Search results for "Coupling"

showing 10 items of 1862 documents

Nonminimal dark sector physics and cosmological tensions

2019

We explore whether non-standard dark sector physics might be required to solve the existing cosmological tensions. The properties we consider in combination are an interaction between the dark matter and dark energy components, and a dark energy equation of state $w$ different from that of the canonical cosmological constant $w=-1$. In principle, these two parameters are independent. In practice, to avoid early-time, superhorizon instabilities, their allowed parameter spaces are correlated. We analyze three classes of extended interacting dark energy models in light of the 2019 Planck CMB results and Cepheid-calibrated local distance ladder $H_0$ measurements of Riess et al. (R19), as well …

PhysicsParticle physicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquation of state (cosmology)FOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsType (model theory)Coupling (probability)01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)13. Climate action0103 physical sciencesDark energysymbolsPlanck010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsQuintessence
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Dynamical Dark sectors and Neutrino masses and abundances

2020

We investigate generalized interacting dark matter-dark energy scenarios with a time-dependent coupling parameter, allowing also for freedom in the neutrino sector. The models are tested in the phantom and quintessence regimes, characterized by an equation of state $w_x-1$, respectively. Our analyses show that for some of the scenarios the existing tensions on the Hubble constant $H_0$ and on the clustering parameter $S_8$ can be significantly alleviated. The relief is either due to \textit{(a)} a dark energy component which lies within the phantom region; or \textit{(b)} the presence of a dynamical coupling in quintessence scenarios. The inclusion of massive neutrinos into the interaction …

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDegrees of freedom (physics and chemistry)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCoupling (probability)01 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologysymbols.namesakeCoupling parameter0103 physical sciencesDark energysymbolsNeutrino010303 astronomy & astrophysicsEnergy (signal processing)Hubble's lawQuintessenceAstrophysics - Cosmology and Nongalactic Astrophysics
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Lepton number asymmetries and the lower bound on the reheating temperature

2017

We show that the reheating temperature of a matter-domination era in the early universe can be pushed down to the neutrino decoupling temperature at around $2 \ {\rm MeV}$ if the reheating takes place through non-hadronic decays of the dominant matter and neutrino-antineutrino asymmetries are still large enough, $|L| \gtrsim \mathcal{O}(10^{-2})$ (depending on the neutrino flavor) at the end of reheating.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsNeutrino decouplingAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLepton numberUpper and lower boundsUniverseGeneral Relativity and Quantum Cosmology0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010303 astronomy & astrophysicsmedia_commonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Yukawa coupling corrections to the decay $H^+ \to W^+ A^0$

1998

We compute the fermionic radiative contributions to the decay $H^+ \to W^{+(*)} A^0$ in the framework of models with two Higgs doublets (2HDM), for the case of an on-shell and off-shell W. We show that, in the majority of the cases, current measurements of the $\rho$ parameter suggest $M_{H^{\pm}}\ge M_A$ and such decays could invalidate current charged Higgs searches or aid detection in the region $M_{H^{\pm}}\approx M_W$. We find that the radiative corrections may approach 50% for small values of $\tan\beta$.

PhysicsParticle physicsCurrent (mathematics)Physics and Astronomy (miscellaneous)High Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesApproxCoupling (probability)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Radiative transferHiggs bosonHigh Energy Physics::ExperimentEngineering (miscellaneous)The European Physical Journal C
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Search for axionlike dark matter with a liquid-state nuclear spin comagnetometer

2019

Physical review letters 122(19), 191302 (2019). doi:10.1103/PhysRevLett.122.191302

PhysicsParticle physicsField (physics)SpinsDark matterGeneral Physics and AstronomyOrder (ring theory)FOS: Physical sciencesCoupling (probability)01 natural sciences530High Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530010306 general physicsNucleonSpin (physics)Axion
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Evidence for the two pole structure of the Lambda(1405) resonance

2005

The K^- p --> pi^0 pi^0 Sigma^0 reaction is studied within a chiral unitary model. The distribution of pi^0 Sigma^0 states forming the Lambda(1405) shows, in agreement with a recent experiment, a peak at 1420 MeV and a relatively narrow width of Gamma = 38 MeV. The mechanism for the reaction is largely dominated by the emission of a pi^0 prior to the K^- p interaction leading to the Lambda(1405). This ensures the coupling of the Lambda(1405) to the K^- p channel, thus maximizing the contribution of the second state found in chiral unitary theories, which is narrow and of higher energy than the nominal Lambda(1405). This is unlike the pi^- p --> K^0 ��Sigma reaction, which gives more w…

