NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = G.M.Fuller Found 17 matches. 2022HE03 Phys.Rev. C 105, 015801 (2022) R.A.Herrera, C.W.Johnson, G.M.Fuller Modified Brink-Axel hypothesis for astrophysical Gamow-Teller transitions RADIOACTIVITY 53,55,56Fe, 57Co(EC), 55Cr(β-); calculated B(GT) for 53Fe to 53Mn, 55Fe to 55Mn, 56Fe to 56Mn, and 57Co to 57Fe from two adjacent initial states with excitation energies near 4.5 MeV, running sums of the strength functions for 53Fe to 53Mn, and 55Cr to 55Mn, transition strength running sums, thermal electron capture rates, and thermal positron emission rates for 57Co to 57Fe. 28Si(EC); calculated running sum of the strength function for 28Si to 28Al. Modified "local" Brink-Axel hypothesis for Gamow-Teller transitions for pf-shell nuclei in astrophysical applications. Relevance to computing accurate thermal weak transition rates for medium-mass nuclei at temperatures occurring in stellar cores near collapse stage.
doi: 10.1103/PhysRevC.105.015801
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
2004KO13 Phys.Rev.Lett. 92, 111101 (2004) E.Kolbe, K.Langanke, G.M.Fuller Neutrino-Induced Fission of Neutron-Rich Nuclei NUCLEAR REACTIONS 232,240,248,256Po, 228,236,244,252,260Rn, 230,238,246,254,262Ra, 232,240,248,256,264Th, 238,246,254,262,270U(ν, F), E=spectrum; calculated neutrino-induced fission σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevLett.92.111101
2003BA87 J.Phys.(London) G29, 2513 (2003) Supernova neutrino-nucleus astrophysics
doi: 10.1088/0954-3899/29/11/007
2001FU09 Nucl.Phys. A688, 322c (2001) The r-Process and Neutrinos
doi: 10.1016/S0375-9474(01)00721-7
2000AB36 Phys.Rev. D62, 093003 (2000) K.Abazajian, G.M.Fuller, X.Shi Increase in the Primordial 4He Yield in the Two-Doublet Four-Neutrino Mixing Scheme
doi: 10.1103/PhysRevD.62.093003
1999MC02 Phys.Rev. C59, 2873 (1999) G.C.McLaughlin, J.M.Fetter, A.B.Balantekin, G.M.Fuller Active-Sterile Neutrino Transformation Solution for r-Process Nucleosynthesis
doi: 10.1103/PhysRevC.59.2873
1998ME25 Phys.Rev. C58, 3696 (1998) B.S.Meyer, G.C.McLaughlin, G.M.Fuller Neutrino Capture and r-Process Nucleosynthesis
doi: 10.1103/PhysRevC.58.3696
1997CA59 Phys.Lett. 413B, 246 (1997) C.Y.Cardall, G.M.Fuller, D.B.Cline Intermediate Baseline Appearance Experiments and Three-Neutrino Mixing Schemes
doi: 10.1016/S0370-2693(97)01057-5
1996FU16 Nucl.Phys. A606, 167 (1996) Neutrino Gravitational Redshift and the Electron Fraction above Nascent Neutron Stars
doi: 10.1016/0375-9474(96)00268-0
1990AL45 Phys.Rev.Lett. 64, 2607 (1990) C.R.Alcock, D.S.Dearborn, G.M.Fuller, G.J.Mathews, B.S.Meyer Late-Time Dissipation of Primordial Baryon-Number Fluctuations and Nucleosynthesis
doi: 10.1103/PhysRevLett.64.2607
1985BL11 Nucl.Phys. A440, 511 (1985) Gamow-Teller Electron Capture Strength Distributions in Stars: Unblocked Iron and Nickel Isotopes RADIOACTIVITY 56,54,60,64Fe, 56Ni(EC); calculated Gamow-Teller strength distributions.
doi: 10.1016/0375-9474(85)90243-X
1985FU07 Astrophys.J. 293, 1 (1985) G.M.Fuller, W.A.Fowler, M.J.Newman Stellar Weak Interaction Rates for Intermediate-Mass Nuclei. IV. Interpolation Procedures for Rapidly Varying Lepton Capture Rates using Effective log(ft)-Values NUCLEAR STRUCTURE 1H, 1n, 48Ca, 48K, 48Sc, 56Fe, 56Mn, 54Co, 54Fe, 56Ni, 56Co, 60Zn, 60Cu; calculated effective log ft for β+, β- decay; deduced neutrino blocking effects.
doi: 10.1086/163208
1985MA40 Phys.Rev. C32, 796 (1985) G.J.Mathews, S.D.Bloom, G.M.Fuller, J.N.Bahcall Shell Model Calculation for the 71Ga(ν, e-)71Ge Solar Neutrino Detector NUCLEAR REACTIONS 71Ga(ν, e-), E not given; calculated Gamow-Teller transition strengths to residual nuclear levels following neutrino capture; deduced solar neutrino capture rate. 72Ge(p, d), 70Zn(3He, d), E not given; calculated spectroscopic factors. NUCLEAR STRUCTURE 71Ga; calculated levels. 71Ge; calculated levels, Gamow-Teller transition strengths.
doi: 10.1103/PhysRevC.32.796
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