Search results for "Física-Modelos matemáticos"

showing 10 items of 30 documents

Stellar structure models in modified theories of gravity: Lessons and challenges

2019

The understanding of stellar structure represents the crossroads of our theories of the nuclear force and the gravitational interaction under the most extreme conditions observably accessible. It provides a powerful probe of the strong field regime of General Relativity, and opens fruitful avenues for the exploration of new gravitational physics. The latter can be captured via modified theories of gravity, which modify the Einstein-Hilbert action of General Relativity and/or some of its principles. These theories typically change the stellar structure equations, thus having a large impact on the astrophysical properties of the corresponding stars and opening a new window to constrain these …

High Energy Physics - TheoryFísica-Modelos matemáticosGeneral relativityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsStellar classification01 natural sciencesGeneral Relativity and Quantum CosmologyGravitation0103 physical sciencesFísica matemáticaAstrophysics::Solar and Stellar AstrophysicsStellar structure010306 general physicsChandrasekhar limitSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsWhite dwarfStarsNeutron starHigh Energy Physics - Theory (hep-th)Astrophysics - Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPhysics Reports
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An infinite class of exact rotating black hole metrics of modified gravity

2022

We build an infinite class of exact axisymmetric solutions of a metric-affine gravity theory, namely, Eddington-inspired Born-Infeld gravity, coupled to an anisotropic fluid as a matter source. The solution-generating method employed is not unique of this theory but can be extended to other Ricci-Based Gravity theories (RBGs), a class of theories built out of contractions of the Ricci tensor with the metric. This method exploits a correspondence between the space of solutions of General Relativity and that of RBGs, and is independent of the symmetries of the problem. For the particular case in which the fluid is identified with non-linear electromagnetic fields we explicitly derive the corr…

High Energy Physics - TheoryGeneral Relativity and Quantum CosmologyFísica-Modelos matemáticosHigh Energy Physics - Theory (hep-th)FOS: Physical sciencesFísica matemáticaAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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New scalar compact objects in Ricci-based gravity theories

2019

Taking advantage of a previously developed method, which allows to map solutions of General Relativity into a broad family of theories of gravity based on the Ricci tensor (Ricci-based gravities), we find new exact analytical scalar field solutions by mapping the free-field static, spherically symmetric solution of General Relativity (GR) into quadratic $f(R)$ gravity and the Eddington-inspired Born-Infeld gravity. The obtained solutions have some distinctive feature below the would-be Schwarzschild radius of a configuration with the same mass, though in this case no horizon is present. The compact objects found include wormholes, compact balls, shells of energy with no interior, and a new …

High Energy Physics - TheoryModified gravityFísica-Modelos matemáticosGeneral relativityGravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesFísica matemáticaWormhole010306 general physicsRicci curvaturePhysics010308 nuclear & particles physicsScalar (physics)Astronomy and AstrophysicsGR black holesBlack holeHigh Energy Physics - Theory (hep-th)Horizon (general relativity)WormholesScalar fieldSchwarzschild radius
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Fingerprints of heavy scales in electroweak effective Lagrangians

2017

The couplings of the electroweak effective theory contain information on the heavy-mass scales which are no-longer present in the low-energy Lagrangian. We build a general effective Lagrangian, implementing the electroweak chiral symmetry breaking $SU(2)_L\otimes SU(2)_R\to SU(2)_{L+R}$, which couples the known particle fields to heavier states with bosonic quantum numbers $J^P=0^\pm$ and $1^\pm$. We consider colour-singlet heavy fields that are in singlet or triplet representations of the electroweak group. Integrating out these heavy scales, we analyze the pattern of low-energy couplings among the light fields which are generated by the massive states. We adopt a generic non-linear realiz…

Nuclear and High Energy PhysicsParticle physicsFísica-Modelos matemáticosHiggs PhysicsFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryFísica matemáticaPartículas (Física nuclear)lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectromagnetismoSymmetry breakingSinglet state010306 general physicsParticles (Nuclear physics)Huellas dactilares.PhysicsQuantum chromodynamics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionCromodinámica cuántica.Technicolor and Composite ModelsQuantum numberLagrangian functions.High Energy Physics - PhenomenologyFingerprints.Simetría (Física)Beyond Standard ModelChiral LagrangiansQuantum chromodynamics.Higgs bosonlcsh:QC770-798Chiral symmetry breakingSymmetry (Physics)Lagrange Funciones de.Journal of High Energy Physics
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Determination of the pole position of the lightest hybrid meson candidate

2019

Mapping states with explicit gluonic degrees of freedom in the light sector is a challenge, and has led to controversies in the past. In particular, the experiments have reported two different hybrid candidates with spin-exotic signature, pi1(1400) and pi1(1600), which couple separately to eta pi and eta' pi. This picture is not compatible with recent Lattice QCD estimates for hybrid states, nor with most phenomenological models. We consider the recent partial wave analysis of the eta(') pi system by the COMPASS collaboration. We fit the extracted intensities and phases with a coupled-channel amplitude that enforces the unitarity and analyticity of the S-matrix. We provide a robust extracti…

