Search results for "Astrophysics"

showing 10 items of 8341 documents

Exploration of jet substructure using iterative declustering in pp and Pb–Pb collisions at LHC energies

2020

The ALICE collaboration at the CERN LHC reports novel measurements of jet substructure in pp collisions at $\sqrt{s}$= 7 TeV and central Pb-Pb collisions at $\sqrt{s_{\rm{NN}}}$ = 2.76 TeV. Jet substructure of track-based jets is explored via iterative declustering and grooming techniques. We present the measurement of the momentum sharing of two-prong substructure exposed via grooming, the $z_{\rm{g}}$, and its dependence on the opening angle, in both pp and Pb-Pb collisions. We also present the first measurement of the distribution of the number of branches obtained in the iterative declustering of the jet, which is interpreted as the number of its hard splittings. In Pb-Pb collisions, we…

jet substructure pp and Pb-Pb collisionsheavy ion: scattering:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Physics::Instrumentation and DetectorsMonte Carlo methodPb-Pbjet quenchin; jet substructure; heavy-ion collisionshiukkasfysiikkapp and Pb-Pb collisionsnucl-expp01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEjetscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]color: coherenceNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentMonte Carlojet ; declustering ; pp ; Pb-PbPhysicsLarge Hadron ColliderPhysicsVDP::Kjerne- og elementærpartikkelfysikk: 431suppressionlcsh:QC1-999PRIRODNE ZNANOSTI. Fizika.CERN LHC Coll:Nuclear and elementary particle physics: 431 [VDP]VDP::Nuclear and elementary particle physics: 431PYTHIAdeclusteringLHCpp collisionsParticle Physics - ExperimentCoherence (physics)Nuclear and High Energy Physicsp p: scatteringAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciencesNuclear physicsheavy-ion; pp collisions; jet substructure; ALICEscattering [heavy ion]0103 physical sciencesddc:530jet substructureNuclear Physics - Experiment010306 general physicsenhancementjet quenchin010308 nuclear & particles physicshep-exheavy-ion collisionsNATURAL SCIENCES. Physics.7000 GeV-cms/nucleon 2760 GeV-cms/nucleonHeavy ion interactionQGPQuark–gluon plasmaheavy-ioncoherence [color]SubstructureHigh Energy Physics::ExperimentLHC jet QGPLHC High-Energy Physicslcsh:Physicsexperimental results
researchProduct

The WEBT BL Lacertae Campaign 2001 and its extension : Optical light curves and colour analysis 1994–2002

2004

BL Lacertae has been the target of four observing campaigns by the Whole Earth Blazar Telescope (WEBT) collaboration. In this paper we present UBVRI light curves obtained by theWEBT from 1994 to 2002, including the last, extended BL Lac 2001 campaign. A total of about 7500 optical observations performed by 31 telescopes from Japan to Mexico have been collected, to be added to the ∼15 600 observations of the BL Lac Campaign 2000. All these data allow one to follow the source optical emission behaviour with unprecedented detail. The analysis of the colour indices reveals that the flux variability can be interpreted in terms of two components: longer-term variations occurring on a fewday time …

jetsAstrophysics::High Energy Astrophysical PhenomenaFluxScale (descriptive set theory)activeAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA01 natural sciencesPower lawlaw.inventionTelescopesymbols.namesakelawBL Lac objects0103 physical sciencesJetsBlazar010303 astronomy & astrophysicsQuasarsAstrophysics::Galaxy AstrophysicsPhysicsactive; galaxies: BL Lacertae objects: general; galaxies: jets; galaxies: quasars: general010308 nuclear & particles physicsActive galaxies ; BL Lacertae objects ; Jets ; Quasarsactive galaxiesAstronomy and AstrophysicsDecoupling (cosmology)galaxies: jetsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]galaxies: quasars: generalSpace and Planetary Scienceactive galaxies; BL Lac objects; jetssymbolsgalaxies: BL Lacertae objects: generalActive galaxiesBL Lacertae objectsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaDoppler effect:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

Laboratory formation of a scaled protostellar jet by coaligned poloidal magnetic field

