NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = W.C.Haxton Found 70 matches. 2023EL07 Phys.Rev. C 108, 035502 (2023) S.R.Elliott, V.N.Gavrin, W.C.Haxton, T.V.Ibragimova, E.J.Rule Gallium neutrino absorption cross section and its uncertainty
doi: 10.1103/PhysRevC.108.035502
2023HA12 Phys.Rev. C 107, 035504 (2023) W.C.Haxton, E.Rule, K.McElvain, M.J.Ramsey-Musolf Nuclear-level effective theory of μ → e conversion: Formalism and applications NUCLEAR REACTIONS 12C, 16O, 19F, 23Na, 27Al, 28Si, 32S, 40Ca, 48Ti, 56Fe, 63,65Cu, 184W, 197Au, 208Pb(μ-, e-), at momentum transfer q=96.54-105.12 MeV; calculated μ to e conversion rates, with derivation of bounds on the coefficients of the charged lepton flavor violation decay (CLFV) operators, and full evaluation of the associated nuclear response functions, and accurate treatment of electron and muon Coulomb effects using advanced shell-model methods. Discussed matching of the nonrelativistic effective theory (NRET) onto higher level effective field theories, and relation of μ to e conversion to μ to e+γ, and μ to 3e. Comparison with results from MEG, MEG II, Mu3e and SINDRUM experiments. Relevance to future μ to e conversion searches at Fermilab (Mu2e) and J-PARC (COMET, DeeMe) experimental facilities to improve and to advance limits to higher orders on charged lepton flavor violation (CLFV) decays of light pseudoscalars via μ to e conversion in Nuclei.
doi: 10.1103/PhysRevC.107.035504
2022BA17 Phys.Rev.Lett. 128, 232501 (2022) V.V.Barinov, B.T.Cleveland, S.N.Danshin, H.Ejiri, S.R.Elliott, D.Frekers, V.N.Gavrin, V.V.Gorbachev, D.S.Gorbunov, W.C.Haxton, T.V.Ibragimova, I.Kim, Y.P.Kozlova, L.V.Kravchuk, V.V.Kuzminov, B.K.Lubsandorzhiev, Y.M.Malyshkin, R.Massarczyk, V.A.Matveev, I.N.Mirmov, J.S.Nico, A.L.Petelin, R.G.H.Robertson, D.Sinclair, A.A.Shikhin, V.A.Tarasov, G.V.Trubnikov, E.P.Veretenkin, J.F.Wilkerson, A.I.Zvir Results from the Baksan Experiment on Sterile Transitions (BEST) NUCLEAR REACTIONS 71Ga(ν, e-), E<1 MeV; measured reaction products, Eβ, Iβ; deduced the deficit of electron neutrinos observed in gallium-based radiochemical measurements with high-intensity neutrino sources, commonly referred to as the gallium anomaly. The Baksan Experiment on Sterile Transitions (BEST).
doi: 10.1103/PhysRevLett.128.232501
2022BA21 Phys.Rev. C 105, 065502 (2022) V.V.Barinov, S.N.Danshin, V.N.Gavrin, V.V.Gorbachev, D.S.Gorbunov, T.V.Ibragimova, Yu.P.Kozlova, L.V.Kravchuk, V.V.Kuzminov, B.K.Lubsandorzhiev, Yu.M.Malyshkin, I.N.Mirmov, A.A.Shikhin, E.P.Veretenkin, B.T.Cleveland, H.Ejiri, S.R.Elliott, I.Kim, R.Massarczyk, D.Frekers, W.C.Haxton, V.A.Matveev, G.V.Trubnikov, J.S.Nico, A.L.Petelin, V.A.Tarasov, A.I.Zvir, R.G.H.Robertson, D.Sinclair, J.F.Wilkerson Search for electron-neutrino transitions to sterile states in the BEST experiment NUCLEAR REACTIONS 71Ga(ν, e-), E<1 MeV; measured reaction products, Eb, Iβ; deduced 71Ge yields, deficit of electron neutrinos observed in gallium-based radiochemical measurements with high-intensity neutrino sources, commonly referred as "the gallium anomaly". The Baksan Experiment on Sterile Transitions (BEST). Neutrinos from decay of the 51Cr decay. RADIOACTIVITY 51Cr(EC); measured Eγ, Iγ, calorimetric heat; deduced T1/2.
