204 research outputs found
Charge conservation and time-varying speed of light
It has been recently claimed that cosmologies with time dependent speed of
light might solve some of the problems of the standard cosmological scenario,
as well as inflationary scenarios. In this letter we show that most of these
models, when analyzed in a consistent way, lead to large violations of charge
conservation. Thus, they are severly constrained by experiment, including those
where is a power of the scale factor and those whose source term is the
trace of the energy-momentum tensor. In addition, early Universe scenarios with
a sudden change of related to baryogenesis are discarded.Comment: 4 page
Illusions of general relativity in Brans-Dicke gravity
Contrary to common belief, the standard tenet of Brans-Dicke theory reducing
to general relativity when omega tends to infinity is false if the trace of the
matter energy-momentum tensor vanishes. The issue is clarified in a new
approach using conformal transformations. The otherwise unaccountable limiting
behavior of Brans-Dicke gravity is easily understood in terms of the conformal
invariance of the theory when the sources of gravity have radiation-like
properties. The rigorous computation of the asymptotic behavior of the
Brans-Dicke scalar field is straightforward in this new approach.Comment: 16 pages, LaTeX, to appear in Physical Review
STATIONARY SOLUTIONS IN BRANS-DICKE STOCHASTIC INFLATIONARY COSMOLOGY
In Brans-Dicke theory the Universe becomes divided after inflation into many
exponentially large domains with different values of the effective
gravitational constant. Such a process can be described by diffusion equations
for the probability of finding a certain value of the inflaton and dilaton
fields in a physical volume of the Universe. For a typical chaotic inflation
potential, the solutions for the probability distribution never become
stationary but grow forever towards larger values of the fields. We show here
that a non-minimal conformal coupling of the inflaton to the curvature scalar,
as well as radiative corrections to the effective potential, may provide a
dynamical cutoff and generate stationary solutions. We also analyze the
possibility of large nonperturbative jumps of the fluctuating inflaton scalar
field, which was recently revealed in the context of the Einstein theory. We
find that in the Brans--Dicke theory the amplitude of such jumps is strongly
suppressed.Comment: 19 pages, LaTe
The scientific potential of space-based gravitational wave detectors
The millihertz gravitational wave band can only be accessed with a
space-based interferometer, but it is one of the richest in potential sources.
Observations in this band have amazing scientific potential. The mergers
between massive black holes with mass in the range 10 thousand to 10 million
solar masses, which are expected to occur following the mergers of their host
galaxies, produce strong millihertz gravitational radiation. Observations of
these systems will trace the hierarchical assembly of structure in the Universe
in a mass range that is very difficult to probe electromagnetically. Stellar
mass compact objects falling into such black holes in the centres of galaxies
generate detectable gravitational radiation for several years prior to the
final plunge and merger with the central black hole. Measurements of these
systems offer an unprecedented opportunity to probe the predictions of general
relativity in the strong-field and dynamical regime. Millihertz gravitational
waves are also generated by millions of ultra-compact binaries in the Milky
Way, providing a new way to probe galactic stellar populations. ESA has
recognised this great scientific potential by selecting The Gravitational
Universe as its theme for the L3 large satellite mission, scheduled for launch
in ~2034. In this article we will review the likely sources for millihertz
gravitational wave detectors and describe the wide applications that
observations of these sources could have for astrophysics, cosmology and
fundamental physics.Comment: 18 pages, 2 figures, contribution to Gravitational Wave Astrophysics,
the proceedings of the 2014 Sant Cugat Forum on Astrophysics; v2 includes one
additional referenc
Ready-to-use food supplement, with or without arginine and citrulline, with daily chloroquine in Tanzanian children with sickle-cell disease: a double-blind, random order crossover trial
Background: Sickle cell disease increases malnutrition risk. Low arginine and nitric oxide [NO] bioavailability are implicated in sickle-related morbidity. Simple interventions are required, especially in low-income settings. We aimed to test the hypotheses: (1) supplementary arginine, citrulline and daily chloroquine increases bioavailable arginine and flow-mediated-dilatation (FMDmax%; a measure of NO-dependent endothelial function), and (2); protein energy supplementation in the form of ready-to-use supplementary-food (RUSF) improves nutritional status in children with sickle cell disease.
