7,125 research outputs found
Future supernovae data and quintessence models
The possibility to unambiguously determine the equation-of-state of the
cosmic dark energy with existing and future supernovae data is investigated. We
consider four evolution laws for this equation-of-state corresponding to four
quintessential models, i.e. i) a cosmological constant, ii) a general
barotropic fluid, iii) a perfect fluid with a linear equation-of-state and iv)
a more physical model based on a pseudo-Nambu-Goldstone boson field. We
explicitly show the degeneracies present not only within each model but also
between the different models : they are caused by the multi-integral relation
between the equation-of-state of dark energy and the luminosity distance.
Present supernova observations are analysed using a standard method
and the minimal values obtained for each model are compared. We
confirm the difficulty to discriminate between these models using present SNeIa
data only. By means of simulations, we then show that future SNAP observations
will not remove all the degeneracies. For example, wrong estimations of
with a good value of could be found if the right
cosmological model is not used to fit the data. We finally give some
probabilities to obtain unambiguous results, free from degeneracies. In
particular, the probability to confuse a cosmological constant with a true
barotropic fluid with an equation-of-state different from -1 is shown to be 95%
at a level.Comment: 12 pages. This improved version has been accepted for publication in
M.N.R.A.
Production of trans-Neptunian binaries through chaos-assisted capture
The recent discovery of binary objects in the Kuiper-belt opens an invaluable
window into past and present conditions in the trans-Neptunian part of the
Solar System. For example, knowledge of how these objects formed can be used to
impose constraints on planetary formation theories. We have recently proposed a
binary-object formation model based on the notion of chaos-assisted capture.
Here we present a more detailed analysis with calculations performed in the
spatial (three-dimensional) three- and four-body Hill approximations. It is
assumed that the potential binary partners are initially following heliocentric
Keplerian orbits and that their relative motion becomes perturbed as these
objects undergo close encounters. First, the mass, velocity, and orbital
element distribu- tions which favour binary formation are identified in the
circular and elliptical Hill limits. We then consider intruder scattering in
the circular Hill four-body problem and find that the chaos-assisted capture
mechanism is consistent with observed, apparently randomly distributed, binary
mutual orbit inclinations. It also predicts asymmetric distributions of
retrograde versus prograde orbits. The time-delay induced by chaos on particle
transport through the Hill sphere is analogous to the formation of a resonance
in a chemical reaction. Implications for binary formation rates are considered
and the 'fine-tuning' problem recently identified by Noll et al. (2007) is also
addressed.Comment: submitted to MNRA
On the dynamics of a collapsing bubble in contact with a rigid wall
This work reveals that the dynamic response of a spherical cap bubble in
contact with a rigid wall depends on the effective contact angle at the instant
prior to collapse. This parameter allows us to discriminate between two regimes
in which the mechanisms of interaction between the collapsing bubble and its
surrounding medium differ significantly: When the contact angle is smaller than
90 degrees a classical jet directed towards the wall is observed whereas if the
initial contact angle is larger than 90 degrees an annular re-entrant jet
parallel to the wall appears. We show that this change of the behaviour can be
explained using the impulse potential flow theory for small times which shows
the presence of a singularity on the initial acceleration of the contact line
when the contact angle is larger then 90 degrees. Direct Numerical Simulations
show that although viscosity regularises the solution at , the solution
remains singular at . In these circumstances numerical and experimental
results show that the collapse of flat bubbles can eventually lead to the
formation of a vortex ring that unexpectedly induces long-range effects. The
role of the bubble geometry at the instant of maximum expansion on the overall
collapse process is shown to be well captured by the impulse potential flow
theory, which can be easily generalised to other bubble shapes. These results
may find direct application in the interpretation of geophysical flows as well
as the control and design of bio-medical, naval, manufacturing and
sonochemistry applications
Metallic phase in stoichiometric CeOBiS 2 revealed by space-resolved ARPES
Recently CeOBiS2 system without any fluorine doping is found to show superconductivity posing question on its origin. Using space resolved ARPES we have found a metallic phase embedded in the morphological defects and at the sample edges of stoichiometric CeOBiS2. While bulk of the sample is semiconducting, the embedded metallic phase is characterized by the usual electron pocket at X point, similar to the Fermi surface of doped BiS2-based superconductors. Typical size of the observed metallic domain is larger than the superconducting correlation length of the system suggesting that the observed superconductivity in undoped CeOBiS2 might be due to this embedded metallic phase at the defects. The results also suggest a possible way to develop new systems by manipulation of the defects in these chalcogenides with structural instability
Nonlocal regularization of abelian models with spontaneous symmetry breaking
We demonstrate how nonlocal regularization is applied to gauge invariant
models with spontaneous symmetry breaking. Motivated by the ability to find a
nonlocal BRST invariance that leads to the decoupling of longitudinal gauge
bosons from physical amplitudes, we show that the original formulation of the
method leads to a nontrivial relationship between the nonlocal form factors
that can appear in the model.Comment: 11 pages, uses amsart. To appear in Mod. Phys. Lett
Bi-layer splitting in overdoped high cuprates
Recent angle-resolved photoemission data for overdoped Bi2212 are explained.