doi: 10.1103/PhysRevC.105.065502
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
2014AN04 Phys.Rev. C 89, 065501 (2014) N.Anand, A.L.Fitzpatrick, W.C.Haxton Weakly interacting massive particle-nucleus elastic scattering response
doi: 10.1103/PhysRevC.89.065501
2012SA07 Rep.Prog.Phys. 75, 036901 (2012) D.W.Savin, N.S.Brickhouse, J.J.Cowan, R.P.Drake, S.R.Federman, G.J.Ferland, A.Frank, M.S.Gudipati, W.C.Haxton, E.Herbst, S.Profumo, F.Salama, L.M.Ziurys, E.G.Zweibel The impact of recent advances in laboratory astrophysics on our understanding of the cosmos
doi: 10.1088/0034-4885/75/3/036901
2011AD03 Rev.Mod.Phys. 83, 195 (2011) E.G.Adelberger, A.Garcia, R.G.H.Robertson, K.A.Snover, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, D.Bemmerer, A.Junghans, D.Bemmerer, A.Junghans, C.A.Bertulani, K.-W.Chen, H.Costantini, P.Prati, M.Couder, E.Uberseder, M.Wiescher, R.Cyburt, B.Davids, S.J.Freedman, M.Gai, D.Gazit, L.Gialanella, G.Imbriani, U.Greife, M.Hass, W.C.Haxton, T.Itahashi, K.Kubodera, K.Langanke, D.Leitner, M.Leitner, P.Vetter, L.Winslow, L.E.Marcucci, T.Motobayashi, A.Mukhamedzhanov, R.E.Tribble, F.M.Nunes, T.-S.Park, R.Schiavilla, E.C.Simpson, C.Spitaleri, F.Strieder, H.-P.Trautvetter, K.Suemmerer, S.Typel Solar fusion cross sections. II. The pp chain and CNO cycles NUCLEAR REACTIONS 2H(p, γ), 3He(3He, 2p), (α, γ), (p, e), 7Be, 12C, 14N, 15N, 17O(p, γ), 15N, 16,17,18O(p, α), E<3 MeV; analyzed and evaluated experimental data; deduced recommended values and uncertainties.
doi: 10.1103/RevModPhys.83.195
2011BA20 Phys.Rev.Lett. 106, 201104 (2011) P.Banerjee, W.C.Haxton, Y.-Z.Qian Long, Cold, Early r Process? Neutrino-Induced Nucleosynthesis in He Shells Revisited NUCLEAR REACTIONS 4He(ν, nν), 3He(n, p), 3H(t, 2n), 4He(ν, νp), E ∼ 30 keV; calculated r-process yields; deduced ν-driven r-process mechanism.
