Search results for "FÍSICAS"

showing 10 items of 251 documents

Charged-particle multiplicities in pp interactions measured with the ATLAS detector at the LHC

2011

Measurements are presented from proton–proton collisions at centre-of-mass energies of \sqrt{s} = 0.9 , 2.36 and 7 TeV recorded with the ATLAS detector at the LHC. Events were collected using a single-arm minimum-bias trigger. The charged-particle multiplicity, its dependence on transverse momentum and pseudorapidity and the relationship between the mean transverse momentum and charged-particle multiplicity are measured. Measurements in different regions of phase space are shown, providing diffraction-reduced measurements as well as more inclusive ones. The observed distributions are corrected to well-defined phase-space regions, using model-independent corrections. The results are compared…

Atlas detectorMonte Carlo methodLarge hadron colliderNuclear physicsGeneral Physics and Astronomy01 natural sciencesTransverse-Momentum SpectraHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Pseudorapidity[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]CollisionsQANuclear ExperimentTransverse momentumQCPhysicsLarge Hadron ColliderPhysicsSettore FIS/01 - Fisica SperimentaleParticle physicsATLAS detector; LHC; pp collisionsATLASSquare-Root-SMonte carlo methodCharged particle3. Good healthPseudorapidityddc:540ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGTsallis distributionFísica nuclearDistributionsLHCpp collisionsParticle Physics - ExperimentParticle physicsCiências Naturais::Ciências FísicasAtlas detector:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesCharged particleInclusive production with identified hadronsPhase spaceddc:500.2530Nuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsATLAS detector010308 nuclear & particles physicsFísicaMultiplicity (mathematics)Perturbative calculationsMultiplicity (mathematics)pp interactions; LHC; ATLAS detectorPhase spaceHADRON-HADRON COLLISIONSExperimental High Energy PhysicsCM EnergiesTevHigh Energy Physics::ExperimentCollider
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ATLAS measurements of the properties of jets for boosted particle searches

2012

Measurements are presented of the properties of high transverse momentum jets, produced in proton-proton collisions at a center-of-mass energy of √s=7  TeV. The data correspond to an integrated luminosity of 35  pb−1 and were collected with the ATLAS detector in 2010. Jet mass, width, eccentricity, planar flow and angularity are measured for jets reconstructed using the anti-kt algorithm with distance parameters R=0.6 and 1.0, with transverse momentum pT>300  GeV and pseudorapidity |η|<2. The measurements are compared to the expectations of Monte Carlo generators that match leading-logarithmic parton showers to leading-order, or next-to-leading-order, matrix elements. The generators describ…

Atlas detectorMonte Carlo methodParton7. Clean energy01 natural sciencesNucleonHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentNUCLEONATLAS; jets; boostedQCDetectors de radiacióQuantum chromodynamicsPhysicsLarge Hadron ColliderAcceleradors de partículesSettore FIS/01 - Fisica SperimentaleATLASINCLUSIVE JET CROSS SECTIONLarge Hadron ColliderPseudorapidityTransverse momentumComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCFRAGMENTATIONNucleonParticle Physics - ExperimentjetsNuclear and High Energy PhysicsParticle physicsCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Partícules (Física nuclear)Proton-proton collisionsNuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsCiencias ExactasScience & TechnologyATLAS detector010308 nuclear & particles physicsFísicaMODELHADRON-HADRON COLLISIONSCol·lisions (Física nuclear)PARTON DISTRIBUTIONSExperimental High Energy PhysicsHigh Energy Physics::ExperimentModel
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Search for excited electrons and muons in root s=8 TeV proton-proton collisions with the ATLAS detector

2013

The ATLAS detector at the Large Hadron Collider is used to search for excited electrons and excited muons in the channel pp → ℓℓ* → ℓℓγ, assuming that excited leptons are produced via contact interactions. The analysis is based on 13 fb[superscript −1] of pp collisions at a centre-of-mass energy of 8 TeV. No evidence for excited leptons is found, and a limit is set at the 95% credibility level on the cross section times branching ratio as a function of the excited-lepton mass m[subscript ℓ*]. For m[subscript ℓ*] ≥ 0.8 TeV, the respective upper limits on σB(ℓ* → ℓγ) are 0.75 and 0.90 fb for the e* and μ* searches. Limits on σB are converted into lower bounds on the compositeness scale Λ. In …

