Search results for "STANDARD MODEL"

showing 10 items of 1206 documents

Neutrino masses and their ordering: global data, priors and models

2018

We present a Bayesian analysis of the combination of current neutrino oscillation, neutrinoless double beta decay and CMB observations. Our major goal is to carefully investigate the possibility to single out one neutrino mass ordering, Normal Ordering or Inverted Ordering, with current data. Two possible parametrizations (three neutrino masses versus the lightest neutrino mass plus the two oscillation mass splittings) and priors (linear versus logarithmic) are examined. We find that the preference for NO is only driven by neutrino oscillation data. Moreover, the values of the Bayes factor indicate that the evidence for NO is strong only when the scan is performed over the three neutrino ma…

AstrofísicaPhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyCosmic background radiationFOS: Physical sciencesAstronomy and AstrophysicsObservableParameter space01 natural sciencesPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesPrior probabilityHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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A White Paper on keV sterile neutrino Dark Matter

2017

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting views and insights from all disciplines involved - cosmology, astrophysics, nuclear, and particle physics - in each case viewed from both theoretical and experimental/observational perspectives. After reviewing the role of active neutrinos in particle physics, astrophysics, and cosmology, we focus on sterile neutrinos in the context of the Dark Matter puzzle. Here, we first review the physics motivation for sterile neutrino Dark Matter, based on challenges and tensions in purely cold Dark Matter scenarios. We then round out the discussion by critically summarizing all known constraints on sterile neutrin…

AstrofísicaSterile neutrinocosmological modelCold dark mattercosmological neutrinosPhysics beyond the Standard Model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matter theory01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)White paperHigh Energy Physics - Phenomenology (hep-ph)X-RAY-EMISSIONMETALLIC MAGNETIC CALORIMETERSQUANTUM-FIELD THEORY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: dark matterCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection010303 astronomy & astrophysicsPhysicsdark matter theorynew physicsDOUBLE-BETA-DECAYhep-phneutrino: sterileCosmological neutrinos; Dark matter experiments; Dark matter theory; Particle physics - cosmology connection; Astronomy and AstrophysicsNuclear & Particles PhysicsHigh Energy Physics - Phenomenologyneutrino: detectorDark matter experimentsparticle physics - cosmology connectionastro-ph.COMILKY-WAY SATELLITESCosmological neutrinos3.5 KEV LINENeutrinoParticle Physics - ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GADark matterLY-ALPHA FORESTreviewFOS: Physical sciencesContext (language use)neutrino: productionX-raySettore FIS/05 - Astronomia e Astrofisica[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]RIGHT-HANDED NEUTRINOS0103 physical sciencesAstronomical And Space Sciencesnumerical calculationsDark matter experimentXMM-NEWTON OBSERVATIONSneutrino: modelParticle Physics - PhenomenologyDWARF SPHEROIDAL GALAXYCosmologia010308 nuclear & particles physicshep-exdark matter experimentsHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsAtomic Molecular Nuclear Particle And Plasma PhysicsCosmological neutrinoAstrophysics - Astrophysics of Galaxies13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Particle physics - cosmology connection[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentneutrino: oscillation[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Cosmology and Astroparticle Physics
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Cosmological analogies in the search for new physics in high-energy collisions

2020

In this paper, analogies between multiparticle production in high-energy collisions and the time evolution of the early universe are discussed. A common explanation is put forward under the assumption of an unconventional early state: a rapidly expanding universe before recombination (last scattering surface), followed by the CMB, later evolving up to present days, versus the formation of hidden/dark states in hadronic collisions followed by a conventional QCD parton shower yielding final-state particles. In particular, long-range angular correlations are considered pointing out deep connections between the two physical cases potentially useful for the discovery of new physics.

