Search results for "ddc:5"

showing 10 items of 1717 documents

First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

2017

Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors. In the case of known pulsars a fully coherent search, based on matched filtering, which uses the position and rotational parameters obtained from electromagnetic observations, can be carried out. Matched filtering maximizes the signal-to-noise (SNR) ratio, but a large sensitivity loss is expected in case of even a very small mismatch between the assumed and the true signal parameters. For this reason, {\it narrow-band} analyses methods have been developed, allowing a fully coherent search for gravitational waves from known …

Gravitational-wave observatoryPhysics and Astronomy (miscellaneous)Astronomy01 natural sciencesrotationneutron starsGeneral Relativity and Quantum Cosmologygravitational waves; LIGO; stochastic gravitational-waveLIGOneutron star010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCpulsarQBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Gravitational Waves neutron stars advanced detectors narrow-band searchDetectorAmplitude[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaasymmetryCoherence (physics)young pulsarinterferometerneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)proper motionadvanced detectorsGravitational wavesPulsar0103 physical sciencesddc:530Gravitational Waves010308 nuclear & particles physicsGravitational wavegravitational radiation530 PhysikLIGOgravitational radiation detectorComputational physicscoherencedetector: sensitivityNeutron starelectromagneticPhysics and AstronomyGravitational waves; Pulsarnarrow-band searchDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]discovery
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Offspring microbiomes differ across breeding sites in a panmictic species.

2019

High dispersal rates are known to homogenize host’s population genetic structure in panmictic species and to disrupt host local adaptation to the environment. Long-distance dispersal might also spread micro-organisms across large geographical areas. However, so far, to which extent selection mechanisms that shape host’s population genetics are mirrored in the population structure of the enteric microbiome remains unclear. High dispersal rates and horizontal parental transfer may homogenize bacterial communities between breeding sites (homogeneous hypothesis). Alternatively, strong selection from the local environment may differentiate bacterial communities between breeding sites (heterogene…

Gut microbiomepopulation differentiationPhoenicopterus roseuslcsh:QR1-502gut microbiomeVerbreitungsökologiegreater flamingosDispersalMicrobiologylcsh:MicrobiologyGastrointestinal MicrobiomeDDC 570 / Life sciences[SDV.MP]Life Sciences [q-bio]/Microbiology and ParasitologyPopulation differentiationddc:570Greater flamingosddc:610Greater flamingodispersalDDC 610 / Medicine & health[SDV.MP] Life Sciences [q-bio]/Microbiology and ParasitologyMicroorganisms DispersalOriginal Research
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Searches for transverse momentum dependent flow vector fluctuations in Pb-Pb and p-Pb collisions at the LHC

2017

The measurement of azimuthal correlations of charged particles is presented for Pb-Pb collisions at $\sqrt{s_{\rm NN}}=$ 2.76 TeV and p-Pb collisions at $\sqrt{s_{\rm NN}}=$ 5.02 TeV with the ALICE detector at the CERN Large Hadron Collider. These correlations are measured for the second, third and fourth order flow vector in the pseudorapidity region $|��|<0.8$ as a function of centrality and transverse momentum $p_{\rm T}$ using two observables, to search for evidence of $p_{\rm T}$-dependent flow vector fluctuations. For Pb-Pb collisions at 2.76 TeV, the measurements indicate that $p_{\rm T}$-dependent fluctuations are only present for the second order flow vector. Similar results hav…

HEAVY-ION COLLISIONSnucl-extransverse momentum dependenceCOLLABORATIONangular correlation [charged particle]High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEmodel: hydrodynamicstransport theory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear ExperimentMonte CarloHeavy Ion Experiments; RELATIVISTIC NUCLEAR COLLISIONS; HEAVY-ION COLLISIONS; QUARK-GLUON; PLASMA; COLLECTIVE FLOW; COLLABORATIONPLASMAfluctuation [geometry]flow: anisotropygeometry: fluctuationQUARK-GLUONCERN LHC CollHeavy Ion Experiments; Nuclear and High Energy PhysicsflowRELATIVISTIC NUCLEAR COLLISIONSHeavy Ion ExperimentQuark-Gluon PlasmaParticle Physics - Experiment2760 GeV/nucleon5020 GeV/nucleonNuclear and High Energy PhysicsCERN LabCOLLECTIVE FLOWFOS: Physical sciencestransverse momentum[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]vector [fluctuation]Heavy Ion Experimentsscattering [heavy ion][ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]factorizationlcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530hydrodynamics [model]Nuclear Physics - Experimentnumerical calculationsinitial stateleadHeavy Ion Experiments Nuclear and High Energy Physics.hep-exboundary conditionrapiditycorrelationviscositylcsh:QC770-798High Energy Physics::Experimentp nucleusentropy: densitycharged particle: angular correlationexperimental results
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Contribution of exclusive diffractive processes to the measured azimuthal asymmetries in SIDIS

