NSR Query Results
Output year order : Descending NSR database version of April 24, 2024. Search: Author = J.Bahcall Found 44 matches. 2004BA79 Phys.Rev. D 70, 033012 (2004) J.N.Bahcall, H.Murayama, C.Pena-Garay What can we learn from neutrinoless double beta decay experiments?
doi: 10.1103/PhysRevD.70.033012
2003BA21 Phys.Rev.Lett. 90, 131301 (2003) J.N.Bahcall, M.C.Gonzalez-Garcia, C.Pena-Garay Does the Sun Shine by pp or CNO Fusion Reactions?
doi: 10.1103/PhysRevLett.90.131301
2002BA06 Phys.Rev. C65, 015802 (2002) How Many σ's is the Solar Neutrino Effect ?
doi: 10.1103/PhysRevC.65.015802
2002BA13 Phys.Rev. C65, 025801 (2002) The Luminosity Constraint on Solar Neutrino Fluxes
doi: 10.1103/PhysRevC.65.025801
2002BA89 Phys.Rev. C66, 035802 (2002) J.N.Bahcall, M.C.Gonzalez-Garcia, C.Pena-Garay If Sterile Neutrinos Exist, How Can One Determine the Total Solar Neutrino Fluxes ?
doi: 10.1103/PhysRevC.66.035802
1998AD12 Rev.Mod.Phys. 70, 1265 (1998) E.G.Adelberger, S.M.Austin, J.B.Bahcall, A.B.Balantekin, G.Bogaert, L.S.Brown, L.Buchmann, F.E.Cecil, A.E.Champagne, L.de Braeckeleer, C.A.Duba, S.R.Elliott, S.J.Freedom, M.Gai, G.Goldring, C.R.Gould, A.Gruzinov, W.C.Haxton, K.M.Heeger, E.Henley, C.W.Johnson, M.Kamionkowski, R.W.Kavanagh, S.E.Koonin, K.Kubodera, K.Langanke, T.Motobayashi, V.Pandharipande, P.Parker, R.G.H.Robertson, C.Rolfs, R.F.Sawyer, N.Shaviv, T.D.Shoppa, K.A.Snover, E.Swanson, R.E.Tribble, S.Turck-Chieze, J.F.Wilkerson Solar Fusion Cross Sections NUCLEAR REACTIONS 7Be, 12,13C, 15N, 16,17,18O(p, γ), 14,15N, 17,18O(p, α), 7Li(d, p), 3He(p, e+), (α, γ), (3He, 2p), 1H(p, e+), E=low; compiled, analyzed S-factor data, calculations; deduced implications for solar neutrino flux calculations.
doi: 10.1103/RevModPhys.70.1265
1998BA21 Nucl.Phys. A631, 29c (1998) Solar Neutrinos: Where we are, what we need
doi: 10.1016/S0375-9474(98)00013-X
1998BA30 Phys.Rev. C57, 2756 (1998) J.N.Bahcall, X.Chen, M.Kamionkowski Electron-Screening Correction for the Proton-Proton Reaction NUCLEAR REACTIONS 1H(p, X), E not given; calculated fusion reaction electron screening effect. Astrophysical implications.
doi: 10.1103/PhysRevC.57.2756
1998BA52 Phys.Lett. 433B, 1 (1998) J.N.Bahcall, S.Basu, M.H.Pinsonneault How Uncertain are Solar Neutrino Predictions ?
doi: 10.1016/S0370-2693(98)00657-1
1998BA84 Phys.Lett. 436B, 243 (1998) Do hep Neutrinos Affect the Solar Neutrino Energy Spectrum ? NUCLEAR REACTIONS 3He(p, e+ν), E=low; analyzed σ, relationship to solar neutrino flux.
doi: 10.1016/S0370-2693(98)00920-4
1998GR18 Astrophys.J. 504, 996 (1998) Screening in Thermonuclear Reaction Rates in the Sun
doi: 10.1086/306116
1997BA03 Phys.Rev. C55, 494 (1997) J.N.Bahcall, P.I.Krastev, E.Lisi Neutrino Oscillations and Moments of Electron Spectra NUCLEAR STRUCTURE 8B; calculated neutrino oscillations effects on solar neutrino; deduced energy distribution first two moments to be sufficient.
doi: 10.1103/PhysRevC.55.494
1997BA11 Phys.Rev. C55, 929 (1997) What Can Be Learned by Measuring the Fluxes of the 7Be and the pep Solar Neutrino Lines ( Question )
doi: 10.1103/PhysRevC.55.929
1997BA73 Phys.Rev. C56, 2839 (1997) Does the Sun Appear Brighter at Night in Neutrinos ( Question )
doi: 10.1103/PhysRevC.56.2839
1997BA87 Nucl.Phys. A625, 893 (1997) The Proton-Proton Reaction, Solar Neutrinos, and a Relativistic Field Theoretic Model of the Deuteron NUCLEAR REACTIONS 1H(p, dX), E not given; analyzed previous calculation; deduced incorrect reaction rate results.