Atlas detectorPhysics::Instrumentation and DetectorsCiencias FísicasGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCPhysicsddc:539Excited leptonsLarge Hadron ColliderLepton ProductionSettore FIS/01 - Fisica SperimentaleBranching ratioHERAATLASLarge Hadron ColliderExcited statePhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGQuarkLHCContact interactionExcited electronsParticle Physics - ExperimentCIENCIAS NATURALES Y EXACTASQuarkParticle physicsCiências Naturais::Ciências Físicas530 PhysicsParticle physics and field theory:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2excited electrons; muons; proton–proton collisions; ATLAS detector530Nuclear physics0103 physical sciencesFysikddc:530High Energy Physics010306 general physicsCentre-of-mass energiesCiencias ExactasHeraScience & TechnologyMuonATLAS detectorProton proton collisions010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyATLAS detectorsFísica//purl.org/becyt/ford/1.3 [https]AstronomíaHADRON-HADRON COLLISIONSExperimental High Energy PhysicsEp CollisionsHigh Energy Physics::Experimentproton-proton collisionsLepton
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Search for strong gravity signatures in same-sign dimuon final states using the ATLAS detector at the LHC

2012

A search for microscopic black holes has been performed in a same-sign dimuon final state using 1.3 fb[superscript −1] of proton–proton collision data collected with the ATLAS detector at a centre of mass energy of 7 TeV at the CERN Large Hadron Collider. The data are found to be consistent with the expectation from the Standard Model and the results are used to derive exclusion contours in the context of a low scale gravity model.

Atlas detectorPhysics::Instrumentation and DetectorsHadron01 natural sciencesHigh Energy Physics - ExperimentMicro black holeHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentDetectors de radiacióPhysicsINTERAÇÕES NUCLEARESLarge Hadron ColliderBLACK HOLEAtlas (topology)Strong gravityAcceleradors de partículesExtra DimensionsSettore FIS/01 - Fisica SperimentaleMicroscopic black holesATLASExtra dimensionsLarge Hadron ColliderComputingMethodologies_DOCUMENTANDTEXTPROCESSINGExtra dimensionsAtlasLHCParticle Physics - ExperimentNuclear and High Energy PhysicsParticle physicsDIMENSIONSCOLLISIONSSame-sign dimuonsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2GRAVITY ON BRANE WORLDS530Partícules (Física nuclear)Nuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsBLACK-HOLESMILLIMETERCiencias ExactasScience & TechnologyROOT-S=7 TEVATLAS detector010308 nuclear & particles physicssame-sign dimuons; microscopic black holes; extra dimensions; lhc; atlasFísicaCollisionLHC; ATLAS; Microscopic black holes; Extra dimensions; Same-sign dimuonsHADRON-HADRON COLLISIONSCol·lisions (Física nuclear)Experimental High Energy PhysicsPhysics::Accelerator PhysicsHigh Energy Physics::Experiment
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Measurement of the distributions of event-by-event flow harmonics in lead-lead collisions at = 2.76 TeV with the ATLAS detector at the LHC

2013

We acknowledge the support of ANPCyT, Argentina; YerPhI, Armenia; ARC, Australia; BMWF and FWF, Austria; ANAS, Azerbaijan; SSTC, Belarus; CNPq and FAPESP, Brazil; NSERC, NRC and CFI, Canada; CERN; CONICYT, Chile; CAS, MOST and NSFC, China; COLCIENCIAS, Colombia; MSMT CR, MPO CR and VSC CR, Czech Republic; DNRF, DNSRC and Lundbeck Foundation, Denmark; EPLANET, ERC and NSRF, European Union; IN2P3-CNRS, CEA-DSM/IRFU, France; GNSF, Georgia; BMBF, DFG, HGF, MPG and AvH Foundation, Germany; GSRT and NSRF, Greece; ISF, MINERVA, GIF, DIP and Benoziyo Center, Israel; INFN, Italy; MEXT and JSPS, Japan; CNRST, Morocco; FOM and NWO, Netherlands; BRF and RCN, Norway; MNiSW, Poland; GRICES and FCT, Portu…

