Search results for "SCALAR"

showing 10 items of 1002 documents

Gravity waves from non-minimal quadratic inflation

2015

We discuss non-minimal quadratic inflation in supersymmetric (SUSY) and non-SUSY models which entails a linear coupling of the inflaton to gravity. Imposing a lower bound on the parameter cR, involved in the coupling between the inflaton and the Ricci scalar curvature, inflation can be attained even for subplanckian values of the inflaton while the corresponding effective theory respects the perturbative unitarity up to the Planck scale. Working in the non-SUSY context we also consider radiative corrections to the inflationary potential due to a possible coupling of the inflaton to bosons or fermions. We find ranges of the parameters, depending mildly on the renormalization scale, with adju…

Inflation (cosmology)PhysicsHigh Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)UnitaritySuperpotentialHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsSupersymmetryAstrophysics::Cosmology and Extragalactic AstrophysicsInflatonCoupling (probability)High Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Effective field theoryScalar curvatureMathematical physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Probing the creatable character of perturbed Friedmann-Robertson-Walker universes

2008

We discuss whether some perturbed Friedmann-Robertson-Walker (FRW) universes could be creatable, i. e., could have vanishing energy, linear momentum and angular momentum, as it could be expectable if the Universe arose as a quantum fluctuation. On account of previous results, the background is assumed to be either closed (with very small curvature) or flat. In the first case, fully arbitrary linear perturbations are considered; whereas in the flat case, it is assumed the existence of: (i) inflationary scalar perturbations, that is to say, Gaussian adiabatic scalar perturbations having an spectrum close to the Harrison-Zel'dovich one, and (ii) arbitrary tensor perturbations. We conclude that…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsAngular momentumGravitational wavemedia_common.quotation_subjectAstrophysics (astro-ph)Scalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyUniverseGeneral Relativity and Quantum Cosmologysymbols.namesakeClassical mechanicsFriedmann–Lemaître–Robertson–Walker metricsymbolsTensorQuantum fluctuationmedia_commonPhysical Review D
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Slinky inflation

2005

We present a new approach to quintessential inflation, in which both dark energy and inflation are explained by the evolution of a single scalar field. We start from a simple scalar potential with both oscillatory and exponential behavior. We employ the conventional reheating mechanism of new inflation, in which the scalar decays to light fermions with a decay width that is proportional to the scalar mass. Because our scalar mass is proportional to the Hubble rate, this gives adequate reheating at early times while shutting off at late times to preserve quintessence and satisfy nucleosynthesis constraints. We discuss a simple model which solves the horizon, flatness, and "why now" problems.…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsCosmic microwave backgroundScalar (mathematics)Astrophysics (astro-ph)FOS: Physical sciencesFísicaScalar potentialAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsTheoretical physicsHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)NucleosynthesisDark energyScalar fieldQuintessence
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Minimal noncanonical cosmologies

2006

We demonstrate how much it is possible to deviate from the standard cosmological paradigm of inflation-assisted LambdaCDM, keeping within current observational constraints, and without adding to or modifying any theoretical assumptions. We show that within a minimal framework there are many new possibilities, some of them wildly different from the standard picture. We present three illustrative examples of new models, described phenomenologically by a noncanonical scalar field coupled to radiation and matter. These models have interesting implications for inflation, quintessence, reheating, electroweak baryogenesis, and the relic densities of WIMPs and other exotics.

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsElectroweak interactionAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsBaryogenesisTheoretical physicsGeneral Relativity and Quantum CosmologyScalar fieldQuintessence
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Inflation might be caused by the right

2009

15 pages, 4 figures.-- ISI article identifier: 000265600800102.-- ArXiv pre-print avaible at: http://arxiv.org/abs/0811.2998

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsBeyond Standard ModelAstrophysics (astro-ph)FOS: Physical sciencesElementary particleFermionInflatonAstrophysicsMassless particleHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino PhysicsNeutrinoScalar fieldComputer Science::DatabasesLeptonCosmology of Theories beyond the SM
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Upper bound on the tensor-to-scalar ratio in GUT-scale supersymmetric hybrid inflation

2014

We explore the upper bound on the tensor-to-scalar ratio r in supersymmetric (F-term) hybrid inflation models with the gauge symmetry breaking scale set equal to the value 2.86⋅1016 GeV2.86⋅1016 GeV, as dictated by the unification of the MSSM gauge couplings. We employ a unique renormalizable superpotential and a quasi-canonical Kähler potential, and the scalar spectral index nsns is required to lie within the two-sigma interval from the central value found by the Planck satellite. In a sizable region of the parameter space the potential along the inflationary trajectory is a monotonically increasing function of the inflaton, and for this case, r≲2.9⋅10−4r≲2.9⋅10−4, while the spectral index…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)SuperpotentialScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryInflatonUpper and lower boundsHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Cosmology and Nongalactic AstrophysicsMinimal Supersymmetric Standard ModelGauge symmetryPhysics Letters B
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2017

