NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = B.Meyer Found 49 matches. 2024LI09 Phys.Lett. B 848, 138385 (2024) M.Li, T.M.Sprouse, B.S.Meyer, M.R.Mumpower Atomic masses with machine learning for the astrophysical r process NUCLEAR STRUCTURE N<160; analyzed available data; deduced mass deviations between Machine-Learning (ML) approach and HFB-32 model, neutron separation energies, abundances, β-decay rates. Comparison with AME 2020 data.
doi: 10.1016/j.physletb.2023.138385
2022LI53 Phys.Rev. C 106, 035803 (2022) Dependence of (n, γ)- (γ, n) equilibrium r-process abundances on nuclear physics properties NUCLEAR STRUCTURE 60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78Cr, 63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78,79Mn, 65,66,67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82Fe, 67,68,69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84Co, 69,70,71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88Ni, 71,72,73,74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93Cu, 74,75,76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96Zn, 76,77,78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101Ga, 78,79,80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104Ge, 80,81,82,83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107As, 83,84,85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111Se, 85,86,87,88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116Br, 88,89,90,91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119Kr, 91,92,93,94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120Rb, 94,95,96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123Sr, 97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125Y, 100,101,102,103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126Zr, 103,104,105,106,107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128Nb, 107,108,109,110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130Mo, 110,111,112,113,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132Tc, 112,114,115,116,117,118,119,120,121,122,123,124,125,126,127,128,129,130,131,132,133,134Ru; 36,37Cl, 37,38,39Ar, 38,39,40,41K, 39,40,41,42,43,44Ca, 40,41,42,43,44,45Sc, 41,42,43,44,45,46,47,48Ti, 42,43,44,45,46,47,48,49,50V, 44,45,46,47,48,49,50,51,52,53Cr, 46,47,48,49,50,51,52,53,54,55,56Mn, 47,48,49,50,51,52,53,54,55,56,57,58Fe, 49,50,51,52,53,54,55,56,57,58,59,60Co, 51,52,53,54,55,56,57,58,59,60,61,62Ni, 53,54,55,56,57,58,59,60,61,62,63,64Cu, 56,57,58,59,60,61,62,63,64,65,66Zn, 58,59,60,61,62,63,64,65,66,67,68Ga, 60,61,62,63,64,65,66,67,68,69,70Ge, 63,64,65,66,67,68,69,70,71As, 65,66,67,68,69,70,71,72,73Se, 68,69,70,71,72,73,74,75Br, 69,70,71,72,73,74,75,76Kr, 72,73,74,75,76,77Rb, 74,75,76,77,78Sr, 76,77,78,79Y, 78,79,80Zr; calculated chemical-potential offset differences for the reference r-process calculations as functions of time step, temperature, and nuclear mass density for the first set of nuclei from A=60-134, and for the second set of nuclei from A=36-80 for the reference νp-process calculations. A=100-220; calculated abundances as a function of nucleon number for the last moment of (n, γ)-(γ, n) equilibrium and the final frozen-out abundances, ratios of masses and partition functions in Z=50 isotopic chain, S(n), isotopic abundances within an isotope chain, equilibrium abundance distributions, normalized equilibrium abundance curves as functions of Coulomb and asymmetry term coefficients. N=40-120; calculated S(n), abundance distribution including the linear and pairing terms of S(n), equilibrium and full abundance distributions for N=50 and N=82 shell crossings as well as for Z=55, 68 and 70 nuclei, S(n) for two shell transitions; deduced effects of nuclear physics inputs on (n, γ)-(γ, n) equilibrium isotopic abundances, and that isotopic abundances versus neutron number in (n, γ)-(γ, n) equilibrium well approximated as Gaussians. Realistic phenomenological nuclear physics model. Comparison with available experimental and evaluated data in REACLIB V2.2 database.
