0000000000294492

AUTHOR

J. I. Porras

showing 3 related works from this author

7Be(n,α) and 7Be(n,p) cross-section measurement for the cosmological lithium problem at the n-TOF facility at CERN

2017

One of the most puzzling problems in Nuclear Astrophysics is the “Cosmological Lithium Problem”, i.e the discrepancy between the primordial abundance of \(^{7}\)Li observed in metal poor halo stars (Asplund et al. in Astrophys J 644:229–259, 2006, [1]), and the one predicted by Big Bang Nucleosynthesis (BBN). One of the reactions that could have an impact on the problem is \(^{7}\)Be(n,p)\(^{7}\)Li. Despite of the importance of this reaction in BBN, the cross-section has never been directly measured at the energies of interest for BBN. Taking advantage of the innovative features of the second experimental area at the n\(\_\)TOF facility at CERN (Sabate-Gilarte et al. in Eur Phys J A 53:210,…

AstrofísicanTOFQC1-999chemistry.chemical_elementNeutronAstrophysics01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Big Bang nucleosynthesisNucleosynthesisCERN0103 physical sciencesNuclear astrophysicsAstrophysics::Solar and Stellar AstrophysicsNeutron010306 general physicsNuclear ExperimentAstrophysics::Galaxy Astrophysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPhysicsAlphaLarge Hadron Collider:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsStarschemistryLithiumHaloNucleosynthesisNucleosíntesi
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Measurement of the Pu-242(n,gamma) cross section from thermal to 500 keV at the Budapest research reactor and CERN n_TOF-EAR1 facilities

2019

The design and operation of innovative nuclear systems requires a better knowledge of the capture and fission cross sections of the Pu isotopes. For the case of capture on 242Pu, a reduction of the uncertainty in the fast region down to 8-12% is required. Moreover, aiming at improving the evaluation of the fast energy range in terms of average parameters, the OECD NEA High Priority Request List (HPRL) requests high-resolution capture measurements with improved accuracy below 2 keV. The current uncertainties also affect the thermal point, where previous experiments deviate from each other by 20%. A fruitful collaboration betwen JGU Mainz and HZ Dresden-Rossendorf within the EC CHANDA project…

PhysicsLarge Hadron ColliderIsotope010308 nuclear & particles physicsFissionPhysicsQC1-999n_TOF 242Pu neutron capture neutron time of flight[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyResonance (particle physics)Nuclear physicsStack (abstract data type)0103 physical sciencesNeutronResearch reactorNuclear Physics - ExperimentNeutron activation analysis010306 general physics
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Radiative neutron capture on Pu242 in the resonance region at the CERN n_TOF-EAR1 facility

2018

The spent fuel of current nuclear reactors contains fissile plutonium isotopes that can be combined with uranium to make mixed oxide (MOX) fuel. In this way the Pu from spent fuel is used in a new reactor cycle, contributing to the long-term sustainability of nuclear energy. However, an extensive use of MOX fuels, in particular in fast reactors, requires more accurate capture and fission cross sections for some Pu isotopes. In the case of Pu242 there are sizable discrepancies among the existing capture cross-section measurements included in the evaluations (all from the 1970s) resulting in an uncertainty as high as 35% in the fast energy region. Moreover, postirradiation experiments evaluat…

PhysicsNuclear fuelFissile material010308 nuclear & particles physicschemistry.chemical_elementUranium01 natural sciences7. Clean energySpent nuclear fuelNeutron temperatureNuclear physicsNeutron capturechemistry13. Climate action0103 physical sciencesNeutron010306 general physicsMOX fuelPhysical Review C
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