Search results for "Particle physics"

showing 10 items of 6826 documents

Theory of Neutrinos: A White Paper

2005

During 2004, four divisions of the American Physical Society commissioned a study of neutrino physics to take stock of where the field is at the moment and where it is going in the near and far future. Several working groups looked at various aspects of this vast field. The summary was published as a main report entitled ``The Neutrino Matrix'' accompanied by short 50 page versions of the report of each working group. Theoretical research in this field has been quite extensive and touches many areas and the short 50 page report provided only a brief summary and overview of few of the important points. The theory discussion group felt that it may be of value to the community to publish the e…

Neutrino mass physics; Matter-antimatter asymmetry of the UniverseParticle physicsSupersymmetric Standard ModelPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaElectric-dipole momentsPhysics beyond the Standard ModelFOS: Physical sciencesGeneral Physics and AstronomyTheoretical researchHigh Energy Physics - Phenomenology (hep-ph)White paperSee-saw mechanismneutriniPublicationParticle Physics - PhenomenologyPhysicsLepton-flavor violationDiscussion groupbusiness.industryHigh Energy Physics::PhenomenologyFísicaMatter-antimatter asymmetry of the UniverseDouble beta decaySettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciEpistemologyElectroweak symmetry-breakingHigh Energy Physics - PhenomenologyLarge extra dimensionsNeutrino mass physicsHeavy Majorana neutrinosHigh Energy Physics::ExperimentRight-handed neutrinoNeutrinoAnomalous magnetic momentWorking groupbusiness
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Testing isotropy of the universe using the Ramsey resonance technique on ultracold neutron spins

2010

Physics at the Planck scale could be revealed by looking for tiny violations of fundamental symmetries in low energy experiments. In 2008, a sensitive test of the isotropy of the Universe using has been performed with stored ultracold neutrons (UCN), this is the first clock-comparison experiment performed with free neutrons. During several days we monitored the Larmor frequency of neutron spins in a weak magnetic field using the Ramsey resonance technique. An non-zero cosmic axial field, violating rotational symmetry, would induce a daily variation of the precession frequency. Our null result constitutes one of the most stringent tests of Lorentz invariance to date.

Neutron electric dipole momentAtomic Physics (physics.atom-ph)FOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Lorentz covariance01 natural sciencesResonance (particle physics)Physics - Atomic PhysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Quantum mechanics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutronNuclear Experiment (nucl-ex)Electrical and Electronic Engineering010306 general physicsNuclear ExperimentLarmor precessionPhysics[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Spins010308 nuclear & particles physicsCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsNeutron spectroscopyUltracold neutrons
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SEARCHES FOR POINT-LIKE AND EXTENDED NEUTRINO SOURCES CLOSE TO THE GALACTIC CENTER USING THE ANTARES NEUTRINO TELESCOPE

2014

A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been found. The most signal-like accumulation of events is located at equatorial coordinates R.A. = -46º.8 and decl. = -64º.9 and corresponds to a 2.2 sigma background fluctuation. In addition, upper limits on the flux normalization of an E-2 muon neutrino energy spectrum have been set for 50 pre-selected astrophysical objects. Finally, motivated by an accumulation of seven events relatively close to the Galactic Center in the recently reported neutrino sample…

Normalization (statistics)AstrofísicaParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicslaw.inventionHigh Energy Physics - ExperimentTelescopeHigh Energy Physics - Experiment (hep-ex)neutrinolaw[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Point (geometry)Muon neutrinoNeutrinsNeutrinosInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonCOSMIC cancer databaseGalaxy: center[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicFísicaneutrinosAstronomy and Astrophysicscenter [Galaxy]Galaxy centerNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionSpace and Planetary Scienceastroparticle physicsFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentNeutrinoAstroparticle physicsMATEMATICA APLICADAAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsastroparticle physics; Galaxy: center; neutrinos
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Performance of the Advanced GAmma Tracking Array at GANIL

2020

The performance of the Advanced GAmma Tracking Array (AGATA) at GANIL is discussed, on the basis of the analysis of source and in-beam data taken with up to 30 segmented crystals. Data processing is described in detail. The performance of individual detectors are shown. The efficiency of the individual detectors as well as the efficiency after $\gamma$-ray tracking are discussed. Recent developments of $\gamma$-ray tracking are also presented. The experimentally achieved peak-to-total is compared with simulations showing the impact of back-scattered $\gamma$ rays on the peak-to-total in a $\gamma$-ray tracking array. An estimate of the achieved position resolution using the Doppler broadeni…

Normalization (statistics)Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesTracking (particle physics)01 natural sciencesOptics0103 physical sciencesNeutron detectionγ -ray trackingGamma spectroscopyNuclear structure[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)AGATA spectrometer010306 general physicsNuclear ExperimentInstrumentationPhysicsData processing010308 nuclear & particles physicsbusiness.industryHPGe detectorsDetectorInstrumentation and Detectors (physics.ins-det)[formula omitted]-ray trackingAGATAbusinessGANIL facilityDoppler broadeningNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Updated determination of the solar neutrino fluxes from solar neutrino data

2016

Journal of High Energy Physics 2016.3 (2016): 132 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)

Normalization (statistics)Particle physicsNuclear and High Energy PhysicsSolar and atmospheric neutrinosSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaBayesian probabilityPosterior probabilitySolar neutrinosFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solars0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsNeutrino oscillationSolar and Stellar Astrophysics (astro-ph.SR)Physics010308 nuclear & particles physicsParticle physicsFísicaMarkov chain Monte CarloNeutrino physicsHigh Energy Physics - PhenomenologyDistribution functionAstrophysics - Solar and Stellar Astrophysics13. Climate actionPhysics::Space PhysicssymbolsAstrophysics::Earth and Planetary AstrophysicsNeutrinoFísica de partícules
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Effects of shadowing on Drell-Yan dilepton production in high energy nuclear collisions

2001

We compute cross sections for the Drell-Yan process in nuclear collisions at next-to-leading order (NLO) in ��_s. The effects of shadowing on the normalization and on the mass and rapidity dependence of these cross sections are presented. An estimate of higher order corrections is obtained from next-to-next-to-leading order (NNLO) calculation of the rapidity-integrated mass distribution. Variations in these predictions resulting from choices of parton distribution sets are discussed. Numerical results for mass distributions at NLO are presented for RHIC and LHC energies, using appropriate rapidity intervals. The shadowing factors in the dilepton mass range 2 < M < 10 GeV are predicted…

Normalization (statistics)PhysicsNuclear and High Energy PhysicsParticle physicsHigh energyLarge Hadron ColliderMass distributionHigh Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Physics and AstronomyPartonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)RapidityHigh Energy Physics::ExperimentNuclear Experiment
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Hard probes in heavy ion collisions at the lhc: pdfs, shadowing and pa collisions

2003

This manuscript is the outcome of the subgroup ``PDFs, shadowing and $pA$ collisions'' from the CERN workshop ``Hard Probes in Heavy Ion Collisions at the LHC''. In addition to the experimental parameters for $pA$ collisions at the LHC, the issues discussed are factorization in nuclear collisions, nuclear parton distributions (nPDFs), hard probes as the benchmark tests of factorization in $pA$ collisions at the LHC, and semi-hard probes as observables with potentially large nuclear effects. Also, novel QCD phenomena in $pA$ collisions at the LHC are considered. The importance of the $pA$ program at the LHC is emphasized.

Nuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear TheoryPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesNuclear ExperimentParticle Physics - Phenomenology
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Photoproduction of the hypertriton

1997

In the framework of the impulse approximation we study the photoproduction of the hypertriton $^3_{\Lambda}$H by using realistic $^3$He wave functions obtained as solutions of Faddeev equations with the Reid soft-core potential for different $^3_{\Lambda}$H wave functions. We obtain relatively small cross sections of the order of 1 nb. We also find that the influence of Fermi motion is important, while the effect of different off-shell assumptions on the cross section is not too significant.

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsFaddeev equationsParticle physicsNuclear TheoryNuclear TheoryFOS: Physical sciencesImpulse (physics)Wave functionLambdaHypertritonFermi Gamma-ray Space TelescopeNuclear Physics A
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Shell-Model Effective Operators for Muon Capture in ^{20}Ne

1999

It has been proposed that the discrepancy between the partially-conserved axial-current prediction and the nuclear shell-model calculations of the ratio $C_P/C_A$ in the muon-capture reactions can be solved in the case of ^{28}Si by introducing effective transition operators. Recently there has been experimental interest in measuring the needed angular correlations also in ^{20}Ne. Inspired by this, we have performed a shell-model analysis employing effective transition operators in the shell-model formalism for the transition $^{20}Ne(0^+_{g.s.})+\mu^- \to ^{20}F(1^+; 1.057 MeV) + \nu_\mu$. Comparison of the calculated capture rates with existing data supports the use of effective transiti…

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryFormalism (philosophy)SHELL modelFOS: Physical sciencesAnisotropyMuon capture
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Chiral restoration from pionic atoms?

2002

We evaluate widths and shifts of pionic atoms using a theoretical microscopical potential in which the pion decay constant $f_\pi$ is changed by an in--medium density dependent one ($f_\pi(\rho)$), predicted by different partial Chiral restoration calculations. We show that the results obtained for shifts and widths are worse than if this modification were not implemented. On the other hand, we argue that in microscopic many body approaches for the pion selfenergy, based on effective Lagrangians, the mechanisms responsible for the change of $f_\pi$ in the medium should be automatically incorporated. Therefore, the replacement of $f_\pi$ by $f_\pi(\rho)$ in the many body derivation of the mi…

Nuclear Theory (nucl-th)PhysicsNuclear and High Energy PhysicsParticle physicsPionNuclear TheoryDensity dependentNuclear TheoryFísicaFOS: Physical sciencesPion decay constantMany bodyPhysics Letters B
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