PhysicsParticle physicsField theory (Physics)HyperonStructure (category theory)Teoria de camps (Física)FOS: Physical sciencesGeneral Physics and AstronomyResonanceFísicaState (functional analysis)Coupling (probability)LambdaLower energyPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Atomic physicsEnergy (signal processing)Particles (Nuclear physics)
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Discovering the h→Zγ decay in tt¯ associated production

2020

We explore the prospects to discover the $h \to Z \gamma$ decay in $t\bar t$-associated production, featuring a signal-to-background ratio of ${\cal O}(1)$. Performing a detailed analysis of the semi-leptonic $t \bar t $-decay channel, we demonstrate that the production mode could lead to a $\sim5\,\sigma$ discovery at the high-luminosity LHC, while the effective $h Z \gamma$ coupling could be extracted with a $\sim15\,\%$ accuracy. Extending the analysis to potential future $pp$ colliders with 27 TeV and 100 TeV center-of-mass energies, we also show that the latter would allow precision measurements at the few percent level, rendering possible precise extractions of the spin and CP propert…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCoupling (probability)01 natural sciences0103 physical sciencesHiggs bosonHigh Energy Physics::ExperimentProduction (computer science)010306 general physicsSpin-½Bar (unit)Physical Review D
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Search for Invisible Decays of a Dark Photon Produced in e+e− Collisions at BaBar

2017

We search for single-photon events in 53  fb^{-1} of e^{+}e^{-} collision data collected with the BABAR detector at the PEP-II B-Factory. We look for events with a single high-energy photon and a large missing momentum and energy, consistent with production of a spin-1 particle A^{'} through the process e^{+}e^{-}→γA^{'}; A^{'}→invisible. Such particles, referred to as "dark photons," are motivated by theories applying a U(1) gauge symmetry to dark matter. We find no evidence for such processes and set 90% confidence level upper limits on the coupling strength of A^{'} to e^{+}e^{-} in the mass range m_{A^{'}}≤8  GeV. In particular, our limits exclude the values of the A^{'} coupling sugges…

PhysicsParticle physicsMuon010308 nuclear & particles physicsElectron–positron annihilationDark matterGeneral Physics and AstronomyCoupling (probability)01 natural sciencesDark photonB-factoryNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentProduction (computer science)010306 general physicsBosonPhysical Review Letters
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A proposal to measure the hadronic contribution to the g-2 in the space-like region

2018

We propose a novel approach to determine the leading hadronic corrections to the muon g-2. It consists in a measurement of the effective electromagnetic coupling in the space-like region. This method may become feasible at flavor factories as well as with μ e scattering resulting in a determination potentially competitive with the dispersive approach via time-like data.

PhysicsParticle physicsMuon010308 nuclear & particles physicsScatteringPhysicsQC1-999HadronSpace (mathematics)01 natural sciencesMeasure (mathematics)0103 physical sciencesElectromagnetic couplingHigh Energy Physics::Experiment010306 general physicsEPJ Web of Conferences
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Search for Dimuon Decays of a Light Scalar Boson in Radiative Transitions Υ→γA0

2009

We search for evidence of a light scalar boson in the radiative decays of the {Upsilon}(2S) and {Upsilon}(3S) resonances: {Upsilon}(2S, 3S) {yields} {gamma}A{sup 0}, A{sup 0} {yields} {mu}{sup +}{mu}{sup -}. Such a particle appears in extensions of the Standaard Model, where a light CP-odd Higgs boson naturally couples strongly to b-quarks. We find no evidence for such processes in the mass range 0.212 {<=} m{sub A{sup 0}} {<=} 9.3 GeV in the samples of 99 x 10{sup 6} {Upsilon}(2S) and 122 x 10{sup 6} {Upsilon}(3S) decays collected by the BABAR detector at the PEP-II B-factory and set stringent upper limits on the effective coupling of the b quark to the A{sup 0}. We also limit the dimuon b…

PhysicsParticle physicsMuonMeson010308 nuclear & particles physicsBranching fractionParticle physicsGeneral Physics and AstronomyElementary particleBABAR detectorScalar bosonCoupling (probability)01 natural sciencesHEPParticle decayBaBar0103 physical sciencesFísica de partículesExperiments010306 general physicsBoson
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