doi: 10.1103/PhysRevLett.106.201104
2009HA24 Nucl.Phys. A827, 42c (2009) Fundamental Symmetries and Conservation Laws
doi: 10.1016/j.nuclphysa.2009.05.017
2008HA06 Phys.Rev. C 77, 034005 (2008) Form of the effective interaction in harmonic-oscillator-based effective theory
doi: 10.1103/PhysRevC.77.034005
2007LI54 Phys.Rev. C 76, 035503 (2007) C.-P.Liu, M.J.Ramsey-Musolf, W.C.Haxton, R.G.E.Timmermans, A.E.L.Dieperink Atomic electric dipole moments: The Schiff theorem and its corrections
doi: 10.1103/PhysRevC.76.035503
2006AB11 Phys.Rev. C 73, 045805 (2006) J.N.Abdurashitov, V.N.Gavrin, S.V.Girin, V.V.Gorbachev, P.P.Gurkina, T.V.Ibragimova, A.V.Kalikhov, N.G.Khairnasov, T.V.Knodel, V.A.Matveev, I.N.Mirmov, A.A.Shikhin, E.P.Veretenkin, V.M.Vermul, V.E.Yants, G.T.Zatsepin, T.J.Bowles, S.R.Elliott, W.A.Teasdale, B.T.Cleveland, W.C.Haxton, J.F.Wilkerson, J.S.Nico, A.Suzuki, K.Lande, Yu.S.Khomyakov, V.M.Poplavsky, V.V.Popov, O.V.Mishin, A.N.Petrov, B.A.Vasiliev, S.A.Voronov, A.I.Karpenko, V.V.Maltsev, N.N.Oshkanov, A.M.Tuchkov, V.I.Barsanov, A.A.Janelidze, A.V.Korenkova, N.A.Kotelnikov, S.Yu.Markov, V.V.Selin, Z.N.Shakirov, A.A.Zamyatina, S.B.Zlokazov Measurement of the response of a Ga solar neutrino experiment to neutrinos from a 37Ar source NUCLEAR REACTIONS 71Ga(ν, e), E=spectrum; measured production rate using 37Ar neutrino source. Comparison with model predictions, implications for solar neutrino experiment discussed.
doi: 10.1103/PhysRevC.73.045805
2006GA38 Phys.Atomic Nuclei 69, 1820 (2006) V.N.Gavrin, J.N.Abdurashitov, V.I.Barsanov, T.J.Bowles, B.T.Cleveland, S.R.Elliott, S.V.Girin, V.V.Gorbachev, P.P.Gurkina, W.C.Haxton, T.V.Ibragimova, A.A.Janelidze, A.V.Kalikhov, N.A.Kotelnikov, K.Lande, V.V.Maltsev, S.Yu.Markov, V.A.Matveev, I.N.Mirmov, O.V.Mishin, J.S.Nico, N.N.Oshkanov, A.N.Petrov, V.M.Poplavsky, V.V.Popov, V.V.Selin, Z.N.Shakirov, A.A.Shikhin, A.Suzuki, W.A.Teasdale, A.M.Tuchkov, B.A.Vasiliev, E.P.Veretenkin, V.M.Vermul, S.A.Voronov, J.F.Wilkerson, V.E.Yants, A.A.Zamyatina, G.T.Zatsepin, S.B.Zlokazov Measurement of the Response of a Ga Solar Neutrino Experiment to 37Ar Source NUCLEAR REACTIONS 71Ga(ν, e), E=spectrum; measured production rate using 37Ar neutrino source. Comparison with model predictions, implications for solar neutrino experiment discussed.
doi: 10.1134/S1063778806110032
2006HA60 Nucl.Phys. A777, 226 (2006) W.C.Haxton, P.D.Parker, C.E.Rolfs Solar hydrogen burning and neutrinos NUCLEAR REACTIONS 3He(3He, 2p), E(cm)=10-1000 keV; 3He(α, γ), E(cm)<950 keV; 3He(d, p), (p, e+ν), E not given; 7Be(p, γ), E(cm)<425 keV; 14N(p, γ), E not given; analyzed astrophysical S-factor data, solar neutrino flux. Impact on pp chain and CN cycle.
doi: 10.1016/j.nuclphysa.2005.02.088
2005HA72 Phys.Rev. C 72, 065501 (2005) W.C.Haxton, K.M.Nollett, K.M.Zurek Piecewise moments method: Generalized Lanczos technique for nuclear response surfaces NUCLEAR STRUCTURE 28Si; calculated electromagnetic response functions. Generalized Lanczos technique.
doi: 10.1103/PhysRevC.72.065501
2005HE02 Phys.Lett. B 606, 258 (2005) A.Heger, E.Kolbe, W.C.Haxton, K.Langanke, G.Martinez-Pinedo, S.E.Woosley Neutrino nucleosynthesis
doi: 10.1016/j.physletb.2004.12.017
2004LU15 Phys.Rev. C 70, 014316 (2004) T.C.Luu, S.Bogner, W.C.Haxton, P.Navratil Effective interactions for the three-body problem NUCLEAR STRUCTURE 3H, 3He; calculated binding energies, contributions from three-body effective interactions.
doi: 10.1103/PhysRevC.70.014316
2002HA21 Phys.Rev. C65, 045502 (2002) W.C.Haxton, C.-P.Liu, M.J.Ramsey-Musolf Nuclear Anapole Moments NUCLEAR STRUCTURE 131In, 131,133Sn, 133Sb, 133Cs, 205,207Tl, 207,209Pb, 209Bi; calculated anapole moments; analyzed data; deduced constraints on parity-nonconserving coupling constants. Meson-exchange approach.
doi: 10.1103/PhysRevC.65.045502
2002HA40 Phys.Rev.Lett. 89, 182503 (2002) Perturbative Effective Theory in an Oscillator Basis?
doi: 10.1103/PhysRevLett.89.182503
2001HA33 Phys.Rev.Lett. 86, 5247 (2001) W.C.Haxton, C.-P.Liu, M.J.Ramsey-Musolf Anapole Moment and Other Constraints on the Strangeness Conserving Hadronic Weak Interaction NUCLEAR STRUCTURE 133Cs, 205Tl; calculated nuclear polarization contributions to anapole moments; deduced constraints on parity-nonconserving meson couplings.
doi: 10.1103/PhysRevLett.86.5247
2001HA43 Nucl.Phys. A690, 15c (2001) The Canonical Nuclear Many-Body Problem as an Effective Theory
doi: 10.1016/S0375-9474(01)00927-7
2001HA64 Ann.Rev.Nucl.Part.Sci. 51, 261 (2001) Atomic Parity Nonconservation and Nuclear Anapole Moments
doi: 10.1146/annurev.nucl.51.101701.132458
2000HA29 Phys.Rev.Lett. 84, 5484 (2000) Morphing the Shell Model into an Effective Theory NUCLEAR STRUCTURE 3He; calculated ground-state wave functions, body effective matrix elements. 2H, 3He; calculated form factors. Bloch-Horowitz equation.
doi: 10.1103/PhysRevLett.84.5484
1999HA01 Phys.Rev. C59, 515 (1999) Solar Neutrino Interactions with 18O in the SuperKamiokande Water Cerenkov Detector
doi: 10.1103/PhysRevC.59.515
1999HA47 Nucl.Phys. A654, 315c (1999) Fundamental Symmetries and Theory
doi: 10.1016/S0375-9474(99)00261-4
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
1998HA35 Phys.Lett. 431B, 110 (1998) Cross Section Uncertainties in the Gallium Neutrino Source Experiments NUCLEAR REACTIONS 71Ga(ν, e), E not given; calculated Ge excited state contribution to σ; deduced implications for solar neutrino detector calibration. Neutrinos from 51Cr source. Large-basis shell model calculations.
doi: 10.1016/S0370-2693(98)00581-4
1997HA16 Phys.Rev.Lett. 78, 2694 (1997) W.C.Haxton, K.Langanke, Y.-Z.Qian, P.Vogel Neutrino-Induced Nucleosynthesis and the Site of the r Process NUCLEAR STRUCTURE A=124-126; A=183-187; analyzed postprocessed abundance distributions. A ≈ 195; analyzed postprocessing neutron emission probabilities; deduced consistency with neutrino induced nucleosynthesis, strong argument for a supernova r-process site.
