NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = G.W.Misch Found 10 matches. 2023HO14 Phys.Rev.Lett. 131, 262701 (2023) D.E.M.Hoff, K.Kolos, G.W.Misch, D.Ray, B.Liu, A.A.Valverde, M.Brodeur, D.P.Burdette, N.Callahan, J.A.Clark, A.T.Gallant, F.G.Kondev, G.E.Morgan, M.R.Mumpower, R.Orford, W.S.Porter, F.Rivero, G.Savard, N.D.Scielzo, K.S.Sharma, K.Sieja, T.M.Sprouse, L.Varriano Direct Mass Measurements to Inform the Behavior of 128mSb in Nucleosynthetic Environments ATOMIC MASSES 128,128mSb; measured cyclotron frequencies; deduced mass excesses, isomer excitation energy. Comparison with AME2020, NUBASE2020, state-of-the-art shell model calculations using the GCN5082 interaction. The phase-imaging ion-cyclotron resonance (PI-ICR) technique with the Canadian Penning Trap (CPT) mass spectrometer at the Californium Rare Isotope Breeder Upgrade facility.
doi: 10.1103/PhysRevLett.131.262701
2022SP02 Astrophys.J. 929, 22 (2022) T.M.Sprouse, G.W.Misch, M.R.Mumpower Isochronic Evolution and the Radioactive Decay of r-process Nuclei
doi: 10.3847/1538-4357/ac470f
2021MI02 Astrophys.J.Suppl.Ser. 252, 2 (2021) G.W.Misch, S.K.Ghorui, P.Banerjee, Y.Sun, M.R.Mumpower Astromers: Nuclear Isomers in Astrophysics RADIOACTIVITY 26Al, 34Cl, 85Kr, 121Sn(IT), 121,123,125,127Sn, 128Sb, 170Ho, 176Lu, 182Hf(IT), 58Mn, 113Cd(β-); calculated thermally mediated transition rates between the ground state and long-lived isomers in nuclei; deduced delimiting a thermalization temperature above which a nucleus may be considered a single species and below which it must be treated as two separate species: a ground-state species and an astrophysical isomer ("astromer") species.
doi: 10.3847/1538-4365/abc41d
2021MI12 Astrophys.J. 913, L2 (2021) G.W.Misch, T.M.Sprouse, M.R.Mumpower Astromers in the Radioactive Decay of r-process Nuclei RADIOACTIVITY 69,71Zn, 79,81Se, 83,85Kr, 93,95,97Nb, 99Tc, 113,115,117Cd, 115,117,119In, 119,121,129Sn, 126,128,130Sb, 125,127,129,131,133Te, 131,133Xe, 137Ba, 144Pr, 166Ho, 189Os, 191,195Ir, 195Pt(IT); analyzed available data; deduced the dynamic population of nuclear isomers in the r process.
doi: 10.3847/2041-8213/abfb74
2021WA45 Phys.Rev.Lett. 127, 172702 (2021) L.-J.Wang, L.Tan, Z.Li, G.W.Misch, Y.Sun Urca Cooling in Neutron Star Crusts and Oceans: Effects of Nuclear Excitations RADIOACTIVITY 31Mg, 25Na(EC); analyzed available data; deduced impact of the excited-state structure of atomic nuclei on nuclear processes in stellar environments.
doi: 10.1103/PhysRevLett.127.172702
2018BA23 Phys.Rev. C 97, 065807 (2018) P.Banerjee, G.W.Misch, S.K.Ghorui, Y.Sun Effective stellar β-decay rates of nuclei with long-lived isomers: 26Al and 34Cl RADIOACTIVITY 26Al, 34Cl(β+), (IT); calculated effective β-decay, and electromagnetic transition rates for ground states, isomeric states, and several low-spin excited states up to about 2.5 MeV at temperatures suitable for stellar environments; deduced time evolution of 26Al abundance. Calculations used NUSHELLX and OXBASH shell model codes with USDB interaction. Comparison with available experimental values from the ENSDF database, and with other theoretical calculations.
doi: 10.1103/PhysRevC.97.065807
2018MI01 Astrophys.J. 852, 43 (2018) Neutrino Spectra from Nuclear Weak Interactions in sd-Shell Nuclei under Astrophysical Conditions NUCLEAR STRUCTURE A=21-35; calculated electron- and positron-capture spectra, isospin-raising reaction neutrino spectra at a temperature and density typical of early core collapse.
doi: 10.3847/1538-4357/aa9c41
2016MI26 Phys.Rev. C 94, 055808 (2016) Nuclear neutrino energy spectra in high temperature astrophysical environments NUCLEAR STRUCTURE 27,28Si, 31S, 30,32P, 27,28Al, 56Fe; calculated charged current process neutrino spectra in high temperature astrophysical environments for electron capture and positron decays from ground and excited states calculated from shell-model calculations. 21,22Ne, 25Mg, 28,30Si, 27,28Al, 31P, 34,36S; calculated neutrino pair emissivities as a function of temperature. 27Al, 28Si; calculated neutral current neutrino and antineutrino spectra, energy-loss rates from neutral current deexcitation of 27Al and electron capture on 28Si.
doi: 10.1103/PhysRevC.94.055808
2014MI24 Phys.Rev. C 90, 065808 (2014) G.W.Misch, G.M.Fuller, B.A.Brown Modification of the Brink-Axel hypothesis for high-temperature nuclear weak interactions NUCLEAR STRUCTURE 28Si, 24,28Mg; calculated B(GT) distributions as a function of excitation energy up to 50 MeV, electron capture rates for 28Si as a function of electron Fermi energy and temperature. Failure of Brink-Axel hypothesis at high initial excitation energies, and proposed its modifications. Shell-model calculations.
doi: 10.1103/PhysRevC.90.065808
2013MI15 Phys.Rev. C 88, 015807 (2013) G.W.Misch, B.A.Brown, G.M.Fuller Neutrino-pair emission from hot nuclei during stellar collapse NUCLEAR STRUCTURE 28Si, 47Ti, 56Fe; calculated neutrino-antineutrino emission transition strength B(GT), energy loss as function of temperature and excitation energy, density of states as function of excitation energy. Shell-model calculations. Effect of residual interaction-induced configuration mixing on B(GT), energy of neutrino pairs, and entropy transport in supernovae.
doi: 10.1103/PhysRevC.88.015807
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