Search results for " asymmetry."

showing 10 items of 257 documents

Baryogenesis in the two doublet and inert singlet extension of the Standard Model

2016

We investigate an extension of the Standard Model containing two Higgs doublets and a singlet scalar field (2HDSM). We show that the model can have a strongly first-order phase transition and give rise to the observed baryon asymmetry of the Universe, consistent with all experimental constraints. In particular, the constraints from the electron and neutron electric dipole moments are less constraining here than in pure two-Higgs-doublet model (2HDM). The two-step, first-order transition in 2HDSM, induced by the singlet field, may lead to strong supercooling and low nucleation temperatures in comparison with the critical temperature, $T_n \ll T_c$, which can significantly alter the usual pha…

Phase transitionCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciences7. Clean energy01 natural sciencesMolecular physicsStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencescosmological phase transitionstwo-Higgs-doublet modelsSinglet state010306 general physicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsextensions of the Standard ModelBaryogenesisHigh Energy Physics - Phenomenologyscalar fieldsHiggs bosonbaryon asymmetryScalar fieldAstrophysics - Cosmology and Nongalactic Astrophysics
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GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

Physics and Astronomy (miscellaneous)AstronomyGravitational wave detection Gravitational wave sources Gravitational waves Astronomical black holesagn discsAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & Fieldsstar-clustersgravitational waves black holesgravitational waves; black holesAGN DISCSgravitational waves; black holes; LIGO; Virgoblack holegeneral relativityLIGOgravitational waveQCQBPhysicsSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)GRAVITATIONAL WAVE-FORMSPROGENITORSCOMPACT BINARIESblack hole: spinPhysicsPERTURBATIONSgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave detectionAstrophysics - High Energy Astrophysical PhenomenaMETALLICITYmass: asymmetrymetallicitydata analysis methodGeneral relativityMERGERSgr-qcAstrophysics::High Energy Astrophysical PhenomenamultipolePREDICTIONSFOS: Physical sciencesgravitational wavesblack holesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionGravitational wavesGeneral Relativity and Quantum CosmologyTheory of relativityBinary black holeSettore FIS/05 - Astronomia e AstrofisicaAstronomical black holesbinary: coalescence0103 physical sciencesnumerical methodsddc:530STAR-CLUSTERS010306 general physicsnumerical calculationsSTFCAstrophysiqueGravitational wave sourcesScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKblack hole: massMass ratioblack holesLIGOEVOLUTIONgravitational radiation detectorBlack holedetector: sensitivityPhysics and Astronomyblack hole: binaryrelativity theorygravitational radiation: emissionmass ratioMultipole expansion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physics
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Theory of Neutrino Masses and Mixing

2002

In this talk I will review our present knowledge on neutrino masses and mixing trying to emphasize what has been definitively proved and what is in the process of being probed. I will also discuss the most important theoretical implications of these results: the existence of new physics, the estimate of the scale of this new physics as well as some other possible consequences such as leptogenesis origin of the baryon asymmetry.

PhysicsHigh Energy Physics - PhenomenologyNuclear and High Energy PhysicsParticle physicsBaryon asymmetryHigh Energy Physics - Phenomenology (hep-ph)LeptogenesisPhysics beyond the Standard ModelFOS: Physical sciencesNeutrinoAtomic and Molecular Physics and OpticsMixing (physics)Particle Physics - Phenomenology
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Links between CP violation in leptogenesis and low energy supersymmetry

2008

The seesaw mechanism makes leptogenesis a very attractive solution to the baryon asymmetry problem. If the baryon asymmetry of the Universe (BAU) was made via leptogenesis, any observation of CP violation in the lepton sector, for instance CP violation in neutrino oscillations, would support leptogenesis by demonstrating that CP is not a symmetry of leptons. The question is whether a stronger link exists between CP violation at low energies and leptogenesis. In our work we address this question, in the framework of a supersymmetric scenario where new constraints given by the low energy footprints of the high energy theory can be imposed, namely the current experimental bounds on lepton flav…

PhysicsHistoryParticle physicsHigh Energy Physics::PhenomenologySupersymmetrySymmetry (physics)Computer Science ApplicationsEducationBaryon asymmetrySeesaw mechanismLeptogenesisCP violationHigh Energy Physics::ExperimentNeutrino oscillationLeptonJournal of Physics: Conference Series
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WIMPy baryogenesis with sterile neutrinos

2015

In this talk we propose a mechanism for baryogenesis from particle decays or annihilations that can work at the TeV scale. Some heavy particles annihilate or decay into a heavy sterile neutrino N (with M 1 TeV) and a "light" one ν (with m 100 GeV), generating an asymmetry among the two helicity degrees of freedom of v. This asymmetry is partially transferred to Standard Model leptons via fast Yukawa interactions and reprocessed into a baryon asymmetry by the electroweak sphalerons. We illustrate this mechanism in a WIMPy baryogenesis model where the helicity asymmetry is generated in the annihilation of dark matter. This model connects the baryon asymmetry, dark matter, and neutrino masses.