doi: 10.1103/PhysRevLett.78.2694
1997QI01 Phys.Rev. C55, 1532 (1997) Y.-Z.Qian, W.C.Haxton, K.Langanke, P.Vogel Neutrino-Induced Neutron Spallation and Supernova r-Process Nucleosynthesis NUCLEAR STRUCTURE A=76-195; calculated r-process associated ν(e) capture rates, average neutron number, multiple neutron probabilities.
doi: 10.1103/PhysRevC.55.1532
1996CU06 Phys.Rev.Lett. 77, 4286 (1996) 3He Transport in the Sun and the Solar Neutrino Problem
doi: 10.1103/PhysRevLett.77.4286
1996HA41 Nucl.Phys. B(Proc.Suppl.) S48, 317 (1996) Nuclear and Atomic Physics of the Solar Neutrino Problem
doi: 10.1016/0920-5632(96)00269-1
1996HA55 Phys.Rev.Lett. 76, 1562 (1996) Salty Water Cerenkov Detectors for Solar Neutrinos
doi: 10.1103/PhysRevLett.76.1562
1995ZH32 Phys.Rev. C52, 2488 (1995) D.C.Zheng, B.R.Barrett, J.P.Vary, W.C.Haxton, C.-L.Song Large-Basis Shell Model Studies of Light Nuclei with a Multivalued G-Matrix Effective Interaction NUCLEAR STRUCTURE 5,4He; calculated levels. 7,6Li; calculated levels, binding energy, μ, quadrupole moment, proton rms radii. Large basis shell model.
doi: 10.1103/PhysRevC.52.2488
1994HA08 Nucl.Phys. A570, 125c (1994) Solar Neutrino Oscillations
doi: 10.1016/0375-9474(94)90276-3
1993AD09 Phys.Lett. 314B, 185 (1993) E.G.Adelberger, L.De Braeckeleer, W.C.Haxton, K.A.Snover Accelerator Calibration of Solar Neutrino Detectors NUCLEAR REACTIONS 12C(p, n), E not given; calculated neutrino flux from 12N source.
doi: 10.1016/0370-2693(93)90447-P
1993HA48 Nucl.Phys. A553, 397c (1993) Nuclear Astrophysics
doi: 10.1016/0375-9474(93)90638-E
1992EN06 Phys.Rev. C46, R2153 (1992) Effective Summation Over Intermediate States in Double-Beta Decay RADIOACTIVITY 48Ca(β-); 48Ti(β+); calculated β-decay Gamow-Teller transition strength. 48Ca(2β-); calculated 2ν-accompained 2β-decay T1/2, Gamow-Teller matrix element.
doi: 10.1103/PhysRevC.46.R2153
1992YI01 Phys.Rev. C45, 1982 (1992) S.Ying, W.C.Haxton, E.M.Henley Charged- and Neutral-Current Solar-Neutrino Cross Sections for Heavy-Water Cherenkov Detectors NUCLEAR REACTIONS 2H(ν, X), E=3.25-160 MeV; calculated charged, neutral current σ. Bonn, Paris, Hamada-Johnson potentials.
doi: 10.1103/PhysRevC.45.1982
1991HA24 Phys.Rev.Lett. 67, 2431 (1991) Double-Beta-Decay Mass Constraints of 17-keV Neutrinos RADIOACTIVITY 76Ge, 128,130Te(2β); analyzed 2ν-, 0ν-decay T1/2 data; deduced 17 keV neutrinos mass constraints.
doi: 10.1103/PhysRevLett.67.2431
1990HA07 Nucl.Phys. A507, 179c (1990) Neutrino Nucleosynthesis in Supernovae: Shell model predictions NUCLEAR STRUCTURE 4He, 8Be, 12C, 14N, 16O, 20Ne, 24Mg, 28Si, 32S, 32S, 36Ar, 40Ca, 44Ti, 48Cr, 56,52Fe, 56Ni, 60Zn, 80Zr; calculated inclusive responses to supernova neutrinos.
