503 research outputs found
Cosmological parameters estimation in the Quintessence Paradigm
We present cosmological parameter constraints on flat cosmologies dominated
by dark energy using various cosmological data including the recent Archeops
angular power spectrum measurements. A likelihood analysis of the existing
Cosmic Microwave Background data shows that the presence of dark energy is not
requested, in the absence of further prior. This comes from the fact that there
exist degeneracies among the various cosmological parameters constrained by the
Cosmic Microwave Background. We found that there is a degeneracy in a
combination of the Hubble parameter H_0 and of the dark energy equation of
state parameter w_Q, but that w_Q is not correlated with the primordial index n
of scalar fluctuations and the baryon content Omega_b h^2. Preferred primordial
index is n = 0.95 \pm 0.05 (68%) and baryon content Omega_b h^2 = 0.021 \pm
0.003. Adding constraint on the amplitude of matter fluctuations on small
scales, sigma_8, obtained from clusters abundance or weak lensing data may
allow to break the degenaracies, although present-day systematics uncertainties
do not allow firm conclusions yet. The further addition of the Hubble Space
Telescope measurements of the local distance scale and of the high redshift
supernovae data allows to obtain tight constraints. When these constraints are
combined together we find that the amount of dark energy is 0.7^{+0.10}_{-0.07}
(95% C.L.) and that its equation of state is very close to those of the vacuum:
w_Q 95% C.L.). In no case do we find that quintessence is prefered
over the classical cosmological constant, although robust data on sigma_8 might
rapidly bring light on this important issue.Comment: 6 pages, 4 figures, submitted to A&
Constraints on CDM cosmology from galaxy power spectrum, CMB and SNIa evolution
We examine the constraints that can be obtained on standard cold dark matter
models from the most currently used data set: CMB anisotropies, type Ia
supernovae and the SDSS luminous red galaxies. We also examine how these
constraints are widened when the equation of state parameter and the
curvature parameter are left as free parameters. For the
CDM model, our 'vanilla' model, cosmological parameters are tightly
constrained and consistent with current estimates from various methods. When
the dark energy parameter is free we find that the constraints remain
mostly unchanged, i.e. changes are smaller than the 1 sigma uncertainties.
Similarly, relaxing the assumption of a flat universe leads to nearly identical
constraints on the dark energy density parameter of the universe
, baryon density of the universe , the optical
depth , the index of the power spectrum of primordial fluctuations ,
with most one sigma uncertainties better than 5%. More significant changes
appear on other parameters: while preferred values are almost unchanged,
uncertainties for the physical dark matter density , Hubble
constant and are typically twice as large. We found that
different methodological approaches on large scale structure estimates lead to
appreciable differences in preferred values and uncertainty widths. We also
found that possible evolution in SNIa intrinsic luminosity does not alter these
constraints by much, except for , for which the uncertainty is twice as
large. At the same time, this possible evolution is severely constrained. We
conclude that systematic uncertainties for some estimated quantities are
similar or larger than statistical ones.Comment: Revised version, 9 pages, 8 figures, accepted for publication in A&
Test Bench Of The Barrel Calorimeter Modules
A systematic procedure to qualify the barrel calorimeter modules is an essential step to guarantee a 0.7% constant term, which is the collaboration objective. The procedure detailed in this note consists of quality monitoring during mechanical assembling and of a set of electrical tests such as electrical continuity, cell and cross-talk capacitance measurement, and high-voltage behaviour. For the whole test, it has been necessary to develop dedicated electronic boards, to develop measurement methods, and the whole operation software. Making the procedure automatic will guarantee the quality of each module during assembling, cabling, and test in liquid argon
Vector field as a quintessence partner
We derive generic equations for a vector field driving the evolution of flat
homogeneous isotropic universe and give a comparison with a scalar filed
dynamics in the cosmology. Two exact solutions are shown as examples, which can
serve to describe an inflation and a slow falling down of dynamical
``cosmological constant'' like it is given by the scalar quintessence. An
attractive feature of vector field description is a generation of ``induced
mass'' proportional to a Hubble constant, which results in a dynamical