doi: 10.1016/S0375-9474(97)00404-1
1997BA92 Phys.Rev. C56, 3391 (1997) Gallium Solar Neutrino Experiments: Absorption cross sections, neutrino spectra, and predicted event rates NUCLEAR REACTIONS 71Ga(ν, X), E=0.24-30 MeV; calculated absorption σ; deduced event rates for gallium-based experiments. Source thermal properties considered.
doi: 10.1103/PhysRevC.56.3391
1997GR27 Astrophys.J. 490, 437 (1997) The 7Be Electron Capture Rate in the Sun NUCLEAR REACTIONS 7Be(e, X), E not given; calculated electron capture rate in solar environment.
doi: 10.1086/304854
1996BA28 Phys.Rev. C54, 411 (1996) J.N.Bahcall, E.Lisi, D.E.Alburger, L.De Braeckeleer, S.J.Freedman, J.Napolitano Standard Neutrino Spectrum from 8B Decay RADIOACTIVITY 8B(β+); compiled, reviewed, analyzed decay data; deduced ν spectrum, absorption σ on Cl, Ga.
doi: 10.1103/PhysRevC.54.411
1996BA30 Phys.Lett. 374B, 1 (1996) J.N.Bahcall, M.Fukugita, P.I.Krastev How Does the Sun Shine ( Question )
doi: 10.1016/0370-2693(96)00187-6
1996BB03 Nucl.Phys. B(Proc.Suppl.) S48, 281 (1996) Ray Davis: The scientist and the man
doi: 10.1016/0920-5632(96)00262-9
1996BB04 Nucl.Phys. B(Proc.Suppl.) S48, 309 (1996) Solar Neutrinos: Where we are, where we are going
doi: 10.1016/0920-5632(96)00266-6
1995BA31 Phys.Lett. 348B, 121 (1995) J.N.Bahcall, P.I.Krastev, E.Lisi Limits on Electron-Neutrino Oscillations from the GALLEX 51Cr Source Experiment
doi: 10.1016/0370-2693(95)00111-W
1994KA02 Phys.Rev. C49, 545 (1994) Vacuum-Polarization Corrections to Solar-Fusion Rates NUCLEAR REACTIONS 1H(p, e+), 3He(3He, 2p), (α, γ), 7Li(p, α), 7Be(p, γ), 3He(p, e+), 14,15N, 16O, 12,13C(p, γ), 15N(p, α), E=low; calculated nuclear reaction rate. 3He(3He, 2p), (α, γ), 7Be, 14N(p, γ), E(cm) ≤ 1 MeV; calculated correction to Gamow penetration factor vs E.
doi: 10.1103/PhysRevC.49.545
1994KA07 Astrophys.J. 420, 884 (1994) The Rate of the Proton-Proton Reaction NUCLEAR REACTIONS 1H(p, e+), E=low; calculated reaction rate, matrix element, overlap integral square. Improved data input.
doi: 10.1086/173612
1993BA48 Phys.Rev.Lett. 71, 2369 (1993) Central Temperature of the Sun Can be Measured via the 7Be Solar Neutrino Line RADIOACTIVITY 7Be(EC); calculated ν line broadening, shift at solar temperatures.
doi: 10.1103/PhysRevLett.71.2369
1993BA86 Phys.Rev. D 47, 1298 (1993) Do solar-neutrino experiments imply new physics?
doi: 10.1103/PhysRevD.47.1298
1991BE54 Phys.Rev. D 44, 2962 (1991) Solar neutrinos and the Mikheyev-Smirnov-Wolfenstein theory
doi: 10.1103/PhysRevD.44.2962
1990BA64 Phys.Rev.Lett. 65, 2233 (1990) A Solution of the Solar-Neutrino Problem
doi: 10.1103/PhysRevLett.65.2233
1989BA95 Phys.Rev. D40, 931 (1989) Matter-Enchanced Neutrino Oscillations in the Standard Solar Model
doi: 10.1103/PhysRevD.40.931
1988BA86 Rev.Mod.Phys. 60, 297 (1988) Solar Models, Neutrino Experiments, and Helioseismology
doi: 10.1103/RevModPhys.60.297
1987BA89 Rev.Mod.Phys. 59, 505 (1987) Neutrino-Electron Scattering and Solar Neutrino Experiments
doi: 10.1103/RevModPhys.59.505
1987KR10 Phys.Lett. 189B, 299 (1987) D.Krofcheck, E.Sugarbaker, A.J.Wagner, J.Rapaport, D.Wang, J.N.Bahcall, R.C.Byrd, C.C.Foster, C.D.Goodman, C.Gaarde, D.J.Horen, T.Carey, T.N.Taddeucci Gamow-Teller Strength Distribution in 81Kr and the Consequences for a 81Br Solar Neutrino Detector NUCLEAR REACTIONS 81Br(p, n), E=190, 200 MeV; measured σ(En). 81Kr transitions deduced Gamow-Teller transition strength distribution. Tof.