Methods: A random-order, double-blind, cross-over trial with two four-month intervention periods (each followed by four-months wash-out) was conducted in Dar-es-Salaam, Tanzania. 119 children aged 8-12 years, naïve to hydroxyurea, were enrolled from the Muhimbili National Hospital Sickle Cohort. The random order sequence and allocation codes were generated centrally. Two formulations of RUSF (500kcal/day) were tested: ‘basic’ with weekly chloroquine (150/225mg base, depending on weight) (RUSF-b) and ‘vascular’ (RUSF-v) fortified with arginine, citrulline designed to achieve mean intakes of 0.2g/0.1g/kg/day and daily chloroquine (max 3mg base/kg/day). The primary outcomes of the comparison of the 2 RUSF formulations were mean FMDmax%, mean plasma arginine to ornithine ratio and mean plasma arginine to asymmetric-di-methylated-arginine (ADMA) ratio. The primary outcomes of the combined effect of both RUSF interventions were mean height and body mass index for age z-scores with analysis by intention to treat. Trial registration: ISRCTN74331412
Findings: 114/119 children had complete data for all reported endpoints. There was no treatment effect of RUSF-v compared to RUSF-b on the ratio of arginine to ornithine (mean within individual difference -0.09, 95% CI -0.03/0.2, p=0.12), or on FMDmax% (-1.00 95% CI -2.47/0.47, p=0.18) but the arginine:ADMA ratio was significantly increased (-0.56, 95% CI -0.81/-0.31, P<0.001). In planned analyses using random effects models to estimate the effect of each intervention compared to baseline/washout, the arginine:ADMA ratio increased following both RUSF-v or RUSF-b (+86%, p<0.001; +41%, p<0.001). Similarly, FMDmax% was higher after
2
RUSF-v (+0.92, p<0.001) but not after RUSF-b intervention (+0.39, p=0.22). Adjusted for covariates, effect estimates for FMDmax% increased: RUSF-v (+1.19, p<0.001) and RUSF-b (+0.93, p=0.008). Following either intervention (RUSF-b and RUSF-v pooled) compared to baseline/wash-outs, body-mass-index-z-score (+0.091, P=0.001) and height-for-age-z-score (+0.013, P=0.081) increased. There were 71 and 81 adverse events of which 21 and 26 were serious during intervention and washout (P=0.31) in 83 participants, 1 of whom died in the 2nd washout period.
Interpretation: RUSF providing 500kcal/day results in small weight gains in children with sickle cell disease. However, RUSF even without arginine and citrulline fortification improves arginine dysregulation and may improve endothelial function. Long-term studies are required to assess if these physiological effects translate to improved clinical outcomes and better growth and development in sickle cell disease
Naked Singularity Formation In f(R) Gravity
We study the gravitational collapse of a star with barotropic equation of
state in the context of theories of gravity.
Utilizing the metric formalism, we rewrite the field equations as those of
Brans-Dicke theory with vanishing coupling parameter. By choosing the
functionality of Ricci scalar as , we
show that for an appropriate initial value of the energy density, if
and satisfy certain conditions, the resulting singularity would be naked,
violating the cosmic censorship conjecture. These conditions are the ratio of
the mass function to the area radius of the collapsing ball, negativity of the
effective pressure, and the time behavior of the Kretschmann scalar. Also, as
long as parameter obeys certain conditions, the satisfaction of the
weak energy condition is guaranteed by the collapsing configuration.Comment: 15 pages, 4 figures, to appear in GR
Categorizing Different Approaches to the Cosmological Constant Problem
We have found that proposals addressing the old cosmological constant problem
come in various categories. The aim of this paper is to identify as many
different, credible mechanisms as possible and to provide them with a code for
future reference. We find that they all can be classified into five different
schemes of which we indicate the advantages and drawbacks.
Besides, we add a new approach based on a symmetry principle mapping real to
imaginary spacetime.Comment: updated version, accepted for publicatio
Light propagation in statistically homogeneous and isotropic universes with general matter content
We derive the relationship of the redshift and the angular diameter distance
to the average expansion rate for universes which are statistically homogeneous
and isotropic and where the distribution evolves slowly, but which have
otherwise arbitrary geometry and matter content. The relevant average expansion
rate is selected by the observable redshift and the assumed symmetry properties
of the spacetime. We show why light deflection and shear remain small. We write
down the evolution equations for the average expansion rate and discuss the
validity of the dust approximation.Comment: 42 pages, no figures. v2: Corrected one detail about the angular
diameter distance and two typos. No change in result
The exposure of the hybrid detector of the Pierre Auger Observatory
The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays.
It consists of a surface array to measure secondary particles at ground level
and a fluorescence detector to measure the development of air showers in the
atmosphere above the array. The "hybrid" detection mode combines the
information from the two subsystems. We describe the determination of the
hybrid exposure for events observed by the fluorescence telescopes in
coincidence with at least one water-Cherenkov detector of the surface array. A
detailed knowledge of the time dependence of the detection operations is
crucial for an accurate evaluation of the exposure. We discuss the relevance of
monitoring data collected during operations, such as the status of the
fluorescence detector, background light and atmospheric conditions, that are
used in both simulation and reconstruction.Comment: Paper accepted by Astroparticle Physic
Search for direct production of charginos and neutralinos in events with three leptons and missing transverse momentum in √s = 7 TeV pp collisions with the ATLAS detector
A search for the direct production of charginos and neutralinos in final states with three electrons or muons and missing transverse momentum is presented. The analysis is based on 4.7 fb−1 of proton–proton collision data delivered by the Large Hadron Collider and recorded with the ATLAS detector. Observations are consistent with Standard Model expectations in three signal regions that are either depleted or enriched in Z-boson decays. Upper limits at 95% confidence level are set in R-parity conserving phenomenological minimal supersymmetric models and in simplified models, significantly extending previous results
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