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciences01 natural sciencesMetric expansion of spaceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear Experiment010306 general physicsParton showerParticle Physics - Phenomenologymedia_commonPhysicsQuantum chromodynamics010308 nuclear & particles physicsScatteringTime evolutionhep-phUniverseHigh Energy Physics - Phenomenologyastro-ph.COAstrophysics - Cosmology and Nongalactic Astrophysics
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Electroweak baryogenesis from a dark sector

2017

Adding an extra singlet scalar $S$ to the Higgs sector can provide a barrier at tree level between a false vacuum with restored electroweak symmetry and the true one. This has been demonstrated to readily give a strong phase transition as required for electroweak baryogenesis. We show that with the addition of a fermionic dark matter particle $\chi$ coupling to $S$, a simple UV-complete model can realize successful electroweak baryogenesis. The dark matter gets a CP asymmetry that is transferred to the standard model through a $CP\ portal\ interaction$, which we take to be a coupling of $\chi$ to $\tau$ leptons and an inert Higgs doublet. The CP asymmetry induced in left-handed $\tau$ lepto…

Astrophysics and AstronomyParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)standard model of particle physicsPhysics beyond the Standard ModelSTANDARD MODELFOS: Physical sciences01 natural sciences7. Clean energy114 Physical sciencesdark matterHiggs sectorStandard Modelpimeä aineHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencesSINGLET010306 general physicsParticle Physics - PhenomenologyPhysicsta114010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::Phenomenologyhiukkasfysiikan standardimalliRADIATIVE NEUTRINO MASShep-phSphaleronBaryogenesisHigh Energy Physics - Phenomenologyastro-ph.COHiggs bosonPHASE-TRANSITIONHigh Energy Physics::ExperimentMATTERAstrophysics - Cosmology and Nongalactic Astrophysics
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Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background

2020

Sterile neutrinos with mass in the eV-scale and large mixings of order $\theta_0\simeq 0.1$ could explain some anomalies found in short-baseline neutrino oscillation data. Here, we revisit a neutrino portal scenario in which eV-scale sterile neutrinos have self-interactions via a new gauge vector boson $\phi$. Their production in the early Universe via mixing with active neutrinos can be suppressed by the induced effective potential in the sterile sector. We study how different cosmological observations can constrain this model, in terms of the mass of the new gauge boson, $M_\phi$, and its coupling to sterile neutrinos, $g_s$. Then, we explore how to probe part of the allowed parameter spa…

Astrophysics and AstronomySterile neutrinoParticle physicsScale (ratio)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesNeutrino oscillation010303 astronomy & astrophysicsParticle Physics - Phenomenologymedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Gauge boson010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyhep-phAstronomy and AstrophysicsUniverse3. Good healthSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Differential branching fractions and isospin asymmetries of B -> K ((*)) μ(+) μ(-) decays

2014

The isospin asymmetries of $B \to K\mu^+\mu^-$ and $B \to K^{*}\mu^+\mu^-$ decays and the partial branching fractions of the $B^0 \to K^0\mu^+\mu^-$, $B^+ \to K^+\mu^+\mu^-$ and $B^+ \to K^{*+}\mu^+\mu^-$ decays are measured as functions of the dimuon mass squared, $q^2$. The data used correspond to an integrated luminosity of 3$~$fb$^{-1}$ from proton-proton collisions collected with the LHCb detector at centre-of-mass energies of 7$\,$TeV and 8$\,$TeV in 2011 and 2012, respectively. The isospin asymmetries are both consistent with the Standard Model expectations. The three measured branching fractions, while individually consistent, all favour lower values than their respective Standard M…

B physic01 natural sciences7. Clean energyB physicsLuminosity/dk/atira/pure/sustainabledevelopmentgoals/clean_water_and_sanitationHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnuclearePhysics Particles & Fields[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]11.30.HvNuclear ExperimentQCPhysics02 Physical SciencesB physics; Branching fraction; Flavour Changing Neutral Currents; Hadron-Hadron Scattering; Rare decayPhysicsParticle physicsNuclear & Particles PhysicsFIS/01 - FISICA SPERIMENTALEIsospinPhysical SciencesBranching fractionFísica nuclearLHCSDG 6 - Clean Water and SanitationParticle Physics - ExperimentParticle physicsNuclear and High Energy Physics14.40.NdFlavour Changing Neutral CurrentsLHCb - Abteilung HofmannHadronsBranching (polymer chemistry)Standard Model0103 physical sciencesLeptonic semileptonic and radiative decays of bottom meson010306 general physicsFlavor symmetrieLarge Hadron Collider (France and Switzerland)01 Mathematical SciencesScience & TechnologyFlavour Changing Neutral CurrentHadron-Hadron Scattering010308 nuclear & particles physicshep-exGran Col·lisionador d'HadronsLHCbRare decay13.20.HeBottom mesons (|B|>0)High Energy Physics::ExperimentFísica de partículesExperimentsRare decay; Branching fraction; B physics; Flavour Changing Neutral Currents; Hadron-Hadron ScatteringFIS/04 - FISICA NUCLEARE E SUBNUCLEARE
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Angular analysis of charged and neutral B → Kμ + μ − decays

