properties of a mixed
cosmic string-inflationary large scale structure formation scenario are
discussed.Comment: 32 pages, uses RevTex. Misprint in a referenc
- …