0000000000214458

AUTHOR

Yuichiro Sekiguchi

showing 6 related works from this author

Measurement of PromptD-Meson Production inp−PbCollisions atsNN=5.02  TeV

2014

The p_{T}-differential production cross sections of the prompt charmed mesons D^{0}, D^{+}, D^{*+}, and D_{s}^{+} and their charge conjugate in the rapidity interval -0.96<y_{cms}<0.04 were measured in p-Pb collisions at a center-of-mass energy sqrt[s_{NN}]=5.02 TeV with the ALICE detector at the LHC. The nuclear modification factor R_{pPb}, quantifying the D-meson yield in p-Pb collisions relative to the yield in pp collisions scaled by the number of binary nucleon-nucleon collisions, is compatible within the 15%-20% uncertainties with unity in the transverse momentum interval 1<p_{T}<24 GeV/c. No significant difference among the R_{pPb} of the four D-meson species is observed. The results…

PhysicsParticle physicsMeson010308 nuclear & particles physicsHadronGeneral Physics and Astronomy7. Clean energy01 natural sciencesNuclear physicsMomentum0103 physical sciencesD mesonHigh Energy Physics::ExperimentProduction (computer science)RapidityNuclear Experiment010306 general physicsEnergy (signal processing)BosonPhysical Review Letters
researchProduct

Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

2021

We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data from the first three observing runs of the Advanced LIGO and Advanced Virgo detectors. For the first time, we include Virgo data in our analysis and run our search with a new efficient pipeline called {\tt PyStoch} on data folded over one sidereal day. We use gravitational-wave radiometry (broadband and narrow band) to produce sky maps of stochastic gravitational-wave backgrounds and to search for gravitational waves from point sources. A spherical harmonic decomposition method is employed to look for gravitational-wave emission from spatially-extended sources. Neither technique found eviden…

gravitational radiation: anisotropyPhysics and Astronomy (miscellaneous)gravitational radiation: stochasticAstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsCosmology & Astrophysicsenergy: fluxenergy: densitygravitational radiation: energyLIGOQCQBPhysicsSettore FIS/01Spectral indexPhysicsGalactic CenterAmplitudeGeneral relativitySidereal timePhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]gravitational radiation: power spectrumGravitationdata analysis methodAnisotropic stochastic gravitational-wave backgroundExperimental studies of gravityFOS: Physical sciencesO3O2General Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsStochastic Background Gravitational Waves LIGO Virgo O1 O2 O3O1Gravitational wavesGeneral Relativity and Quantum CosmologyUPPER LIMITSstatistical analysis0103 physical sciencesadvanced LIGO and Virgoddc:530KAGRAKAGRACosmology &amp; Astrophysics010306 general physicsSTFCgravitational waves; LIGO; VirgoGravitational WavesScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundRCUKGalaxyLIGOVIRGOgravitational radiation: emissionspectrum: densityRADIATIONCROSS-CORRELATION SEARCHStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikgalaxyExperimental studies of gravity; General relativity; Gravitational waves
researchProduct

Azimuthal anisotropy ofD-meson production in Pb-Pb collisions atsNN=2.76TeV

2014

The production of the prompt charmed mesons D0, D+, and D*+ relative to the reaction plane was measured in Pb-Pb collisions at a center-of-mass energy per nucleon-nucleon collision of √sNN=2.76TeV with the ALICE detector at the CERN Large Hadron Collider. D mesons were reconstructed via their hadronic decays at central rapidity in the transverse-momentum (p_T) interval 2–16 GeV/c. The azimuthal anisotropy is quantified in terms of the second coefficient v2 in a Fourier expansion of the D-meson azimuthal distribution and in terms of the nuclear modification factor R_AA, measured in the direction of the reaction plane and orthogonal to it. The v2 coefficient was measured with three different …

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderMeson010308 nuclear & particles physicsPlane (geometry)Hadron01 natural sciences7. Clean energyNuclear physicsYield (chemistry)0103 physical sciencesD mesonHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsAnisotropyPhysical Review C
researchProduct

Multi-particle azimuthal correlations in p-Pb and Pb-Pb collisions at the CERN Large Hadron Collider

