Search results for "dark energy"

showing 9 items of 89 documents

The virial theorem and the dark matter problem in hybrid metric-Palatini gravity

2012

Hybrid metric-Palatini gravity is a recently proposed theory, consisting of the superposition of the metric Einstein-Hilbert Lagrangian with an f(R) term constructed a la Palatini. The theory predicts the existence of a long-range scalar field, which passes the Solar System observational constraints, even if the scalar field is very light, and modifies the cosmological and galactic dynamics. Thus, the theory opens new possibilities to approach, in the same theoretical framework, the problems of both dark energy and dark matter. In this work, we consider the generalized virial theorem in the scalar-tensor representation of the hybrid metric-Palatini gravity. More specifically, taking into ac…

Physicsdark matter theory010308 nuclear & particles physicsDark matterVelocity dispersionFOS: Physical sciencesAstronomy and AstrophysicsVirial massAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesPotential energyGeneral Relativity and Quantum CosmologyVirial theoremTheoretical physicsGeneral Relativity and Quantum CosmologyPhysics - General PhysicsGeneral Physics (physics.gen-ph)Gravitational field0103 physical sciencesDark energygalaxy clusters010303 astronomy & astrophysicsScalar fieldmodified gravity
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Large-scale inhomogeneities may improve the cosmic concordance of supernovae

2010

We reanalyze the supernovae data from the Union Compilation including the weak lensing effects caused by inhomogeneities. We compute the lensing probability distribution function for each background solution described by the parameters Omega_M, Omega_L and w in the presence of inhomogeneities, approximately modeled with a single-mass population of halos. We then perform a likelihood analysis in the space of FLRW-parameters and compare our results with the standard approach. We find that the inclusion of lensing can move the best-fit model significantly towards the cosmic concordance of the flat LCDM model, improving the agreement with the constraints coming from the cosmic microwave backgro…

Physicseducation.field_of_studyCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundPopulationDark matterGeneral Physics and AstronomyFOS: Physical sciencesLambda-CDM modelAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyObservational cosmology0103 physical sciencesDark energyBaryon acoustic oscillationseducation010303 astronomy & astrophysicsWeak gravitational lensingAstrophysics - Cosmology and Nongalactic Astrophysics
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Euclid preparation - XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields

2022

Artículo escrito por un elevado núnmero de autores, sólo se referencian el qque aparece en primer lugar, los autores pertenecientes a la UAM y el nombre del grupo de colaboración, si lo hubiere

SAMPLELarge-scale structure of UniverseDATA RELEASEFormationSurveysobservations Dark energy Dark matter Galaxy: formation Large-scale structure of Universe Surveys [Cosmology]kosmologiaAstrophysicsCosmology: observationdark mattergalaksijoukotpimeä ainesurveysDark energyDark matterobservations [Cosmology]dark energyObservationsLEGACY SURVEYAstrophysics of GalaxiesFísicaAstronomy and Astrophysics115 Astronomy Space scienceEVOLUTIONCosmologygalaksitGALAXIESCosmology: observations; Dark energy; Dark matter; Galaxy: formation; Large-scale structure of Universe; SurveysGalaxyformation [Galaxy]Space and Planetary ScienceGalaxy: formationcosmology: observationslarge-scale structure of Universepimeä energiaCosmology and Nongalactic Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Observational constraints on inhomogeneous cosmological models without dark energy

2011

It has been proposed that the observed dark energy can be explained away by the effect of large-scale nonlinear inhomogeneities. In the present paper we discuss how observations constrain cosmological models featuring large voids. We start by considering Copernican models, in which the observer is not occupying a special position and homogeneity is preserved on a very large scale. We show how these models, at least in their current realizations, are constrained to give small, but perhaps not negligible in certain contexts, corrections to the cosmological observables. We then examine non-Copernican models, in which the observer is close to the center of a very large void. These models can gi…

