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NSR database version of May 24, 2024.

Search: Author = G.Fuller

Found 24 matches.

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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
Citations: PlumX Metrics


2022SC17      J.Phys.(London) G49, 110502 (2022)

H.Schatz, A.D.Becerril Reyes, A.Best, E.F.Brown, K.Chatziioannou, K.A.Chipps, C.M.Deibel, R.Ezzeddine, D.K.Galloway, C.J.Hansen, F.Herwig, A.P.Ji, M.Lugaro, Z.Meisel, D.Norman, J.S.Read, L.F.Roberts, A.Spyrou, I.Tews, F.X.Timmes, C.Travaglio, N.Vassh, C.Abia, P.Adsley, S.Agarwal, M.Aliotta, W.Aoki, A.Arcones, A.Aryan, A.Bandyopadhyay, A.Banu, D.W.Bardayan, J.Barnes, A.Bauswein, T.C.Beers, J.Bishop, T.Boztepe, B.Cote, M.E.Caplan, A.E.Champagne, J.A.Clark, M.Couder, A.Couture, S.E.de Mink, S.Debnath, R.J.deBoer, J.den Hartogh, P.Denissenkov, V.Dexheimer, I.Dillmann, J.E.Escher, M.A.Famiano, R.Farmer, R.Fisher, C.Frohlich, A.Frebel, C.Fryer, G.Fuller, A.K.Ganguly, S.Ghosh, B.K.Gibson, T.Gorda, K.N.Gourgouliatos, V.Graber, M.Gupta, W.C.Haxton, A.Heger, W.R.Hix, W.C.G.Ho, E.M.Holmbeck, A.A.Hood, S.Huth, G.Imbriani, R.G.Izzard, R.Jain, H.Jayatissa, Z.Johnston, T.Kajino, A.Kankainen, G.G.Kiss, A.Kwiatkowski, M.La Cognata, A.M.Laird, L.Lamia, P.Landry, E.Laplace, K.D.Launey, D.Leahy, G.Leckenby, A.Lennarz, B.Longfellow, A.E.Lovell, W.G.Lynch, S.M.Lyons, K.Maeda, E.Masha, C.Matei, J.Merc, B.Messer, F.Montes, A.Mukherjee, M.R.Mumpower, D.Neto, B.Nevins, W.G.Newton, L.Q.Nguyen, K.Nishikawa, N.Nishimura, F.M.Nunes, E.O'Connor, B.W.O'Shea, W.-J.Ong, S.D.Pain, M.A.Pajkos, M.Pignatari, R.G.Pizzone, V.M.Placco, T.Plewa, B.Pritychenko, A.Psaltis, D.Puentes, Y.-Z.Qian, D.Radice, D.Rapagnani, B.M.Rebeiro, R.Reifarth, A.L.Richard, N.Rijal, I.U.Roederer, J.S.Rojo, J.S K, Y.Saito, A.Schwenk, M.L.Sergi, R.S.Sidhu, A.Simon, T.Sivarani, A.Skuladottir, M.S.Smith, A.Spiridon, T.M.Sprouse, S.Starrfield, A.W.Steiner, F.Strieder, I.Sultana, R.Surman, T.Szucs, A.Tawfik, F.Thielemann, L.Trache, R.Trappitsch, M.B.Tsang, A.Tumino, S.Upadhyayula, J.O.Valle Martinez, M.Van der Swaelmen, C.Viscasillas Vazquez, A.Watts, B.Wehmeyer, M.Wiescher, C.Wrede, J.Yoon, R.G.T.Zegers, M.A.Zermane, M.Zingale, the Horizon 2020 Collaborations

Horizons: nuclear astrophysics in the 2020s and beyond

doi: https://dx.doi.org/10.1088/1361-6471/ac8890
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2018MI01      Astrophys.J. 852, 43 (2018)

G.W.Misch, Y.Sun, G.M.Fuller

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
Citations: PlumX Metrics


2016MI26      Phys.Rev. C 94, 055808 (2016)

G.W.Misch, G.M.Fuller

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
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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
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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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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
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2003BA87      J.Phys.(London) G29, 2513 (2003)

A.B.Balantekin, G.M.Fuller

Supernova neutrino-nucleus astrophysics

doi: 10.1088/0954-3899/29/11/007
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2001FU09      Nucl.Phys. A688, 322c (2001)

G.M.Fuller

The r-Process and Neutrinos

doi: 10.1016/S0375-9474(01)00721-7
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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
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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
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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
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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
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1996FU16      Nucl.Phys. A606, 167 (1996)

G.M.Fuller, Y.-Z.Qian

Neutrino Gravitational Redshift and the Electron Fraction above Nascent Neutron Stars

doi: 10.1016/0375-9474(96)00268-0
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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
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1985BL11      Nucl.Phys. A440, 511 (1985)

S.D.Bloom, G.M.Fuller

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
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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
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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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1976FU06      J.Phys.Chem.Ref.Data 5, 835 (1976)

G.H.Fuller

Nuclear Spins and Moments

COMPILATION A=1-253; compiled μ, quadrupole moment, I.

doi: 10.1063/1.555544
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1976FU10      J.Phys.Chem.Ref.Data 5, 835 (1976)

G.H.Fuller

Nuclear Spins and Moments

doi: 10.1063/1.555544
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1972FU01      Priv.Comm. (March 1972); See Also 69FuCo

G.F.Fuller


1971FU02      Priv.Comm. (March 1971)

G.Fuller


1969FU11      Nucl.Data Tables A5, 433 (1969)

G.H.Fuller, V.W.Cohen

Nuclear Spins and Moments


1959FU99      1959 Nuclear Data Tables, p.127. U.S.Government Printing Office, Washington, D.C. 20402( 1.00)

G.H.Fuller

Relative Isotopic Abundances


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Note: The following list of authors and aliases matches the search parameter G.Fuller: , G.F.FULLER, G.H.FULLER, G.M.FULLER