6533b7d3fe1ef96bd126160d

RESEARCH PRODUCT

Beta-decay studies for applied and basic nuclear physics

J. L. TainM. FallotAlejandro AlgoraAlejandro AlgoraBerta RubioW. Gelletly

subject

safetyNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaPenning trapFOS: Physical sciencesnucleus: structure functionnuclear model[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energylaw.inventionNuclear physicslawnuclear physics0103 physical sciencesNuclear fusionNeutronDecay heatNuclear Experiment (nucl-ex)n: capture010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsantineutrino: spectrum010308 nuclear & particles physicsPandemonium effectsemileptonic decayNuclear reactorNeutron capturemonitoring13. Climate actionnuclear reactorDelayed neutronElectron neutrinoabsorption

description

In this review we will present the results of recent beta-decay studies using the total absorption technique that cover topics of interest for applications, nuclear structure and astrophysics. The decays studied were selected primarily because they have a large impact on the prediction of a) the decay heat in reactors, important for the safety of present and future reactors and b) the reactor electron antineutrino spectrum, of interest for particle/nuclear physics and reactor monitoring. For these studies the total absorption technique was chosen, since it is the only method that allows one to obtain beta decay probabilities free from a systematic error called the Pandemonium effect. The measurements presented and discussed here were performed mainly at the IGISOL facility of the University of Jyvaskyla (Finland) using isotopically pure beams provided by the JYFLTRAP Penning trap. Examples are presented to show that the results of our measurements on selected nuclei have had a large impact on predictions of both the decay heat and the anti-neutrino spectrum from reactors. Some of the cases involve beta delayed neutron emission thus one can study the competition between gamma- and neutron-emission from states above the neutron separation energy. The gamma-to-neutron emission ratios can be used to constrain neutron capture (n,gamma)cross sections for unstable nuclei of interest in astrophysics. The information obtained from the measurements can also be used to test nuclear model predictions of half-lives and Pn values for decays of interest in astrophysical network calculations. These comparisons also provide insights into aspects of nuclear structure in particular regions of the nuclear chart.

10.1140/epja/s10050-020-00316-4http://dx.doi.org/10.1140/epja/s10050-020-00316-4