doi: 10.1016/0375-9474(90)90577-9
1990HA35 Phys.Rev.Lett. 65, 1325 (1990) Weak-Interaction Rates in 16O NUCLEAR STRUCTURE 16O; calculated levels, B(λ), Gamow-Teller transition strength, weak interaction rates. Shell model.
doi: 10.1103/PhysRevLett.65.1325
1989BA95 Phys.Rev. D40, 931 (1989) Matter-Enchanced Neutrino Oscillations in the Standard Solar Model
doi: 10.1103/PhysRevD.40.931
1989HA11 Phys.Rev. C39, 2081 (1989) Reply to ' Comment on ' 37Ar as a Calibration Source for Solar Neutrino Detectors ' ' RADIOACTIVITY 37Ar(EC); analyzed internal bremsstrahlung yield implications.
doi: 10.1103/PhysRevC.39.2081
1989HA22 Phys.Rev.Lett. 63, 949 (1989) W.C.Haxton, E.M.Henley, M.J.Musolf Nucleon and Nuclear Anapole Moments NUCLEAR STRUCTURE 19F, 133Cs; calculated one-body, polarization, exchange-current contribution to the anapole matrix element. Shell model.
doi: 10.1103/PhysRevLett.63.949
1988AV02 Phys.Rev. D37, 618 (1988) F.T.Avignone III, C.Baktash, W.C.Barker, F.P.Calaprice, R.W.Dunford, W.C.Haxton, D.Kahana, R.T.Kouzes, H.S.Miley, D.M.Moltz Search for Axions from the 1115-keV Transition of 65Cu RADIOACTIVITY 65Zn(EC), (β+); measured γγ-coin; deduced axion search constraints.
doi: 10.1103/PhysRevD.37.618
1988HA05 Phys.Rev.Lett. 60, 768 (1988) Radiochemical Neutrino Detection via 127I(ν(e), e-)127Xe NUCLEAR REACTIONS 127I(ν, e-), E ≈ 664 keV; calculated 127Xe production rate; deduced neutrino detector sensitivity.
doi: 10.1103/PhysRevLett.60.768
1988HA22 Phys.Rev. C37, 2660 (1988) Neutrino Reactions on Oxygen and a Proposed Measurement of the Weinberg Angle NUCLEAR REACTIONS 16,17,18O(ν, e-), E=muon decay spectrum; calculated σ(θ); deduced θ(Weinberg) estimate feasibility.
doi: 10.1103/PhysRevC.37.2660
1988HA31 Can.J.Phys. 66, 503 (1988) Parity Nonconservation in the Nucleon-Nucleon System: Nuclear structure issues NUCLEAR STRUCTURE 14N, 18,19F, 21Ne; compiled, analyzed parity mixing features.
doi: 10.1139/p88-082
1988HA34 Phys.Rev. C38, 2474 (1988) 37Ar as a Calibration Source for Solar Neutrino Detectors NUCLEAR REACTIONS 36Ar(n, γ), E=thermal; analyzed capture σ data; deduced high intensity 37Ar neutrino source production possibility.
doi: 10.1103/PhysRevC.38.2474
1987AD05 Phys.Rev. C36, 879 (1987) 37Cl Solar Neutrino Capture Cross Section RADIOACTIVITY 37Ca(β+p); calculated β-delayed p-emission effects; deduced 37Cl solar neutrino detector consequences. 37K levels deduced β-delayed proton branching ratios, Gamow-Teller transition strength.
doi: 10.1103/PhysRevC.36.879
1985FR08 Phys.Rev. C31, 2027 (1985) Current Conservation and the Transverse Electric Multipole Field NUCLEAR REACTIONS 12C(e, e'), E not given; calculated longitudinal, transverse form factors.