2019

Hadron leptoproduction in Semi-Inclusive measurements of Deep-Inelastic Scattering (SIDIS) on unpolarised nucleons allows one to get information on the intrinsic transverse momentum of quarks in a nucleon and on the Boer-Mulders function through the measurement of azimuthal modulations in the cross section. These modulations were recently measured by the HERMES experiment at DESY on proton and deuteron targets, and by the COMPASS experiment using the CERN SPS muon beam and a $^6$LiD target. In both cases, the amplitudes of the $\cos\phi_h$ and $\cos 2\phi_h$ modulations show strong kinematic dependences for both positive and negative hadrons. It has been known since some time that the measu…

HERMES experimentvirtual [photon]Hadronleptoproduction [hadron]measurement methodsNuclear TheoryVirtual particleHERMES01 natural sciencesSIDISCOMPASShadron: leptoproductionHigh Energy Physics - Experimentazimthal asymmetrieproduction [diffraction]High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)semi-inclusive reaction [deep inelastic scattering][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]COMPASS experimentNuclear ExperimentPhysicsdeep inelastic scattering: semi-inclusive reactionnucleonhep-phphoton: energyTMD obsvervableangular dependenceHigh Energy Physics - Phenomenologymodulationhadron: final stateTMD obsvervablesbeam [muon]asymmetry [angular distribution]interpretation of experimentsdeuteron: targettransverse momentum [quark]Nucleondiffraction: productionParticle Physics - ExperimentQuarkNuclear and High Energy PhysicsParticle physicsazimthal asymmetriesexclusive reactionangular distribution: asymmetryMesonFOS: Physical sciences530vector meson: production0103 physical scienceskinematics: effectlcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530final state [hadron]010306 general physicsParticle Physics - PhenomenologyMuonmuon: beam010308 nuclear & particles physicsproduction [vector meson]hep-exenergy [photon]CERN SPSeffect [kinematics]lcsh:QC770-798quark: transverse momentumHigh Energy Physics::ExperimentTMD obsvervables; azimthal asymmetries; SIDIStarget [deuteron]photon: virtual
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Search for high-mass resonances decaying to dimuons at CDF.

2009

We present a search for high-mass neutral resonances using dimuon data corresponding to an integrated luminosity of 2.3 fb(-1) collected in pp collisions at s=1.96 TeV by the CDF II detector at the Fermilab Tevatron. No significant excess above the standard model expectation is observed in the dimuon invariant-mass spectrum. We set 95% confidence level upper limits on sigma BR(pp -> X ->mu mu), where X is a boson with spin-0, 1, or 2. Using these cross section limits, we determine lower mass limits on sneutrinos in R-parity-violating supersymmetric models, Z(') bosons, and Kaluza-Klein gravitons in the Randall-Sundrum model.

HIGH MASS RESONANCEParticle physicsFermilab TevatronTevatronGeneral Physics and AstronomyFOS: Physical sciencesddc:500.2114 Physical sciencesResonance7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsTellurium compoundsHigh Energy Physics - Experiment (hep-ex)Integrated luminosities0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsBosonsBosonPhysicsMuonMass spectrometryhep-ex010308 nuclear & particles physicsPhysicsInvariant-mass spectrum13.85.Rm 13.85.Qk 12.60.Cn 14.70.Pw 04.50.-hHigh Energy Physics::PhenomenologyConfidence levelsGravitonSupersymmetryUpper limitsSupersymmetric modelsCross sectionsRandall–Sundrum modelThe standard modelsMass spectrumCDFHigh Energy Physics::ExperimentPhysical review letters
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Constraints on Minute-Scale Transient Astrophysical Neutrino Sources

2019

High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets, and neutron star mergers. IceCube's optical and x-ray follow-up program searches for such transient sources by looking for two or more muon neutrino candidates in directional coincidence and arriving within 100 s. The measured rate of neutrino alerts is consistent with the expected rate of chance coincidences of atmospheric background events and no likely electromagnetic counterparts have been identified in Swift follow-up observations. Here, we calculate generic bounds on the neutrino flux of short-lived transient so…

