Search results for "Hub"

showing 10 items of 207 documents

Cosmological parameters degeneracies and non-Gaussian halo bias

2010

We study the impact of the cosmological parameters uncertainties on the measurements of primordial non-Gaussianity through the large-scale non-Gaussian halo bias effect. While this is not expected to be an issue for the standard Lambda CDM model, it may not be the case for more general models that modify the large-scale shape of the power spectrum. We consider the so-called local non-Gaussianity model, parametrized by the f(NL) non-Gaussianity parameter which is zero for a Gaussian case, and make forecasts on f(NL) from planned surveys, alone and combined with a Planck CMB prior. In particular, we consider EUCLID- and LSST-like surveys and forecast the correlations among f(NL) and the runni…

AstrofísicaCúmuls de galàxiesParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundFOS: Physical sciencesGalaxy clustersAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesPower spectrumsymbols.namesake0103 physical sciencesPlanck010303 astronomy & astrophysicsRedshift surveysPhysicsSpectral indexCosmological parameters from LSSCosmologiaClusters of galaxies010308 nuclear & particles physicsEquation of state (cosmology)Order (ring theory)Spectral densityAstronomy and AstrophysicsCosmologyHubble volumeDark energysymbolsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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A Standard Siren Measurement of the Hubble Constant from GW170817 without the Electromagnetic Counterpart

2019

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817. Instead, we consider each galaxy within the GW170817 localization region as a potential host; combining the redshift from each galaxy with the distance estimate from GW170817 provides an estimate of the Hubble constant, $H_0$. We then combine the $H_0$ values from all the galaxies to provide a final measurement of $H_0$. We explore the dependence of our results on the thresholds by which galaxies are included in our sample, as well as the impact of weighting the galaxies by stellar mass and star-formation rate. Co…

AstrofísicaGravitacióCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesStellar massStar (game theory)AstronomyFOS: Physical sciencesPREDICTIONSInterval (mathematics)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsMASSdistance scale01 natural sciencessymbols.namesake0103 physical sciencesRange (statistics)distance scale; gravitational waves010303 astronomy & astrophysicsgravitational waveAstrophysics::Galaxy AstrophysicsQB0105 earth and related environmental sciencesPhysicsSettore FIS/01Science & TechnologyAstronomy and AstrophysicsAstronomy and AstrophysicRedshiftGalaxyWeightingGALAXIESdistance scale; gravitational waves; Astronomy and Astrophysics; Space and Planetary SciencePhysics and Astronomygravitational wavesSpace and Planetary SciencePhysical Sciencessymbols[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawAstrophysical Journal Letters
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Testing standard and nonstandard neutrino physics with cosmological data

2012

Cosmological constraints on the sum of neutrino masses and on the effective number of neutrino species in standard and nonstandard scenarios are computed using the most recent available cosmological data. Our cosmological data sets include the measurement of the baryonic acoustic oscillation (BAO) feature in the data release 9 CMASS sample of the baryon oscillation spectroscopic survey. We study in detail the different degeneracies among the parameters, as well as the impact of the different data sets used in the analyses. When considering bounds on the sum of the three active neutrino masses, the information in the BAO signal from galaxy clustering measurements is approximately equally pow…

AstrofísicaNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic background radiationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesCosmologyPower spectrumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino oscillationTelescope010303 astronomy & astrophysicsDigital sky surveyPhysicsHubble constantCosmologia010308 nuclear & particles physicsMatter power spectrumBig-bang nucleosynthesisCMB cold spotHigh Energy Physics - Phenomenology13. Climate actionParameterssymbolsBaryon acoustic-oscillationsBaryon acoustic oscillationsNeutrinoData releaseAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawPhysical Review D
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New horizons for fundamental physics with LISA

2022

K. G. Arun et al.

AstrofísicaPROTOPLANET MIGRATIONFísica-Modelos matemáticosPhysics and Astronomy (miscellaneous)gr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)GRAVITATIONAL-WAVEShorizonFundamental physicGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational wavesLIGO (Observatory)Tests of general relativitySettore FIS/05 - Astronomia e AstrofisicaDARK-MATTERFísica matemáticaKOZAI MECHANISMHigh Energy PhysicsGENERAL-RELATIVITYFundamental physics; Gravitational waves; LISA; Tests of general relativityFundamental physicsPRIMORDIAL BLACK-HOLESLISAScience & TechnologyGeneral Relativity and Cosmology83CXXPhysicsgravitation: interactiongravitational radiationFísicaCompactQUANTUM-GRAVITYPhysical SciencesAstronomia[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]fundamental physics; gravitational waves; LISA; test of general relativityMODIFIED GRAVITYtest of general relativityGravitational waveMULTIPOLE MOMENTSHUBBLE CONSTANT
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Dark radiation sterile neutrino candidates after Planck data

2013

Recent Cosmic Microwave Background (CMB) results from the Planck satellite, combined with previous CMB data and Hubble constant measurements from the Hubble Space Telescope, provide a constraint on the effective number of relativistic degrees of freedom 3.62(-0.48)(+0.50) at 95% CL. New Planck data provide a unique opportunity to place limits on models containing relativistic species at the decoupling epoch. We present here the bounds on sterile neutrino models combining Planck data with galaxy clustering information. Assuming N-eff active plus sterile massive neutrino species, in the case of a Planck+WP+HighL+HST analysis we find m(nu,sterile)(eff) < 0.36 eV and 3.14 < N-eff < 4.15 at 95% …