doi: 10.1103/PhysRevC.31.2027
1984HA60 Prog.Part.Nucl.Phys. 12, 409 (1984) W.C.Haxton, G.J.Stephenson, Jr. Double beta decay
doi: 10.1016/0146-6410(84)90006-1
1983AD03 Phys.Rev. C27, 2833 (1983) E.G.Adelberger, M.M.Hindi, C.D.Hoyle, H.E.Swanson, R.D.Von Lintig, W.C.Haxton Beta Decays of 18Ne and 19Ne and Their Relation to Parity Mixing in 18F and 19F NUCLEAR STRUCTURE 18,19F, 19,21Ne, 21Na; calculated B(λ). 18,19Ne, 21Na; calculated Gamow-Teller transition strengths. Shell model. RADIOACTIVITY 18Ne(β+) [from O(3He, xn), E=12 MeV]; 19Ne(β+) [from 19F(p, n), E=6.4 MeV]; measured Eγ, Iγ; deduced ft. 18,19F levels deduced β-branching ratios, relative Iγ, parity mixing effects. Shell model. Natural O2, SF6 gas targets.
doi: 10.1103/PhysRevC.27.2833
1983GA09 Phys.Rev. C28, 294 (1983) M.M.Gazzaly, N.M.Hintz, M.A.Franey, J.Dubach, W.C.Haxton Neutron and Proton Transition Matrix Elements for 90Zr from a Microscopic Analysis of 0.8 GeV Proton Inelastic Scattering NUCLEAR REACTIONS 90Zr(p, p'), E=0.8 GeV; measured absolute σ(θ). 90Zr levels deduced core to total deformation parameter ratio, enhancement factors, neutron, proton matrix element ratios. DWIA, shell model transition densities.
doi: 10.1103/PhysRevC.28.294
1983HA13 Phys.Rev. C28, 458 (1983) W.C.Haxton, G.J.Stephenson, Jr. Comment on ' Nilsson-Pairing Model for Double Beta Decay ' RADIOACTIVITY 76Ge(β-β-); calculated double β-decay Gamow-Teller matrix element. Nilsson pairing model.
doi: 10.1103/PhysRevC.28.458
1983HA14 Phys.Rev. C28, 467 (1983) W.C.Haxton, G.A.Cowan, M.Goldhaber Radiochemical Tests of Double Beta Decay RADIOACTIVITY 238U, 232Th(β-β-); calculated double β-decay Gamow-Teller matrix element, T1/2 esimates. Nilsson pairing model.
doi: 10.1103/PhysRevC.28.467
1981HA06 Phys.Rev.Lett. 46, 698 (1981) Parity Nonconservation in 18F and Meson-Exchange Contributions to the Axial Charge Operator RADIOACTIVITY 18Ne; calculated β+-decay rate. 18F deduced strength of parity-nonconserving effects. Meson exchange contributions to axial charge operator.
doi: 10.1103/PhysRevLett.46.698
1981HA21 Phys.Rev.Lett. 47, 153 (1981) W.C.Haxton, G.J.Stephenson, Jr., D.Strottman Double Beta Decay and the Majorana Mass of the Electron Neutrino RADIOACTIVITY 76Ge, 82Se; calculated double β-decay T1/2; deduced ν(e) Majorana mass constraint. Two-neutrino, neutrinoless decay mechanisms.
doi: 10.1103/PhysRevLett.47.153
1981HA35 Nucl.Phys. A367, 517 (1981) The Solar Neutrino Capture Cross Section for 81Br NUCLEAR REACTIONS 81Br(ν, e), E at rest; calculated σ; deduced Gamow-Teller transition dominance. Solar neutrino, weak interaction models.
doi: 10.1016/0375-9474(81)90663-1
1981SE05 Phys.Rev. C23, 1293 (1981) R.M.Sealock, H.S.Caplan, G.J.Lolos, W.C.Haxton Low Energy Angular Distributions for the 12C(e, π+e') Reaction NUCLEAR REACTIONS 12C(e, π+e'), E=200 MeV; measured σ(E(π), θ). DWBA calculations.
