Search results for "Astrophysics and Cosmology"

showing 10 items of 28 documents

The Gaia-ESO Survey: Extracting diffuse interstellar bands from cool star spectra DIB-based interstellar medium line-of-sight structures at the kpc s…

2014

We study how diffuse interstellar bands (DIBs) measured toward distance-distributed target stars can be used to locate dense interstellar (IS) clouds in the Galaxy and probe a line-of-sight (LOS) kinematical structure, a potential useful tool when gaseous absorption lines are saturated or not available in the spectral range. Cool target stars are numerous enough for this purpose. We have devised automated DIB fitting methods appropriate to cool star spectra and multiple IS components. The data is fitted with a combination of a synthetic stellar spectrum, a synthetic telluric transmission, and empirical DIB profiles. In parallel, stellar distances and extinctions are estimated self-consisten…

Milky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSpectral line0103 physical sciencesAstronomy Astrophysics and CosmologyISM: general; dust extinction; ISM: lines and bandsEmission spectrum010303 astronomy & astrophysicsGalaxy: generalgeneral [Galaxy]Dust extinctionAstrophysics::Galaxy AstrophysicsISM: generalPhysicsLine-of-sightSpiral galaxygeneral [ISM]010308 nuclear & particles physicsextinctionAstronomy and AstrophysicsAstronomy and AstrophysicISM: lines and bandAstrophysics - Astrophysics of GalaxiesGalaxyISM: lines and bandsAstronomíaInterstellar mediumStars13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)lines and bands [ISM]dust
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Measurements of the center-of-mass energies of e+e- collisions at BESIII

2021

Chinese physics / C 45(10), 103001 (2021). doi:10.1088/1674-1137/ac1575

Nuclear and High Energy PhysicsParticle physicsFOS: Physical sciences53001 natural sciencescenter-of-mass energy; e(+)e(-) annihilation; BESIIINO030218 nuclear medicine & medical imagingHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)03 medical and health sciences0302 clinical medicineAstronomi astrofysik och kosmologi0103 physical sciencesSubatomic PhysicsAstronomy Astrophysics and Cosmologyddc:530Instrumentationcenter-of-mass energyPhysicscenter-of-mass energy e+e- annihilation BESIII010308 nuclear & particles physicsBESIIIE+e-annihilationAstronomy and Astrophysicse(+)e(-) annihilationannihilationExcited stateCenter of masscenter-of-mass energy e+e-
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Measurements of Sigma(+) and Sigma(-) time-like electromagnetic form factors for center-of-mass energies from 2.3864 to 3.0200 GeV

2021

Physics letters / B 814, 136110 (2021). doi:10.1016/j.physletb.2021.136110

Nuclear and High Energy Physicselectric [form factor]Electron–positron annihilationFOS: Physical sciencesSigma hyperonannihilation [electron positron]BESIII; Cross section; Electromagnetic form factor; Σ hyperonhyperon53001 natural sciencesHigh Energy Physics - ExperimentNOSubatomär fysikHigh Energy Physics - Experiment (hep-ex)Angular distributionAstronomi astrofysik och kosmologi0103 physical sciencesSubatomic PhysicsAstronomy Astrophysics and Cosmologyddc:530angular distributionstructure010306 general physicsElectromagnetic form factorPhysics2.3864-3.0200 GeV-cmsBESelectron positron --> Sigma+ Sigma-Cross section010308 nuclear & particles physicsHyperonBESIIIBeijing Storlcsh:QC1-999Sigma HyperonBaryonΣ hyperonmagnetic [form factor]ratio [form factor]valence [quark]colliding beams [electron positron]High Energy Physics::Experimentpair production [Sigma+]Atomic physicsform factor [Sigma-]electromagnetic [form factor]lcsh:Physicsform factor [Sigma+]experimental results
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Measurement of the absolute branching fractions for purely leptonic D+s decays

2021

We report new measurements of the branching fraction $\cal B(D_s^+\to \ell^+\nu)$, where $\ell^+$ is either $\mu^+$ or $\tau^+(\to\pi^+\bar{\nu}_\tau)$, based on $6.32$ fb$^{-1}$ of electron-positron annihilation data collected by the BESIII experiment at six center-of-mass energy points between $4.178$ and $4.226$ GeV. Simultaneously floating the $D_s^+\to\mu^+\nu_\mu$ and $D_s^+\to\tau^+\nu_\tau$ components yields $\cal B(D_s^+\to \tau^+\nu_\tau) = (5.21\pm0.25\pm0.17)\times10^{-2}$, $\cal B(D_s^+\to \mu^+\nu_\mu) = (5.35\pm0.13\pm0.16)\times10^{-3}$, and the ratio of decay widths $R=\frac{\Gamma(D_s^+\to \tau^+\nu_\tau)}{\Gamma(D_s^+\to \mu^+\nu_\mu)} = 9.73^{+0.61}_{-0.58}\pm 0.36$, whe…

