Search results for "MBD"

showing 10 items of 646 documents

Astrophysical constraints on extended gravity models

2015

We investigate the propagation of gravitational waves in the context of fourth order gravity nonminimally coupled to a massive scalar field. Using the damping of the orbital period of coalescing stellar binary systems, we impose constraints on the free parameters of extended gravity models. In particular, we find that the variation of the orbital period is a function of three mass scales which depend on the free parameters of the model under consideration; we can constrain these mass scales from current observational data.

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Wave propagationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyTheory of relativityPulsarBinary starRELATIVITYphysics of the early universemodified gravityCOSMOLOGICAL CONSTANTANISOTROPYPhysicsGravitational waveAstronomy and AstrophysicsSUPERNOVAEPULSARgravitational waves / theoryLAMBDASupernovaStarsDERIVATIVE QUANTUM-GRAVITY; COSMOLOGICAL CONSTANT; LAGRANGIANS; RELATIVITY; SUPERNOVAE; ANISOTROPY; LAMBDA; PULSARClassical mechanicsHigh Energy Physics - Theory (hep-th)LAGRANGIANSDERIVATIVE QUANTUM-GRAVITYAstrophysics - Cosmology and Nongalactic Astrophysics
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Effective interactions in Ricci-Based Gravity below the non-metricity scale

2020

We show how minimally-coupled matter fields of arbitrary spin, when coupled to Ricci-Based Gravity theories, develop non-trivial effective interactions that can be treated perturbatively only below a characteristic high-energy scale $\Lambda_Q$. Our results generalize to arbitrary matter fields those recently obtained for spin 1/2 fields in \cite{Latorre:2017uve}. We then use this interactions to set bounds on the high-energy scale $\Lambda_Q$ that controls departures of Ricci-Based Gravity theories from General Relativity. Particularly, for Eddington-inspired Born-Infeld gravity we obtain the strong bound $ |\kappa|<3.5 \times 10^{-14} \text{ m}^5 \text{kg}^{-1}\text{s}^{-2} $.

High Energy Physics - TheoryGravity (chemistry)Physics and Astronomy (miscellaneous)General relativityFOS: Physical sciencesScale (descriptive set theory)lcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Lambda01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics - Phenomenology (hep-ph)Born–Infeld model0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Spin-½Mathematical physicsPhysics010308 nuclear & particles physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798
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Differential Regularization of a Non-relativistic Anyon Model

1994

Differential regularization is applied to a field theory of a non-relativistic charged boson field $\phi$ with $\lambda (\phi {}^{*} \phi)^2$ self-interaction and coupling to a statistics-changing $U(1)$ Chern-Simons gauge field. Renormalized configuration-space amplitudes for all diagrams contributing to the $\phi {}^{*} \phi {}^{*} \phi \phi$ 4-point function, which is the only primitively divergent Green's function, are obtained up to 3-loop order. The renormalization group equations are explicitly checked, and the scheme dependence of the $\beta$-function is investigated. If the renormalization scheme is fixed to agree with a previous 1-loop calculation, the 2- and 3-loop contributions …

High Energy Physics - TheoryPhysicsFOS: Physical sciencesLie groupFísicaRenormalization groupSymmetry groupLambdaRenormalizationHigh Energy Physics - Theory (hep-th)Quantum mechanicsRegularization (physics)Gauge theoryBoson
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Dark energy cosmologies for codimension-two branes

2005

A six-dimensional universe with two branes in the "football-shaped" geometry leads to an almost realistic cosmology. We describe a family of exact solutions with time dependent characteristic size of internal space. After a short inflationary period the late cosmology is either of quintessence type or turns to a radiation dominated Friedmann universe where the cosmological constant appears as a free integration constant of the solution. The radiation dominated universe with relativistic fermions is analyzed in detail, including its dimensional reduction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBig RipFOS: Physical sciencesNon-standard cosmologyLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsMetric expansion of spaceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyScale factor (cosmology)
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Gravitational waves in the presence of a cosmological constant

2011

We derive the effects of a non-zero cosmological constant $\Lambda$ on gravitational wave propagation in the linearized approximation of general relativity. In this approximation we consider the situation where the metric can be written as $g_{\mu\nu}= \eta_{\mu\nu}+ h_{\mu\nu}^\Lambda + h_{\mu\nu}^W$, $h_{\mu\nu}^{\Lambda,W}<< 1$, where $h_{\mu\nu}^{\Lambda}$ is the background perturbation and $h_{\mu\nu}^{W}$ is a modification interpretable as a gravitational wave. For $\Lambda \neq 0$ this linearization of Einstein equations is self-consistent only in certain coordinate systems. The cosmological Friedmann-Robertson-Walker coordinates do not belong to this class and the derived linearized…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmologiaGravitational waveGeneral relativityPlane waveFísicaFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)LambdaGeneral Relativity and Quantum CosmologyGravitational wavesCosmologySupernovaGeneral Relativity and Quantum CosmologyAmplitudeHigh Energy Physics - Theory (hep-th)Ones gravitacionalsQuantum mechanicsMinkowski space
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Limits on the parameters of the equation of state for interacting dark energy

