Search results for "Early Universe"

showing 10 items of 26 documents

Revising the Predictions of Inflation for the Cosmic Microwave Background Anisotropies

2009

4 pages, 1 figure.-- PACS nrs.: 98.70.Vc; 11.10.Gh; 98.80.Cq.-- ArXiv pre-print available at: http://arxiv.org/abs/0901.0439

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Cosmic microwave backgroundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)[PACS] Cosmic background radiations01 natural sciencesGeneral Relativity and Quantum CosmologySpectral lineRenormalizationHigh Energy Physics - Phenomenology (hep-ph)[PACS] Particle-theory and field-theory models of the early UniverseQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsSpectral densityCMB cold spot3. Good healthHigh Energy Physics - Phenomenology[PACS] Renormalization in quantum field theoryHigh Energy Physics - Theory (hep-th)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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On gravitational waves in Born-Infeld inspired non-singular cosmologies

2017

We study the evolution of gravitational waves for non-singular cosmological solutions within the framework of Born-Infeld inspired gravity theories, with special emphasis on the Eddington-inspired Born-Infeld theory. We review the existence of two types of non-singular cosmologies, namely bouncing and asymptotically Minkowski solutions, from a perspective that makes their features more apparent. We study in detail the propagation of gravitational waves near these non-singular solutions and carefully discuss the origin and severity of the instabilities and strong coupling problems that appear. We also investigate the role of the adiabatic sound speed of the matter sector in the regularisatio…

High Energy Physics - Theorycosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th][ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GravitationTheoretical physicsGeneral Relativity and Quantum CosmologyBorn–Infeld modelgravitational radiation: propagation0103 physical sciencesMinkowski spacestrong couplingphysics of the early universeMinkowski010306 general physicsAdiabatic processmodified gravityPhysics010308 nuclear & particles physicsGravitational waveNon singular[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astronomy and Astrophysicsalternatives to inflationstabilityvelocity: acousticBorn-Infeld modelregularizationHigh Energy Physics - Theory (hep-th)gravitationRegularization (physics)adiabaticStrong coupling[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]primordial gravitational waves (theory)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Born–Infeld inspired modifications of gravity

2017

General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own limit of validity. In particular, the breakdown of unitarity near the Planck scale strongly suggests that General Relativity needs to be modified at high energies and quantum gravity effects are expected to be important. This is related to the existence of spacetime singularities when the solutions of General Relativity are extrapolated to regimes where curvatures are large. In this sense, Born-Infeld inspired modifications of gravity have shown an extraordin…

High Energy Physics - Theorystar: compactcosmological model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]space-time: black holeGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Gravitationquantum gravity: effectBorn–Infeld gravityPhysicsenergy: highBlack holes[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationCosmologyregularizationcurvaturewormhole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational singularitySingularitiesAstrophysics - Cosmology and Nongalactic AstrophysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityEarly universegeneral relativity: solutionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Theoretical physicsGeneral Relativity and Quantum Cosmologyspace-time: singularity0103 physical sciencesunitaritystructureWormholeinflation010306 general physicsCompact objectsSpacetime010308 nuclear & particles physicsscale: PlanckBlack holeBorn-Infeld modelHigh Energy Physics - Theory (hep-th)gravitationQuantum gravity[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Decoherence in supernova neutrino transformations suppressed by deleptonization

2007

16 pages, 12 figures.-- PACS nrs.: 14.60.Pq; 97.60.Bw.-- ISI Article Identifier: 000251987300100.-- ArXiv pre-print available at: http://arxiv.org/abs/0706.2498

HistoryParticle physicsNuclear and High Energy PhysicsQuantum decoherence[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PACS] Supernovae[PACS] Neutrino mass and mixingAstrophysicsAsymmetryMeasure (mathematics)01 natural sciences7. Clean energyEarly UniverseStandard ModelEducationLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesInvariant massddc:530High Energy Physics010306 general physicsMixing (physics)media_commonPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaWeinberg angleFunction (mathematics)Atomic and Molecular Physics and OpticsComputer Science Applications3. Good healthSupernovaHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]PhenomenologyHigh Energy Physics::ExperimentNeutrino
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Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA

2013

Supernova (SN) explosions are crucial engines driving the evolution of galaxies by shock heating gas, increasing the metallicity, creating dust, and accelerating energetic particles. In 2012 we used the Atacama Large Millimeter/Submillimeter Array to observe SN 1987A, one of the best-observed supernovae since the invention of the telescope. We present spatially resolved images at 450um, 870um, 1.4mm, and 2.8mm, an important transition wavelength range. Longer wavelength emission is dominated by synchrotron radiation from shock-accelerated particles, shorter wavelengths by emission from the largest mass of dust measured in a supernova remnant (>0.2Msun). For the first time we show unambig…

MetallicityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSubmillimeter ArrayEARLY UNIVERSEindividual (1987A) [supernovae]Magellanic CloudsAstrophysics::Solar and Stellar AstrophysicsEjectaSupernova remnantSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsISM [galaxies]supernova remnants [ISM]Astronomy and AstrophysicsOPTICAL-PROPERTIESHUBBLE-SPACE-TELESCOPEAstrophysics - Astrophysics of GalaxiesEVOLUTIONGalaxyParticle accelerationEJECTASupernovaPhysics and AstronomyAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)REVERSE SHOCKREMNANTAstrophysics::Earth and Planetary AstrophysicsEMISSIONAstrophysics - High Energy Astrophysical PhenomenaMASSIVE STARSSN 1987A
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Bounds on very low reheating scenarios after Planck

2015

9 pages.- 9 figures

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaEarly universeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsUpper and lower boundsCosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisPlanckPhysicsCosmology Big Bang NucleosynthesisOscillationHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologysymbolsProduction (computer science)High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsPrimordial abundance
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Updated BBN bounds on the cosmological lepton asymmetry for non-zero 13

2011

We discuss the bounds on the cosmological lepton number from Big Bang Nucleosynthesis (BBN), in light of recent evidences for a large value of the neutrino mixing angle theta13. The largest asymmetries for electron and muon or tau neutrinos compatible with 4He and 2H primordial yields are computed versus the neutrino mass hierarchy and mixing angles. The flavour oscillation dynamics is traced till the beginning of BBN and neutrino distributions after decoupling are numerically computed. The latter contains in general, non thermal distortion due to the onset of flavour oscillations driven by solar squared mass difference in the temperature range where neutrino scatterings become inefficient …

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPhysics of the early UniverseFOS: Physical sciences01 natural sciencesAsymmetryPartícules (Física nuclear)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesPrimordial asymmetriesPlanckNeutrinos010306 general physicsNeutrino oscillationmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDecoupling (cosmology)Lepton numberHigh Energy Physics - PhenomenologysymbolsHigh Energy Physics::ExperimentNeutrinoLeptonAstrophysics - Cosmology and Nongalactic Astrophysics
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Tachyonic production of dark relics : a non-perturbative quantum study

2023

We study production of dark relics during reheating after the end of inflation in a system consisting of a non-minimally coupled spectator scalar field and the inflaton. We derive a set of renormalized quantum transport equations for the one-point function and the two-point function of the spectator field and solve them numerically. We find that our system can embody both tachyonic and parametric instabilities. The former is an expected result due to the non-minimal coupling, but the latter displays new features driven by a novel interplay of the two-point function with the Ricci scalar. We find that when the parametric instability driven by the two-point function takes place, it dominates …

Nuclear and High Energy Physicsearly universe particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)hiukkasfysiikka114 Physical sciencesGeneral Relativity and Quantum Cosmologypimeä aineHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nonperturbative Effectsnonperturbative effectsNon-Equilibrium Field TheoryModels for Dark Matternon-equilibrium field theorymodels for dark matterAstrophysics - Cosmology and Nongalactic AstrophysicsEarly Universe Particle Physics
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Precision calculations of dark matter relic abundance

2019

The dark matter annihilation channels sometimes involve sharp resonances. In such cases the usual momentum averaged approximations for computing the DM abundance may not be accurate. We develop an easily accessible momentum dependent framework for computing the DM abundance accurately and efficiently near such features. We apply the method to the case of a singlet scalar dark matter $s$ interacting with SM through higgs portal $\lambda_{\rm hs}s^2 h^2$ and compare the results with different momentum averaged methods. The accuracy of the latter depend strongly on the strength of the elastic interactions and corrections are large if WIMP has negligible interactions beyond the main annihilatio…

Particle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Dark matterFOS: Physical sciencesKinetic energykosmologia01 natural sciencesStandard ModelMomentumpimeä aineHigh Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciencesphysics of the early universeCOSMIC ABUNDANCES010306 general physicsParticle Physics - PhenomenologyPhysicsdark matter theoryAnnihilation010308 nuclear & particles physicsdark matter experimentsAstronomy and Astrophysicshep-ph115 Astronomy Space scienceHigh Energy Physics - PhenomenologyHiggs bosonastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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Early Universe Higgs dynamics in the presence of the Higgs-inflaton and non-minimal Higgs-gravity couplings

2017

Apparent metastability of the electroweak vacuum poses a number of cosmological questions. These concern evolution of the Higgs field to the current vacuum, and its stability during and after inflation. Higgs-inflaton and non-minimal Higgs-gravity interactions can make a crucial impact on these considerations potentially solving the problems. In this work, we allow for these couplings to be present simultaneously and study their interplay. We find that different combinations of the Higgs-inflaton and non-minimal Higgs-gravity couplings induce effective Higgs mass during and after inflation. This crucially affects the Higgs stability considerations during preheating. In particular, a wide ra…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectHigh Energy Physics::LatticeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Metastability0103 physical sciencesphysics of the early universeinflationparticle physicscosmology connectionELECTROWEAK VACUUM010306 general physicscosmology of theories beyond the SMmedia_commonInflation (cosmology)PhysicsSTABILITY010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsBOSONInflaton115 Astronomy Space scienceUniverseHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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