PhysicsHistoryParticle physicsSterile neutrinoAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectHigh Energy Physics::PhenomenologyDark matterElectroweak interactionAsymmetryComputer Science ApplicationsEducationBaryogenesisNuclear physicsBaryon asymmetryHigh Energy Physics::ExperimentNeutrinoLeptonmedia_commonJournal of Physics: Conference Series
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Baryogenesis from a right-handed neutrino condensate

2010

We show that the baryon asymmetry of the Universe can be generated by a strongly coupled right handed neutrino condensate which also drives inflation. The resulting model has only a small number of parameters, which completely determine not only the baryon asymmetry of the Universe and the mass of the right handed neutrino but also the inflationary phase. This feature allows us to make predictions that will be tested by current and planned experiments. As compared to the usual approach our dynamical framework is both economical and predictive.

PhysicsInflation (cosmology)Strongly coupledNuclear and High Energy PhysicsParticle physicsRight handedHigh Energy Physics::PhenomenologyPhase (waves)FOS: Physical sciencesFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsBaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetryHigh Energy Physics::ExperimentNeutrinoJournal of High Energy Physics
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Excitation energy dependence of fragment-mass distributions from fission of 180,190 Hg formed in fusion reactions of 36 Ar + 144,154 Sm

2015

Physics letters / B 748, 89 - 94 (2015). doi:10.1016/j.physletb.2015.06.068

PhysicsNuclear and High Energy PhysicsMass asymmetryCluster decayIsotopeFissionNuclear Theory180190HgFusion–fissionActinide530lcsh:QC1-999Mass asymmetric fissionMass spectrumNuclear fusionddc:530Atomic physicsNuclear Experimentlcsh:PhysicsExcitationPhysics Letters B
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Tri/Bi-maximal lepton mixing and leptogenesis

2009

In models with flavour symmetries added to the gauge group of the Standard Model the CP-violating asymmetry necessary for leptogenesis may be related with low-energy parameters. A particular case of interest is when the flavour symmetry produces exact Tri-Bimaximal lepton mixing leading to a vanishing CP-violating asymmetry. In this paper we present a model-independent discussion that confirms this always occurs for unflavoured leptogenesis in type I see-saw scenarios, noting however that Tri-Bimaximal mixing does not imply a vanishing asymmetry in general scenarios where there is interplay between type I and other see-saws. We also consider a specific model where the exact Tri-Bimaximal mi…

PhysicsNuclear and High Energy PhysicsParticle physics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy010308 nuclear & particles physicsmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesAsymmetrySymmetry (physics)Standard Model (mathematical formulation)High Energy Physics - PhenomenologyBaryon asymmetryHigh Energy Physics - Phenomenology (hep-ph)Gauge groupLeptogenesis0103 physical sciencesCP violationHigh Energy Physics::ExperimentSDG 7 - Affordable and Clean Energy010306 general physicsMixing (physics)media_commonParticle Physics - Phenomenology
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CP Violation in the SUSY Seesaw: Leptogenesis and Low Energy

2008

We suppose that the baryon asymmetry is produced by thermal leptogenesis (with flavour effects), at temperatures $\sim 10^{9} - 10^{10}$ GeV, in the supersymmetric seesaw with universal and real soft terms. The parameter space is restricted by assuming that $l_\alpha \to l_\beta \gamma$ processes will be seen in upcoming experiments. We study the sensitivity of the baryon asymmetry to the phases of the lepton mixing matrix, and find that leptogenesis can work for any value of the phases. We also estimate the contribution to the electric dipole moment of the electron, arising from the seesaw, and find that it is (just) beyond the sensitivity of next generation experiments ($\lsim 10^{-29} e$…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixFísicaFOS: Physical sciencesSupersymmetryParameter space01 natural sciencesHigh Energy Physics - PhenomenologyElectric dipole momentBaryon asymmetryHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryLeptogenesis[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesCP violation010306 general physics
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Is the baryon asymmetry of the Universe related to galactic magnetic fields?

2009

A tiny hypermagnetic field generated before the electroweak phase transition (EWPT) associated to the generation of elementary particle masses can polarize the early Universe hot plasma at huge redshifts z >= 10(15). The anomalous violation of the right-handed electron current characteristic of the EWPT converts the lepton asymmetry into a baryon asymmetry. Under reasonable approximations, the magnetic field strength inferred by requiring such "leptogenic'' origin for the observed baryon asymmetry of the Universe matches the large-scale cosmological magnetic field strengths estimated from current astronomical observations.

PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::PhenomenologyFOS: Physical sciencesFísicaMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetryElectron currentHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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