2014

Measurements of multi-particle azimuthal correlations (cumulants) for charged particles in p-Pb and Pb-Pb collisions are presented. They help address the question of whether there is evidence for global, flow-like, azimuthal correlations in the p-Pb system. Comparisons are made to measurements from the larger Pb-Pb system, where such evidence is established. In particular, the second harmonic two-particle cumulants are found to decrease with multiplicity, characteristic of a dominance of few-particle correlations in p-Pb collisions. However, when a $|\Delta \eta|$ gap is placed to suppress such correlations, the two-particle cumulants begin to rise at high-multiplicity, indicating the prese…

Pb-Pb collisionsazimuthal correlationsPb-Pb and p-Pb collisions at the LHCPpb CollisionsHigh multiplicityppQUARK-GLUON PLASMAALICEp-Pb collisionsRoot-S(Nn)=5.02 Tevcharged particlesPbPbNuclear Experiment (nucl-ex)Nuclear ExperimentPhysicsLarge Hadron Colliderazimuthal correlations; p-Pb collisions; Pb-Pb collisionsFlowPhysicsLong-RangeCharged particle3. Good health:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]AzimuthPRIRODNE ZNANOSTI. Fizika.LHCThird harmonicLHC; ALICE; pp; PbPb; Azimuthal correlationsParticle Physics - ExperimentParticle physicsNuclear and High Energy PhysicsVDP::Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431FOS: Physical sciencesEccentricities[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear physicsNuclear Physics - ExperimentDependenceCumulantNUCLEUS-NUCLEUS COLLISIONS; QUARK-GLUON PLASMA; ANGULAR-CORRELATIONSTransverse-Momentumta114VDP::Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431NUCLEUS-NUCLEUS COLLISIONS:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]ALICE experimentMultiplicity (mathematics)ANGULAR-CORRELATIONSNATURAL SCIENCES. Physics.Quark–gluon plasma
researchProduct

Efficient magnetic-field amplification due to the Kelvin-Helmholtz instability in binary neutron star mergers

2015

We explore magnetic-field amplification due to the Kelvin-Helmholtz instability during binary neutron star mergers. By performing high-resolution general relativistic magnetohydrodynamics simulations with a resolution of $17.5$ m for $4$--$5$ ms after the onset of the merger on the Japanese supercomputer "K", we find that an initial magnetic field of moderate maximum strength $10^{13}$ G is amplified at least by a factor of $\approx 10^3$. We also explore the saturation of the magnetic-field energy and our result shows that it is likely to be $\gtrsim 4 \times 10^{50}$ erg, which is $\gtrsim 0.1\%$ of the bulk kinetic energy of the merging binary neutron stars.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Nuclear TheoryAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesBinary numberGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinetic energyInstabilityGeneral Relativity and Quantum CosmologyMagnetic fieldNuclear Theory (nucl-th)Numerical relativityNeutron starAstrophysics - Solar and Stellar AstrophysicsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaSaturation (magnetic)Solar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
researchProduct

Nuclear matter effects onJ/ψproduction in asymmetric Cu + Au collisions atsNN=200GeV

2014

We report on J/psi production from asymmetric Cu + Au heavy-ion collisions at root S-NN = 200 GeV at the Relativistic Heavy Ion Collider at both forward (Cu-going direction) and backward (Au-going direction) rapidities. The nuclear modification of J/psi yields in Cu + Au collisions in the Au-going direction is found to be comparable to that inAu + Au collisions when plotted as a function of the number of participating nucleons. In the Cu-going direction, J/psi production shows a stronger suppression. This difference is comparable in magnitude and has the same sign as the difference expected from shadowing effects due to stronger low-x gluon suppression in the larger Au nucleus.

PhysicsNuclear and High Energy PhysicsQuantitative Biology::Neurons and Cognition010308 nuclear & particles physicsNuclear TheoryNuclear matter01 natural sciences7. Clean energyGluonNuclear physicsmedicine.anatomical_structure0103 physical sciencesmedicineEnergy densityHigh Energy Physics::ExperimentAngular dependenceAtomic physicsNuclear Experiment010306 general physicsNucleonRelativistic Heavy Ion ColliderNucleusPhysical Review C
researchProduct