0000000000162819

AUTHOR

Iris Dillmann

showing 15 related works from this author

New accurate measurements of neutron emission probabilities for relevant fission products

2017

We have performed new accurate measurements of the beta-delayed neutron emission probability for ten isotopes of the elements Y, Sb, Te and I. These are fission products that either have a significant contribution to the fraction of delayed neutrons in reactors or are relatively close to the path of the astrophysical r process. The measurements were performed with isotopically pure radioactive beams using a constant and high efficiency neutron counter and a low noise beta detector. Preliminary results are presented for six of the isotopes and compared with previous measurements and theoretical calculations. peerReviewed

Neutron emissionQC1-999Nuclear physicsNeutronAstrophysics7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesNeutron010306 general physicsNuclear Experimentastro nuclear physicsPhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]Fission productsPnta114Isotope:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsDetectorBeta (plasma physics)r-processFísica nuclearDelayed neutronNeutron emission
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First Measurement of Severalβ-Delayed Neutron Emitting Isotopes BeyondN=126

2016

The β-delayed neutron emission probabilities of neutron rich Hg and Tl nuclei have been measured together with β-decay half-lives for 20 isotopes of Au, Hg, Tl, Pb, and Bi in the mass region N≳126. These are the heaviest species where neutron emission has been observed so far. These measurements provide key information to evaluate the performance of nuclear microscopic and phenomenological models in reproducing the high-energy part of the β-decay strength distribution. This provides important constraints on global theoretical models currently used in r-process nucleosynthesis.

PhysicsIsotope010308 nuclear & particles physicsNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and Astronomy01 natural sciencesMass formulaNuclear physics13. Climate actionNucleosynthesis0103 physical sciencesr-processNeutronNuclear Experiment010306 general physicss-processDelayed neutronPhysical Review Letters
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Approaching the precursor nuclei of the third r-process peak with RIBs

2013

The rapid neutron nucleosynthesis process involves an enormous amount of very exotic neutron-rich nuclei, which represent a theoretical and experimental challenge. Two of the main decay properties that affect the final abundance distribution the most are half-lives and neutron branching ratios. Using fragmentation of a primary $^{238}$U beam at GSI we were able to measure such properties for several neutron-rich nuclei from $^{208}$Hg to $^{218}$Pb. This contribution provides a short update on the status of the data analysis of this experiment, together with a compilation of the latest results published in this mass region, both experimental and theoretical. The impact of the uncertainties …

HistoryNeutron emissionNuclear TheoryFOS: Physical sciencesNeutronPhysics and Astronomy(all)nucl-ex01 natural sciences530EducationNuclear physicsNucleosynthesis/dk/atira/pure/subjectarea/asjc/31000103 physical sciencesNuclear Physics - Experimentddc:530NeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]010308 nuclear & particles physicsBranching fractionNuclear energyComputer Science ApplicationsUranium-238r-processEnergia nuclears-processNucleosynthesisRadioactive decay
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Development of a Reference Database for Beta-Delayed Neutron Emission

2021

Beta-delayed neutron emission is important for nuclear structure and astrophysics as well as for reactor applications. Significant advances in nuclear experimental techniques in the past two decades have led to a wealth of new measurements that remain to be incorporated in the databases. We report on a coordinated effort to compile and evaluate all the available beta-delayed neutron emission data. The different measurement techniques have been assessed and the data have been compared with semi-microscopic and microscopic-macroscopic models. The new microscopic database has been tested against aggregate total delayed neutron yields, time-dependent group parameters in 6-and 8-group re-present…

Nuclear and High Energy PhysicsFissile material010308 nuclear & particles physicsNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaAggregate (data warehouse)Nuclear TheoryNuclear dataFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear physicsBeta (plasma physics)0103 physical sciencesReference databaseEnvironmental scienceNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentDelayed neutronNuclear Experiment
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r -process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos

2018

This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star merger GW170817 was observed in extraordinary detail with gravitational waves and electromagnetic radiation from radio to gamma rays. The very red color of the associated kilonova suggests that neutron star mergers are an important r-process site. Astrophysical simulations of neutron star mergers and core collapse supernovae are making rapid progress. Detection of both, electron neutrinos and antineutrinos from the next galactic supernova will constrain the composition of neutrino-driven winds and provide unique nucleosynthesis information. Finally FRIB and other rare-isotope beam facilities will s…

Nuclear and High Energy PhysicsNuclear Theorymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsKilonova01 natural sciences7. Clean energyNuclear Theory (nucl-th)Nucleosynthesis0103 physical sciencesBinary starddc:530Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentStellar evolutionNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsmedia_commonPhysics010308 nuclear & particles physicsAstronomyUniverseNeutron starSupernovaAstrophysics - Solar and Stellar Astrophysicsr-processJournal of Physics G: Nuclear and Particle Physics
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Commissioning of the BRIKEN beta-delayed neutron detector for the study of exotic neutron-rich nuclei

