Search results for "GRAVITY"

showing 10 items of 537 documents

Update of the search for supersymmetric particles in scenarios with Gravitino LSP and Sleptons NLSP

2001

An update of the search for sleptons, neutralinos and charginos in the context of scenarios where the lightest supersymmetric particle is the gravitino and the next-to-lightest supersymmetric particle is a slepton, is presented, together with the update of the search for heavy stable charged particles in light gravitino scenarios and Minimal Supersymmetric Standard Models. Data collected in 1999 with the DELPHI detector at centre-of-mass energies around 192, 196, 200 and 202 GeV were analysed. No evidence for the production of these supersymmetric particles was found. Hence, new mass limits were derived at 95% confidence level.

NEUTRALINOSNuclear and High Energy PhysicsParticle physicsMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; E(+)E(-) COLLISIONS; 2-PHOTON PROCESSES; PAIR PRODUCTION; MISSING ENERGY; STAU NLSP; BREAKING; SUPERGRAVITY; NEUTRALINOSLOWEST ORDER CALCULATIONSPAIR PRODUCTIONMONTE-CARLO SIMULATIONFOS: Physical sciences2-PHOTON PROCESSESContext (language use)01 natural sciencesLightest Supersymmetric ParticlePartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SUPERGRAVITY010306 general physicsDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLARGE ELECTRON POSITRON COLLIDERCharged particleSTAU NLSPPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIParticlePARTICLE PHYSICSMISSING ENERGYGravitinoFísica nuclearHigh Energy Physics::ExperimentParticle Physics - ExperimentBREAKING
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What is the final state of a black hole merger?

2018

In this short paper we discuss the possibility of testing the nature of astrophysical black holes using the recently observed black hole mergers. We investigate the possibility that a secondary black hole is created in the merger of two astrophysical black holes and discuss potential astrophysical signatures. We point out that black hole mergers are a possible astrophysical mechanism for the creation of quantum black holes with masses close to the Planck mass.

Nuclear and High Energy PhysicsBlack holeAstrophysics::High Energy Astrophysical PhenomenaShort paperPlanck massFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesquantum black holes.10. No inequality010306 general physicsQuantumQBPhysics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsBlack holeblack hole mergerquantum gravityQuantum gravityModern Physics Letters A
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Standard and Z2-Regge theory in two dimensions

1998

Abstract We qualitatively compare two versions of quantum Regge calculus by means of Monte Carlo simulations. In Standard Regge Calculus the quadratic link lengths of the triangulation vary continuously, whereas in the Z2-Regge Model they are restricted to two possible values. The goal is to determine whether the computationally more easily accessible Z2 model retains the characteristics of standard Regge theory.

Nuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyMonte Carlo methodTriangulation (social science)Regge calculusAtomic and Molecular Physics and OpticsRegge theoryHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyQuadratic equationQuantum electrodynamicsQuantum gravityHigh Energy Physics::ExperimentStatistical physicsLink (knot theory)QuantumMathematicsNuclear Physics B - Proceedings Supplements
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Measurement of quantum states of neutrons in the Earth's gravitational field

2003

The lowest stationary quantum state of neutrons in the Earth's gravitational field is identified in the measurement of neutron transmission between a horizontal mirror on the bottom and an absorber/scatterer on top. Such an assembly is not transparent for neutrons if the absorber height is smaller than the ``height'' of the lowest quantum state.

Nuclear and High Energy PhysicsNeutron transportAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Gravitational fieldQuantum stateQuantum mechanics0103 physical sciencesNeutronQuantum field theory010306 general physicsNuclear ExperimentPhysics03.65.Ta010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]FermionQuantum numberquantum theoryneutron reflectionComputational physicsHigh Energy Physics - Phenomenologyneutron absorptionquantum gravity[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Quantum gravity
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Flavour violation at the LHC: type-I versus type-II seesaw in minimal supergravity

2009

20 pages, 13 figures.-- ISI article identifier:000267789100003.-- ArXiv pre-print avaible at:http://arxiv.org/abs/0903.1408

Nuclear and High Energy PhysicsParticle physicsFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesNeutrino Physics010306 general physicsNeutrino oscillationPhysicsLarge Hadron Collider010308 nuclear & particles physicsSupergravityMass generationHigh Energy Physics::PhenomenologyFísicaRare decaysHigh Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics::ExperimentBeyond standard modelNeutrinoLeptonSupersymmetric standard model
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Measurement and Interpretation of Fermion-Pair Production at LEP Energies of 183 and 189 GeV

2000

An analysis of the data collected in 1997 and 1998 with the DELPHI detector at e+e- collision energies close to 183 and 189 GeV was performed in order to extract the hadronic and leptonic fermion-pair cross-sections, as well as the leptonic forward-backward asymmetries and angular distributions. The data are used to put limit on contact interactions between fermions, the exchange of R-parity violating SUSY sneutrinos, Z' bosons and the existence of gravity in extra dimensions.

