0000000000079943

AUTHOR

Matthew Mumpower

showing 8 related works from this author

Precision mass measurements on neutron-rich rare-earth isotopes at JYFLTRAP - reduced neutron pairing and implications for the $r$-process calculatio…

2018

The rare-earth peak in the $r$-process abundance pattern depends sensitively on both the astrophysical conditions and subtle changes in nuclear structure in the region. This work takes an important step elucidating the nuclear structure and reducing the uncertainties in $r$-process calculations via precise atomic mass measurements at the JYFLTRAP double Penning trap. $^{158}$Nd, $^{160}$Pm, $^{162}$Sm, and $^{164-166}$Gd have been measured for the first time and the precisions for $^{156}$Nd, $^{158}$Pm, $^{162,163}$Eu, $^{163}$Gd, and $^{164}$Tb have been improved considerably. Nuclear structure has been probed via two-neutron separation energies $S_{2n}$ and neutron pairing energy metrics…

Nuclear TheoryastrofysiikkaRare earthnuclear astrophysicsGeneral Physics and AstronomyFOS: Physical sciences7. Clean energy01 natural sciencesbinding energy and massesNuclear Theory (nucl-th)0103 physical sciencesNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentSolar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Isotopeta114010308 nuclear & particles physicsNuclear structureharvinaiset maametallitPenning trapAtomic mass3. Good healthAstrophysics - Solar and Stellar Astrophysics13. Climate actionPairingr-processAtomic physicsydinfysiikkaAstrophysics - High Energy Astrophysical Phenomena
researchProduct

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
researchProduct

Exploring the mass surface near the rare-earth abundance peak via precision mass measurements at JYFLTRAP

2019

The JYFLTRAP double Penning trap at the Ion Guide Isotope Separator On-Line (IGISOL) facility has been used to measure the atomic masses of 13 neutron-rich rare-earth isotopes. Eight of the nuclides, $^{161}$Pm, $^{163}$Sm, $^{164,165}$Eu, $^{167}$Gd, and $^{165,167,168}$Tb, were measured for the first time. The systematics of the mass surface has been studied via one- and two-neutron separation energies as well as neutron pairing-gap and shell-gap energies. The proton-neutron pairing strength has also been investigated. The impact of the new mass values on the astrophysical rapid neutron capture process has been studied. The calculated abundance distribution results in a better agreement w…

EFFICIENCYrare and new isotopesastrofysiikkanuclear astrophysicsNuclear Theoryr processFOS: Physical sciencesnucl-ex01 natural sciences7. Clean energybinding energy and massesIonPENNING TRAPS0103 physical sciencesNuclear Physics - ExperimentNeutronNuclideIONNuclear Experiment (nucl-ex)Nuclear Experiment010306 general physicsNuclear ExperimentDETECTORPhysicsScience & TechnologySTABILITYIsotope010308 nuclear & particles physicsPhysicsR-PROCESSRAMSEY METHODPenning trapnuclear structure and decaysAtomic massNeutron capturePhysics NuclearSPECTROMETRY13. Climate actionPairingPhysical SciencesELECTRONAtomic physicsydinfysiikkaDECAYPhysical Review C
researchProduct

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
researchProduct

Novel Techniques for Constraining Neutron-capture Rates relevant to Heavy-element Nucleosynthesis

2017

In this contribution we discuss new experimental approaches to indirectly provide information on neutron-capture rates relevant to the $r$-process. In particular, we focus on applications of the Oslo method to extract fundamental nuclear properties for reaction-rate calculations: the nuclear level density and the $\gamma$ strength function. Two methods are discussed in detail, the Oslo method in inverse kinematics and the beta-Oslo method. These methods present a first step towards constraining neutron-capture rates of importance to the $r$-process.

Nuclear physicsPhysicsFocus (computing)Neutron captureInverse kinematicsNucleosynthesisStrength functionHeavy elementNuclear ExperimentProceedings of The 26th International Nuclear Physics Conference — PoS(INPC2016)
researchProduct

Experimental Neutron Capture Rate Constraint Far from Stability

2016

Nuclear reactions where an exotic nucleus captures a neutron are critical for a wide variety of applications, from energy production and national security, to astrophysical processes, and nucleosynthesis. Neutron capture rates are well constrained near stable isotopes where experimental data are available; however, moving far from the valley of stability, uncertainties grow by orders of magnitude. This is due to the complete lack of experimental constraints, as the direct measurement of a neutron-capture reaction on a short-lived nucleus is extremely challenging. Here, we report on the first experimental extraction of a neutron capture reaction rate on ^{69}Ni, a nucleus that is five neutro…

Nuclear reactionPhysics010308 nuclear & particles physicsStable isotope ratioAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and Astronomy7. Clean energy01 natural sciencesStability (probability)Nuclear physicsNeutron captureOrders of magnitude (time)13. Climate actionValley of stabilityNucleosynthesis0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysical Review Letters
researchProduct

First Exploration of Neutron Shell Structure below Lead and beyond N=126

2020

The nuclei below lead but with more than 126 neutrons are crucial to an understanding of the astrophysical r process in producing nuclei heavier than A∼190. Despite their importance, the structure and properties of these nuclei remain experimentally untested as they are difficult to produce in nuclear reactions with stable beams. In a first exploration of the shell structure of this region, neutron excitations in ^{207}Hg have been probed using the neutron-adding (d,p) reaction in inverse kinematics. The radioactive beam of ^{206}Hg was delivered to the new ISOLDE Solenoidal Spectrometer at an energy above the Coulomb barrier. The spectroscopy of ^{207}Hg marks a first step in improving our…

PhysicsNuclear reactionSpectrometerSolenoidal vector fieldNuclear TheoryGeneral Physics and AstronomyCoulomb barrier01 natural sciencesNuclear physicsLead (geology)0103 physical sciencesr-processPhysics::Accelerator PhysicsNeutron010306 general physicsSpectroscopyNuclear Experimentydinfysiikka
researchProduct

Astrophysics with the Laser Interferometer Space Antenna

2023

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massi…

AstrofísicaACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Black holeAstronomyStellar remnantFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)TIDAL DISRUPTION EVENTSGeneral Relativity and Quantum CosmologyGravitational wavesMOCCA-SURVEY DATABASESettore FIS/05 - Astronomia e AstrofisicaStellar remnantsSoftware ScienceMulti-messengerGRAVITATIONAL-WAVE SOURCESInstrumentation and Methods for Astrophysics (astro-ph.IM)Extreme mass ratio in-spiralsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)Black holes; Extreme mass ratio in-spirals; Gravitational waves; Multi-messenger; Stellar remnantsBlack holesData ScienceAstrophysics::Instrumentation and Methods for AstrophysicsExtreme mass ratio in-spiralAM-CVN STARSAstrophysics - Astrophysics of GalaxiesWHITE-DWARF BINARIESDOUBLE NEUTRON-STARSAstrophysics - Solar and Stellar Astrophysics[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)AstronomiaMASSIVE BLACK-HOLEAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsX-RAY BINARIESCOMMON-ENVELOPE EVOLUTIONGravitational waveAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct