Search results for "física nuclear"

showing 10 items of 900 documents

Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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First search for point sources of high-energy cosmic neutrinos with the ANTARES neutrino telescope

2011

Results are presented of a search for cosmic sources of high-energy neutrinos with the ANTARES neutrino telescope. The data were collected during 2007 and 2008 using detector configurations containing between 5 and 12 detection lines. The integrated live time of the analyzed data is 304 days. Muon tracks are reconstructed using a likelihood-based algorithm. Studies of the detector timing indicate a median angular resolution of 0.5 0.1deg. The neutrino flux sensitivity is 7.5 ¿ 10 -8(E ¿/ GeV) -2 GeV -1 s -1 cm -2 for the part of the sky that is always visible (¿ < -48deg), which is better than limits obtained by previous experiments. No cosmic neutrino sources have been observed.

FLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesDeclinationneutrinos; cosmic rays; astroparticle physicscosmic rays0103 physical sciencesAngular resolutionALGORITHMNeutrinosDETECTOR010303 astronomy & astrophysicsCosmic raysmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorneutrinosASTRONOMYAstronomy and Astrophysicsastroparticle physics13. Climate actionSpace and Planetary ScienceSkyFISICA APLICADAddc:520Física nuclearHigh Energy Physics::ExperimentNeutrinoAstroparticle physicsAstrophysics - High Energy Astrophysical Phenomena
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New antineutrino energy spectra predictions from the summation of beta decay branches of the fission products

2012

In this paper, we study the impact of the inclusion of the recently measured beta decay properties of the $^{102;104;105;106;107}$Tc, $^{105}$Mo, and $^{101}$Nb nuclei in an updated calculation of the antineutrino energy spectra of the four fissible isotopes $^{235, 238}$U, and $^{239,241}$Pu. These actinides are the main contributors to the fission processes in Pressurized Water Reactors. The beta feeding probabilities of the above-mentioned Tc, Mo and Nb isotopes have been found to play a major role in the $\gamma$ component of the decay heat of $^{239}$Pu, solving a large part of the $\gamma$ discrepancy in the 4 to 3000\,s range. They have been measured using the Total Absorption Techni…

FissionFOS: Physical sciencesGeneral Physics and Astronomy[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Absorption (logic)Nuclear Experiment (nucl-ex)Decay heat010306 general physicsNuclear ExperimentPhysicsFission productsIsotope010308 nuclear & particles physicsPandemonium effectBeta decay3. Good healthHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclear
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Measurement of the heaviest Beta-delayed 2-neutron emitter: 136Sb

2017

The Beta-delayed neutron emission probability, Pn , of very exotic nuclei is crucial for the understanding of nuclear structure properties of many isotopes and astrophysical processes such as the rapid neutron capture process (r-process). In addition Beta-delayed neutrons are important in a nuclear power reactor operated in a prompt sub-critical, delayed critical condition, as they contribute to the decay heat inducing fission reactions after a shut down. The study of neutron-rich isotopes and the measurement of Beta-delayed one-neutron emitters (Beta1n) is possible thanks to the Rare Isotope Beam (RIB) facilities, where radioactive beams allow the production of exotic nuclei of interest, w…

FissionNeutron emissionQC1-999Astrophysics::High Energy Astrophysical PhenomenaNuclear TheoryNuclear physicsNeutronAstrophysics7. Clean energy01 natural sciencesNuclear physicsEmission0103 physical sciencesNeutronDecay heat010306 general physicsNuclear Experimentastro nuclear physicsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPnIsotopeta114:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsBranching fractionPhysicsNeutron capture13. Climate actionr-processPhysics::Accelerator PhysicsFísica nuclearAtomic physics
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Laboratorio de Física Nuclear y de Partículas

2018

Guiones de apoyo para el desarrollo de las actividades de laboratorio de la asignatura de Física Nuclear y de Partículas (1.5 créditos ECTS), cuyo material docente teórico está disponible en esta plataforma con el identificador http://roderic.uv.es/handle/10550/65281. Incluye tres bloques de experimentos: 1) Estadística de recuento y espectrometría beta con un detector Geiger-Mueller; 2) Espectroscopia gamma y vidas medias con un detector de NaI(Tl); 3) La cámara de niebla de difusión. Support scripts for the development of the laboratory activities of the subject of Nuclear and Particle Physics (1.5 ECTS credits), whose theoretical teaching material is available on this platform with ident…

Física NuclearDetectores de radiaciónUNESCO::FÍSICAFísica de PartículasAceleradores de partículas
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Measurements of direct CP asymmetries in B -> X-s gamma decays using sum of exclusive decays