2014

International audience; Although bipolar jets are seen emerging from a wide variety of astrophysical systems, the issue of their formation and morphology beyond their launching is still under study. Our scaled laboratory experiments, representative of young stellar object outflows, reveal that stable and narrow collimation of the entire flow can result from the presence of a poloidal magnetic field whose strength is consistent with observations. The laboratory plasma becomes focused with an interior cavity. This gives rise to a standing conical shock from which the jet emerges. Following simulations of the process at the full astrophysical scale, we conclude that it can also explain recentl…

jetsPhysicsJet (fluid)MultidisciplinaryShock (fluid dynamics)Young stellar objectAstrophysics::High Energy Astrophysical PhenomenaFlow (psychology)PlasmaConical surfaceAstrophysics01 natural sciencesSIMULATIONS010305 fluids & plasmasMagnetic fieldCOLLIMATION[PHYS.COND.CM-S]Physics [physics]/Condensed Matter [cond-mat]/Superconductivity [cond-mat.supr-con]DISCOVERY0103 physical sciencesDG-TAURI010303 astronomy & astrophysicsACCRETION DISCSAstrophysics::Galaxy AstrophysicsDRIVEN JETS
researchProduct

Determining the infrared radiative effects of Saharan dust: a radiative transfer modelling study based on vertically resolved measurements at Lampedu…

2018

Detailed measurements of radiation, atmospheric and aerosol properties were carried out in summer 2013 during the Aerosol Direct Radiative Impact on the regional climate in the MEDiterranean region (ADRIMED) campaign in the framework of the Chemistry-Aerosol Mediterranean Experiment (ChArMEx) experiment. This study focusses on the characterization of infrared (IR) optical properties and direct radiative effects of mineral dust, based on three vertical profiles of atmospheric and aerosol properties and IR broadband and narrowband radiation from airborne measurements, made in conjunction with radiosonde and ground-based observations at Lampedusa, in the central Mediterranean. Satellite IR spe…

lcsh:Chemistrylcsh:QD1-999Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPhysics::Atmospheric and Oceanic PhysicsAstrophysics::Galaxy Astrophysicslcsh:Physicslcsh:QC1-999Atmospheric Chemistry and Physics
researchProduct

Calibration of high voltages at the ppm level by the difference of $$^{83{\mathrm{m}}}$$ 83m Kr conversion electron lines at the KATRIN experiment

2018

The neutrino mass experiment KATRIN requires a stability of 3 ppm for the retarding potential at − 18.6 kV of the main spectrometer. To monitor the stability, two custom-made ultra-precise high-voltage dividers were developed and built in cooperation with the German national metrology institute Physikalisch-Technische Bundesanstalt (PTB). Until now, regular absolute calibration of the voltage dividers required bringing the equipment to the specialised metrology laboratory. Here we present a new method based on measuring the energy difference of two $$^{83{\mathrm{m}}}$$ 83m Kr conversion electron lines with the KATRIN setup, which was demonstrated during KATRIN’s commissioning measurements …

lcsh:QB460-466lcsh:QC770-798lcsh:Astrophysicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityEuropean Physical Journal C: Particles and Fields
researchProduct

Theoretical estimates of supernova-neutrino cross sections for the stable even-even lead isotopes: Charged-current reactions

2016

A detailed study of the charged-current supernova electron neutrino and electron antineutrino scattering off the stable even-mass lead isotopes A = 204, 206, and 208 is reported in this work. The proton-neutron quasiparticle random-phase approximation (pnQRPA) is adopted to construct the nuclear final and initial states. Three different Skyrme interactions are tested for their isospin and spin-isospin properties and then applied to produce (anti)neutrino-nucleus scattering cross sections for (anti)neutrino energies below 80 MeV. Realistic estimates of the nuclear responses to supernova (anti)neutrinos are computed by folding the computed cross sections with a two-parameter Fermi-Dirac distr…

lead isotopesAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNuclear TheoryscatteringHigh Energy Physics::Experimentneutrino-nucleus interactionselectron neutrinoNuclear Experimentelectron antineutrinosupernova neutrinos
researchProduct

Theoretical study of supernova neutrino and antineutrino scattering off the stable cadmium and lead isotopes

2017

In this thesis work, an extensive study of neutrino- and antineutrino-nucleus interactions is performed. The work is focused on supernova-neutrino scattering off the stable cadmium and lead isotopes. The studied nuclei are of interest for the investigations of neutrino-properties and for neutrino-detection experiments. The adopted nuclear-structure models are based on the quasiparticle random-phase approximation (QRPA) and the microscopic quasiparticle- phonon model (MQPM) and the cross-sections calculations are based on the Donnelly-Walecka formalism. The computed cross sections are folded with a two-parameter Fermi-Dirac distribution to obtain realistic estimates of the nuclear responses …

leadisotoopitcadmiumAstrophysics::High Energy Astrophysical PhenomenaNuclear Theoryscatteringneutriinotstable isotopesneutrinosnucleisirontalyijyNuclear Experimentsupernova neutrinoskadmium
researchProduct

