Search results for "Theoretical physics"

showing 10 items of 751 documents

Violation of the equivalence principle from light scalar dark matter

2018

In this paper, we study the local observational consequences of a violation of the Einstein Equivalence Principle induced by models of light scalar Dark Matter (DM). We focus on two different models where the scalar field couples linearly or quadratically to the standard model of matter fields. For both these cases, we derive the solutions of the scalar field. We also derive from first principles the expressions for two types of observables: (i) the local comparison of two atomic sensors that are differently sensitive to the constants of Nature and (ii) the local differential acceleration between two test-masses with different compositions. For the linear coupling, we recover that the signa…

General relativityAtomic Physics (physics.atom-ph)Dark matteralternative theories of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)local position invariance01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics - Atomic Physicsspace-time: oscillationdark matter: couplingGravitationTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Gravitational field0103 physical sciencesDark Matteruniversalityequivalence principle: violationdark matter: scalarEquivalence principle010306 general physicsmodified gravityPhysics010308 nuclear & particles physicsScalar (physics)Yukawa potentialtorsioncoupling: linearuniversality of free fall[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]field theory: scalarHigh Energy Physics - Phenomenologypotential: YukawaGeneral relativitytests of gravitygravitation[SDU]Sciences of the Universe [physics][PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]expansion: accelerationScalar field
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Classical and relativistic n-body problem: from Levi-Civita to the most advanced interplanetary missions

2022

The n-body problem is one of the most important issue in Celestial Mechanics. This article aims to retrace the historical and scientific events that led the Paduan mathematician, Tullio Levi-Civita, to deal with the problem first from a classic and then a relativistic point of view. We describe Levi-Civita's contributions to the theory of relativity focusing on his epistolary exchanges with Einstein, on the problem of secular acceleration and on the proof of Brillouin's cancellation principle. We also point out that the themes treated by Levi-Civita are very topical. Specifically, we analyse how the mathematical formalism used nowadays to test General Relativity can be found in Levi-Civita'…

General relativityComputer sciencen-body problemn-body problemComplex systemPhysics - History and Philosophy of PhysicsFOS: Physical sciencesGeneral Physics and AstronomyAcceleration (differential geometry)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesSpace explorationCelestial mechanicsGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsTheory of relativity0103 physical sciencessymbolsHistory and Philosophy of Physics (physics.hist-ph)Einstein010306 general physicsSettore MAT/07 - Fisica Matematica010303 astronomy & astrophysicsThe European Physical Journal PLus
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Statistical physics: Some basic principles of fluctuation and noise theory

1983

Abstract Models have traditionally played a significant role in statistical mechanics. In view of the complexity of the system which statistical mechanics attempt to describe, this is not at all surprising. The study of simplified models has frequently revealed the underlying mathematical structure of many physical questions and in so doing the study of models has contributed directly to a clarification of several paradoxes which beset statistical mechanics. In this paper some of the models which appear to be useful for the discussion of non-equilibrium phenomena are examined in some detail. As usual these models are extremely simplified versions of the actual situations. It is, finally, as…

Generating FunctionPopulation DynamicStatistical mechanicsBartlett formalismNoise TheoryEpistemologyTheoretical physicsStochastic ProceNuclear Energy and EngineeringThe SymbolicNoise (video)Mathematical structureSettore ING-IND/19 - Impianti NucleariMathematicsAnnals of Nuclear Energy
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The Inverse Seesaw Family: Dirac And Majorana

2021

After developing a general criterion for deciding which neutrino mass models belong to the category of inverse seesaw models, we apply it to obtain the Dirac analogue of the canonical Majorana inverse seesaw model. We then generalize the inverse seesaw model and obtain a class of inverse seesaw mechanisms both for Majorana and Dirac neutrinos. We further show that many of the models have double or multiple suppressions coming from tiny symmetry breaking "$\mu$-terms". These models can be tested both in colliders and with the observation of lepton flavour violating processes.

Global SymmetriesPhysicsNuclear and High Energy PhysicsClass (set theory)010308 nuclear & particles physicsDirac (video compression format)High Energy Physics::PhenomenologyFOS: Physical sciencesInverse01 natural sciencesMAJORANATheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryBeyond Standard Model0103 physical scienceslcsh:QC770-798Neutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityHigh Energy Physics::ExperimentSymmetry breakingNeutrino010306 general physicsLepton
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On the canonical structure of higher-derivative field theories. The gravitational WZW-model

1992

Abstract A general expression for the symplectic structure of a higher-derivative lagrangian field theory is given. General relativity and the gravitational WZW-model are considered in this framework. In the second case we work out explicitly the Poisson bracket for both chiral solutions giving rise, in two different ways, to the classical exchange algebra of the SL q (2) group.

