0000000000409944

AUTHOR

D. Nakajima

showing 20 related works from this author

Summary of the HypHI Phase 0 experiment and future plans with FRS at GSI (FAIR Phase 0)

2016

WOS: 000381331200014

PhysicsNuclear and High Energy PhysicsCOLLISIONSLifetime measurement010308 nuclear & particles physicsInvariant massLIFETIMEHeavy ion induced reactionHYPERNUCLEAR SPECTROSCOPY01 natural sciencesNuclear physicsShort lifetimeStatistical analysesFRS and Super-FRS0103 physical sciencesRI-beamHeavy ionInvariant massLIGHT HYPERFRAGMENTS010306 general physicsSpectroscopyRELATIVISTIC HYPERNUCLEINuclear Physics A
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Scintillating fiber detectors for the HypHI project at GSI

2009

WOS: 000270326800009

PhysicsNuclear and High Energy PhysicsHydrogenProjectileDetectorPhase (waves)chemistry.chemical_elementTracking (particle physics)Charged particleHypernuclear spectroscopyNuclear physicsTracking detectorschemistryScintillating fiber detectorsDeposition (phase transition)InstrumentationImage resolution
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NEW RESULTS ON NONMESONIC WEAK DECAY OF Lambda HYPERNUCLEI WITH FINUDA

2010

The FINUDA experiment has performed a systematic study of the NonMesonic Weak Decay (NMWD) of Λ hypernuclei analizing all the data collected from 2003 up to 2007. The results of a measurement of the spectra of protons coming from the NMWD of [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text] and [Formula: see text] are the subject of this paper.

Nuclear physicsPhysicsNuclear and High Energy PhysicsFINUDAHypernuclei; nonmesonic weak decay; proton spectraHypernucleiGeneral Physics and AstronomySpectral linenonmesonic weak decayproton spectra
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The HypHI Phase 0 experiment

2010

10th International Conference on Hypernuclear and Strange Particle Physics -- SEP 14-18, 2009 -- Tokai, JAPAN

PhysicsNuclear and High Energy PhysicsCarbon graphiteProjectilehypernuclear spectroscopyPhase (waves)LambdaNuclear physicsheavy ion induced reactioninvariant massHeavy ionENERGY NUCLEAR COLLISIONSAtomic physicsSpectroscopyNuclear Physics A
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Recent results on mesonic weak decay of Λ-hypernuclei

2010

The FINUDA experiment has performed a systematic study of mesonic weak decay of p-shell Λ-hypernuclei. Recent results on the mesonic decay spectra and ratios are illustrated and discussed.

Hypernuclei; mesonic weak decayPhysicsNuclear and High Energy PhysicsFINUDANuclear TheoryLambda-hypernucleiΛ-hypernucleiGeneral Physics and AstronomyLambda-hypernuclei; mesonic decay; spin assignmentAstrophysicsMesonic decayLambdaSpectral lineNuclear physicsSpin assignmentmesonic weak decayΛ-hypernuclei; Mesonic decay; Spin assignmentHypernucleiHigh Energy Physics::ExperimentNuclear Experiment
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In-beam tests of scintillating fibre detectors at MAMI and at GSI

2008

The performance of scintillating fibre detectors was studied with electrons at the spectrometer facility of the Mainz microtron MAMI, as well as in a C-12 beam of 2 AGeV energy and in a beam of different particle species at GSI. Multi-anode photomultipliers were used to read out one or more bundles of 128 fibres each in different geometries. For electrons a time resolution of FWHM = 1 ns was measured in a single detector plane with a detection efficiency epsilon > 99%. A time resolution of 310 ps (FWHM) between two planes of fibres was achieved for carbon ions, leading to a FWHM = 220 ps for a single detector. The hit position residual was measured with a width of FWHM = 0.27 mm. The var…