We show that the dynamics of the Higgs field during inflation is not affected by metric fluctuations if the Higgs is an energetically subdominant light spectator. For Standard Model parameters we find that couplings between Higgs and metric fluctuations are suppressed by $\mathcal{O}(10^{-7})$. They are negligible compared to both pure Higgs terms in the effective potential and the unavoidable non-minimal Higgs coupling to background scalar curvature. The question of the electroweak vacuum instability during high energy scale inflation can therefore be studied consistently using the Jordan frame action in a Friedmann--Lemaitre--Robertson--Walker metric, where the Higgs-curvature coupling en…

Inflation (cosmology)PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionScalar (mathematics)Astronomy and Astrophysics01 natural sciencesStandard ModelGeneral Relativity and Quantum CosmologyHiggs field0103 physical sciencesMetric (mathematics)Higgs bosonHigh Energy Physics::Experiment010306 general physicsScalar curvatureJournal of Cosmology and Astroparticle Physics
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Isocurvature Constraints on Portal Couplings

2016

We consider portal models which are ultraweakly coupled with the Standard Model, and confront them with observational constraints on dark matter abundance and isocurvature perturbations. We assume the hidden sector to contain a real singlet scalar $s$ and a sterile neutrino $\psi$ coupled to $s$ via a pseudoscalar Yukawa term. During inflation, a primordial condensate consisting of the singlet scalar $s$ is generated, and its contribution to the isocurvature perturbations is imprinted onto the dark matter abundance. We compute the total dark matter abundance including the contributions from condensate decay and nonthermal production from the Standard Model sector. We then use the Planck lim…

Inflation (cosmology)PhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesStandard ModelPseudoscalarHidden sectorHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencessymbolsPlanck010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Performance and energy optimisation in CPUs through fuzzy knowledge representation

2019

Abstract This paper presents an automatic design space exploration using processor design knowledge for the multi-objective optimisation of a superscalar microarchitecture enhanced with selective load value prediction (SLVP). We introduced new important SLVP parameters and determined their influence regarding performance, energy consumption, and thermal dissipation. We significantly enlarged initial processor design knowledge expressed through fuzzy rules and we analysed its role in the process of automatic design space exploration. The proposed fuzzy rules improve the diversity and quality of solutions, and the convergence speed of the design space exploration process. Experiments show tha…

Information Systems and ManagementComputer scienceDesign space exploration02 engineering and technologyFuzzy logicMulti-objective optimizationTheoretical Computer ScienceProcessor design knowledgeArtificial IntelligenceEnergy savingSuperscalar0202 electrical engineering electronic engineering information engineeringAutomatic design space exploration Processor design knowledge Superscalar microarchitecture Dynamic value prediction Energy savingProcessor design05 social sciencesProcess (computing)050301 educationEnergy consumptionComputer Science ApplicationsMicroarchitectureComputer engineeringControl and Systems EngineeringDynamic value prediction020201 artificial intelligence & image processingAutomatic design space exploration; Processor design knowledge; Superscalar microarchitecture; Dynamic value prediction; Energy savingSuperscalar microarchitecture0503 educationAutomatic design space explorationSoftwareEnergy (signal processing)Information Sciences
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Exploiting selective instruction reuse and value prediction in a superscalar architecture

2009

In our previously published research we discovered some very difficult to predict branches, called unbiased branches. Since the overall performance of modern processors is seriously affected by misprediction recovery, especially these difficult branches represent a source of important performance penalties. Our statistics show that about 28% of branches are dependent on critical Load instructions. Moreover, 5.61% of branches are unbiased and depend on critical Loads, too. In the same way, about 21% of branches depend on MUL/DIV instructions whereas 3.76% are unbiased and depend on MUL/DIV instructions. These dependences involve high-penalty mispredictions becoming serious performance obstac…

Instructions per cycleSpeedupComputer scienceSpeculative executionSpec#Thread (computing)Parallel computingReuseHardware and ArchitectureSuperscalarHardware_CONTROLSTRUCTURESANDMICROPROGRAMMINGcomputerData cacheSoftwarecomputer.programming_languageJournal of Systems Architecture
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