GravitationPhysicsNuclear and High Energy PhysicsPoisson bracketField (physics)General relativityGroup (mathematics)Structure (category theory)Field theory (psychology)Mathematics::Symplectic GeometryGeneral Theoretical PhysicsMathematical physicsSymplectic geometryPhysics Letters B
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Post-post-Newtonian effects on a clean nearly-Newtonian binary

1983

Etude du taux de changement temporel moyen de l'energie newtonienne et du moment d'une binaire presque newtonienne, ponctuelle. On trouve qu'il faut ajouter quelques termes post-post newtoniens non seculaires aux flux radiatifs seculaires standards. Les termes post-post newtoniens tendent vers zero pour l'observateur du centre de masse newtonien dans le cas de l'energie mais pas dans le cas du moment. Du fait de la longue periode de ces termes ils sont observationnellement significatifs, c'est-a-dire qu'ils vont apparaitre comme s'ils etaient des effets seculaires

GravitationPhysicsTheoretical physicsSpace and Planetary ScienceGravitational waveBinary starNewtonian fluidBinary numberAstronomy and AstrophysicsCenter of massMathematical physicsMonthly Notices of the Royal Astronomical Society
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Mapping nonlinear gravity into General Relativity with nonlinear electrodynamics

2018

We show that families of nonlinear gravity theories formulated in a metric-affine approach and coupled to a nonlinear theory of electrodynamics can be mapped into General Relativity (GR) coupled to another nonlinear theory of electrodynamics. This allows to generate solutions of the former from those of the latter using purely algebraic transformations. This correspondence is explicitly illustrated with the Eddington-inspired Born-Infeld theory of gravity, for which we consider a family of nonlinear electrodynamics and show that, under the map, preserve their algebraic structure. For the particular case of Maxwell electrodynamics coupled to Born-Infeld gravity we find, via this corresponden…

Gravity (chemistry)Physics and Astronomy (miscellaneous)Algebraic structureGeneral relativityFOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationlcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Metric-affine approachPhysics010308 nuclear & particles physicsNumerical analysisNonlinear theoryPower (physics)Nonlinear gravity theoriesNonlinear systemQuantum electrodynamicslcsh:QC770-798Regular Article - Theoretical Physics
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D6-brane model building onZ2×Z6: MSSM-like and left–right symmetric models

2015

Abstract We perform a systematic search for globally defined MSSM-like and left–right symmetric models on D6-branes on the T 6 / ( Z 2 × Z 6 × Ω R ) orientifold with discrete torsion. Our search is exhaustive for models that are independent of the value of the one free complex structure modulus. Preliminary investigations suggest that there exists one prototype of visible sector for MSSM-like and another for left–right symmetric models with differences arising from various hidden sector completions to global models. For each prototype, we provide the full matter spectrum, as well as the Yukawa and other three-point couplings needed to render vector-like matter states massive. This provides …

Hidden sectorQuarkPhysicsNuclear and High Energy PhysicsTheoretical physicsParticle physicsOrientifoldHigh Energy Physics::PhenomenologyYukawa potentialBraneAxionLeptonMinimal Supersymmetric Standard ModelNuclear Physics B
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Completion of the universal I-Love-Q relations in compact stars including the mass

2017

In a recent paper we applied a rigorous perturbed matching framework to show the amendment of the mass of rotating stars in Hartle's model. Here, we apply this framework to the tidal problem in binary systems. Our approach fully accounts for the correction to the Love numbers needed to obtain the universal $I$-Love-$Q$ relations. We compute the corrected mass vs radius configurations of rotating quark stars, revisiting a classical paper on the subject. These corrections allow us to find a universal relation involving the second-order contribution to the mass $\delta M$. We thus complete the set of universal relations for the tidal problem in binary systems, involving four perturbation param…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGravitational waveFOS: Physical sciencesPerturbation (astronomy)Binary numberAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesUniversal relationGeneral Relativity and Quantum CosmologyStarsTheoretical physicsQuark starSpace and Planetary Science0103 physical sciencesAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics
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Instability of twisted magnetar magnetospheres

2019

We present three-dimensional force-free electrodynamics simulations of magnetar magnetospheres that demonstrate the instability of certain degenerate, high energy equilibrium solutions of the Grad-Shafranov equation. This result indicates the existence of an unstable branch of twisted magnetospheric solutions and allows to formulate an instability criterion. The rearrangement of magnetic field lines as a consequence of this instability triggers the dissipation of up to 30% of the magnetospheric energy on a thin layer above the magnetar surface. During this process, we predict an increase of the mechanical stresses onto the stellar crust, which can potentially result in a global mechanical f…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsnumerical [Methods]bursts [X-rays]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsneutron [Stars]MagnetarInstabilitymagnetars [Stars]Theoretical physicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsCost actionAstrophysics - High Energy Astrophysical PhenomenaPartial supportSolar and Stellar Astrophysics (astro-ph.SR)Astronomía y Astrofísica
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