Search results for "General relativity and quantum cosmology"

showing 10 items of 941 documents

Supermanifolds, symplectic geometry and curvature

2015

We present a survey of some results and questions related to the notion of scalar curvature in the setting of symplectic supermanifolds.

Mathematics - Differential GeometryGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryDifferential Geometry (math.DG)FOS: MathematicsFOS: Physical sciencesMathematics::Differential GeometryMathematical Physics (math-ph)58A50 58C50 53D35Mathematics::Symplectic GeometryMathematical Physics
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Modeling and simulation of an offshore crane

2018

This paper presents a mathematical modeling of a crane system using robot modeling theory as well as the numerical simulation of the dynamics of a crane and a marine craft. The simulations are performed in SimulationX and Matlab Simulink. The simulation platform includes a SimulationX-model of the crane, a realistic model of a marine craft using the Marine Systems Simulator(MSS) and the hydrodynamic sea-keeping calculations (VERES program code). The simulation results show a very good picture of the dynamic behavior of the real crane in offshore environment and verify the validation and effectiveness of the presented modeling approach.

Modeling and simulationGeneral Relativity and Quantum CosmologyComputer simulationComputingMethodologies_SIMULATIONANDMODELINGComputer scienceMathematics::Category TheoryComputerApplications_COMPUTERSINOTHERSYSTEMSSubmarine pipelineNumerical modelsKinematicsSimulation2018 13th IEEE Conference on Industrial Electronics and Applications (ICIEA)
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Modeling quitessential inflation

2001

We develop general criteria to construct unified frameworks for inflation and quintessence which employ a unique scalar field to drive both. By using such a minimal theoretical framework we avoid having to fine-tune couplings and mass-scales. In particular the initial conditions for quintessence are already fixed at the end of the inflationary epoch. We provide concrete realizations of the method which meet all inflationary and quintessence requirements, such as the COBE normalization and the resulting spectral index n = 0.97, which is in excellent agreement with the latest CMB data.

Normalization (statistics)Inflation (cosmology)PhysicsPhysics::General PhysicsCosmic microwave backgroundAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsHigh Energy Physics - PhenomenologyTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Inflationary epochScalar fieldQuintessence
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Cuckoo's Eggs in Neutron Stars: Can LIGO Hear Chirps from the Dark Sector?

2018

We explore in detail the possibility that gravitational wave signals from binary inspirals are affected by a new force that couples only to dark matter particles. We discuss the impact of both the new force acting between the binary partners as well as radiation of the force carrier. We identify numerous constraints on any such scenario, ultimately concluding that observable effects on the dynamics of binary inspirals due to such a force are not possible if the dark matter is accrued during ordinary stellar evolution. Constraints arise from the requirement that the astronomical body be able to collect and bind at small enough radius an adequate number of dark matter particles, from the requ…

Nuclear and High Energy PhysicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)General relativitymedia_common.quotation_subjectgr-qcDark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsStellar evolutionmedia_commonParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsStar formationGravitational wavehep-exGeneral Relativity and CosmologyFifth forcehep-phCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyNeutron starBeyond Standard Modelastro-ph.COlcsh:QC770-798Particle Physics - ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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What is the final state of a black hole merger?

2018

In this short paper we discuss the possibility of testing the nature of astrophysical black holes using the recently observed black hole mergers. We investigate the possibility that a secondary black hole is created in the merger of two astrophysical black holes and discuss potential astrophysical signatures. We point out that black hole mergers are a possible astrophysical mechanism for the creation of quantum black holes with masses close to the Planck mass.

Nuclear and High Energy PhysicsBlack holeAstrophysics::High Energy Astrophysical PhenomenaShort paperPlanck massFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesquantum black holes.10. No inequality010306 general physicsQuantumQBPhysics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsBlack holeblack hole mergerquantum gravityQuantum gravityModern Physics Letters A
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Dynamical analysis of anisotropic inflation

2016

Inflaton coupling to a vector field via the $f^2(\phi)F_{\mu\nu}F^{\mu\nu}$ term is used in several contexts in the literature, such as to generate primordial magnetic fields, to produce statistically anisotropic curvature perturbation, to support anisotropic inflation and to circumvent the $\eta$-problem. Here, I perform dynamical analysis of such a system allowing for most general Bianchi I initial conditions. I also confirm the stability of attractor equilibrium points in phase-space directions that had not been investigated before.

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dynamical systems theoryFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Fixed point01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)anisotropic Bianchi cosmologies0103 physical sciencesAttractorBoundary value probleminflation010306 general physicsInflation (cosmology)Physicsta114010308 nuclear & particles physicsAstronomy and Astrophysicsdynamical systemsInflatonHigh Energy Physics - PhenomenologyClassical mechanicsPhase spaceVector fieldvector fieldsAstrophysics - Cosmology and Nongalactic AstrophysicsModern Physics Letters A
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Critical point Higgs inflation in the Palatini formulation

2021

We study Higgs inflation in the Palatini formulation with the renormalisation group improved potential in the case when loop corrections generate a feature similar to an inflection point. Assuming that there is a threshold correction for the Higgs quartic coupling $\lambda$ and the top Yukawa coupling $y_t$, we scan the three-dimensional parameter space formed by the two jumps and the non-minimal coupling $\xi$. The spectral index $n_s$ can take any value in the observationally allowed range. The lower limit for the running is $\alpha_s>-3.5\times10^{-3}$, and $\alpha_s$ can be as large as the observational upper limit. Running of the running is small. The tensor-to-scalar ratio is $2.2\tim…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesRIEMANNGeneral Relativity and Quantum Cosmology (gr-qc)Parameter spaceINITIAL CONDITIONSkosmologia01 natural sciences114 Physical sciencesGeneral Relativity and Quantum CosmologyEINSTEINCritical point (thermodynamics)0103 physical sciencesRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. Radioactivityteoreettinen fysiikkaGENERAL-RELATIVITY010306 general physicscosmology of theories beyond the SMDISSIPATIONBosonMathematical physicsInflation (cosmology)Physics010308 nuclear & particles physicsYukawa potentialCONSTRAINTSBOSONGRAVITATIONRenormalization groupAFFINE VARIATIONAL-PRINCIPLESCosmology of Theories beyond the SMInflection pointHiggs bosonSCALARONlcsh:QC770-798renormalization groupAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Standard and Z2-Regge theory in two dimensions

1998

Abstract We qualitatively compare two versions of quantum Regge calculus by means of Monte Carlo simulations. In Standard Regge Calculus the quadratic link lengths of the triangulation vary continuously, whereas in the Z2-Regge Model they are restricted to two possible values. The goal is to determine whether the computationally more easily accessible Z2 model retains the characteristics of standard Regge theory.

Nuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyMonte Carlo methodTriangulation (social science)Regge calculusAtomic and Molecular Physics and OpticsRegge theoryHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyQuadratic equationQuantum electrodynamicsQuantum gravityHigh Energy Physics::ExperimentStatistical physicsLink (knot theory)QuantumMathematicsNuclear Physics B - Proceedings Supplements
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Inertial modes in stratified rotating neutron stars : An evolutionary description

2005

With (non-barotropic) equations of state valid even when the neutron, proton and electron content of neutron star cores is not in beta equilibrium, we study inertial and composition gravity modes of relativistic rotating neutron stars. We solve the relativistic Euler equations in the time domain with a three dimensional numerical code based on spectral methods, in the slow rotation, relativistic Cowling and anelastic approximations. Principally, after a short description of the gravity modes due to smooth composition gradients, we focus our analysis on the question of how the inertial modes are affected by non-barotropicity of the nuclear matter. In our study, the deviation with respect to …

Nuclear and High Energy PhysicsInertial frame of referenceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics7. Clean energy01 natural sciencesGeneral Relativity and Quantum CosmologyGravitation[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols.namesake0103 physical sciencesNeutron010303 astronomy & astrophysicsPhysics[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010308 nuclear & particles physicsAstrophysics (astro-ph)Nuclear matterRelativistic Euler equationsComputational physicsEuler equationsNumerical relativityNeutron starClassical mechanics[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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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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