doi: 10.1103/PhysRevC.106.035803
2019PE11 Phys.Rev. C 100, 015810 (2019) A.Petrovici, A.S.Mare, O.Andrei, B.S.Meyer Impact of 68Se and 72Kr stellar weak interaction rates on rp-process nucleosynthesis and energetics RADIOACTIVITY 68Se, 72Kr(β+), (EC); calculated stellar weak interaction rates of ground state and low-lying excited states using the beyond-mean-field complex excited Vampir model. Discussed impact on rp-process nucleosynthesis in type-I x-ray bursts and energetics.
doi: 10.1103/PhysRevC.100.015810
2018TA12 Phys.Rev. C 97, 055801 (2018) R.Talwar, M.J.Bojazi, P.Mohr, K.Auranen, M.L.Avila, A.D.Ayangeakaa, J.Harker, C.R.Hoffman, C.L.Jiang, S.A.Kuvin, B.S.Meyer, K.E.Rehm, D.Santiago-Gonzalez, J.Sethi, C.Ugalde, J.R.Winkelbauer Experimental study of 38Ar + α reaction cross sections relevant to the 41Ca abundance in the solar system NUCLEAR REACTIONS 4He(38Ar, p), (38Ar, n), (38Ar, α'), E=133 MeV; measured energies and yields of reaction products, energy- and angle integrated σ(E) using multisampling ionization chamber (MUSIC) detector at the ATLAS-ANL facility. Comparison with previous experimental values, and with statistical model calculations using TALYS code. 41K(p, α)38Ar, 41Ca(n, α)38Ar, T=0.1-10.0 GK; deduced astrophysical reaction rates, and compared with statistical model calculations, and with REACLIB fits. Discussed relevance to 41Ca abundance in the solar system.
doi: 10.1103/PhysRevC.97.055801
2018TE04 Phys.Rev.Lett. 121, 112701 (2018) M.Tessler, M.Paul, S.Halfon, B.S.Meyer, R.Pardo, R.Purtschert, K.E.Rehm, R.Scott, M.Weigand, L.Weissman, S.Almaraz-Calderon, M.L.Avila, D.Baggenstos, P.Collon, N.Hazenshprung, Y.Kashiv, D.Kijel, A.Kreisel, R.Reifarth, D.Santiago-Gonzalez, A.Shor, I.Silverman, R.Talwar, D.Veltum, R.Vondrasek Stellar 36, 38Ar(n, γ)37, 39Ar Reactions and Their Effect on Light Neutron-Rich Nuclide Synthesis NUCLEAR REACTIONS 36,38Ar(n, γ), E ∼ 30 keV; measured reaction products, Eβ, Iβ; deduced thermal σ, Maxwellian average cross sections (MACS). Comparison with available data.
doi: 10.1103/PhysRevLett.121.112701
2017AR04 Prog.Part.Nucl.Phys. 94, 1 (2017) A.Arcones, D.W.Bardayan, T.C.Beers, L.A.Bernstein, J.C.Blackmon, B.Messer, B.A.Brown, E.F.Brown, C.R.Brune, A.E.Champagne, A.Chieffi, A.J.Couture, P.Danielewicz, R.Diehl, M.El Eid, J.E.Escher, B.D.Fields, C.Frohlich, F.Herwig, W.R.Hix, C.Iliadis, W.G.Lynch, G.C.McLaughlin, B.S.Meyer, A.Mezzacappa, F.Nunes, B.W.O'Shea, M.Prakash, B.Pritychenko, S.Reddy, E.Rehm, G.Rogachev, R.E.Rutledge, H.Schatz, M.S.Smith, I.H.Stairs, A.W.Steiner, T.E.Strohmayer, F.X.Timmes, D.M.Townsley, M.Wiescher, R.G.T.Zegers, M.Zingale White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics
doi: 10.1016/j.ppnp.2016.12.003
2017CL05 Geochim.Cosmochim.Act. 221, 47 (2017) Graphite grain-size spectrum and molecules from core-collapse supernovae ATOMIC MASSES C, O; calculated abundances of carbon atomic complexes that emerge from the C + O cores of core-collapse supernovae.
doi: 10.1016/j.gca.2017.06.027
2017SI11 J.Phys.(London) G44, 064006 (2017) A.Simon, M.Beard, B.S.Meyer, B.Roach Impact of the α optical model potential on the γ-process nucleosynthesis NUCLEAR REACTIONS 156,158,160Dy, 152,154Er, 168Yb(α, γ), E<5 GK; 106Cd, 112Sn, 144Sm, 151Eu, 168Yb, 197Au(α, n), E(cm)<24 MeV; calculated σ, astrophysical reaction rates. NON-SMOKER, TALYS nuclear model codes, comparison with available data.
doi: 10.1088/1361-6471/aa6bb4
2016TV01 Phys.Rev. C 94, 025804 (2016) G.M.Tveten, A.Spyrou, R.Schwengner, F.Naqvi, A.C.Larsen, T.K.Eriksen, F.L.Bello Garrote, L.A.Bernstein, D.L.Bleuel, L.Crespo Campo, M.Guttormsen, F.Giacoppo, A.Gorgen, T.W.Hagen, K.Hadynska-Klek, M.Klintefjord, B.S.Meyer, H.T.Nyhus, T.Renstrom, S.J.Rose, E.Sahin, S.Siem, T.G.Tornyi Completing the nuclear reaction puzzle of the nucleosynthesis of 92Mo NUCLEAR REACTIONS 92Mo(p, p'), E=16.5 MeV; measured Ep, Ip, Eγ, Iγ pγ-coin, angular distributions using SiRi silicon ΔE-E telescopes for protons and CACTUS scintillator detector array for γ rays at Oslo Cyclotron Laboratory; deduced nuclear level density (NLD) and γ-strength function (γSF) of 92Mo. 91Nb(p, γ)92Mo, T9=1.8-3.5; deduced astrophysical reaction rates using TALYS 1.6 code and NLD and γSF input from present experiment; discussed puzzle of the nucleosynthesis of 92Mo in the context of p process. Comparison with previous experimental results from 92Mo(γ, γ') and 92,94,95,96Mo(γ, n) reactions, and shell model calculations.
doi: 10.1103/PhysRevC.94.025804
2015LO04 Phys.Rev.Lett. 114, 192501 (2015) G.Lorusso, S.Nishimura, Z.Y.Xu, A.Jungclaus, Y.Shimizu, G.S.Simpson, P.-A.Soderstrom, H.Watanabe, F.Browne, P.Doornenbal, G.Gey, H.S.Jung, B.Meyer, T.Sumikama, J.Taprogge, Zs.Vajta, J.Wu, H.Baba, G.Benzoni, K.Y.Chae, F.C.L.Crespi, N.Fukuda, R.Gernhauser, N.Inabe, T.Isobe, T.Kajino, D.Kameda, G.D.Kim, Y.-K.Kim, I.Kojouharov, F.G.Kondev, T.Kubo, N.Kurz, Y.K.Kwon, G.J.Lane, Z.Li, A.Montaner-Piza, K.Moschner, F.Naqvi, M.Niikura, H.Nishibata, A.Odahara, R.Orlandi, Z.Patel, Zs.Podolyak, H.Sakurai, H.Schaffner, P.Schury, S.Shibagaki, K.Steiger, H.Suzuki, H.Takeda, A.Wendt, A.Yagi, K.Yoshinaga β-Decay Half-Lives of 110 Neutron-Rich Nuclei across the N=82 Shell Gap: Implications for the Mechanism and Universality of the Astrophysical r Process RADIOACTIVITY 134,135,136,137,138,139Sn, 128,129,130,131,132,133,134,135,136,137In, 126,127,128,129,130,131,132,133,134Cd, 124,125,126,127,128,129,130,131,132Ag, 121,122,123,124,125,126,127,128,129Pd, 118,119,120,121,122,123,124,125,126,127Rh, 116,117,118,119,120,121,122,123,124Ru, 112,113,114,115,116,117,118,119,120,121Tc, 109,110,111,112,113,114,115,116,117,118Mo, 107,108,109,110,111,112,113,114,115Nb, 106,107,108,109,110,111,112Zr, 104,105,106,107,108,109Y, 103,104,105,106Sr, 102,103Rb(β-) [from Be(238U, X), E=345 MeV/nucleon]; measured decay products, Eγ, Iγ; deduced T1/2; Calculated r-process abundances. Comparison with available data.