2014

We measure the direct CP violation asymmetry, A(CP), in B -> X-s gamma and the isospin difference of the asymmetry, Delta A(CP), using 429 fb(-1) of data collected at Upsilon(4S) resonance with the BABAR detector at the PEP- II asymmetric- energy e(+)e(-) storage rings operating at the SLAC National Accelerator Laboratory. B mesons are reconstructed from ten charged B final states and six neutral B final states. We find A(CP) = +(1.7 +/- 1.9 +/- 1.0)%, which is in agreement with the Standard Model prediction and provides an improvement on the world average. Moreover, we report the first measurement of the difference between A(CP) for charged and neutral decay modes, Delta A(CP) = +(5.0 +/- …

Física nuclear
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New lifetime measurements in Pd-109 and the onset of deformation at N=60

2015

Several new subnanosecond lifetimes were measured in Pd-109 using the fast-timing beta gamma gamma (t) method. Fission fragments of the A = 109 mass chain were produced by bombarding natural uranium with 30 MeV protons at the Jyvaskyla Ion Guide Isotope Separator On-Line (IGISOL) facility. Lifetimes were obtained for excited states in Pd-109 populated following beta decay of Rh-109. The new lifetimes provide some insight into the evolution of nuclear structure in this mass region. In particular, the distinct structure of the two low-lying 7/2(+) states occurring systematically across the Pd isotopic chain is supported by the new lifetime measurements. The available nuclear data indicate a s…

Física nuclear
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Effective lifetime measurements in the B-s(0) -> K+K-, B-0 -> K+pi(-) and B-s(0) -> pi K-+(-) decays

2014

Measurements of the effective lifetimes in the B-s(0) -> K+K-, B-0 -> K+pi(-) and B-s(0) -> pi K-+(-) decays are presented using 1.0 fb(-1)of pp collision data collected at a centre-of-mass energy of 7 TeV by the LHCb experiment. The analysis uses a data-driven approach to correct for the decay time acceptance. The measured effective lifetimes are tau(Bs0 -> K+K-) = 1.407 +/- 0.016 (stat) +/- 0.007 (syst) ps, tau(Bs0 -> K+pi-) = 1.524 +/- 0.011 (stat) +/- 0.004 (syst) ps, tau(Bs0 ->pi+K-) = 1.60 +/- 0.06 (stat) +/- 0.01 (syst) ps. This is the most precise determination to date of the effective lifetime in the B-s(0) -> K+K- decay and provides constraints on contributions from physics beyond…

Física nuclear
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Search for D-(s)(+) -> pi(+)mu(+)mu(-) and D-(s)(+) -> pi(-)mu(+)mu(+) decays

2013

A search for non-resonant D-(s)(+) -> pi(+)mu(+)mu(-) and D-(s)(+) -> pi(-)mu(+)mu(+) decays is performed using protonproton collision data, corresponding to an integrated luminosity of 1.0 fb(-1), at root s = 7 TeV recorded by the LHCb experiment in 2011. No signals are observed and the 90% (95%) confidence level (CL) limits on the branching fractions are found to be B(D+ -> pi(+)mu(+)mu(-)) pi(+)mu(+)mu(-)) pi(+)mu(+)mu(-)) pi(+)mu(+)mu(-)) < 1.2 (1.4) x 10(-7). These limits are the most stringent to date.

Física nuclear
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Observation of the suppressed ADS modes B-+/- -> [pi K-+/-(-/+)pi(+)pi(-)](D)K-+/- and B-+/- -> [pi K-+/-(-/+)pi(+)pi(-)](D)pi(+/-)

2013

An analysis of and B-+/- -> DK +/- and B-+/- -> D pi(+/-) decays is presented where the D meson is reconstructed in the four-body final state K-+/-pi(-/+)pi(+)pi(-). Using LHCb data corresponding to an integrated luminosity of 1.0 fb(-1), first observations are made of the suppressed ADS modes B-+/- ->[pi K-+/-(-/+)pi(+)pi(-)](D)K-+/- and B +/- -> [pi K-+/-(-/+)pi(+)pi(-)](D)pi(+/-) with a significance of 5.1 sigma and greater than 10 sigma, respectively. Measurements of CP asymmetries and CP-conserving ratios of partial widths from this family of decays are also performed. The magnitude of the ratio between the suppressed and favoured B-+/- -> DK +/- amplitudes is determined to be r(B)(K) …

Física nuclear
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