Of the peak-dip-hump structure, the peak corresponds the component
of a hole condensate which appears at . The fluctuating part of this same
condensate produces the hump. The bilayer splitting is large enough to produce
a bonding hole and an electron antibonding quasiparticle Fermi surface. Smaller
bilayer splittings observed in some experiments reflect the interaction of the
peak structure with quasiparticle states near, but not at, the Fermi surface.Comment: 4 pages with 2 figures - published versio
Cosmological scalar fields that mimic the cosmological model
We look for cosmologies with a scalar field (dark energy without cosmological
constant), which mimic the standard cosmological model yielding
exactly the same large-scale geometry described by the evolution of the Hubble
parameter (i.e. photometric distance and angular diameter distance as functions
on ). Asymptotic behavior of the field solutions is studied in the case of
spatially flat Universe with pressureless matter and separable scalar field
Lagrangians (power-law kinetic term + power-law potential). Exact analytic
solutions are found in some special cases. A number of models have the field
solutions with infinite behavior in the past or even singular behavior at
finite redshifts. We point out that introduction of the cosmological scalar
field involves some degeneracy leading to lower precision in determination of
. To remove this degeneracy additional information is needed beyond
the data on large-scale geometry.Comment: VIII International Conference "Relativistic Astrophysics, Gravitation
and Cosmology": May 21-23, 2008, Kyiv, Ukrain
An 8 GEV Linac As The Booster Replacement In The Fermilab Power Upgrade
Increasing the Fermilab Main Injector (MI) beam power above ~1.2 MW requires
replacement of the 8 GeV Booster by a higher intensity alternative. Earlier,
rapid-cycling synchrotron and linac solutions were considered for this purpose.
In this paper, we consider the linac version that produces 8 GeV H- beam for
injection into the Recycler Ring (RR) or MI The new linac takes ~1 GeV beam
from the PIP-II linac and accelerates it to ~ 2 GeV in a 650 MHz SRF linac, and
then accelerates to ~8 GeV in an SRF pulsed linac using 1300 MHz cryomodules.
The linac components incorporate recent improvements in SRF technology. This
Booster Replacement linac (BRL) will increase MI beam power to DUNE to more
than 2.5 MW and enable next-generation intensity frontier experiments.Comment: arXiv admin note: text overlap with arXiv:2203.0505
Density functional electronic spectrum of the cluster and possible local Jahn-Teller distorsions in the La-Ba-Cu-O superconductor
We present a density functional theory (DFT) calculation in the generalized
gradient approximation to study the possibility for the existence of
Jahn-Teller (JT) or pseudo Jahn-Teller (PJT) type local distortions in the
La-Ba-Cu-O superconducting system. We performed the calculation and
correspondingly group theory classification of the electronic ground state of
the CuO elongated octahedra cluster, immersed in a background
simulating the superconductor. Part of the motivation to do this study is that
the origin of the apical deformation of the CuO cluster is not
due to a pure JT effect, having therefore a non {\it a priori} condition to
remove the degeneracy of the electronic ground state of the parent regular
octahedron. We present a comparative analysis of the symmetry classified
electron spectrum with previously reported results using unrestricted
Hartree-Fock calculations (UHF). Both the DFT and UHF calculations produced a
non degenerate electronic ground state, not having therefore the necessary
condition for a pure JT effect. However, the appearance of a degenerate E
state near to the highest occupied molecular orbital in the DFT calculation,
suggests the possibility for a PJT effect responsible for a local distortion of
the oxidized CuO cluster.Comment: 12 pages, 3 figures, submitted to International Journal of Modern
Physics B (IJMPB
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