Nuclear and High Energy PhysicsParticle physicsHadronSTANDARD MODELFOS: Physical sciences7. Clean energy01 natural sciencesPartícules (Física nuclear)CROSS-SECTIONSHigh Energy Physics - ExperimentPHYSICSHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesMONTE-CARLO PROGRAM[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]EXTRA DIMENSIONSLimit (mathematics)010306 general physicsQCBosonDELPHIPhysicsCondensed Matter::Quantum Gaseshigh energy collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCONSTRAINTSLEPSupersymmetryFermionZ(0)CollisionLARGE ELECTRON POSITRON COLLIDERExtra dimensionsFIS/01 - FISICA SPERIMENTALEPair productionOF-MASS ENERGIESQUANTUM-GRAVITYPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIMONTE-CARLO PROGRAM; OF-MASS ENERGIES; STANDARD MODEL; EXTRA DIMENSIONS; QUANTUM-GRAVITY; CROSS-SECTIONS; CONSTRAINTS; PHYSICS; TESTS; Z(0)TESTSPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentParticle Physics - Experiment
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Determination of the atmospheric neutrino flux and searches for new physics with AMANDA-II

2009

The AMANDA-II detector, operating since 2000 in the deep ice at the geographic South Pole, has accumulated a large sample of atmospheric muon neutrinos in the 100 GeV to 10 TeV energy range. The zenith angle and energy distribution of these events can be used to search for various phenomenological signatures of quantum gravity in the neutrino sector, such as violation of Lorentz invariance (VLI) or quantum decoherence (QD). Analyzing a set of 5511 candidate neutrino events collected during 1387 days of livetime from 2000 to 2006, we find no evidence for such effects and set upper limits on VLI and QD parameters using a maximum likelihood method. Given the absence of evidence for new flavor-…

Nuclear and High Energy PhysicsParticle physicsOscillationsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaConfidence-IntervalsGravityFOS: Physical sciencesGeneratorLorentz covariance01 natural sciences7. Clean energyHigh Energy Physics - ExperimentScatteringHigh Energy Physics - Experiment (hep-ex)SensitivityQuantum Decoherence0103 physical sciencesddc:530Muon neutrino010306 general physicsNeutrino oscillationTelescopeAstroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSmall SignalsLorentz Invariance Violation
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Probing neutralino properties in minimal supergravity with bilinear R-parity violation

2012

Supersymmetric models with bilinear R-parity violation (BRPV) can account for the observed neutrino masses and mixing parameters indicated by neutrino oscillation data. We consider minimal supergravity versions of BRPV where the lightest supersymmetric particle (LSP) is a neutralino. This is unstable, with a large enough decay length to be detected at the CERN Large Hadron Collider (LHC). We analyse the LHC potential to determine the LSP properties, such as mass, lifetime and branching ratios, and discuss their relation to neutrino properties.

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsBilinear interpolationFOS: Physical sciencesSupergravity01 natural sciences7. Clean energyLightest Supersymmetric ParticleSupergravitaciónHigh Energy Physics - Phenomenology (hep-ph)R-parity0103 physical sciencesNeutrinos010306 general physicsNeutrino oscillationPhysicsNeutrinesLarge Hadron Collider010308 nuclear & particles physicsSupergravityHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyNeutralinoHigh Energy Physics::ExperimentNeutrino
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Constraint on the coupling of axionlike particles to matter via ultracold neutron gravitational experiment

2006

We present a new constraint for the axion monopole-dipole coupling in the range of 1 micrometer to a few millimeters, previously unavailable for experimental study. The constraint was obtained using our recent results on the observation of neutron quantum states in the Earth's gravitational field. We exploit the ultimate sensitivity of ultra-cold neutrons (UCN) in the lowest gravitational states above a material surface to any additional interaction between the UCN and the matter, if the characteristic interaction range is within the mentioned domain. In particular, we find that the upper limit for the axion monopole-dipole coupling constant is (g_p g_s)/(\hbar c)<2 x 10^{-15} for the ax…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciencesElementary particle01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Gravitational field14.80.Mz 04.80.-ygravitational experiments0103 physical sciencesultracold neutronsNeutron010306 general physicsNuclear ExperimentAxionPhysics010308 nuclear & particles physicsFermionCoupling (probability)Quantum numbergravityCP invarianceHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Ultracold neutrons
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Search for associated production of charginos and neutralinos in the trilepton final state using 2.3 fb-1 of data

2009

We report the results of a search for associated production of charginos and neutralinos using a data set corresponding to an integrated luminosity of 2.3 fb-1 collected with the D0 experiment during Run II of the Tevatron proton-antiproton collider. Final states containing three charged leptons and missing transverse energy are probed for a signal from supersymmetry with four dedicated trilepton event selections. No evidence for a signal is observed, and we set limits on the product of production cross section and leptonic branching fraction. Within minimal supergravity, these limits translate into bounds on m_0 and m_1/2 that are well beyond existing limits.

Nuclear and High Energy PhysicsParticle physicsTevatronFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Experimentlaw.inventionNuclear physicsHigh Energy Physics - Experiment (hep-ex)law0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsColliderPhysicsLuminosity (scattering theory)010308 nuclear & particles physicsBranching fractionSupergravityHigh Energy Physics::PhenomenologySupersymmetryD0 experimentExperimental High Energy PhysicsHigh Energy Physics::ExperimentLepton
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