PhysicsNuclear and High Energy PhysicsPhotomultiplierSpectrometerbusiness.industryDetectorFOS: Physical sciencesCharged particleParticle detectorNuclear physicsFull width at half maximumOpticsNuclear Experiment (nucl-ex)businessInstrumentationMicrotronNuclear ExperimentBeam (structure)
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Multiband variability studies and novel broadband SED modeling of Mrk 501 in 2009

2017

Astronomy and astrophysics 603, A31 (2017). doi:10.1051/0004-6361/201629540

extragalactic background lightmultiwavelength observationsAstrophysics::High Energy Astrophysical Phenomenabl-lacertae objectsGalaxies: BL Lacertae objects: individual: Markarian 501 ; Methods: data analysis ; observational ; Polarizationspectral energy-distributionFluxFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionindividual: Markarian 501 [BL Lacertae objects]lawCoincident0103 physical sciencesddc:530MAGIC (telescope)crab-nebulaBlazardata analysis [Methods]010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)tev blazars010308 nuclear & particles physicsstochastic accelerationtelescope observationsInstitut für Physik und AstronomieAstronomy and AstrophysicsAstronomy and Astrophysicgamma-ray emissionmethods: data analysis520BL Lacertae objects: individual: Markarian 501; Methods: data analysisSynchrotrondata analysi [Methods]BL Lacertae objects: individual: Markarian 501; Methods: data analysis; Astronomy and Astrophysics; Space and Planetary ScienceBL Lacertae objects: individual: Markarian 501x-raySpace and Planetary Scienceddc:520ElectrónicaFísica nuclearElectricidadDegeneracy (mathematics)Astrophysics - High Energy Astrophysical PhenomenaFlareBL Lac object
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First Multi-wavelength Campaign on the Gamma-ray-loud Active Galaxy IC 310

2017

The extragalactic VHE gamma-ray sky is rich in blazars. These are jetted active galactic nuclei viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a larger angle are known so far to emit above 100 GeV. Multi-wavelength studies of such objects up to the highest energies provide new insights into the particle and radiation processes of active galactic nuclei. We report the results from the first multi-wavelength campaign observing the TeV detected nucleus of the active galaxy IC 310, whose jet is observed at a moderate viewing angle of 10 deg - 20 deg. The multi-instrument campaign was conducted between 2012 Nov. and 2013 Jan., and involved observations with MAG…

Active galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesEnergy fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxies: active; Galaxies: individual: IC 310; Gamma rays: galaxies; Astronomy and Astrophysics; Space and Planetary Science01 natural scienceslaw.inventionlawGalaxies: individual: IC 3100103 physical sciencesindividual: IC 310 [galaxies]Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgalaxie [Gamma rays]010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsGalaxies: activeAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesSynchrotrongamma rays: galaxies ; galaxies: active ; individual (IC 310)Gamma rays: galaxiesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)active [galaxies]galaxies [gamma rays]ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGSpectral energy distributionddc:520Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeFlare
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Hypernuclear production cross section in the reaction of 6Li + 12C at 2 A GeV

2015

WOS: 000358624800021

Particle physicsNuclear and High Energy PhysicsPopulationH-4(LAMBDA)BEAMLIFETIMEStrangenessHEAVY-ION COLLISIONSLambdaParticle identificationNuclear physicsHypernucleiInvariant massRapidityeducationNuclear ExperimentPhysicseducation.field_of_studyHeavy ion collisionHyperonRelativistic energyHypernucleuslcsh:QC1-999STATEProduction cross sectionQUANTUM MOLECULAR-DYNAMICSLIGHT HYPERNUCLEIYield ratioDECAYlcsh:PhysicsRELATIVISTIC HYPERNUCLEIPhysics Letters B
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Hypernuclear spectroscopy of products from Li-6 projectiles on a carbon target at 2 A GeV