2017

Beta-delayed neutron emission (Beta-n) is a form of radioactive decay in which an electron, an anti-neutrino and one or more neutrons are emitted. This process arises if the energy window of the decay Q_Beta is greater than the neutron separation energy S n of the daughter. The probability in each decay of emitting neutrons is called the Pn value. This form of decay plays a key role in the synthesis of chemical elements in the Universe via the rapid neutron capture process, or r-process. The r-process proceeds far from the valley of nuclear stability, and leads to very neutron-rich nuclei that then decay to the line of stability. Most of these nuclei are ßn emitters. The initial abundance d…

AstrofísicaNeutron emissionQC1-999Astrophysics::High Energy Astrophysical PhenomenaNeutron detectorNuclear TheoryElectronNeutronAstrophysics01 natural sciencesNuclear physics0103 physical sciencesNeutron detectionNeutron010306 general physicsNuclear ExperimentDelayed neutronsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Neutrons:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear structureDetectorNeutron captureDelayed neutronRadioactive decay
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Dawning of the N=32 shell closure seen through precision mass measurements of neutron-rich titanium isotopes

2018

A precision mass investigation of the neutron-rich titanium isotopes 51 − 55 Ti was performed at TRIUMF’s Ion Trap for Atomic and Nuclear science (TITAN). The range of the measurements covers the N = 32 shell closure, and the overall uncertainties of the 52 − 55 Ti mass values were significantly reduced. Our results conclusively establish the existence of the weak shell effect at N = 32 , narrowing down the abrupt onset of this shell closure. Our data were compared with state-of-the-art ab initio shell model calculations which, despite very successfully describing where the N = 32 shell gap is strong, overpredict its strength and extent in titanium and heavier isotones. These measurements a…

Materials scienceNuclear Theorynucl-thNuclear TheoryAb initioGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Mass spectrometrynucl-ex01 natural sciencesNuclear Theory (nucl-th)symbols.namesake0103 physical sciencesPhysics::Atomic and Molecular ClustersNeutron[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentIsotope010308 nuclear & particles physicsStarke Wechselwirkung und exotische Kerne – Abteilung BlaumPenning trapchemistry13. Climate actionsymbolsIon trapAtomic physicsTitan (rocket family)Titanium
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The BRIKEN Project: Extensive Measurements of $\beta $-delayed Neutron Emitters for the Astrophysical r Process

2018

An ambitious program to measure decay properties, primarily β-delayed neutron emission probabilities and half-lives, for a significant number of nuclei near or on the path of the rapid neutron capture process, has been launched at the RIKEN Nishina Center. We give here an overview of the status of the project.

AstrofísicaDelayed neutronNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear dataNuclear TheoryMeasure (physics)General Physics and AstronomyNeutronAstrophysics01 natural sciencesNuclear physics0103 physical sciencesNeutronNuclear Experiment010306 general physics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPhysics:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNuclear dataNeutron capture:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]r-processDelayed neutronActa Physica Polonica B
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β-delayed neutron emission of r-process nuclei at the N = 82 shell closure

2021

This experiment was performed at RI Beam Factory operated by RIKEN Nishina Center and CNS, University of Tokyo. O.H, T.D, P.J.W, C.G.B, C.J.G and D.K would like to thank STFC, UK for support. This research was sponsored in part by the Office of Nuclear Physics, U.S. Department of Energy under Award No. DE-FG02-96ER40983 (UTK) and DEAC05-00OR22725 (ORNL), and by the National Nuclear Security Administration under the Stewardship Science Academic Alliances program through DOE Award No. DENA0002132. This work was supported by National Science Foundation under Grants No. PHY-1430152 (JINA Center for the Evolution of the Elements), No. PHY-1565546 (NSCL), and No. PHY-1714153 (Central Michigan Uni…

Nuclear and High Energy PhysicsNational securityQC1-999ß-delayedNuclear physicsLibrary scienceNeutrons--Capturaβ-delayed neutron emission7. Clean energy01 natural sciencesNeutrons--CaptureAstrophysical0103 physical sciencesEuropean commissionr-processimportant010306 general physicsChinaNuclear ExperimentNeutron emissionr-processPhysics:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsbusiness.industryr-processPhysicsChinese academy of sciencesbeta-delayed neutron emissionResearch councilChristian ministryFísica nuclearNational laboratorybusinessAdministration (government)Physics Letters B
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Superallowed Gamow-Teller decay of the doubly magic nucleus $^{100}$Sn

2012

Expérience au GSI; The shell structure of atomic nuclei is associated with 'magic numbers' and originates in the nearly independent motion of neutrons and protons in a mean potential generated by all nucleons. During b1-decay, a proton transforms into a neutron in a previously not fully occupied orbital, emitting a positron-neutrino pair with either parallel or antiparallel spins, in a Gamow-Teller or Fermi transition, respectively. The transition probability, or strength, of a Gamow-Teller transition depends sensitively on the underlying shell structure and is usually distributed among many states in the neighbouring nucleus. Here we report measurements of the half-life and decay energy fo…