doi: 10.1103/PhysRevLett.114.192501
2014BO04 Phys.Rev. C 89, 025807 (2014) Explosive nucleosynthesis of 15Na in a massive-star model NUCLEAR REACTIONS 14N(α, γ)18F, 18F(n, α)15N, 18O(p, α)15N, E at stellar temperatures; calculated mass fraction of 15N in explosive nucleosynthesis through different pathways in helium-rich outer layers of massive stars over all the 707 zones available in the presupernova stars including neutrino-nucleus interactions, time evolution of mass fractions of neutrons, protons, 14,15N, 18O and 18F; discussed competition between the production and destruction of 15N, latter through 15N(p, α)12C and 15N(α, γ)19F reactions. Comparison of presupernova and postsupernova values, and with previous calculations A simple but realistic model of shock passage using open-source, freely available codes.
doi: 10.1103/PhysRevC.89.025807
2014WU06 Phys.Rev. C 90, 011601 (2014), Erratum Phys.Rev. C 90, 019903 (2014) S.Wuenschel, H.Zheng, K.Hagel, B.Meyer, M.Barbui, E.J.Kim, G.Ropke, J.B.Natowitz Nucleation and cluster formation in low-density nucleonic matter: A mechanism for ternary fission NUCLEAR REACTIONS 241Pu(n, F), E=thermal; calculated ternary fission yields as a function of mass and charge of products of A<40. Nucleation and cluster formation in the low-density neck between the two large fragments. Nuclear statistical equilibrium (NSE) calculations. Comparison with experimental data. 242Pu(SF); plotted experimental relative yields of ternary cluster isotopes.
doi: 10.1103/PhysRevC.90.011601
2013FA04 J.Phys.:Conf.Ser. 445, 012025 (2013) M.Famiano, R.N.Boyd, T.Kajino, B.Meyer, Y.Motizuki, I.Roederer Implementing the r-process in metal-poor stars via black hole collapse and relevance to the light element enhancement
doi: 10.1088/1742-6596/445/1/012025
2013QU01 Phys.Rev. C 88, 011603 (2013) S.J.Quinn, A.Spyrou, A.Simon, A.Battaglia, M.Couder, P.A.DeYoung, A.C.Dombos, X.Fang, J.Gorres, A.Kontos, Q.Li, S.Lyons, B.S.Meyer, G.F.Peaslee, D.Robertson, K.Smith, M.K.Smith, E.Stech, W.P.Tan, X.D.Tang, M.Wiescher Probing the production mechanism of the light p-process nuclei NUCLEAR REACTIONS 74Ge(p, γ)75As, E=1.6-4.2 MeV; measured Eγ, Iγ, σ(E) using the NSCL SuN detector at Notre Dame facility; deduced astrophysical S(E) factors, reaction rates at T9=0.10-10.0, cumulative mass fraction of 74Se in a Type II Supernova model. Comparison with previous experimental data, and with theoretical predictions using NON-SMOKER and TALYS nuclear reaction codes.
