Search results for "Particle physics"

showing 10 items of 6826 documents

Search for new phenomena in final states with large jet multiplicities and missing transverse momentum at s√=8 TeV proton-proton collisions using the…

2013

A search is presented for new particles decaying to large numbers (7 or more) of jets, with missing transverse momentum and no isolated electrons or muons. This analysis uses 20.3 fb[superscript −1] of pp collision data at s√ = 8 TeV collected by the ATLAS experiment at the Large Hadron Collider. The sensitivity of the search is enhanced by considering the number of b-tagged jets and the scalar sum of masses of large-radius jets in an event. No evidence is found for physics beyond the Standard Model. The results are interpreted in the context of various simplified supersymmetry-inspired models where gluinos are pair produced, as well as an mSUGRA/CMSSM model.

ExoticsPhysics::Instrumentation and DetectorsCiencias FísicasPhysics beyond the Standard ModelElectron01 natural sciences7. Clean energyHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Jets[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QChadron-hadron scatteringPhysicsGluinoLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleATLAS experimentSupersymmetryATLASJet physicsPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCParticle Physics - ExperimentCIENCIAS NATURALES Y EXACTASNuclear and High Energy PhysicsParticle physicsHadron-Hadron Scattering; Jet physics; Supersymmetry ExoticsCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]Scalar (mathematics)FOS: Physical sciencesHadron-hadron scattering530Nuclear physics0103 physical sciencesFysikddc:530High Energy Physics010306 general physicsScience & TechnologyMuon010308 nuclear & particles physicssupersymmetry; hadron-hadron scattering; jet physics; exoticsHigh Energy Physics::PhenomenologyexoticsFísica//purl.org/becyt/ford/1.3 [https]Hadron scatteringAstronomíaHADRON-HADRON COLLISIONSExperimental High Energy PhysicsHigh Energy Physics::ExperimentSupersymmetrysupersymmetry
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Combination of CDF and D0 measurements of the W boson helicity in top quark decays

2012

Aaltonen, T. et al.

FERMILAB TEVATRON COLLIDERNuclear and High Energy PhysicsParticle physicsTop quark[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TevatronW helicityValue (computer science)FOS: Physical sciencesTOP QUARK7. Clean energy01 natural sciencesHigh Energy Physics - Experimentlaw.inventionStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)law0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]FermilabTEVATRON010306 general physicsColliderBosonPhysicsW BOSONp-pbar collider; FERMILAB TEVATRON COLLIDER; W bosons; W helicity010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]W bosonsHelicityD0p-pbar colliderExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGCDFPhysical Review. D, Particles, Fields, Gravitation, and Cosmology
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Higgs boson studies at the Tevatron

2013

We combine searches by the CDF and D0 Collaborations for the standard model Higgs boson with mass in the range 90-200 GeV/c2 produced in the gluon-gluon fusion, WH, ZH, tt̄H, and vector boson fusion processes, and decaying in the H→bb̄, H→W+W-, H→ZZ, H→τ+τ-, and H→γγ modes. The data correspond to integrated luminosities of up to 10 fb-1 and were collected at the Fermilab Tevatron in pp̄ collisions at √s=1.96 TeV. The searches are also interpreted in the context of fermiophobic and fourth generation models. We observe a significant excess of events in the mass range between 115 and 140 GeV/c2. The local significance corresponds to 3.0 standard deviations at mH=125 GeV/c2, consistent with the…

FERMILAB TEVATRON COLLIDERNuclear and High Energy PhysicsParticle physicsproton antiproton collisions; FERMILAB TEVATRON COLLIDER; Standard Model Higgs boson; BROKEN SYMMETRIESSTANDARD MODELP(P)OVER-BAR COLLISIONSTevatronFOS: Physical sciencesContext (language use)ATLAS DETECTORddc:500.2Standard Model Higgs boson7. Clean energy01 natural sciencesStandard ModelVector bosonHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesBibliography[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]BROKEN SYMMETRIESFermilab010306 general physicsPhysicsHIGGS BOSONB-JET IDENTIFICATIONLarge Hadron ColliderPP COLLISIONS010308 nuclear & particles physics4. EducationHigh Energy Physics::PhenomenologyROOT-S=1.96 TEVPARTON DISTRIBUTIONSExperimental High Energy PhysicsHiggs bosonproton antiproton collisionsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGSYMMETRIESCDFB-JET IDENTIFICATION; STANDARD MODEL; ATLAS DETECTOR; PP COLLISIONS; P(P)OVER-BAR COLLISIONS; PARTON DISTRIBUTIONS; ROOT-S=1.96 TEV; SEARCH; LHC; SYMMETRIESHigh Energy Physics::ExperimentLHC
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Evidence for a Particle Produced in Association with Weak Bosons and Decaying to a Bottom-Antibottom Quark Pair in Higgs Boson Searches at the Tevatr…

2012

Aaltonen, T. et al.