2013

WOS: 000322848900009

Nuclear reaction(Li-6E=2 GeV/nucleonNuclear and High Energy PhysicsMaximum likelihoodWEAK DECAYFOS: Physical sciencesLIFETIMET-1/2. Compared with other datadeduced Lambda massC-12(LAMBDA)H-4)T-1/2measured Lambda H-3H-4 Lambda-hypernuclei invariant mass distribution T-1/2measured LambdaInvariant massNuclear Experiment (nucl-ex)LIGHT HYPERFRAGMENTSSpectroscopyNuclear ExperimentX)PhysicsH-4 Lambda-hypernuclei invariant mass distributionH-3ProjectileSignificance valueslifetime measurementdeduced Lambda mass H-3H-4 Lambda-hypernuclei mass T-1/2. Compared with other data lifetime measurementNUCLEAR REACTIONS C(Li-6Decay timeLAMBDA-HYPERNUCLEIAtomic physicst)NUCLEAR REACTIONS C(Li-6 X) (Li-6 t) (Li-6 H-4) E=2 GeV/nucleonH-4 Lambda-hypernuclei massHypertritonRELATIVISTIC HYPERNUCLEINuclear Physics A
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Production of hypernuclei in peripheral HI collisions: The HypHI project at GSI

2012

ECT Workshop on Strange Hadronic Matter -- SEP 26-30, 2011 -- Trento, ITALY

PhysicsNuclear and High Energy PhysicsPhase (waves)chemistry.chemical_elementInvariant massLIFETIMEHeavy ion induced reactionHypernuclear spectroscopyNuclear physicschemistryMass spectrumLithiumHeavy ionInvariant massENERGY NUCLEAR COLLISIONSAtomic physicsSpectroscopyRELATIVISTIC HYPERNUCLEI
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The HypHI project: Hypernuclear spectroscopy with stable heavy ion beams and rare isotope beams at GSI and FAIR

2009

The HypHI collaboration aims to perform a precise hypernuclear spectroscopy with stable heavy ion beams and rare isotope beams at GSI and fAIR in order to study hypernuclei at extreme isospin, especially neutron rich hypernuclei to look insight hyperon-nucleon interactions in the neutron rich medium, and hypernuclear magnetic moments to investigate baryon properties in the nuclei. We are currently preparing for the first experiment with $^6$Li and $^{12}$C beams at 2 AGeV to demonstrate the feasibility of a precise hypernuclear spectroscopy by identifying $^{3}_{\Lambda}$H, $^{4}_{\Lambda}$H and $^{5}_{\Lambda}$He. The first physics experiment on these hypernuclei is planned for 2009. In th…

PhysicsNuclear and High Energy PhysicsIsotopeMagnetic momentNuclear TheoryGeneral Physics and AstronomyOrder (ring theory)FOS: Physical sciencesLambdaBaryonNuclear physicsIsospinNeutronNuclear Experiment (nucl-ex)Nuclear ExperimentSpectroscopyNuclear Experiment
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Mesonic and Non-Mesonic Weak Decay of Hypernuclei with FINUDA

2009

Abstract The FINUDA experiment performed a systematic study of both mesonic and non-mesonic weak decay of p - shell Λ-hypernuclei. Recent results on the mesonic decay rates and the non-mesonic decay ratios are illustrated and briefly discussed.

PhysicsNuclear and High Energy PhysicsΛ-hypernuclei mesonic decay non-mesonic decay FINUDA experimentHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyNuclear TheoryΛ-hypernucleiShell (structure)FINUDA experimentweak decaymesonic decayNuclear physicsHypernuclei; weak decayHypernucleinon-mesonic decayHigh Energy Physics::ExperimentNuclear ExperimentFINUDA experiment; mesonic decay; non-mesonic decay; Λ-hypernuclei
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Event reconstruction methods for the HypHI Phase 0 experiment at GSI

2010

WOS: 000282530300034

PhysicsNuclear and High Energy PhysicsEvent reconstructionPhase (waves)Kalman filterHypHICollisionHough transformlaw.inventionHypernuclear spectroscopyNuclear physicsHough transformlawHeavy ionKalman filterSpectroscopyInstrumentationEvent reconstruction
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On the measured lifetime of light hypernuclei 3ΛH and 4ΛH