PhysicsMultidisciplinaryProton010308 nuclear & particles physicsProton decayNuclear Theory[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesBeta decayNuclear physicsDecay energy0103 physical sciencesAtomic nucleusPhysical SciencesFysikNeutronAtomic physics010306 general physicsNucleonNuclear ExperimentRadioactive decay
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β-delayed neutron emission measurements around the third r-process abundance peak

2013

This contribution summarizes an experiment performed at GSI (Germany) in the neutron-rich region beyond N=126. The aim of this measurement is to provide the nuclear physics input of relevance for r-process model calculations, aiming at a better understanding of the third r-process abundance peak. Many exotic nuclei were measured around 211Hg and 215Tl. Final ion identification diagrams are given in this contribution. For most of them, we expect to derive halflives and and β-delayed neutron emission probabilities. The detectors used in this experiment were the Silicon IMplantation and Beta Absorber (SIMBA) detector, based on an array of highly segmented silicon detectors, and the BEta deLayE…

PhysicsNuclear physicsPhysics::Instrumentation and DetectorsNucleosynthesisNeutron emissionDouble beta decayDetectorr-processNuclear ExperimentDelayed neutronAbundance of the chemical elementsIon
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Measurement of the 241Am neutron capture cross section at the n-TOF facility at CERN

2016

New neutron cross section measurements of minor actinides have been performed recently in order to reduce the uncertainties in the evaluated data, which is important for the design of advanced nuclear reactors and, in particular, for determining their performance in the transmutation of nuclear waste. We have measured the 241 Am(n,γ) cross section at the n TOF facility between 0.2 eV and 10 keV with a BaF2 Total Absorption Calorimeter, and the analysis of the measurement has been recently concluded. Our results are in reasonable agreement below 20 eV with the ones published by C. Lampoudis et al. in 2013, who reported a 22% larger capture cross section up to 110 eV compared to experimental …

Nuclear reactionNuclear transmutationnTOFQC1-999Neutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Cross section (physics)Nuclear reactorsReactors nuclears0103 physical sciencesCERNNeutron cross sectionNuclear Physics - Experimentddc:530Neutron010306 general physicsAbsorption (electromagnetic radiation)PhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]Large Hadron ColliderCross section:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear reactionCalorimeter
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β-decay and β-delayed Neutron Emission Measurements at GSI-FRS Beyond N=126, for r-process Nucleosynthesis

2014

New measurements of very exotic nuclei in the neutron-rich region beyond N=126 have been performed at the GSI facility with the fragment separator (FRS). The aim of the experiment is to determine half-lives and β-delayed neutron emission branching ratios of isotopes of Hg, Tl and Pb in this region. This contribution summarizes final counting statistics for identification and for implantation, as well as the present status of the data analysis of the half-lives. In summary, isotopes of Pt, Au, Hg, Tl, Pb, Bi, Po, At, Rn and Fr were clearly identified and several of them (208-211Hg, 211-215Tl, 214-218Pb) were implanted with enough statistics to determine their half-lives. About half of them a…

PhysicsNuclear and High Energy PhysicsIsotope010308 nuclear & particles physicsNeutron emissionBranching fraction01 natural sciencesNuclear physicsNucleosynthesis0103 physical sciencesr-processNeutron010306 general physicss-processDelayed neutronNuclear Data Sheets
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A new reference database for beta-delayed neutrons

2019

International audience; A new database containing all available experimental and evaluated β-delayed neutron data is presented in this paper. The database is the product of an international effort coordinated by the International Atomic Energy Agency. It comprises a microscopic section including all available experimental data on beta-decay half-lives, β-delayed neutron emission probabilities and spectra, as well as new systematics and global theoretical calculations for comparison. The beta-delayed neutron data for individual precursors have been benchmarked against available data on macroscopic properties such as total delayed-neutron yields and spectra, delayed-neutron decay curves and t…

Physics010308 nuclear & particles physicsPhysicsQC1-999Experimental data[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesDecay curveNuclear physics0103 physical sciencesReference databaseNeutronBeta (velocity)Nuclear Experiment010306 general physicsDelayed neutron
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Compilation and Evaluation of Beta-Delayed Neutron Emission Probabilities and Half-Lives for Z > 28 Precursors

2020

Abstract We present a compilation and evaluation of experimental β-delayed neutron emission probabilities (Pn) and half-lives (T1/2) for known or potential β-delayed neutron precursors with atomic number Z > 28 (73Cu–233Fr). This article includes the recommended values of both of these quantities, together with a compilation of experimental measurements when available. Some notable cases, as well as proposed standards for β-delayed neutron measurements are also discussed. Evaluated data has also been compared to systematics using three different approaches. The literature cut-off date for this work is August 15, 2020.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsNeutron emissionNuclear data01 natural sciencesNuclear physics0103 physical sciencesEvaluated dataNeutronBeta (velocity)Atomic number010306 general physicsDelayed neutronNuclear Data Sheets
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