Atlas detectorUnfolding01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Heavy-ion collisionNaturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)RELATIVISTIC HEAVY-ION COLLISIONSNuclear ExperimentNuclear ExperimentQCunfoldingPhysicsLarge Hadron ColliderAtlas (topology)4. EducationSettore FIS/01 - Fisica SperimentaleEvent-By-Event FluctuationElliptic flowHeavy-Ion CollisionsHarmonic FlowCharged particlehadron-hadron scattering; harmonic flow; event-by-event fluctuation; unfolding; heavy-ion collisionHarmonicsImpact parameterNatural Sciencesharmonic flowParticle Physics - ExperimentNuclear and High Energy PhysicsParticle physicsCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesComputer Science::Digital Libraries530Nuclear physics0103 physical sciencesHeavy ion collisionsddc:530Rapidity010306 general physicsevent-by-event fluctuationCiencias ExactasScience & TechnologyHadron-Hadron Scattering010308 nuclear & particles physicsFísicaheavy ion collisionHeavy-ion collision; harmonic flow; event-by-event fluctuation; unfolding; Hadron-Hadron Scattering
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Observation of an Excited $B^{\pm}_c$ Meson State with the ATLAS Detector

2014

A search for excited states of the B±c meson is performed using 4.9 fb-1 of 7 TeV and 19.2 fb-1 of 8 TeV pp collision data collected by the ATLAS experiment at the LHC. A new state is observed through its hadronic transition to the ground state, with the latter detected in the decay B±c→J/ψπ±. The state appears in the m(Bc±π+π-)-m(Bc±)-2m(π±) mass difference distribution with a significance of 5.2 standard deviations. The mass of the observed state is 6842±4±5 MeV, where the first error is statistical and the second is systematic. The mass and decay of this state are consistent with expectations for the second S-wave state of the B±c meson, B±c(2S).

B-C meson; spectroscopy; equationEquationБольшой адронный коллайдер550Atlas detectorlarge hadron colliderGeneral Physics and Astronomyhadronic decay [excited state]7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareSubatomär fysikHigh Energy Physics - Experiment (hep-ex)B/c* --&gt; B/c+ pi+ pi-Subatomic Physicsexcited stateddc:550EQUATION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]ATLAS Detector; Meson StateB mesonGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)SpectroscopyQCPhysics8000 GeV-cms [7000]Large Hadron ColliderSPECTROSCOPYATLAS experimentSettore FIS/01 - Fisica SperimentaleATLASB-C MESON:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]B/c* --> B/c+ pi+ pi-medicine.anatomical_structureCERN LHC CollExcited statePhysical Sciences7000: 8000 GeV-cmsLHCParticle Physics - ExperimentB-C MesonParticle physicsp p: scatteringMeson530 PhysicsCiências Naturais::Ciências FísicasAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesmass [excited state]столкновение частиц530hadronic decay [B/c+]Nuclear physicsPhysics and Astronomy (all)(J/psi(3100) pi+) [mass spectrum]B/c+ --&gt; J/psi(3100) pi+Atlas (anatomy)TheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITY0103 physical sciencesmedicineFysikHigh Energy Physics010306 general physicsB/c+ --> J/psi(3100) pi+Ciencias ExactasScience & TechnologyATLAS detector010308 nuclear & particles physicsHigh Energy Physics::Phenomenology:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]FísicaState (functional analysis)B/c+: hadronic decaymass differencemass spectrum: (J/psi(3100) pi+)B-C MESON; SPECTROSCOPY; EQUATIONB/c+excited state: massexcited state: hadronic decayExperimental High Energy PhysicsмезоныHigh Energy Physics::Experimentproton-proton collisionsATLAS детекторexperimental results
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Detailed study of SNR G306.3–0.9 using XMM-Newton and Chandra observations

