Search results for " 25.30.Pt"

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Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam

2011

The T2K experiment observes indications of $\nu_\mu\rightarrow \nu_e$ appearance in data accumulated with $1.43\times10^{20}$ protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with $|\Delta m_{23}^2|=2.4\times10^{-3}$ eV$^2$, $\sin^2 2\theta_{23}=1$ and $\sin^2 2\theta_{13}=0$, the expected number of such events is 1.5$\pm$0.3(syst.). Under this hypothesis, the probability to observe six or more candidate events is 7$\times10^{-3}$, equivalent to 2.5$\sigma$ significance. At 90% C.L., the data are consistent with 0.03(0.04)$<\sin^2 2\theta_{13}<$ 0.28(0.34) for $\delta_{\rm CP}=0$ and a normal (inverted) hierarchy.

Particle physicsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2CHOOZ01 natural sciencesParticle identificationHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)neutrino14.60.Pq 13.15.+g 25.30.Pt 95.55.Vj0103 physical sciencesneutrino oscillationMuon neutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSPhysicsNOνATribimaximal mixinghep-ex010308 nuclear & particles physicsT2K experimentFísicaT2K Collaborationparticle identificationElectron neutrinoexperimental resultsPhysical Review Letters
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Nuclear liquid-gas phase transition and supernovae evolution

2004

It is shown that the large density fluctuations appearing at the onset of the first order nuclear liquid-gas phase transition can play an important role in the supernovae evolution. Due to these fluctuations, the neutrino gas may be trapped inside a thin layer of matter near the proto-neutron star surface. The resulting increase of pressure may induce strong particle ejection a few hundred milliseconds after the bounce of the collapse, contributing to the revival of the shock wave. The Hartree-Fock+RPA scheme, with a finite-range nucleon-nucleon effective interaction, is employed to estimate the effects of the neutrino trapping due to the strong density fluctuations, and to discuss qualitat…

Shock waveNuclear and High Energy PhysicsPhase transition97.60.Bw; 26.50.+x; 25.30.Pt; 21.60.JzNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]supernovaeAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesTrappingAstrophysics7. Clean energy01 natural sciencesNuclear Theory (nucl-th)Nuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsLiquid gasAstrophysics (astro-ph)FísicaneutrinosNuclear matterSupernovaphase transitionnuclear matterParticleNeutrino
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