Search results for " Low"

showing 10 items of 972 documents

Update of the search for charginos nearly mass-degenerate with the lightest neutralino

2000

The data collected by DELPHI in 1998 at the centre-of-mass energy of 189 GeV have been used to update the search for charginos nearly mass-degenerate with the lightest supersymmetric particle, which is assumed to be the lightest neutralino. Mass differences below \Delta M = 3 GeV/c^2 are considered. No excess of events with respect to the Standard Model expectation has been observed, and exclusions in the plane of \Delta M versus chargino mass are given. The new \Delta M independent lower limit on the mass of the chargino is 62.4 GeV/c^2 in the higgsino scenario (which includes the gaugino mass unification scenario), if all sfermions are heavier than the lightest chargino. In the approximat…

Nuclear and High Energy PhysicsParticle physicsCOLLISIONSField (physics)LOWEST ORDER CALCULATIONSENERGIESMONTE-CARLO SIMULATIONFOS: Physical sciences2-PHOTON PROCESSES01 natural sciencesLightest Supersymmetric ParticlePartícules (Física nuclear)Standard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)MONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; RADIATIVE-CORRECTIONS; 2-PHOTON PROCESSES; COLLISIONS; ENERGIES; PROGRAMChargino0103 physical sciencesPROGRAM[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONSHiggsino010306 general physicsNuclear ExperimentDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGauginoLEPLARGE ELECTRON POSITRON COLLIDERSfermionNeutralinoPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentParticle Physics - Experiment
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Neutrino Mass from Cosmology

2012

Neutrinos can play an important role in the evolution of the Universe, modifying some of the cosmological observables. In this contribution we summarize the main aspects of cosmological relic neutrinos and we describe how the precision of present cosmological data can be used to learn about neutrino properties, in particular their mass, providing complementary information to beta decay and neutrinoless double-beta decay experiments. We show how the analysis of current cosmological observations, such as the anisotropies of the cosmic microwave background or the distribution of large-scale structure, provides an upper bound on the sum of neutrino masses of order 1 eV or less, with very good p…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Article SubjectCosmic microwave backgroundFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyUpper and lower boundsPartícules (Física nuclear)CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyObservableBeta decaylcsh:QC1-999High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Bounds on very low reheating scenarios after Planck

2015

9 pages.- 9 figures

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaEarly universeFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsUpper and lower boundsCosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisPlanckPhysicsCosmology Big Bang NucleosynthesisOscillationHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologysymbolsProduction (computer science)High Energy Physics::ExperimentNeutrinoAstrophysics - Cosmology and Nongalactic AstrophysicsPrimordial abundance
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SUSY-GUTs, SUSY-Seesaw and the Neutralino Dark Matter

2007

19 pages, 7 figures.-- ISI Article Identifier: 000249788800048.-- ArXiv pre-print available at: http://arxiv.org/abs/0704.3518

Nuclear and High Energy PhysicsParticle physicsDark matterFOS: Physical sciencesAstrophysics01 natural sciencesUpper and lower bounds[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesGUTFlavor violation010306 general physicsPhysics[PHYS]Physics [physics]Relic density010308 nuclear & particles physicsAstrophysics (astro-ph)Yukawa potentialSupersymmetryCMB cold spotSupersymmetry phenomenologyHigh Energy Physics - PhenomenologyProbe WMAP observations[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]NeutralinoStau coannihilationNeutrinoMSSM
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Constraining neutrinoless double beta decay

2011

A class of discrete flavor-symmetry-based models predicts constrained neutrino mass matrix schemes that lead to specific neutrino mass sum-rules (MSR). We show how these theories may constrain the absolute scale of neutrino mass, leading in most of the cases to a lower bound on the neutrinoless double beta decay effective amplitude.

Nuclear and High Energy PhysicsParticle physicsFOS: Physical sciences01 natural sciencesUpper and lower boundsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationAbsolute scaleNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaMass matrixHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics::ExperimentNeutrino
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Novel mechanism for primordial perturbations in minimal extensions of the Standard Model

2020

Abstract We demonstrate that light spectator fields in their equilibrium can source sizeable CMB anisotropies through modulated reheating even in the absence of direct couplings to the inflaton. The effect arises when the phase space of the inflaton decay is modulated by the spectator which generates masses for the decay products. We call the mechanism indirect modulation and using the stochastic eigenvalue expansion show that it can source perturbations even four orders of magnitude larger than the observed amplitude. Importantly, the indirect mechanism is present in the Standard Model extended with right- handed neutrinos. For a minimally coupled Higgs boson this leads to a novel lower bo…