Searches for lepton number violation and resonances in K± → πμμ decays

2017

The NA48/2 experiment at CERN collected a large sample of charged kaon decays to final states with multiple charged particles in 2003–2004. A new upper limit on the rate of the lepton number violating decay K±→π∓μ±μ± is reported: B(K±→π∓μ±μ±)<8.6×10−11 at 90% CL. Searches for two-body resonances X in K±→πμμ decays (such as heavy neutral leptons N4 and inflatons χ ) are also presented. In the absence of signals, upper limits are set on the products of branching fractions B(K±→μ±N4)B(N4→πμ) and B(K±→π±X)B(X→μ+μ−) for ranges of assumed resonance masses and lifetimes. The limits are in the (10−11,10−9) range for resonance lifetimes below 100 ps.

leptonBEAM01 natural sciences7. Clean energyPhysics Particles & FieldsHigh Energy Physics - ExperimentLIMITSkaon physicsCERNIntermediate statelepton number violation neutrinos dark matter kaon physicsPhysicsVMSMLarge Hadron ColliderPhysicsCharge KaonsneutrinosNuclear and High Energy Physics; CERN; leptonsHigh Energy Physics - Experiment; Charge Kaons; Lepton number violationNuclear & Particles PhysicsCharged particlelcsh:QC1-999NEUTRAL HEAVY-LEPTONSPhysics Nuclearlepton number violationPhysical SciencesParticle physicsNuclear and High Energy Physicsleptonskaon decays lepton number violationNuclear and High Energy Physics lepton kaon meson lepton number violation NA48Socio-culturaleAstronomy & AstrophysicsUPPER-BOUNDSdark matterNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physics0103 physical sciencesDARK-MATTERPARTICLES010306 general physicsScience & Technologykaon decays010308 nuclear & particles physicsBranching fractionResonanceInflatonLepton numberkaon mesonNA48High Energy Physics::Experimentlcsh:PhysicsLepton
researchProduct

Preliminary analysis of CH3D from 3250 to 3700 cm(-1)

2006

International audience; The infrared spectrum of CH3D from 3250 to 3700 cm(-1) was studied for the first time to assign transitions involving the nu(2) + nu(3), nu(2) + nu(5), nu(2) + nu(6), nu(3) + 2(nu 6) and 3 nu(6) vibrational states. Line positions and intensities were measured at 0.011 cm(-1) resolution using Fourier transform spectra recorded at Kitt Peak with isotopically enriched samples. Some 2852 line positions (involving over 900 upper state levels) and 874 line intensities were reproduced with RMS values of 0.0009 cm(-1) and 4.6%, respectively. The strongest bands were found to be nu(2) + nu(3) at 3499.7 cm(-1) and nu(2) + nu(6) at 3342.5 cm(-1) with integrated strengths, respe…

line intensitieshot bands010504 meteorology & atmospheric sciencesInfraredmonodeuterated methaneFourier transform spectra01 natural sciencesPreliminary analysisRoot mean squaresymbols.namesake0103 physical sciencesline positionsPhysical and Theoretical Chemistry010303 astronomy & astrophysicsSpectroscopydatabase0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Physics33.20.EaAtomic and Molecular Physics and OpticsCH3D[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph][ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]symbols[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physicsGround stateHamiltonian (quantum mechanics)
researchProduct

Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino

2017

We detected the seasonal modulation of the $^7$Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99\% C.L. The data are analyzed using three methods: the sinusoidal fit, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.

liquid scintillators detectorsPhysics - Instrumentation and Detectorsexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinolow background detectorsSolar neutrinos01 natural sciencesflux: time dependenceneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Liquid scintillators detectors; Low background detectors; Neutrino oscillations; Solar neutrinos; Astronomy and Astrophysics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Borexinoneutrino: interactionMSW effectPhysicsNeutrino oscillationsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)neutrino electron: elastic scatteringmodulationAmplitudeModulationsolar neutrinosBorexinoNeutrinoLiquid scintillators detectorFLUXLow background detectordata analysis methodNeutrino oscillationFOS: Physical sciencesSolar neutrinoNuclear physicsTIME-SERIES ANALYSIS[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Low background detectorsLiquid scintillators detectorsSEARCH0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SPACED DATA010306 general physicsNeutrino oscillationbackground: radioactivityneutrino oscillations010308 nuclear & particles physicsAstronomy and AstrophysicsEMPIRICAL MODE DECOMPOSITIONberylliumGran SassoHigh Energy Physics::Experimentneutrino: oscillationEvent (particle physics)experimental results
researchProduct