suppression of actual cosmological constant during the evolution.Comment: 14 pages, LaTeX file, iopart class, discussion extended, reference
adde
Jet energy measurement with the ATLAS detector in proton-proton collisions at √s = 7 TeV
The jet energy scale and its systematic uncertainty are determined for jets measured with the ATLAS detector at the LHC in proton-proton collision data at a centre-of-mass energy of √s = 7 TeV corresponding to an integrated luminosity of 38 pb−1. Jets are reconstructed with the anti-kt algorithm with distance parameters R = 0.4 or R = 0.6. Jet energy and angle corrections are determined from Monte Carlo simulations to calibrate jets with transverse momenta pT ≥ 20 GeV and pseudorapidities |η| < 4.5. The jet energy systematic uncertainty is estimated using the single isolated hadron response measured in situ and in test-beams, exploiting the transverse momentum balance between central and forward jets in events with dijet topologies and studying systematic variations in Monte Carlo simulations. The jet energy uncertainty is less than 2.5 % in the central calorimeter region (|η| < 0.8) for jets with 60 ≤ pT < 800 GeV, and is maximally 14 % for pT < 30 GeV in the most forward region 3.2 ≤ |η| < 4.5. The jet energy is validated for jet transverse momenta up to 1 TeV to the level of a few percent using several in situ techniques by comparing a well-known reference such as the recoiling photon pT, the sum of the transverse momenta of tracks associated to the jet, or a system of low-pT jets recoiling against a high-pT jet. More sophisticated jet calibration schemes are presented based on calorimeter cell energy density weighting or hadronic properties of jets, aiming for an improved jet energy resolution and a reduced flavour dependence of the jet response. The systematic uncertainty of the jet energy determined from a combination of in situ techniques is consistent with the one derived from single hadron response measurements over a wide kinematic range. The nominal corrections and uncertainties are derived for isolated jets in an inclusive sample of high-pT jets. Special cases such as event topologies with close-by jets, or selections of samples with an enhanced content of jets originating e-mail: [email protected] from light quarks, heavy quarks or gluons are also discussed and the corresponding uncertainties are determined.Fil: Aad, G.. Albert Ludwigs Universität; AlemaniaFil: Abbott, B.. University of Oklahoma; Estados UnidosFil: Abdallah, J.. Universitat Autònoma de Barcelona; EspañaFil: Abdelalim, A. A.. Universidad de Ginebra; SuizaFil: Abdesselam, A.. University of Oxford; Reino UnidoFil: Anduaga, Xabier Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: González Silva, María Laura. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Monticelli, Fernando Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Otero y Garzon, Gustavo Javier. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Piegaia, Ricardo Nestor. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Romeo, Gaston Leonardo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Tripiana, Martin Fernando. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Zhuang, X.. Ludwig Maximilians Universitat; AlemaniaFil: Zhuravlov, V.. Max-Planck Institut für Physik; AlemaniaFil: Zieminska, D.. Indiana University; Estados UnidosFil: Zimmermann, R.. Universitaet Bonn; AlemaniaFil: Zimmermann, S.. Universitaet Bonn; AlemaniaFil: Zimmermann, S.. Albert Ludwigs Universität; AlemaniaFil: Zinonos, Z.. Università degli Studi di Pisa; ItaliaFil: Ziolkowski, M.. Universität Siegen; AlemaniaFil: Zitoun, R.. Université de Savoie; FranciaFil: Živković, L.. Columbia University; Estados UnidosFil: Zmouchko, V. V.. State Research Center Institute for High Energy Physics; RusiaFil: Zobernig, G.. University of Wisconsin; Estados UnidosFil: Zoccoli, A.. Università di Bologna; ItaliaFil: Zolnierowski, Y.. Université de Savoie; FranciaFil: Zsenei, A.. Cern - European Organization For Nuclear Research; SuizaFil: zur Nedden, M.. Humboldt University; AlemaniaFil: Zutshi, V.. Northern Illinois University; Estados UnidosFil: Zwalinski, L.. Cern - European Organization For Nuclear Research; Suiz
Shrinking a large dataset to identify variables associated with increased risk of Plasmodium falciparum infection in Western Kenya
Large datasets are often not amenable to analysis using traditional single-step approaches. Here, our general objective was to apply imputation techniques, principal component analysis (PCA), elastic net and generalized linear models to a large dataset in a systematic approach to extract the most meaningful predictors for a health outcome. We extracted predictors for Plasmodium falciparum infection, from a large covariate dataset while facing limited numbers of observations, using data from the People, Animals, and their Zoonoses (PAZ) project to demonstrate these techniques: data collected from 415 homesteads in western Kenya, contained over 1500 variables that describe the health, environment, and social factors of the humans, livestock, and the homesteads in which they reside. The wide, sparse dataset was simplified to 42 predictors of P. falciparum malaria infection and wealth rankings were produced for all homesteads. The 42 predictors make biological sense and are supported by previous studies. This systematic data-mining approach we used would make many large datasets more manageable and informative for decision-making processes and health policy prioritization