2014

A statistical combination of the experimental lifetime estimations available in the literatures is performed for 3 Λ H and 4 Λ H, including several recent measurements. The combined average values of the lifetime for 3 Λ H and 4 Λ H are respectively 216−16+19 ps and 192−18+20 ps with a reduced χ2 of 0.89 and 0.48. A new insight into the lifetime estimation of the HypHI Phase 0 experiment by a Bayesian approach is also presented. In this approach, several different prior distributions including the combination of previous lifetime data and a Jeffrey prior are used. The principal mode and the smallest credible interval at 68% of the posterior distribution, given by the prior belief of the pre…

PhysicsNuclear physicsNuclear and High Energy PhysicsLifetime measurementPosterior probabilityHypernucleiBayesian approachCredible intervalddc:530LambdaHypertritonAveraged combinationPhysics Letters B
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Black hole lightning due to particle acceleration at subhorizon scales

2015

Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio interferometry, but still suffer from insufficient angular resolution. An alternative method to resolve small structures is to measure the time variability of their emission. Here, we report on gamma-ray observations of the radio galaxy IC 310 obtained with the MAGIC telescopes revealing variability with doubling time scales faster than 4.8 min. Causality constrains the size of the emission region to be smaller than 20\% of the gravitational radius of its central black hole. We suggest that the emission is associated …

Black HolesRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsVery High Energy Gamma AstronomyBlack Holes Very High Energy Gamma Astronomy Active Galactic NucleiX-shaped radio galaxysupermassive black hole ; jet formation ; IC 310 ; MAGIC telescopesAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HESupermassive black holeta115MultidisciplinaryPhysicsActive Galactic NucleiAstronomy and AstrophysicsGalaxyIntermediate-mass black holeStellar black holeElectrónicaFísica nuclearddc:500Spin-flipElectricidadAstrophysics - High Energy Astrophysical PhenomenaSchwarzschild radius
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Hypernuclear spectroscopy with heavy ion beams: The HypHI project at GSI and fair

2010

The HypHI experiment for precise hypernuclear spectroscopy with induced reactions of stable heavy ion beams and rare isotope beams is currently under preparation at GSI. The main goal of the HypHI project is to study neutron and proton rich hypernuclei and to measure directly hypernuclear magnetic moments at GSI and FAIR. In the first HypHI experiment (Phase 0) planned in 2009, the feasibility of precise hypernuclear spectroscopy with heavy ion beams will be demonstrated by observing π- decay channels of [Formula: see text], [Formula: see text] and [Formula: see text] with 6 Li projectiles at 2 A GeV impinging on a 12 C target. An overview of the HypHI project and the details of the Phase …

PhysicsNuclear and High Energy PhysicsRI-beamsProtonNuclear TheoryGeneral Physics and AstronomyHypernuclear spectroscopyNuclear physicsmagnetic momentsexotic hypernucleiPhysics::Accelerator PhysicsHeavy ionNeutronheavy ion beamsENERGY NUCLEAR COLLISIONSSpectroscopyNuclear Experiment
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New results on mesonic weak decay of p-shell Lambda-hypernuclei

2009

The FINUDA experiment performed a systematic study of the charged mesonic weak decay channel of $p$-shell $\Lambda$-hypernuclei. Negatively charged pion spectra from mesonic decay were measured with magnetic analysis for the first time for ${^{7}_{\Lambda}Li}$, ${^{9}_{\Lambda}Be}$, ${^{11}_{\Lambda}B}$ and ${^{15}_{\Lambda}N}$. The shape of the $\pi^{-}$ spectra was interpreted through a comparison with pion distorted wave calculations that take into account the structure of both hypernucleus and daughter nucleus. Branching ratios $\Gamma_{\pi^{-}}/\Gamma_{tot}$ were derived from the measured spectra and converted to $\pi^{-}$ decay rates $\Gamma_{\pi^{-}}$ by means of known or extrapolate…