Particle physicsFOS: Physical sciences53001 natural sciencesHigh Energy Physics - ExperimentNOStandard ModelSubatomär fysikHigh Energy Physics - Experiment (hep-ex)Astronomi astrofysik och kosmologiSubatomic Physics0103 physical sciencesAstronomy Astrophysics and Cosmologyddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsPhysicsAnnihilation010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixBranching fractionHigh Energy Physics::PhenomenologyDecayHigh Energy Physics::ExperimentEnergy (signal processing)LeptonPhysical Review D
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The ATLAS Inner Detector commissioning and calibration

2010

The ATLAS Inner Detector is a composite tracking system consisting of silicon pixels, silicon strips and straw tubes in a 2 T magnetic field. Its installation was completed in August 2008 and the detector took part in data-taking with single LHC beams and cosmic rays. The initial detector operation, hardware commissioning and insitu calibrations are described. Tracking performance has been measured with 7.6 million cosmic-ray events, collected using a tracking trigger and reconstructed with modular pattern-recognition and fitting software. The intrinsic hit efficiency and tracking trigger efficiencies are close to 100%. Lorentz angle measurements for both electrons and holes, specific energ…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsAstronomyTracking (particle physics)Modules7. Clean energy01 natural sciencesATLAS; calibrationHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Heavy IonsDetectors and Experimental TechniquesDetectors de radiacióPhysicsLarge Hadron ColliderDetectorSettore FIS/01 - Fisica SperimentaleInstrumentation and Detectors (physics.ins-det)ATLASAstrophysics and CosmologyTransition radiation detectormedicine.anatomical_structureIonization EnergyComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCElementary ParticlesQuantum Field TheoryParticle physicsFOS: Physical sciencesCosmic rayddc:500.2HadronsSilicon Pixel Sensors530OpticsQuantum Field TheoriesAtlas (anatomy)0103 physical sciencesCalibrationmedicineddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Measurement Science and InstrumentationOptoelectronics010306 general physicsString TheoryEngineering (miscellaneous)ReadoutNuclear PhysicsATLAS detectorbusiness.industry010308 nuclear & particles physicsFísicaSemiconductor TrackerTransition radiationExperimental High Energy Physicsbusiness
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Complete sets of logarithmic vector fields for integration-by-parts identities of Feynman integrals

2018

Integration-by-parts identities between loop integrals arise from the vanishing integration of total derivatives in dimensional regularization. Generic choices of total derivatives in the Baikov or parametric representations lead to identities which involve dimension shifts. These dimension shifts can be avoided by imposing a certain constraint on the total derivatives. The solutions of this constraint turn out to be a specific type of syzygies which correspond to logarithmic vector fields along the Gram determinant formed of the independent external and loop momenta. We present an explicit generating set of solutions in Baikov representation, valid for any number of loops and external mome…

PhysicsHigh Energy Physics - TheoryPure mathematicsLogarithmLaplace transform010308 nuclear & particles physicsFOS: Physical sciencesAlgebraic geometry01 natural sciencesLoop integralLoop (topology)Dimensional regularizationHigh Energy Physics - PhenomenologyMathematics - Algebraic GeometryHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Astronomi astrofysik och kosmologi0103 physical sciencesFOS: MathematicsAstronomy Astrophysics and CosmologyVector fieldIntegration by parts010306 general physicsAlgebraic Geometry (math.AG)Physical Review D
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Study of $e^{+}e^{-} \to D^{+} D^{-} \pi^{+} \pi^{-} $ at center-of-mass energies from 4.36 to 4.60 GeV