Void (astronomy)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physics0103 physical sciencesHomogeneity (physics)98.62.Sb010303 astronomy & astrophysicsPhysics010308 nuclear & particles physics98.80.EsObservable95.36.+xCopernican principleNonlinear systemDark energysymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]98.65.DxAstrophysics - Cosmology and Nongalactic AstrophysicsSpecial position
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Euclid preparation : XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography

2021

The analysis of weak gravitational lensing in wide-field imaging surveys is considered to be a major cosmological probe of dark energy. Our capacity to constrain the dark energy equation of state relies on an accurate knowledge of the galaxy mean redshift ⟨z⟩. We investigate the possibility of measuring ⟨z⟩ with an accuracy better than 0.002 (1 + z) in ten tomographic bins spanning the redshift interval 0.2  99.8%. The zPDF approach can also be successful if the zPDF is de-biased using a spectroscopic training sample. This approach requires deep imaging data but is weakly sensitive to spectroscopic redshift failures in the training sample. We improve the de-biasing method and confirm our fi…

galaksijoukotgalaksitstatistical [methods]distances and redshifts [galaxies]Astrophysics::Cosmology and Extragalactic Astrophysicsdark energypimeä energiakosmologia
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Review of Particle Physics

2020

The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, …

high energyleptonmixing [neutrino]High Energy Physics::LatticeCosmic microwave backgrounddiffractionTechnicolorAstrophysicsOmega01 natural sciencesPhysics Particles & Fieldshiggs-boson productionBig Bang nucleosynthesiscosmological model: parameter spacetaudark energyMonte CarlofieldspentaquarkinstrumentationSettore FIS/01gauge bosonAnomalous magnetic dipole momentdeep-inelastic scatteringnew physicsPhysicsDOUBLE-BETA-DECAYElectroweak interactiondensity [dark matter]HEAVY FLAVOURQuarkoniumreview; particle; physicsSUPERSYMMETRIC STANDARD MODELsquare-root-sPhysics Nucleargrand unified theoryboson: heavystatisticsPhysical SciencesHiggs bosonaxion: massflavor: violationNeutrinoELECTROWEAK SYMMETRY-BREAKINGnumerical calculations: Monte Carlophysicson-lineS013EPHQuarkheavy [boson]particle[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Physics Multidisciplinaryanomalous magnetic-momentelectroweak radiative-correctionsdark matter: densityHiggs particlemesonneutrino masses neutrino mixing; neutrino oscillations114 Physical sciencesCHIRAL PERTURBATION-THEORYneutrino mixingStandard Modelquark0202 Atomic Molecular Nuclear Particle And Plasma PhysicsNucleosynthesisquantum chromodynamicsCP: violationDark matterddc:530particle physicsStrong Interactions010306 general physicssparticleS013DFgrand unified theoriesPRODUCTIONGauge bosonScience & Technologyneutrino oscillationsneutrino masses010308 nuclear & particles physicsC50 Other topics in experimental particle physicsParticle Data GroupAstronomy and AstrophysicsDeep inelastic scatteringto-leading-order* Automatic Keywords *heavy bosonaxiontables (particle physics)Tetraquarkproton-proton collisionsSupersymmetryhadronneutrino: mixing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyVolume (compression)HIGGS-BOSONUB-VERTICAL-BARcosmological modeldark energy densityexperimental methodsddc:539.72021Physics beyond the Standard Modelstandard modelgroup theoryGeneral Physics and Astronomytables particle physicshigh energy physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamicsPhysicsenergy: highE Rev 2016[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Settore FIS/01 - Fisica SperimentalephotonSupersymmetryNuclear & Particles Physicsparameter space [cosmological model]dark energy: densityhigh [energy]M013WXfermion-pair productionNuclear and High Energy PhysicsParticle physicsHiggs bosonreviewAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics530dark matterstatistical analysisDouble beta decay0103 physical sciencesconservation lawcold dark-matterTAU LEPTONSAstrophysics::Galaxy AstrophysicstablesDEEP-INELASTIC-SCATTERINGelectroweak interactionHigh Energy Physics::Phenomenology750 GeV diphoton excessPRODUCTION CROSS-SECTIONbaryondensity [dark energy]Physics and AstronomygravitationCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentsupersymmetryMinimal Supersymmetric Standard Model
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Euclid preparation. XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses

2021

Pocino, A., et al. (Euclid Collaboration)

luminous red galaxiesCosmological parameterAstrophysicsSurveys01 natural sciencesCosmologytechniques: photometricgalaxiesGalaxies: distances and redshiftdistances and redshiftsSurvey010303 astronomy & astrophysicsWeak gravitational lensingPhysicsRedshift surveylsstastro-ph.COgalaxies: distances and redshiftsconstraintsAstrophysics - Cosmology and Nongalactic Astrophysicsredshift surveyCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmological parametersFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsphotometricSettore FIS/05 - Astronomia e Astrofisicasurveys0103 physical sciencesdistances and redshifts [Galaxies]cosmological parametersSpurious relationshipCluster analysisdark energy surveyAstrophysics::Galaxy Astrophysics010308 nuclear & particles physicsphotometric [Techniques]Astronomy and Astrophysicsspace115 Astronomy Space scienceRedshiftGalaxySpace and Planetary ScienceCosmological parameters; Galaxies: distances and redshifts; Surveys; Techniques: photometrictechniquesFocus (optics)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologycosmic shearintrinsic alignments
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Shell-model computed cross sections for charged-current scattering of astrophysical neutrinos off 40Ar

2018

Charged-current (anti)neutrino-$^{40}\mathrm{Ar}$ cross sections for astrophysical neutrinos have been calculated. The initial and final nuclear states were calculated using the nuclear shell model. The folded solar-neutrino scattering cross section was found to be $1.78(23)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}42}\phantom{\rule{4pt}{0ex}}{\mathrm{cm}}^{2}$, which is higher than what the previous papers have reported. The contributions from the ${1}^{\ensuremath{-}}$ and ${2}^{\ensuremath{-}}$ multipoles were found to be significant at supernova-neutrino energies, confirming the random-phase approximation (RPA) result of a previous study. The effects of neutrino flavor conve…

solar radiationSHELL model01 natural sciencesdark matternucleus-neutrino interactionsNuclear physicspimeä aineCross section (physics)0103 physical sciences010306 general physicsauringonsäteilydark energyCharged currentPhysicsta114010308 nuclear & particles physicsScatteringNuclear shell modelneutriinotshell modelneutrinosDistribution (mathematics)solar neutrinosHigh Energy Physics::ExperimentNeutrinopimeä energiaParametrizationPhysical Review C
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Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography

2021

Ilbert, O., et al. (Euclid Collaboration)

statistical [Methods]IMPACTUNIVERSEAstrophysics01 natural sciencesDark energyGalaxies: distances and redshiftdark energyPHOTOMETRIC REDSHIFTS010303 astronomy & astrophysicsWeak gravitational lensingPhotometric redshiftmedia_commonPhysicsdistances and redshift [Galaxies]Dark energy; Galaxies: distances and redshifts; Methods: statisticalSIMULATIONastro-ph.CO3103 Astronomy and AstrophysicsProbability distributionSpectral energy distributiongalaxies: distances and redshiftsAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)530 Physicsastro-ph.GAmedia_common.quotation_subjectFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics1912 Space and Planetary Science0103 physical sciencesdistances and redshifts [Galaxies]/dk/atira/pure/subjectarea/asjc/1900/1912DISTRIBUTIONSmethods: statistical010308 nuclear & particles physicsAstronomy and AstrophysicsPERFORMANCE115 Astronomy Space scienceAstrophysics - Astrophysics of GalaxiesEVOLUTIONGalaxyUniverseRedshiftSTELLARRESOLUTIONSpace and Planetary Science10231 Institute for Computational ScienceAstrophysics of Galaxies (astro-ph.GA)Dark energy/dk/atira/pure/subjectarea/asjc/3100/3103[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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