Particle physicsFísica-Modelos matemáticosMesonPartial wave analysisLattice field theoryGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesResonance (particle physics)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all); energy; meson photoproductionPhysics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesFísica matemática010306 general physicsS-matrixPOMERONQuantum chromodynamicsPhysicsUnitarityRESTLattice QCDmeson photoproductionETA-PIMODELHigh Energy Physics - PhenomenologyPhysics and AstronomyEXOTICSSTATESWAVEPI(-)PSYSTEMenergy
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Double Polarization Observables in Pentaquark Photoproduction

2019

We investigate the properties of the hidden charm pentaquark-like resonances first observed by LHCb in 2015, by measuring the polarization transfer KLL between the incident photon and the outgoing proton in the exclusive photoproduction of J/psi near threshold. We present a first estimate of the sensitivity of this observable to the pentaquark photocouplings and hadronic branching ratios, and extend our predictions to the case of initial state helicity correlation ALL, using a polarized target. These results serve as a benchmark for the SBS experiment at Jefferson Lab, which proposes to measure for the first time the helicity correlations ALL and KLL in J/psi exclusive photoproduction, in o…

Particle physicsFísica-Modelos matemáticosPhotonHadronpentaquarksFOS: Physical sciences01 natural sciencesexotic hadronsHigh Energy Physics - ExperimentPolarized targetHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPhoton polarizationNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsexotic hadrons; pentaquarks; hadron spectroscopy010308 nuclear & particles physicshadron spectroscopyObservablePolarization (waves)HelicityPentaquarkHigh Energy Physics - PhenomenologyHigh Energy Physics::Experiment
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Improved unitarized heavy baryon chiral perturbation theory for πN scattering to fourth order

2004

We extend our previous analysis of the unitarized pion-nucleon scattering amplitude including up to fourth order terms in heavy baryon chiral perturbation theory. We pay special attention to the stability of the generated Delta(1232) resonance, the convergence problems, and the power counting of the chiral parameters.

PhysicsChiral anomalyNuclear and High Energy PhysicsParticle physicsChiral perturbation theoryFísica-Modelos matemáticosUnitarityHeavy baryon chiral perturbation theoryScatteringPartial wave analysisHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyFísicaResonance (particle physics)Scattering amplitudeQuantum electrodynamicsFísica matemáticaNuclear Experiment
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Parameterized nonrelativistic limit of stellar structure equations in Ricci-based gravity theories

2021

We present the non-relativistic limit of the stellar structure equations of Ricci-based gravities, a family of metric-affine theories whose Lagrangian is built via contractions of the metric with the Ricci tensor of an a priori independent connection. We find that this limit is characterized by four parameters that arise in the expansion of several geometric quantities in powers of the stress-energy tensor of the matter fields. We discuss the relevance of this result for the phenomenology of non-relativistic stars, such as main-sequence stars as well as several substellar objects.

PhysicsFísica-Modelos matemáticosFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyConnection (mathematics)StarsMetric (mathematics)Astrophysics::Solar and Stellar AstrophysicsFísica matemáticaStellar structureLimit (mathematics)TensorAstrophysics::Earth and Planetary AstrophysicsPhenomenology (particle physics)Ricci curvatureMathematical physics
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Junction conditions in Palatinif(R) gravity

2020

We work out the junction conditions for $f(R)$ gravity formulated in metric-affine (Palatini) spaces using a tensor distributional approach. These conditions are needed for building consistent models of gravitating bodies with an interior and exterior regions matched at some hypersurface. Some of these conditions depart from the standard Darmois-Israel ones of General Relativity and from their metric $f(R)$ counterparts. In particular, we find that the trace of the stress-energy momentum tensor in the bulk must be continuous across the matching hypersurface, though its normal derivative need not to. We illustrate the relevance of these conditions by considering the properties of stellar sur…

PhysicsFísica-Modelos matemáticosPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsGeneral relativityFOS: Physical sciencesPolytropic processGeneral Relativity and Quantum Cosmology (gr-qc)Directional derivative01 natural sciencesDomain (mathematical analysis)General Relativity and Quantum CosmologyMomentumGeneral Relativity and Quantum CosmologyHypersurface0103 physical sciencesFísica matemáticaf(R) gravityTensor010306 general physicsMathematical physics
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Rotating black holes in Eddington-inspired Born-Infeld gravity: an exact solution

2020

We find an exact, rotating charged black hole solution within Eddington-inspired Born-Infeld gravity. To this end we employ a recently developed correspondence or {\it mapping} between modified gravity models built as scalars out of contractions of the metric with the Ricci tensor, and formulated in metric-affine spaces (Ricci-Based Gravity theories) and General Relativity. This way, starting from the Kerr-Newman solution, we show that this mapping bring us the axisymmetric solutions of Eddington-inspired Born-Infeld gravity coupled to a certain model of non-linear electrodynamics. We discuss the most relevant physical features of the solutions obtained this way, both in the spherically sym…

PhysicsHigh Energy Physics - TheoryGravity (chemistry)Modified gravityFísica-Modelos matemáticos010308 nuclear & particles physicsGeneral relativityRotational symmetryFOS: Physical sciencesAstronomy and AstrophysicsGR black holesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black hole01 natural sciencesGravitational-wave astronomyGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyExact solutions in general relativityHigh Energy Physics - Theory (hep-th)0103 physical sciencesMetric (mathematics)Física matemáticaWormholesRicci curvature
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