Search results for "Cosmology"

showing 10 items of 2905 documents

Discovery of a new accreting millisecond X-ray pulsar in the globular cluster NGC 2808

2016

We report on the discovery of coherent pulsations at a period of 2.9 ms from the X-ray transient MAXI J0911-655 in the globular cluster NGC 2808. We observed X-ray pulsations at a frequency of $\sim339.97$ Hz in three different observations of the source performed with XMM-Newton and NuSTAR during the source outburst. This newly discovered accreting millisecond pulsar is part of an ultra-compact binary system characterised by an orbital period of $44.3$ minutes and a projected semi-major axis of $\sim17.6$ lt-ms. Based on the mass function we estimate a minimum companion mass of 0.024 M$_{\odot}$, which assumes a neutron star mass of 1.4 M$_{\odot}$ and a maximum inclination angle of $75^{\…

X-rays: binaries pulsars: general stars: neutron accretion accretion disks binaries: generalMetallicityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsWhite dwarfAstronomy and Astrophysicsbinaries pulsars: general stars: neutron accretion accretion disks binaries: general [X-rays]Orbital periodNeutron starSpace and Planetary ScienceGlobular clusterAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-ray pulsar
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First Dark Matter Search Results from the XENON1T Experiment

2017

We report the first dark matter search results from XENON1T, a ∼2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042±12)-kg fiducial mass and in the [5,40] keVnr energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93±0.25)×10-4 events/(kg×day×keVee), the lowest ever achieved in such a dark matter detector. A profile likelihood analysis shows that the data are consisten…

Xenon[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Massive particleGeneral Physics and Astronomy01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)RecoilXenonWIMPS046DM2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matter[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]PhysicsRange (particle radiation)Time projection chamberDetectorHigh Energy Physics - Phenomenologydark matter: scatteringTPCAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPDark matterFOS: Physical scienceschemistry.chemical_elementWIMP: massS030DI2Nuclear physicsPhysics and Astronomy (all)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesrecoil[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physique010308 nuclear & particles physicsbackgrounddark matter: detectorAstronomieGran SassochemistryDirect Searchtime projection chamber: xenoninterpretation of experiments: XENON[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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A detailed study of the rise phase of a long duration X-ray flare in the young star TWA 11B

2010

We analyzed a long duration flare observed in a serendipitous XMM-Newton detection of the M star CD-39 7717B (TWA 11B), member of the young stellar association TW Hya (~ 8 Myr). Only the rise phase (with a duration of ~ 35 ks) and possibly the flare peak were observed. We took advantage of the high count-rate of the X-ray source to carry out a detailed analysis of its spectrum during the whole exposure. After a careful analysis, we interpreted the rise phase as resulting from the ignition of a first group of loops (event A) which triggered a subsequent two-ribbon flare (event B). Event A was analyzed using a single-loop model, while a two-ribbon model was applied for event B. Loop semi-leng…

Young stellar objectAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicslaw.inventionSettore FIS/05 - Astronomia E AstrofisicalawIonizationAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)X-rayAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesStarsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)astrofisica fisica stellare flares stars: activity stars: coronae stars: flare stars: individual: CD-39 7717B TWA 11B stars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)Flare
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New view of the corona of classical T Tauri stars: Effects of flaring activity in circumstellar disks

2019

Classical T Tauri stars (CTTSs) are young low-mass stellar objects accreting mass from their circumstellar disks. They are characterized by high levels of coronal activity as revealed by X-ray observations. This activity may affect the disk stability and the circumstellar environment. Here we investigate if an intense coronal activity due to flares occurring close to the accretion disk may perturb the inner disk stability, disrupt the inner part of the disk and, possibly, trigger accretion phenomena with rates comparable with those observed. We model a magnetized protostar surrounded by an accretion disk through 3D magnetohydrodinamic simulations. We explore cases characterized by a dipole …

Young stellar objectStars: flareAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesX-rays: starsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsaccretion accretion disk01 natural sciencesmagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferProtostarAstrophysics::Solar and Stellar AstrophysicsStars: coronae010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]accretion disksStellar magnetic fieldAstronomy and Astrophysics[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]CoronaAccretion (astrophysics)T Tauri starAstrophysics - Solar and Stellar AstrophysicsHeat flux13. Climate actionSpace and Planetary ScienceStars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysics
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"Table 2" of "Measurement of ZZ production in pp collisions at sqrt(s)=7 TeV and limits on anomalous ZZZ and ZZgamma couplings with the ATLAS detecto…

2014

The measured total cross sections. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity, the second is the luminosity.

Z ProductionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross Section7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 1" of "Measurement of ZZ production in pp collisions at sqrt(s)=7 TeV and limits on anomalous ZZZ and ZZgamma couplings with the ATLAS detecto…

2014

The measured fiducial cross sections. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity, the second is the luminosity.

Z ProductionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross Section7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 16" of "Measurement of the production cross section for Z/gamma* in association with jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS d…

2014

Measured normalized leading jet differential cross section 1/sigma_DY dsigma/dpt for the electron channel and the muon channel in the individual lepton fiducial regions and uncorrected for QED effects.

Z ProductionHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionInclusiveSingle Differential Cross SectionP P --> Z0 JET XP P --> GAMMA* JET XProton-Proton ScatteringHigh Energy Physics::ExperimentDSIG/DPTTransverse Momentum DependenceComputer Science::Information Theory
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"Table 15" of "Measurement of the production cross section for Z/gamma* in association with jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS d…

2014

Measured normalized inclusive jet differential cross section 1/sigma_DY dsigma/dpt for the electron channel and the muon channel in the individual lepton fiducial regions and uncorrected for QED effects.

Z ProductionHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionInclusiveSingle Differential Cross SectionP P --> Z0 JET XP P --> GAMMA* JET XProton-Proton ScatteringHigh Energy Physics::ExperimentDSIG/DPTTransverse Momentum DependenceComputer Science::Information Theory
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"Table 13" of "Measurement of the production cross section for Z/gamma* in association with jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS d…

2014

Cross section for Inclusive Jet Multiplicity for the electron channel and the muon channel in the individual lepton fiducial regions and uncorrected for QED effects.

Z ProductionHigh Energy Physics::PhenomenologyIntegrated Cross SectionAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionCross SectionSIGInclusiveP P --> Z0 JET XP P --> GAMMA* JET XProton-Proton ScatteringHigh Energy Physics::ExperimentComputer Science::Information Theory
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"Table 5" of "Measurement of differential Z / gamma* + jet + X cross sections in p anti-p collisions at s**(1/2) = 1.96-TeV"

2008

Integrated cross section.. The second DSYS error is from the muon identification and the third from the luminosity measurement.

Z ProductionPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionCross SectionSIGMuon productionInclusivePhysics::Accelerator PhysicsHigh Energy Physics::ExperimentPBAR P --> Z0 JET XPBAR P --> GAMMA* JET X1960.0
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