FERMILAB TEVATRON COLLIDERTop quarkParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Higgs-Boson decaysSTANDARD MODEL; PARTON DISTRIBUTIONS; SYMMETRIES; proton antiproton collisions; FERMILAB TEVATRON COLLIDER; Standard Model Higgs boson; HIGGS-BOSON production; Higgs-Boson decaysSTANDARD MODELGeneral Physics and AstronomyFOS: Physical sciencesElementary particleStandard Model Higgs boson7. Clean energy01 natural sciencesVector bosonStandard ModelHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsTEVATRONBosonStandard-model Higgs bosonsPhysicsHIGGS-BOSON productionHIGGS BOSON010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyScalar bosonW and Z bosonsPARTON DISTRIBUTIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHiggs bosonSYMMETRIESproton antiproton collisionsCDFLimits on production of particlesHigh Energy Physics::Experiment
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Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

2015

A diffuse flux of astrophysical neutrinos above $100\,\mathrm{TeV}$ has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to $35\,\mathrm{TeV}$ and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmospheric backgrounds for shower-like events, we obtain a shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013. We demonstrate consistency with the $(f_e:f_{\mu}:f_\tau)_\oplus\approx(1:1:1)_\oplus$ flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sou…

FLUXAMANDAParticle physicsPhysics::Instrumentation and DetectorsENERGIESAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayAstrophysicsACCELERATION01 natural sciencesflavor : ratioHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)PionObservatory0103 physical sciencesddc:550010306 general physicsNeutrino oscillationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsSigmashowersCOSMIC-RAYSatmosphere : backgroundtracksneutrino : flavor : rationeutrino : oscillationfluxobservatoryPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomenaneutrino : VHEpi : decay
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Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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Search for relativistic magnetic monopoles with IceCube

2012

We present the first results in the search for relativistic magnetic monopoles with the IceCube detector, a subsurface neutrino telescope located in the South Polar ice cap containing a volume of 1 km$^{3}$. This analysis searches data taken on the partially completed detector during 2007 when roughly 0.2 km$^{3}$ of ice was instrumented. The lack of candidate events leads to an upper limit on the flux of relativistic magnetic monopoles of $\Phi_{\mathrm{90%C.L.}}\sim 3\e{-18}\fluxunits$ for $\beta\geq0.8$. This is a factor of 4 improvement over the previous best experimental flux limits up to a Lorentz boost $\gamma$ below $10^{7}$. This result is then interpreted for a wide range of mass …

FLUXSELECTIONAMANDANuclear and High Energy PhysicsParticle physicsProton decayCherenkov detectorPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleFOS: Physical sciencesddc:500.201 natural scienceslaw.inventionIceCube Neutrino ObservatoryPhysics::GeophysicsIceCubelaw0103 physical sciencesGrand Unified Theoryddc:530NEUTRINO TELESCOPE010306 general physicsCherenkov radiationPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsFIELDS85-05Physics and AstronomyNeutrino detectorAstrophysics - High Energy Astrophysical Phenomena
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Search for sterile neutrino mixing using three years of IceCube DeepCore data

2017

Physical review / D 95(11), 112002(2017). doi:10.1103/PhysRevD.95.112002

FLUXSterile neutrinoParticle physicsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences530High Energy Physics - ExperimentOSCILLATION EXPERIMENTSHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTRACK RECONSTRUCTIONddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomySolar neutrino problemLINE-EXPERIMENT-SIMULATORMODELHigh Energy Physics - PhenomenologyNeutrino detectorPhysics and AstronomyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrino
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First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

2011

Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 0.1deg. The neutrino flux sensitivity is 7.5 ¿ 10 -8(E ¿/ GeV) -2 GeV -1 s -1 cm -2 for the part of the sky that is always visible (¿ < -48deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.

FLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesAngular resolutionALGORITHMNeutrinosDETECTOR010303 astronomy & astrophysicsCosmic raysmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorneutrinosASTRONOMYAstronomy and Astrophysicsastroparticle physics13. Climate actionSpace and Planetary ScienceSkyFISICA APLICADAddc:520Física nuclearHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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Faraday patterns in bose-Einstein condensates.

2002

Temporal periodic modulation of the interatomic s-wave scattering length in Bose-Einstein condensates is shown to excite subharmonic patterns of atom density through a parametric resonance. The dominating wavelength of the spatial structures is shown to be primarily selected by the excitation frequency but also affected by the depth of the spatial modulation via a nonlinear resonance. These phenomena represent macroscopic quantum analogues of the Faraday waves excited in vertically shaken liquids.

FOS: Physical sciencesGeneral Physics and AstronomyPattern formationPattern Formation and Solitons (nlin.PS)Resonance (particle physics)law.inventionFaraday wavesymbols.namesakelawQuantum mechanicsFaraday effectFaraday cageFeshbach resonanceCondensed Matter - Statistical MechanicsPhysicsCondensed Matter::Quantum GasesStatistical Mechanics (cond-mat.stat-mech)Condensed matter physicsScatteringCondensed Matter::OtherResonanceScattering lengthNonlinear Sciences - Pattern Formation and SolitonsSymmetry (physics)Magnetic fieldModulationNonlinear resonanceExcited statesymbolsDissipative systemState of matterAtomic physicsParametric oscillatorExcitationBose–Einstein condensatePhysical review letters
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