Constraints on dark energy evolution
We investigate a class of dark energy models in which the equation of state
undergoes a rapid transition and for which the Hubble SN Ia diagram is known to
be poorly discriminant. Interestingly enough, we find that transitions at high
redshift can lead to distortion in the correlation function of dark matter at
lower redshift. We therefore use a combination of the SN Ia Hubble diagram,
Cosmic Microwave Background data and power spectrum from the Sloan Digital Sky
Survey Luminous Red Galaxies (SDSS LRG) to constrain the redshift of a possible
transition. We find that the fundamental cosmological parameters are well
constrained independently of the presence of a transition. Acceptable
transitions from an equation of state close to to a value close to -1
are strongly rejected at redshifts much higher than those for which Large Scale
Structure and SN Ia data are available: the transition redshift can be rejected
up to a value as high as 10. We conclude that no preference for a transition
appears from present-day data.Comment: 11 pages, 9 figures, final version, accepted for publication n A&
Study of CP violation in Dalitz-plot analyses of B0 --> K+K-KS, B+ --> K+K-K+, and B+ --> KSKSK+
We perform amplitude analyses of the decays , , and , and measure CP-violating
parameters and partial branching fractions. The results are based on a data
sample of approximately decays, collected with the
BABAR detector at the PEP-II asymmetric-energy factory at the SLAC National
Accelerator Laboratory. For , we find a direct CP asymmetry
in of , which differs
from zero by . For , we measure the
CP-violating phase .
For , we measure an overall direct CP asymmetry of
. We also perform an angular-moment analysis of
the three channels, and determine that the state can be described
well by the sum of the resonances , , and
.Comment: 35 pages, 68 postscript figures. v3 - minor modifications to agree
with published versio
Studying the Underlying Event in Drell-Yan and High Transverse Momentum Jet Production at the Tevatron
We study the underlying event in proton-antiproton collisions by examining
the behavior of charged particles (transverse momentum pT > 0.5 GeV/c,
pseudorapidity |\eta| < 1) produced in association with large transverse
momentum jets (~2.2 fb-1) or with Drell-Yan lepton-pairs (~2.7 fb-1) in the
Z-boson mass region (70 < M(pair) < 110 GeV/c2) as measured by CDF at 1.96 TeV
center-of-mass energy. We use the direction of the lepton-pair (in Drell-Yan
production) or the leading jet (in high-pT jet production) in each event to
define three regions of \eta-\phi space; toward, away, and transverse, where
\phi is the azimuthal scattering angle. For Drell-Yan production (excluding the
leptons) both the toward and transverse regions are very sensitive to the
underlying event. In high-pT jet production the transverse region is very
sensitive to the underlying event and is separated into a MAX and MIN
transverse region, which helps separate the hard component (initial and
final-state radiation) from the beam-beam remnant and multiple parton
interaction components of the scattering. The data are corrected to the
particle level to remove detector effects and are then compared with several
QCD Monte-Carlo models. The goal of this analysis is to provide data that can
be used to test and improve the QCD Monte-Carlo models of the underlying event
that are used to simulate hadron-hadron collisions.Comment: Submitted to Phys.Rev.
Measurement of the Production Cross Section and Search for Anomalous and Couplings in Collisions at TeV
This Letter describes the current most precise measurement of the boson
pair production cross section and most sensitive test of anomalous
and couplings in collisions at a center-of-mass energy of 1.96
TeV. The candidates are reconstructed from decays containing two charged
leptons and two neutrinos, where the charged leptons are either electrons or
muons. Using data collected by the CDF II detector from 3.6 fb of
integrated luminosity, a total of 654 candidate events are observed with an
expected background contribution of events. The measured total
cross section is pb, which is in good agreement
with the standard model prediction. The same data sample is used to place
constraints on anomalous and couplings.Comment: submitted to Phys. Rev. Let
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