PhysicsGround-state spin assignmentNuclear and High Energy Physicsp-Shell Lambda-hypernuclei; Mesonic decayNuclear Theorylambda hypernuclei; mesonic decaylambda hypernucleiHypernucleusMesonic decaySpectral linemesonic decayPionmedicine.anatomical_structurep-Shell Lambda-hypernucleimedicineHigh Energy Physics::Experimentp-Shell Λ-hypernucleiAtomic physicsMagnetic analysisNuclear ExperimentNuclear ExperimentNucleus
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First measurements of Λ and hyperons in elementary electroproduction at MAMI

2010

Abstract Since 2008 the magnetic spectrometer Kaos , dedicated to the detection of charged kaons, is operating at the 1.5 GeV electron beam of MAMI at the Institut fur Kernphysik in Mainz, Germany. The strangeness programme performed in 2008–9 is addressing some important issues in the field of elementary kaon photoelectro-production reactions. The identification of Λ and Σ 0 hyperons in the missing mass spectra from kaon production off a liquid hydrogen target demonstrates the capability of the extended facility to perform strangeness electro-production spectroscopy at low momentum transfers Q 2 0.5 ( GeV / c ) 2 . Systematic uncertainties in the cross-section extraction from the data are …

PhysicsNuclear and High Energy PhysicsParticle physicsSpectrometerField (physics)010308 nuclear & particles physicsNuclear TheoryHyperonStrangeness01 natural sciencesNuclear physicsMomentum0103 physical sciencesMass spectrumHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsSpectroscopyNuclear Physics A
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Multifrequency Studies of the Peculiar Quasar 4C +21.35 during the 2010 Flaring Activity

2014

著者人数: 290名

AstrofísicaelectronPhotontorusAstrophysics01 natural scienceslaw.inventiongalaxies: active – gamma rays: general – quasars: general – quasars: individual (4C +21.35) – radiation mechanisms: non-thermalactive gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermal [galaxies]lawblack hole: Kerrgalaxies: active; gamma rays: general; quasars: general; quasars: individual: 4C +21.35; radiation mechanisms: non-thermalopticalGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsenergy: highPhysicsphotonRadiusnon-thermal [radiation mechanisms]Synchrotrongamma ray: emissionactive [galaxies]astro-ph.COElectrónicaFísica nuclearElectricidadGalaxies: active; Gamma rays: general; Quasars: general; Quasars: individual (4C +21.35); Radiation mechanisms: non-thermal; Nuclear and High Energy PhysicsAstrophysics - High Energy Astrophysical Phenomenaquasars: individual (4C +21.35)Astrophysics - Cosmology and Nongalactic AstrophysicsFlareradiation mechanisms: non-thermal; galaxies: active; quasars: general; quasars: individual (4C +21.35); gamma rays: observationsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)astro-ph.GAAstrophysics::High Energy Astrophysical Phenomenaeducationgalaxies: activeFOS: Physical sciencesquasars: individual: 4C +21.35Astrophysics::Cosmology and Extragalactic AstrophysicsVHEGLASTemission: modelTelescopeX-rayquasars: general0103 physical sciencessynchrotrongalaxies: active gamma rays: general quasars: general quasars: individual: 4C +21.35 radiation mechanisms: non-thermalquasarflux: densityindividual: 4C +21.35 [quasars]Astrophysics::Galaxy AstrophysicsAstronomia Observacionsgeneral [quasars]010308 nuclear & particles physicsAstronomy and AstrophysicsQuasargamma rays: generalradiation mechanisms: non-thermalAstrophysics - Astrophysics of GalaxiesMAGICRotating black holeSpace and Planetary SciencegravitationAstrophysics of Galaxies (astro-ph.GA)ddc:520spectral[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [gamma rays]Fermi Gamma-ray Space Telescope
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