HIGH-ENERGY NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaPopulationGeneral Physics and AstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energy0103 physical sciencesMuon neutrinoddc:530education010303 astronomy & astrophysicsPhysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyMuon010308 nuclear & particles physicsSupernovaNeutron starPhysics and Astronomy13. Climate actionPhysique des particules élémentairesHigh Energy Physics::ExperimentNeutrinoGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube

2015

Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere dataset consisting primarily of nu_e and nu_tau charged current and neutral current (cascade) neutrino interactions. In the analysis presented here, a data sample of approximately 35,000 muon neutrinos from the Northern sky was extracted from data taken during 659.5 days of livetime recorded between May 2010 and May 2012. While this sample is composed primarily of neutrinos produced by cosmic ray interactions in the Earth's atmosphere, the highest energy events are inconsistent with a hypothesis of …

HIGH-ENERGY NEUTRINOSFLUXESATMOSPHERIC MUONAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics01 natural sciencesIceCube Neutrino ObservatoryRATIO0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsSolar neutrino problemPhysics and AstronomyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena
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Tau neutrinos in the next decade: from GeV to EeV

2022

Tau neutrinos are the least studied particle in the standard model. This whitepaper discusses the current and expected upcoming status of tau neutrino physics with attention to the broad experimental and theoretical landscape spanning long-baseline, beam-dump, collider, and astrophysical experiments. This whitepaper was prepared as a part of the NuTau2021 Workshop.

HIGH-ENERGY NEUTRINOSMAGNETIC-MOMENTAstrophysics and AstronomyNuclear and High Energy PhysicsRADIO PULSESPhysics::Instrumentation and Detectorstau neutrinosFOS: Physical sciencesCHERENKOV LIGHT YIELDGeV530High Energy Physics - Experimenttau neutrino theorySubatomär fysikHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)neutrino experimentsSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Particle Physics - PhenomenologyAIR-SHOWERSLEPTON FLAVORastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)hep-exPhysicshep-phtau neutrinos; neutrino experiments; tau neutrino theorylandscapeCOSMIC-RAYSHigh Energy Physics - PhenomenologyQUANTUM-GRAVITYCHARGED-PARTICLES[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]beam dumpPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentLORENTZ VIOLATION[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Experiment
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Atmospheric and astrophysical neutrinos above 1 TeV interacting in IceCube

2015

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A search for $\gtrsim 100$~TeV neutrinos interacting inside the instrumented volume has recently provided evidence for an isotropic flux of such neutrinos. At lower energies, IceCube collects large numbers of neutrinos from the weak decays of mesons in cosmic-ray air showers. Here we present the results of a search for neutrino interactions inside IceCube's instrumented volume between 1~TeV and 1~PeV in 641 days of data taken from 2010--2012, lowering the energy threshold for neutrinos from the southern sky below 10 TeV for the first time, far bel…

HIGH-ENERGY NEUTRINOSNuclear and High Energy PhysicsParticle physicsAMANDAMesonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESFOS: Physical sciencesCosmic rayAstrophysicsFLUX PREDICTIONS01 natural sciencesIceCube Neutrino ObservatoryIceCubeObservatorySEARCH0103 physical sciencesddc:530Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYPERFORMANCEBLAZARSPROMPT LEPTONSGAMMA-RAYPhysics and AstronomyHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsPhysical Review D
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First search for atmospheric and extraterrestrial neutrino-induced cascades with the IceCube detector

2011

We report on the first search for atmospheric and for diffuse astrophysical neutrino-induced showers (cascades) in the IceCube detector using 257 days of data collected in the year 2007-2008 with 22 strings active. A total of 14 events with energies above 16 TeV remained after event selections in the diffuse analysis, with an expected total background contribution of $8.3\pm 3.6$. At 90% confidence we set an upper limit of $E^2\Phi_{90%CL}<3.6\times10^{-7} GeV \cdot cm^{-2} \cdot s^{-1}\cdot sr^{-1} $ on the diffuse flux of neutrinos of all flavors in the energy range between 24 TeV and 6.6 PeV assuming that $\Phi \propto E^{-2}$ and that the flavor composition of the $\nu_e : \nu_\mu : \nu…

HIGH-ENERGY NEUTRINOSSELECTIONNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaHigh-energy neutrinosFOS: Physical sciencesFluxCosmic rayElementary particleAstrophysicsParticle detectorIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SCATTERINGddc:530High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMICEHigh Energy Physics::Phenomenology004Massless particlePhysics and AstronomyNeutrino detectorAMANDA-IIHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomenainfo:eu-repo/classification/ddc/004LeptonPhysical Review D
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