doi: 10.1103/PhysRevC.88.011603
2013SP04 Phys.Rev. C 88, 045802 (2013) A.Spyrou, S.J.Quinn, A.Simon, T.Rauscher, A.Battaglia, A.Best, B.Bucher, M.Couder, P.A.DeYoung, A.C.Dombos, X.Fang, J.Gorres, A.Kontos, Q.Li, L.Y.Lin, A.Long, S.Lyons, B.S.Meyer, A.Roberts, D.Robertson, K.Smith, M.K.Smith, E.Stech, B.Stefanek, W.P.Tan, X.D.Tang, M.Wiescher Measurement of the 90, 92Zr(p, γ)91, 93Nb reactions for the nucleosynthesis of elements near A=90 NUCLEAR REACTIONS 90,92Zr(p, γ)91Nb/93Nb, E=2.0-5.0 MeV; measured Eγ, Iγ, σ(E) using NSCL SuN detector at Notre Dame accelerator facility; deduced astrophysical S factors, reaction rates, sensitivity of reaction to widths in Hauser-Feshbach model. Comparison with standard NON-SMOKER model, and two TALYS calculations. Relevance to synthesis and abundances of light p nuclei.
doi: 10.1103/PhysRevC.88.045802
2007NI12 667, L159 (2007) r-Process Nucleosynthesis in Shocked Surface Layers of O-Ne-Mg Cores
doi: 10.1086/522372
2006HI17 Nucl.Phys. A777, 188 (2006) Thermonuclear kinetics in astrophysics
doi: 10.1016/j.nuclphysa.2004.10.009
2004JO20 Astrophys.J. 617, L131 (2004) Nucleosynthesis in fast expansions of high-entropy, proton-rich matter
doi: 10.1086/427233
2003JO20 Phys.Rev. C 68, 065801 (2003) G.C.Jordan IV, S.S.Gupta, B.S.Meyer Nuclear reactions important in α-rich freeze-outs NUCLEAR REACTIONS 57Ni(n, p), 55Co, 59Cu(p, γ), 59Cu(p, α), E=low; calculated astrophysical reactions rates. Sensitivity of supernova observables to nuclear reaction rates discussed.
doi: 10.1103/PhysRevC.68.065801
2003ME19 Nucl.Phys. A719, 13c (2003) Neutrinos, supernovae, molybdenum, and extinct 92Nb
doi: 10.1016/S0375-9474(03)00952-7
2002ME23 Phys.Rev.Lett. 89, 231101 (2002) r-Process Nucleosynthesis without Excess Neutrons
doi: 10.1103/PhysRevLett.89.231101
2001GU21 Phys.Rev. C64, 025805 (2001) Internal Equilibration of a Nucleus with Metastable States: 26Al as an example NUCLEAR STRUCTURE 26Al; analyzed equilibration of ground, metastable states in astrophysical environment. Multistep transitions, application to nucleosynthesis calculations discussed.
doi: 10.1103/PhysRevC.64.025805
2001TH22 Astrophys.J. 562, 887 (2001) T.A.Thompson, A.Burrows, B.S.Meyer The Physics of Proto-Neutron Star Winds: Implications for r-Process Nucleosynthesis
doi: 10.1086/323861
2000ME22 Phys.Rep. 333-334, 1 (2000) Nucleocosmochronology
doi: 10.1016/S0370-1573(00)00012-0
2000TH09 Astrophys.J. 533, 998 (2000) L.-S.The, M.F.El Eid, B.S.Meyer A New Study of s-Process Nucleosynthesis in Massive Stars
doi: 10.1086/308677
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
1998TH07 Astrophys.J. 504, 500 (1998) L.-S.The, D.D.Clayton, L.Jin, B.S.Meyer Nuclear Reactions Governing the Nucleosynthesis of 44Ti NUCLEAR REACTIONS 44Ti, 36Ar, 40Ca(α, p), 8Be, 40Ca, 44Ti, 12C, 36Ar(α, γ), 45V, 57Ni, 58Cu, 44Ti, 57Co(p, γ), 57Co(p, n), 57Ni(n, γ), 54Fe(α, n), E not given; analyzed reaction rates influence on 44Ti nucleosynthesis.