AstrofísicaSterile neutrinocosmological neutrinosHadronCosmic microwave backgroundAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPartícules (Física nuclear)symbols.namesake0103 physical sciencesneutrino properties; dark energy theory; neutrino theory; cosmological neutrinosdark energy theoryPlanck010303 astronomy & astrophysicsAxionAstrophysics::Galaxy Astrophysicsneutrino propertiesPhysicsCosmologia010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsDecoupling (cosmology)neutrino theory13. Climate actionDark radiationsymbolsHigh Energy Physics::ExperimentHubble's law
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Coupled dark matter-dark energy in light of near Universe observations

2010

Cosmological analysis based on currently available observations are unable to rule out a sizeable coupling among the dark energy and dark matter fluids. We explore a variety of coupled dark matter-dark energy models, which satisfy cosmic microwave background constraints, in light of low redshift and near universe observations. We illustrate the phenomenology of different classes of dark coupling models, paying particular attention in distinguishing between effects that appear only on the expansion history and those that appear in the growth of structure. We find that while a broad class of dark coupling models are effectively models where general relativity (GR) is modified - and thus can b…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEnergia fosca (Astronomia)01 natural sciencesRedshift-space distortionssymbols.namesake0103 physical sciencesDark energy (Astronomy)010303 astronomy & astrophysicsPhysicsCosmologia010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxyRedshiftCosmologyDark matter (Astronomy)symbolsDark energyMatèria fosca (Astronomia)Astrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Morphological Differences in Neuromasts of the Blind Cave Fish &lt;i&gt;Astyanax hubbsi &lt;/i&gt;and the Sighted River Fish &lt;i&gt;Astyanax mexica…

1990

Vital staining and scanning electron microscopy were used to study the morphology of superficial neuromasts in the blind cave fish, Astyanax hubbsi, and its sighted congener, <i&

Astyanax hubbsigeographygeography.geographical_feature_categoryZoologyCavefishAnatomyBiologybiology.organism_classificationhumanitiesbody regionsCharacidaeBehavioral NeuroscienceDevelopmental NeuroscienceCaveFish <Actinopterygii>Brain, Behavior and Evolution
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Driven Bose-Hubbard Model with a Parametrically Modulated Harmonic Trap

2016

We investigate a one-dimensional Bose–Hubbard model in a parametrically driven global harmonic trap. The delicate interplay of both the local interaction of the atoms in the lattice and the driving of the global trap allows us to control the dynamical stability of the trapped quantum many-body state. The impact of the atomic interaction on the dynamical stability of the driven quantum many-body state is revealed in the regime of weak interaction by analyzing a discretized Gross–Pitaevskii equation within a Gaussian variational ansatz, yielding a Mathieu equation for the condensate width. The parametric resonance condition is shown to be modified by the atom interaction strength. In particul…

Bose–Hubbard modelquantum many-body systemsFOS: Physical sciencesHarmonic (mathematics)02 engineering and technologyBose–Hubbard modelWeak interaction01 natural sciencessymbols.namesakeQuantum mechanics0103 physical sciencesAtomquantum gas010306 general physicsQuantumAnsatzPhysicsCondensed Matter::Quantum Gasesta114021001 nanoscience & nanotechnologyMathieu functionQuantum Gases (cond-mat.quant-gas)symbolsParametric oscillator0210 nano-technologyCondensed Matter - Quantum Gasesharmonic trap
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Probing the bond order wave phase transitions of the ionic Hubbard model by superlattice modulation spectroscopy

2017

An exotic phase, the bond order wave, characterized by the spontaneous dimerization of the hopping, has been predicted to exist sandwiched between the band and Mott insulators in systems described by the ionic Hubbard model. Despite growing theoretical evidences, this phase still evades experimental detection. Given the recent realization of the ionic Hubbard model in ultracold atomic gases, we propose here to detect the bond order wave using superlattice modulation spectroscopy. We demonstrate, with the help of time-dependent density-matrix renormalization group and bosonization, that this spectroscopic approach reveals characteristics of both the Ising and Kosterlitz-Thouless transitions …

BosonizationHubbard model[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]SuperlatticeGeneral Physics and AstronomyIonic bondingFOS: Physical sciences01 natural sciencesCondensed Matter - Strongly Correlated ElectronsPhysics and Astronomy (all)0103 physical sciencesBosonizationCold atoms010306 general physicsPhysicsCondensed Matter::Quantum GasesCondensed matter physicsDensity Matrix Renormalization GroupStrongly Correlated Electrons (cond-mat.str-el)010308 nuclear & particles physicsMott insulatorBerezinskii-Kosterlitz-Thouless transitionIsing transitionRenormalization groupBond orderQuantum Gases (cond-mat.quant-gas)Ising modelCondensed Matter::Strongly Correlated ElectronsCondensed Matter - Quantum Gases
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Accessing finite momentum excitations of the one-dimensional Bose-Hubbard model using superlattice modulation spectroscopy

2018

We investigate the response to superlattice modulation of a bosonic quantum gas confined to arrays of tubes emulating the one-dimensional Bose-Hubbard model. We demonstrate, using both time-dependent density matrix renormalization group and linear response theory, that such a superlattice modulation gives access to the excitation spectrum of the Bose-Hubbard model at finite momenta. Deep in the Mott-insulator, the response is characterized by a narrow energy absorption peak at a frequency approximately corresponding to the onsite interaction strength between bosons. This spectroscopic technique thus allows for an accurate measurement of the effective value of the interaction strength. On th…

BosonizationPhysicsCondensed Matter::Quantum GasesCondensed matter physics[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]Density matrix renormalization groupMott insulatorSuperlatticeFOS: Physical sciencesBose–Hubbard model01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasSuperfluidityBose-Hubbard modelQuantum Gases (cond-mat.quant-gas)Atomic and Molecular PhysicsDMRG0103 physical sciencesBosonizationand Optics010306 general physicsCondensed Matter - Quantum GasesFrequency modulationBoson
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