2014

The angular distributions of the rare decays B → K+µ+µ- and B0 → K0 <inf>a</inf>Sμ+μ- are studied with data corresponding to 3 fb-1 of integrated luminosity, collected in proton-proton collisions at 7 and 8TeV centre-of-mass energies with the LHCb detector. The angular distribution is described by two parameters, FH and the forward-backward asymmetry of the dimuon system AFB, which are determined in bins of the dimuon mass squared. The parameter F<inf>H</inf> is a measure of the contribution from (pseudo)scalar and tensor amplitudes to the decay width. The measurements of A<inf>FB</inf> and F<inf>H</inf> reported here are the most precise to d…

B physic12.15.MmB physicsSettore FIS/04 - Fisica Nucleare e SubnucleareLuminosityNeutral currentFlavor physicsMathematics::ProbabilityNuclear Experimentmedia_commonPhysicsB physics; Flavor physics; Flavour changing neutral currents; Hadron-hadron scattering; Rare decayPhysicsPHYSICS PARTICLES & FIELDSParticle physicsAmplitudePhysical SciencesFísica nuclearLHCNuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subject14.40.NdScalar (mathematics)Flavour Changing Neutral CurrentsMathematics::Analysis of PDEsLHCb - Abteilung HofmannHadronsMeasure (mathematics)AsymmetryMathematics::Numerical AnalysisStandard ModelAngular distributionTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYLeptonic semileptonic and radiative decays of bottom mesonSDG 7 - Affordable and Clean EnergyTensorLarge Hadron Collider (France and Switzerland)Science & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyHadron-Hadron ScatteringGran Col·lisionador d'HadronsFlavour changing neutral currentLHCbRare decay13.20.HeFlavor physicBottom mesons (|B|>0)High Energy Physics::ExperimentFísica de partículesExperiments
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Sensitivity to charged scalars in B -> D-(*)tau nu(tau) and B -> tau nu(tau) decays

2013

We analyze the recent experimental evidence for an excess of tau-lepton production in several exclusive semileptonic B-meson decays in the context of two-Higgs-doublet models. These decay modes are sensitive to the exchange of charged scalars and constrain strongly their Yukawa interactions. While the usual Type-II scenario cannot accommodate the recent BaBar data, this is possible within more general models in which the charged-scalar couplings to up-type quarks are not as suppressed. Both the B -> D-(*)tau nu(tau) and the B -> tau nu(tau) data can be fitted within the framework of the Aligned Two-Higgs-Doublet Model, but the resulting parameter ranges are in conflict with the constraints …

B-PhysicsBeyond Standard ModelHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentPartícules (Física nuclear)
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The Belle II Physics Book

2019

cd. autorów: L. Cao48,‡, G. Caria145,‡, G. Casarosa57,‡, C. Cecchi56,‡,D. Cˇ ervenkov10,‡,M.-C. Chang22,‡, P. Chang92,‡, R. Cheaib146,‡, V. Chekelian83,‡, Y. Chen154,‡, B. G. Cheon28,‡, K. Chilikin77,‡, K. Cho70,‡, J. Choi14,‡, S.-K. Choi27,‡, S. Choudhury35,‡, D. Cinabro170,‡, L. M. Cremaldi146,‡, D. Cuesta47,‡, S. Cunliffe16,‡, N. Dash33,‡, E. de la Cruz Burelo9,‡, E. de Lucia52,‡, G. De Nardo54,‡, †Editor. ‡Belle II Collaborator. §Theory or external contributing author. M. De Nuccio16,‡, G. De Pietro59,‡, A. De Yta Hernandez9,‡, B. Deschamps129,‡, M. Destefanis60,‡, S. Dey116,‡, F.Di Capua54,‡, S.Di Carlo75,‡, J. Dingfelder129,‡, Z. Doležal10,‡, I. Domínguez Jiménez125,‡, T.V. Dong30,26,…