2016

Aims. We aim to study the spatial distribution of the physical and chemical properties of the X-ray emitting plasma of the supernova remnant (SNR) G306.3-0.9 in detail to obtain constraints on its ionization stage, the progenitor supernova explosion, and the age of the remnant. Methods. We used combined data from XMM-Newton and Chandra observatories to study the X-ray morphology of G306.3-0.9 in detail. A spatially resolved spectral analysis was used to obtain physical and geometrical parameters of different regions of the remnant. Spitzer infrared observations, available in the archive, were also used to constrain the progenitor supernova and study the environment in which the remnant evol…

Ciencias AstronómicasInfraredCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaISM [Infrared]FOS: Physical sciencesthermal [radiation mechanism]individual objects: SNR G306.3–0.9 [ISM]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral line//purl.org/becyt/ford/1 [https]ISM: individual objects: SNR G306.3IonizationISM [X-ray]0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsISM [X-rays]Radio continuum: ISMEjectaSupernova remnant010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy AstrophysicsISM: supernova remnantsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Infrared: ISM010308 nuclear & particles physicssupernova remnants [ISM]Astronomy and AstrophysicsPlasma//purl.org/becyt/ford/1.3 [https]Astronomy and AstrophysicISM: individual objects: SNR G306.3–0.9ISM [Radio continuum]Radiation mechanisms: thermalX-rays: ISMindividual objects: G306.3-0.9 [ISM]Interstellar mediumAstronomíaSupernovathermal [Radiation mechanisms]Space and Planetary ScienceISM; ISM: individual objects: SNR G306.3; ISM: supernova remnants; Radiation mechanisms: thermal; Radio continuum: ISM; X-rays: ISM; Astronomy and Astrophysics; Space and Planetary Science [0.9; Infrared]0.9Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory an…

2014

Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 1019 eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 1019 eV. No significant devia…

Ciencias FísicasAstronomyRaysAstrophysicsAstroparticle physics; Cosmic rays01 natural scienceslaw.inventionPierrelawAnisotropyTelescope010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[PHYS]Physics [physics]Energy[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for Astrophysicsastroparticle physicRadiación cósmicaAugerCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsCIENCIAS NATURALES Y EXACTASHigh[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raySURFACE DETECTORICECUBETelescopeAIR-SHOWER ARRAYDirectionscosmic rays0103 physical sciencesInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsArraySpectral densitySpherical harmonicsFísicaAstronomy and AstrophysicsASTROFÍSICAUltra[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AstronomíaDipoleRESOLUTIONSpace and Planetary ScienceExperimental High Energy PhysicsQuadrupoleObservatoryAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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SHOCK-CLOUD INTERACTION AND PARTICLE ACCELERATION IN THE SOUTHWESTERN LIMB OF SN 1006

2014

The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relatively tenuous and uniform environment despite interacting with an atomic cloud in its northwestern limb. The X-ray image of SN 1006 reveals an indentation in the southwestern part of the shock front and the H I maps show an isolated (southwestern) cloud, having the same velocity as the northwestern cloud, whose morphology fits perfectly in the indentation. We performed spatially resolved spectral analysis of a set of small regions in the southwestern nonthermal limb and studied the deep X-ray spectra obtained within the XMM-Newton SN 1006 Large Program. We also analyzed archive H I data, obtain…

Ciencias FísicasAstrophysics::High Energy Astrophysical PhenomenaHadronSynchrotron radiationAstrophysicsSpectral lineISM: cloudIndentationSupernova remnantISM: individual objects (SN 1006)acceleration of particleISM: supernova remnantAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicssupernova remnants X-rays: ISM [ISM]Astronomy and AstrophysicsX-rays: ISMShock (mechanics)Particle accelerationAstronomíaSpace and Planetary Scienceindividual objects: SN 1006 [ISM]clouds [ISM]CIENCIAS NATURALES Y EXACTASFermi Gamma-ray Space Telescope
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