2020

We report a study of the $e^{+}e^{-} \to D^{+} D^{-} \pi^{+} \pi^{-}$ process using $e^{+}e^{-}$ collision data samples with an integrated luminosity of $2.5\,\rm{fb}^{-1}$ at center-of-mass energies from 4.36 to $4.60 \rm{GeV}$, collected with the BESIII detector at the BEPCII storage ring. The $D_{1}(2420)^+$ is observed in the $D^{+} \pi^{+} \pi^{-}$ mass spectrum. The mass and width of the $D_{1}(2420)^+$ are measured to be $(2427.2\pm 1.0_{\rm stat.}\pm 1.2_{\rm syst.}) \rm{MeV}/c^2$ and $(23.2\pm 2.3_{\rm stat.} \pm2.3_{\rm syst.}) \rm{MeV}$, respectively. The first errors are statistical and the second ones are systematic. In addition, the Born cross sections of the $e^{+}e^{-} \to D…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsElectron–positron annihilationAnalytical chemistry01 natural sciences530lcsh:QC1-999High Energy Physics - ExperimentLuminosityNOSubatomär fysikAstronomi astrofysik och kosmologiSubatomic Physics0103 physical sciencesMass spectrumAstronomy Astrophysics and Cosmologyddc:530Center of mass010306 general physicslcsh:Physics
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GRB 030227: The first multiwavelength afterglow of an INTEGRAL GRB

2003

We present multiwavelength observations of a gamma-ray burst detected by INTEGRAL (GRB 030227) between 5.3 hours and ~1.7 days after the event. Here we report the discovery of a dim optical afterglow (OA) that would not have been detected by many previous searches due to its faintess (R~23). This OA was seen to decline following a power law decay with index Alpha_R= -0.95 +/- 0.16. The spectral index Beta_opt/NIR yielded -1.25 +/- 0.14. These values may be explained by a relativistic expansion of a fireball (with p = 2.0) in the cooling regime. We also find evidence for inverse Compton scattering in X-rays.

PhysicsSpectral indexBurstsAstrophysics (astro-ph)Gamma raysCompton scatteringbursts [gamma rays]FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGamma rays ; Bursts ; Photometric ; Cosmology observationsPhotometricUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsCosmology observationsPower law:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]observations [cosmology]Afterglowphotometric [techniques]Space and Planetary ScienceAstronomy Astrophysics and CosmologyUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Neutrino oscillation studies with IceCube-DeepCore

2016

IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make…

Physics::Instrumentation and DetectorsSolar neutrinopoleinteraction [neutrino nucleon]PINGU01 natural sciences7. Clean energyneutrino nucleon: interactionIceCubeenergy: thresholdAstronomi astrofysik och kosmologineutrino: atmosphereAstronomy Astrophysics and Cosmologydetector [neutrino]Physicsneutrino: energy spectrumoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicsatmosphere [neutrino]threshold [energy]mass difference [neutrino]Cosmic neutrino backgroundneutrino: detectorNeutrino detectorPhysique des particules élémentairesMeasurements of neutrino speedNeutrinoperformanceNuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceddc:500.2530neutrino: energySOUTH-POLE0103 physical sciencesddc:530010306 general physicsNeutrino oscillation010308 nuclear & particles physicsICEenergy spectrum [neutrino]Solar neutrino problemneutrino: mixing anglePhysics and Astronomyenergy [neutrino]High Energy Physics::Experimentneutrino: oscillationNeutrino astronomyMATTERSYSTEMmixing angle [neutrino]experimental results
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Multiplicities of charged pions and charged hadrons from deep-inelastic scattering of muons off an isoscalar target

2017

Multiplicities of charged pions and charged hadrons produced in deep-inelastic scattering were measured in three-dimensional bins of the Bjorken scaling variable x , the relative virtual-photon energy y and the relative hadron energy z . Data were obtained by the COMPASS Collaboration using a 160GeV muon beam and an isoscalar target ( 6 LiD). They cover the kinematic domain in the photon virtuality Q2>1(GeV/c)2 , 0.004 1(GeV/c$)^2$, $0.004 < x < 0.4$, $0.2 < z < 0.85$ and $0.1 < y < 0.7$. In addition, a leading-order pQCD analysis was performed using the pion multiplicity results to extract quark fragmentation functions.

QuarkNuclear and High Energy PhysicsPhotonIsoscalarHadronNuclear TheoryHERMEStarget: isoscalar[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex01 natural sciencesCOMPASSscaling: BjorkenNuclear physicsPionAstronomi astrofysik och kosmologi[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astronomy Astrophysics and CosmologyPion multiplicitiesNuclear Physics - Experiment[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]quantum chromodynamics: perturbation theory010306 general physicsNuclear ExperimentRICHDeep inelastic scattering; Fragmentation functions; Pion multiplicities; Nuclear and High Energy PhysicsPhysicsquark: fragmentation functionMuonpi: multiplicityhep-ex010308 nuclear & particles physicsScatteringmuon: beamhigher-order: 0Fragmentation functionphotonFragmentation functionsDeep inelastic scatteringhadron: energylcsh:QC1-999kinematicsPion multiplicitieHigh Energy Physics::ExperimentParticle Physics - Experimentlcsh:PhysicsDeep inelastic scattering
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