B: semileptonic decayPhysics beyond the Standard ModelHadronelectroproduction [charmonium]General Physics and AstronomyComputingMilieux_LEGALASPECTSOFCOMPUTINGB: radiative decayannihilation [electron positron]7. Clean energy01 natural sciencescharmonium: electroproductionB physicsHigh Energy Physics - Experimentlaw.inventionHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Z'law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Charm (quantum number)dark sector searchesPhysicslifetimeradiative decay [B]doublet [Higgs particle]new physicsPhysicsHigh Energy Physics - Lattice (hep-lat)ddc:530Electroweak interactionlepton: flavor: violationhep-phParticle Physics - LatticeMonte Carlo [numerical calculations]electron positron: colliding beamsQuarkoniumasymmetry: CPquarkonium physicselectroweak interaction: penguinHigh Energy Physics - PhenomenologyImproved performancecolliding beams [electron positron]CP violationinterfaceelectroproduction [quarkonium]electroweak precision measurementsnumerical calculations: Monte CarlophysicsParticle Physics - ExperimentperformanceParticle physicsflavor: violation [lepton]reviewhep-latFOS: Physical sciencesBELLEHigh Energy Physics - Experiment; High Energy Physics - Experiment; High Energy Physics - Lattice; High Energy Physics - Phenomenologyelectron positron: annihilationquarkonium: electroproductionCP [asymmetry]E(6)Higgs particle: doubletmixing [D0 anti-D0]Theoretical physicsCP: violation: time dependenceHigh Energy Physics - LatticeKEK-B0103 physical sciencesquantum chromodynamicshidden sector [photon]ddc:530composite010306 general physicsColliderParticle Physics - PhenomenologyHigh Energy Physics - Experiment; High Energy Physics - Lattice; High Energy Physics - Phenomenologyphoton: hidden sectorhep-ex010308 nuclear & particles physics[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]C50 Other topics in experimental particle physicsviolation: time dependence [CP]D0 anti-D0: mixingB2TiP530 PhysikExperimental physicsB: leptonic decayCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]penguin [electroweak interaction]leptonic decay [B]semileptonic decay [B]charmparticle identificationexperimental results
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New physics in $B$ meson mixing: future sensitivity and limitations

2020

The mixing of neutral mesons is sensitive to some of the highest scales probed in laboratory experiments. In light of the planned LHCb Upgrade II, a possible upgrade of Belle II, and the broad interest in flavor physics in the tera-Z phase of the proposed FCC-ee program, we study constraints on new physics contributions to Bd and Bs mixings which can be obtained in these benchmark scenarios. We explore the limitations of this program, and identify the measurement of |Vcb| as one of the key ingredients in which progress beyond current expectations is necessary to maximize future sensitivity. We speculate on possible solutions to this bottleneck. Given the current tension with the standard mo…

BELLE: upgradeLHC-B: upgradeParticle physicsMesonPhysics beyond the Standard ModelFOS: Physical sciences01 natural sciencesAtomicStandard ModelHigh Energy Physics - ExperimentPhenomenological aspects of field theoryHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Particle and Plasma Physicseffective field theory0103 physical sciencesEffective field theory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]B mesonNuclearmeson: mixing010306 general physicsMixing (physics)PhysicsQuantum Physics010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixhep-exMolecularhep-phFCC-eesensitivityNuclear & Particles Physicsgeneral methodsHigh Energy Physics - PhenomenologyUpgradeCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentluminosity: highAstronomical and Space Sciences
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