0000000000147471

AUTHOR

M. Carmona-gallardo

showing 8 related works from this author

Precise Determination of the UnperturbedB8Neutrino Spectrum

2012

A measurement of the final state distribution of the B-8 beta decay, obtained by implanting a 8B beam in a double-sided silicon strip detector, is reported here. The present spectrum is consistent with a recent independent precise measurement performed by our collaboration at the IGISOL facility, Jyvaskyla [O. S. Kirsebom et al., Phys. Rev. C 83, 065802 ( 2011)]. It shows discrepancies with previously measured spectra, leading to differences in the derived neutrino spectrum. Thanks to a low detection threshold, the neutrino spectrum is for the first time directly extracted from the measured final state distribution, thus avoiding the uncertainties related to the extrapolation of R-matrix fi…

PhysicsParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsSolar neutrinoExtrapolationGeneral Physics and AstronomyFlux01 natural sciencesBeta decaySpectral line0103 physical sciencesMeasurements of neutrino speedNeutrino010306 general physicsNeutrino oscillationPhysical Review Letters
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Relative proton andγwidths of astrophysically important states in30S studied in theβ-delayed decay of31Ar

2013

Resonances just above the proton threshold in S-30 affect the P-29(p, gamma)S-30 reaction under astrophysical conditions. The (p,gamma)-reaction rate is currently determined indirectly and depends on the properties of the relevant resonances. We present here a method for finding the ratio between the proton and gamma partial widths of resonances in S-30. The widths are determined from the beta 2p- and beta p gamma-decay of Ar-31, which is produced at the ISOLDE radioactive ion beam facility at the European research organization CERN. Experimental limits on the ratio between the proton and gamma partial widths for astrophysical relevant levels in S-30 have been found for the first time. A le…

PhysicsNuclear and High Energy PhysicsLarge Hadron ColliderProtonIon beam010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaEuropean researchGamma ray01 natural sciencesGamma gamma0103 physical sciencesBeta (velocity)Atomic physics010306 general physicsPhysical Review C
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Multiparticle emission in the decay ofAr31

2014

A multihit capacity setup was used to study the decay of the dripline nucleus Ar-31, produced at the ISOLDE facility at CERN. A spectroscopic analysis of the beta-delayed three-proton decay of Ar-31 is presented for the first time together with a quantitative analysis of the beta-delayed 2p gamma decay. A new method for determination of the spin of low-lying levels in the beta p daughter 30S using proton-proton angular correlations is presented and used to determine that the spin of the 5.2-MeV level is most likely 3(+) with 4(+) also possible. The half-life of Ar-31 is found to be 15.1(3) ms. An improved analysis of the Fermi beta strength including the beta 3p-decay mode gives a total mea…

PhysicsNuclear and High Energy PhysicsProton010308 nuclear & particles physicsBranching fractionGamma ray7. Clean energy01 natural sciencesNuclear physicsmedicine.anatomical_structure0103 physical sciencesmedicineIsobaric processBeta (velocity)Atomic physics010306 general physicsNucleusSpin-½Fermi Gamma-ray Space TelescopePhysical Review C
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Relative proton and γ widths of astrophysically important states in 30S studied in the β-delayed decay of 31Ar

2013

Resonances just above the proton threshold in 30S affect the 29P(p,gamma)30S reaction under astrophysical conditions. The (p,gamma)-reaction rate is currently determined indirectly and depends on the properties of the relevant resonances. We present here a method for finding the ratio between the proton and gamma partial widths of resonances in 30S. The widths are determined from the beta-2p and beta-p-gamma decay of 31Ar, which is produced at the ISOLDE facility at the European research organization CERN. Experimental limits on the ratio between the proton and gamma partial widths for astrophysical relevant levels in 30S have been found for the first time. A level at 4688(5) keV is identif…

26.30.−k 23.40.Hc 27.30.+tAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:530Experimental nuclear physics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experiment
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Sizeable beta-strength in $^{31}$Ar (β3p) decay

2014

5 pags. ; 7 figs. ; Open Access funded by SCOAP3 - Sponsoring Consortium for Open Access Publishing in Particle Physics

Nuclear and High Energy PhysicsFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex01 natural sciencesNuclear physicsESPECTROSCOPÍA0103 physical sciencesNuclear Physics - ExperimentBeta (velocity)Nuclear Experiment (nucl-ex)010306 general physicsFÍSICA NUCLEARNuclear ExperimentPhysicsta114Isotope010308 nuclear & particles physicsIsotopes of chlorineIsotopes of argonSPECTROSCOPICBeta decaylcsh:QC1-999DESINTEGRATION3. Good healthFísica nuclearHigh Energy Physics::ExperimentAtomic physicsEMISSIONlcsh:PhysicsFÍSICAEnergy (signal processing)ExcitationRadioactive decay
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Multiparticle emission in the decay of Ar 31

2014

A multihit capacity setup was used to study the decay of the dripline nucleus 31Ar, produced at the ISOLDE facility at CERN. A spectroscopic analysis of the β-delayed three-proton decay of 31Ar is presented for the first time together with a quantitative analysis of the β-delayed 2pγ decay. A new method for determination of the spin of low-lying levels in the βp daughter 30S using proton-proton angular correlations is presented and used to determine that the spin of the 5.2-MeV level is most likely 3+ with 4+ also possible. The half-life of 31Ar is found to be 15.1(3) ms. An improved analysis of the Fermi β strength including the β3p-decay mode gives a total measured branching ratio of 3.60…

NUCLEAR EXPERIMENTmultiparticle emissionCIENCIAANÁLISIS ESPECTROSCÓPICOBETA DESINTEGRATIONPROTONFÍSICA NUCLEARFÍSICA
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Multi-particle emission in the decay of $^{31}$Ar

2014

A multi-hit capacity setup was used to study the decay of the dripline nucleus 31Ar, produced at the ISOLDE facility at CERN. A spectroscopic analysis of the beta-delayed three-proton decay of 31Ar is presented for the first time together with a quantitative analysis of the beta-delayed two-proton-gamma-decay. A new method for determination of the spin of low-lying levels in the beta-proton-daughter 30S using proton-proton angular correlations is presented and used for the level at 5.2 MeV, which is found to be either a 3+ or 4+ level, with the data pointing towards the 3+. The half-life of 31Ar is found to be 15.1(3) ms. An improved analysis of the Fermi beta-strength gives a total measure…

Physics::Accelerator PhysicsFOS: Physical sciencesNuclear Physics - Experiment[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experiment23.40.Hc 27.30.+t
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Precise Determination of the Unperturbed 8B Neutrino Spectrum

2012

The measurement was performed at the Kernfysisch Versneller Instituut (KVI) at the University of Groningen, The Netherlands.; A measurement of the final state distribution of the 8B $\beta$ decay, obtained by implanting a 8B beam in a double-sided silicon strip detector, is reported here. The present spectrum is consistent with a recent independent precise measurement performed by our collaboration at the IGISOL facility, Jyvâskylä [O. S. Kirsebom et al., Phys. Rev. C 83, 065802 (2011)]. It shows discrepancies with previously measured spectra, leading to differences in the derived neutrino spectrum. Thanks to a low detection threshold, the neutrino spectrum is for the first time directly ex…

nuclear spectroscopyneutrino oscillationsPhysics::Instrumentation and Detectorsaccelerator-based physics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]kiihdytinpohjainen fysiikkaKVIydinrakenne8Bnuclear structureydinspektroskopiaimplantationydinfysiikka23.40.Bw 26.65.+t 27.20.+nbeta-decay
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