Nuclear and High Energy PhysicsParticle physicsHiggs Physicshiukkasfysiikka114 Physical sciences01 natural sciencesUpper and lower boundsPhysics Particles & FieldsStandard Model0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicscosmology of theories beyond the SM0206 Quantum PhysicsPhysicsScience & Technology0105 Mathematical Physics010308 nuclear & particles physicsHiggsin bosoniPhysicshep-thHigh Energy Physics::PhenomenologyHiggs physicshep-phInflatonCosmology of Theories beyond the SMNuclear & Particles PhysicsAmplitudeOrders of magnitude (time)Phase spacePhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma Physicsastro-ph.COHiggs bosonlcsh:QC770-798NeutrinoJournal of High Energy Physics
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Single intermediate vector boson production in e(+)e(-) collisions at root s=183 and 189 GeV

2001

The cross sections for the production of single charged and neutral intermediate vector bosons were measured using integrated luminosities of 52 pb-1 and 154 pb-1 collected by the experiment at centre-of-mass energies of 182.6 GeV and 188.6 GeV, respectively. The cross sections for the reactions were determined in limited kinematic regions. The results found are in agreement with the Standard Model predictions for these channels. © 2001 Elsevier Science B.V.

Nuclear and High Energy PhysicsParticle physicsLOWEST ORDER CALCULATIONSMONTE-CARLO SIMULATIONFOS: Physical sciences2-PHOTON PROCESSESKinematics01 natural sciencesPartícules (Física nuclear)Standard ModelVector bosonHigh Energy Physics - ExperimentPHYSICSHigh Energy Physics - Experiment (hep-ex)BHABHA SCATTERINGLEP20103 physical sciencesPROGRAM[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]DELPHIPhysics010304 chemical physics010308 nuclear & particles physicsCOUPLINGSLARGE ELECTRON POSITRON COLLIDERPhysique atomique et nucléaire3. Good healthMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; 2-PHOTON PROCESSES; BHABHA SCATTERING; PROGRAM; DELPHI; COUPLINGS; COLLIDERS; PHYSICS; LEP2COLLIDERSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSProduction (computer science)High Energy Physics::ExperimentParticle Physics - Experiment
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Admixture of quasi-Dirac and Majorana neutrinos with tri-bimaximal mixing

2011

7 páginas, 1 tabla.-- El Pdf es la versión pre-print: arXiv:1104.4961v2

Nuclear and High Energy PhysicsParticle physicsNeutrino hierarchyDiscrete symmetriesFOS: Physical sciences01 natural sciencesUpper and lower boundsHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesTri-bimaximal mixingNeutrino masses and mixingsNeutrinoless double beta decay010306 general physicsMixing (physics)Majorana equationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFlavor symmetries3. Good healthMassless particleMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoLepton
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Mass Varying Neutrinos in the Sun

2005

In this work we study the phenomenological consequences of the dependence of mass varying neutrinos on the neutrino density in the Sun, which we precisely compute in each point along the neutrino trajectory. We find that a generic characteristic of these scenarios is that they establish a connection between the effective Delta m^2 in the Sun and the absolute neutrino mass scale. This does not lead to any new allowed region in the oscillation parameter space. On the contrary, due to this effect, the description of solar neutrino data worsens for large absolute mass. As a consequence a lower bound on the level of degeneracy can be derived from the combined analysis of the solar and KamLAND da…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoFOS: Physical sciencesParameter spaceAstrophysics01 natural sciences7. Clean energyUpper and lower boundsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsStandard solar model010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaSolar neutrino problemHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Improved measurements of cross sections and asymmetries at the Z0 resonance

1994

During the 1992 running period of the LEP e+e- collider, the DELPHI experiment accumulated approximately 24 pb-1 of data at the Z0 peak. The decays into hadrons and charged leptons have been analysed to give values for the cross sections and leptonic forward-backward asymmetries which are significantly improved with respect to those previously published by the DELPHI collaboration. Incorporating these new data, more precise values for the Z0 resonance parameters are obtained from model-independent fits. The results are interpreted within the framework of the Standard Model, yielding for the top quark mass m(t) = 157(-48)+36(expt.)-20(+19)(Higgs) GeV, and for the effective mixing angle sin2 …

Nuclear and High Energy PhysicsParticle physicsTop quarkLUND MONTE-CARLOElectron–positron annihilationLEP-SLC ENERGIESElementary particle7. Clean energy01 natural sciencesJET FRAGMENTATIONStandard ModelPHYSICSNuclear physicsBHABHA SCATTERINGParticle decay0103 physical sciencesPROGRAM[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONSZ0010306 general physicsDELPHIPhysicsLOWEST-ORDER CALCULATIONScross section010308 nuclear & particles physicsDELPHI; Bhabha scattering; cross section; Z0High Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERLUND MONTE-CARLO; ELECTRON-POSITRON COLLISIONS; LOWEST-ORDER CALCULATIONS; LEP-SLC ENERGIES; BHABHA SCATTERING; RADIATIVE-CORRECTIONS; JET FRAGMENTATION; PROGRAM; PHYSICSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderHiggs bosonPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentELECTRON-POSITRON COLLISIONSParticle Physics - ExperimentLepton
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