doi: 10.1103/PhysRevC.23.1293
1980HA18 Phys.Lett. 92B, 37 (1980) Pion Production and the Optical Potential NUCLEAR REACTIONS 12C(γ, π+), E not given; 12C(π+, π+), E=38.9, 50 MeV; 12C(e, e'), E not given; calculated σ(θ). Optical model analysis.
doi: 10.1016/0370-2693(80)90298-1
1980HA41 Phys.Rev.Lett. 45, 1677 (1980) W.C.Haxton, B.F.Gibson, E.M.Henley Parity Nonconservation in 18F, 19F, and 21Ne NUCLEAR STRUCTURE 18,19F, 21Ne; calculated γ-circular polarization, γ-asymmetry; deduced parity nonconserving interaction matrix elements. Weinberg-Salam model.
doi: 10.1103/PhysRevLett.45.1677
1979DO16 At.Data Nucl.Data Tables 23, 103 (1979) Multipole Operators in Semileptonic Weak and Electromagnetic Interactions with Nuclei: Harmonic Oscillator Single-Particle Matrix Elements NUCLEAR REACTIONS 27Al(e, e), E not given; calculated M1, M3, M5 contributions to transverse form factor; derived multipole operators for semileptonic weak, electromagnetic interactions with nuclei. Harmonic oscillator basis.
doi: 10.1016/0092-640X(79)90003-2
1979FL08 Phys.Rev.Lett. 43, 1922 (1979) J.B.Flanz, R.S.Hicks, R.A.Lindgren, G.A.Peterson, J.Dubach, W.C.Haxton Electron Scattering, Isospin Mixing, and the Structure of the 12.71- and 15.11-MeV Levels in 12C NUCLEAR REACTIONS 12C(e, e'), E not given; measured form factors at θ=180°; deduced charge-dependent isospin-mixing matrix element. 12C levels deduced isospin mixing, structure.
doi: 10.1103/PhysRevLett.43.1922
1978DU12 Phys.Rev.Lett. 41, 1453 (1978) Nuclear Structure and (e, e') Reactions: The Significance of High-Momentum-Transfer Data and Meson-Exchange Currents NUCLEAR STRUCTURE 12C; calculated inelastic electron scattering form factor.
doi: 10.1103/PhysRevLett.41.1453
1978HA34 Phys.Lett. 76B, 165 (1978) Threshold Pion Photoproduction in 12C and the 15.11 MeV M1 Form Factor NUCLEAR REACTIONS 12C(γ, π-); calculated σ.
doi: 10.1016/0370-2693(78)90266-6
1978HA36 Nucl.Phys. A306, 429 (1978) Threshold Pion Electroproduction and the Nuclear Response Surface NUCLEAR REACTIONS 12C, 16O(e, π), E=280 MeV; calculated σ.
doi: 10.1016/0375-9474(78)90473-6
1977DO12 Nucl.Phys. A287, 506 (1977) Neutrino Reactions in the Mass-37 System NUCLEAR REACTIONS 37Cl(ν, e); calculated total σ for solar neutrino capture. 37Cl, 37Ar, 37K, 37Ca; calculated levels.
doi: 10.1016/0375-9474(77)90060-4
1975DO10 Nucl.Phys. A251, 353 (1975) T.W.Donnelly, J.Dubach, W.C.Haxton Semi-Leptonic Weak and Electromagnetic Interactions in the Goldhaber-Teller Model NUCLEAR STRUCTURE 12C, 16O; T=1 giant resonances calculated β+, β- decay rates. NUCLEAR REACTIONS 16O(e, e); calculated form factors. 16O(ν, e), (ν-bar, e+), E=250 MeV; 40Ca(ν, e), (ν-bar, e+), E=500 MeV; calculated σ. 12C, 16O, 28Si, 40Ca(μ-, X); calculated muon capture rates.
doi: 10.1016/0375-9474(75)90535-7
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