2010

Under the assumption that cold dark matter and dark energy interact with each other through a small coupling term, $Q$, we constrain the parameter space of the equation of state $w$ of those dark energy fields whose variation of the field since last scattering do not exceed Planck's mass. We use three parameterizations of $w$ and two different expressions for $Q$. Our work extends previous ones.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsEquation of stateCosmology and Nongalactic Astrophysics (astro-ph.CO)Hot dark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyThermodynamics of the universeHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum electrodynamicsMixed dark matterWarm dark matterDark energyLight dark matterDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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p−p, p−Λ, and Λ−Λ correlations studied via femtoscopy in pp reactions at √s = 7 TeV

2019

We report on the first femtoscopic measurement of baryon pairs, such as p−p, p−Λ, and Λ−Λ, measured by ALICE at the Large Hadron Collider (LHC) in proton-proton collisions at √s=7 TeV. This study demonstrates the feasibility of such measurements in pp collisions at ultrarelativistic energies. The femtoscopy method is employed to constrain the hyperon-nucleon and hyperon-hyperon interactions, which are still rather poorly understood. A new method to evaluate the influence of residual correlations induced by the decays of resonances and experimental impurities is hereby presented. The p−p, p−Λ, and Λ−Λ correlation functions were fitted simultaneously with the help of a new tool developed spec…

High Energy Physics::Experimentproton-proton collisionslambda baryonshiukkasfysiikkaNuclear Experiment
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Hidden charm N and Delta resonances with heavy-quark symmetry

2013

A model is developed to describe odd-parity baryon resonances generated dynamically through a unitary baryon-meson coupled-channels approach. The scheme applies to channels with light- and/or heavy-quark content. Distinct features of the model are that i) the interaction is an S-wave contact one, ii) it reduces to the SU(3) Weinberg-Tomozawa Hamiltonian when light pseudoscalar mesons are involved, thus respecting chiral symmetry, iii) spin-flavor is preserved in the light-quark sector, and iv) heavy-quark spin symmetry is fulfilled in the heavy-quark sector. In particular, baryon-meson states with different content in c or in (c) over bar do not mix. The model is a minimal one and it contai…

High Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaCHIRAL DYNAMICSMESON-BARYON SCATTERINGMASSCOUPLED-CHANNELLAMBDA(+)(C)MODELHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)CHROMODYNAMICSSTATESUnitary Spin IndepenceUNITARY SPIN INDEPENDENCEKAON-NUCLEON INTERACTIONSHigh Energy Physics::ExperimentNuclear ExperimentKaon-nucleon interactions
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Recent results on mesonic weak decay of Λ-hypernuclei

2010

The FINUDA experiment has performed a systematic study of mesonic weak decay of p-shell Λ-hypernuclei. Recent results on the mesonic decay spectra and ratios are illustrated and discussed.

Hypernuclei; mesonic weak decayPhysicsNuclear and High Energy PhysicsFINUDANuclear TheoryLambda-hypernucleiΛ-hypernucleiGeneral Physics and AstronomyLambda-hypernuclei; mesonic decay; spin assignmentAstrophysicsMesonic decayLambdaSpectral lineNuclear physicsSpin assignmentmesonic weak decayΛ-hypernuclei; Mesonic decay; Spin assignmentHypernucleiHigh Energy Physics::ExperimentNuclear Experiment
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Rapidity correlations in Lambda baryon and proton production in hadronic Z0 decays

1998

In an analysis of multihadronic events recorded at LEP by DELPHI in the years 1992 through 1994, charged hadrons are identified using the measurement of their energy loss and their Cherenkov angle. Rapidity correlations of \La-\La, proton-proton, and \La-proton pairs are compared. The agreement with the string and cluster fragmentation models is tested. For those pairs that frame a meson in terms of rapidity the compensation of strangeness is studied. For \La{}$\overline{\mathrm{p}}$ pairs the additional correlation with respect to charged kaons is analysed.

IMAGING CHERENKOV DETECTOR; DELPHIParticle physicsNuclear and High Energy PhysicsMesonElectron–positron annihilationHadronNuclear TheoryStrangenessLambdaLambda baryon01 natural sciencesPartícules (Física nuclear)Nuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Rapidity010306 general physicsNuclear ExperimentDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERIMAGING CHERENKOV DETECTORLarge Electron–Positron ColliderPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentParticle Physics - Experiment
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