doi: 10.1016/0370-2693(87)91436-5
1986BA21 Phys.Rev. C33, 2121 (1986) Solar Neutrinos from the Decay of 8B RADIOACTIVITY 8B(β+); calculated σ(Eν) following β-decay; deduced ν absorption σ in 37Cl. Forbidden corrections in weak interactions.
doi: 10.1103/PhysRevC.33.2121
1986BA51 Phys.Lett. 178B, 324 (1986) J.N.Bahcall, M.Baldo-Ceolin, D.B.Cline, C.Rubbia Predictions for a Liquid Argon Solar Neutrino Detector NUCLEAR REACTIONS 40Ar(ν, γ), E=solar neutrino; calculated absorption σ, σ(E(e)); deduced liquid argon solar neutrino detector feasibility.
doi: 10.1016/0370-2693(86)91519-4
1985KR10 Phys.Rev.Lett. 55, 1051 (1985) D.Krofcheck, E.Sugarbaker, J.Rapaport, D.Wang, J.N.Bahcall, R.C.Byrd, C.C.Foster, C.D.Goodman, I.J.Van Heerden, C.Gaarde, J.S.Larsen, D.J.Horen, T.N.Taddeucci Gamow-Teller Strength Function in 71Ge via the (p, n) Reaction at Medium Energies NUCLEAR REACTIONS 71Ga(p, n), E=120, 200 MeV; measured σ(En), σ(θ, En); deduced neutrino capture σ corrections in 71Ga detector. 71Ge deduced Gamow-Teller strength function, transition strength fragmentation.
doi: 10.1103/PhysRevLett.55.1051
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
1985RA11 Phys.Rev.Lett. 54, 2325 (1985) J.Rapaport, P.Welch, J.Bahcall, E.Sugarbaker, T.N.Taddeucci, C.D.Goodman, C.F.Foster, D.Horen, C.Gaarde, J.Larsen, T.Masterson Solar-Neutrino Detection: Experimental determination of Gamow-Teller strengths via the 98Mo and 115In(p, n) reactions NUCLEAR REACTIONS 98Mo, 115In(p, n), E=120, 200 MeV; measured σ(En, θ=0°); deduced target solar neutrino absorption σ. 98Tc, 115Sn deduced Gamow-Teller strengths.
doi: 10.1103/PhysRevLett.54.2325
1982BA80 Rev.Mod.Phys. 54, 767 (1982) J.N.Bahcall, W.F.Huebner, S.H.Lubow, P.D.Parker, R.K.Ulrich Standard Solar Models and the Uncertainties in Predicted Capture Rates of Solar Neutrinos
doi: 10.1103/RevModPhys.54.767
1981BA63 Phys.Rev. C24, 2216 (1981) 81Br and 79Br as Detectors of Solar Neutrinos RADIOACTIVITY 79,81Br; calculated neutrino absorption σ.
doi: 10.1103/PhysRevC.24.2216
1964BA58 Phys.Lett. 12, 300 (1964) Solar Neutrinos. I. Theoretical NUCLEAR REACTIONS 1H(p, e+ν), 2H(p, γ), 3He(3He, 2p), 3He(α, γ), 7Be(e-, ν), 7Li(p, α), 3He(α, γ), 7Be(p, γ), 8B(e+, ν), E not given; analyzed available data; deduced solar neutrino flux and reactions.
doi: 10.1103/PhysRevLett.12.300
1963BA21 Phys.Rev. 129, 2683 (1963) Overlap and Exchange Effects in Beta Decay NUCLEAR STRUCTURE 37Ar; measured not abstracted; deduced nuclear properties.
doi: 10.1103/PhysRev.129.2683
1963BA72 Phys.Rev. 132, 362 (1963) Exchange and Overlap Effects in Electron Capture and in Related Phenomena
doi: 10.1103/PhysRev.132.362
1963BA74 Phys.Rev. 131, 1756 (1963) Effect of Exchange on M/L Electron Capture Ratios
doi: 10.1103/PhysRev.131.1756
1962BA45 Phys.Rev.Letters 9, 500 (1962) Effect of Exchange on L to K Capture Ratios
doi: 10.1103/PhysRevLett.9.500
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