doi: 10.1086/306057
1997CL04 Nucl.Phys. A621, 391c (1997) D.D.Clayton, T.D.Krishnan, B.S.Meyer Origin of 48Ca NUCLEAR STRUCTURE 48Ca; analyzed reaction rates variation; deduced 48Ca survival dependence on expansion type in nucleosynthesis.
doi: 10.1016/S0375-9474(97)00277-7
1997JI04 Nucl.Phys. A621, 319c (1997) L.Jin, B.S.Meyer, L.-S.The, D.D.Clayton Nuclear Reaction Rates Governing the Nucleosynthesis of 44Ti NUCLEAR STRUCTURE 44Ti; analyzed, surveyed nuclear reaction rates; deduced 44Ti production dependence on certain reaction rates, astrophysical implication. Large reaction network.
doi: 10.1016/S0375-9474(97)00263-7
1997ME09 Nucl.Phys. A621, 409c (1997) r-Process Surveys NUCLEAR STRUCTURE A=195; calculated abundance peak synthesis; deduced r-process conditions constraints role.
doi: 10.1016/S0375-9474(97)00281-9
1997ME23 Astrophys.J.Suppl.Ser. 112, 199 (1997) Survey of r-Process Models
doi: 10.1086/313032
1997SU19 Phys.Rev.Lett. 79, 1809 (1997) R.Surman, J.Engel, J.R.Bennett, B.S.Meyer Source of the Rare-Earth Element Peak in r-Process Nucleosynthesis NUCLEAR STRUCTURE A=150-175; analyzed r-process abundance distribution; deduced rare-earth element peak associated features in nucleosynthesis.
doi: 10.1103/PhysRevLett.79.1809
1996HO29 Nucl.Instrum.Methods Phys.Res. A380, 117 (1996) D.M.Hofmann, W.Stadler, P.Christmann, B.K.Meyer Defects in CdTe and Cd(1-x)Zn(x)Te
doi: 10.1016/S0168-9002(96)00287-2
1996SI14 Nucl.Instrum.Methods Phys.Res. A369, 340 (1996) Activity Measurement of 204Tl by Direct Liquid Scintillation Method RADIOACTIVITY 204Tl(β-), (EC); measured activity. 4π (X, e)-X(K) coincidence counting.
doi: 10.1016/S0168-9002(96)80005-2
1994ME26 Ann.Rev.Astron.Astrophys. 32, 153 (1994) The r-, s-, and p-Processes in Nucleosynthesis
doi: 10.1146/annurev.astro.32.1.153
1994SI21 Nucl.Instrum.Methods Phys.Res. A339, 14 (1994) Direct Activity Measurement of Pure Beta-Emitting Radionuclides by the TDCR Efficiency Calculation Technique RADIOACTIVITY 3H(β-); 63Ni(β-); 14C(β-); 99Tc(β-); measured activity. Triple-to-double coincidence ratio efficiency calculation technique.
doi: 10.1016/0168-9002(94)91771-X
1994SI26 Appl.Radiat.Isot. 45, 669 (1994) Standardization and Half-Life of 201Tl by the 4π(x, e)-γ Coincidence Method with Liquid Scintillation Counting in the 4π-Channel RADIOACTIVITY 201Tl(EC); measured (X-ray)γ-, (electron)γ-coin; deduced source standardization. 201Tl deduced T1/2. Liquid scintillation counting in 4π channel.
doi: 10.1016/0969-8043(94)90245-3
1994WO06 Astrophys.J. 433, 229 (1994) S.E.Woosley, J.R.Wilson, G.J.Mathews, R.D.Hoffman, B.S.Meyer The r-Process and Neutrino-Heated Supernova Ejecta
doi: 10.1086/174638
1993BO13 Phys.Rev. C47, 2369 (1993) R.N.Boyd, C.A.Mitchell, B.S.Meyer Reaction Rate for Destruction of 7Li and Primordial Nucleosynthesis NUCLEAR REACTIONS 7Li(d, X), E ≈ resonance; calculated target destruction rate; deduced 7Li abundance prediction implications.
doi: 10.1103/PhysRevC.47.2369
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
1990ME05 Appl.Radiat.Isot. 41, 375 (1990) A Direct Method for 55Fe Activity Measurement RADIOACTIVITY 55Fe; measured activity. Direct method, theoretical counting efficiency, liquid scintillators.
doi: 10.1016/0883-2889(90)90146-8
1990ST03 Appl.Radiat.Isot. 41, 315 (1990) G.F.Steyn, S.J.Mills, F.M.Nortier, B.R.S.Simpson, B.R.Meyer Production of 52Fe via Proton-Induced Reactions on Manganese and Nickel NUCLEAR REACTIONS, ICPND 55Mn(p, 4n), E=40-200 MeV; 27Al(p, X)22Na, E=75-200 MeV; Ni(p, X)52Fe, E=45-200 MeV; measured residual production σ(E).
doi: 10.1016/0883-2889(90)90197-O
1989ME06 Phys.Rev. C39, 1876 (1989) B.S.Meyer, W.M.Howard, G.J.Mathews, K.Takahashi, P.Moller, G.A.Leander Beta-Delayed Fission and Neutron Emission Calculations for the Actinide Cosmochronometers NUCLEAR STRUCTURE 234,244,252Fr, 246,248,252,264Ac, 250,252,254,260,270Pa, 252,254,276Np, 251,258,264,277Am; calculated Gamow-Teller strength functions; deduced beta-delayed fission, beta delayed neutron emission, galactic age uncertainities. Actinide cosmochronometers.
doi: 10.1103/PhysRevC.39.1876
1989SI19 Appl.Radiat.Isot. 40, 819 (1989) The Half-Life of 125I RADIOACTIVITY 125I(EC); measured T1/2. Linearized weighted least square data analysis, direct activity measurement.
doi: 10.1016/0883-2889(89)90103-2
1974DE09 Nucl.Phys. A225, 317 (1974); Priv.Comm. (March 1974) F.W.N.de Boer, P.F.A.Goudsmit, P.Koldewijn, B.J.Meyer Decay Properties of Three 166Lu Isomers and the Decay of 166Hf RADIOACTIVITY 166Lu, 166Hf [from 169Tm(3He, 6n), 170Yb(p, 5n)]; measured Eγ, Iγ, I(ce), γγ-coin, Eγ-coin, Xγ delay. 166Yb, 166Lu deduced levels, T1/2, Q-value, J, log ft, π, ICC multipolarities, Ge(Li), Si(Li), NaI(Tl), plastic detectors. Enriched, natural targets.
doi: 10.1016/0375-9474(74)90544-2
1973DE04 Priv.Comm. (1973) F.W.N.de Boer, P.F.A.Goudsmit, B.J.Meyer
1973SO03 Phys.Rev. C7, 1564 (1973) H.W.Sobel, A.A.Hruschka, W.R.Kropp, J.Lathrop, F.Reines, M.F.Crouch, B.S.Meyer, J.P.F.Sellschop High-Energy Gamma Rays from Spontaneous Fission of 238U RADIOACTIVITY, Fission 238U(SF); measured γ-spectrum. Deduced absolute photon yield.
doi: 10.1103/PhysRevC.7.1564
1973ST19 Int.J.Appl.Radiat.Isotop. 24, 369 (1973) Production of 67Ga by Deuteron Bombardment of Natural Zinc NUCLEAR REACTIONS Zn(d, xn), E=0-16 MeV; measured σ(E). 66,67Ga deduced production rates.
doi: 10.1016/0020-708X(73)90015-X
1969ME17 Priv.Comm. (1969)
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