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Search: Author = W.Haxton

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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
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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
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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
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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
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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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2020GA34      J.Phys.(London) G47, 045108 (2020)

J.Galan, X.Chen, H.Du, C.Fu, K.Giboni, F.Giuliani, K.Han, B.Jiang, X.Ji, H.Lin, Y.Lin, J.Liu, K.Ni, X.Ren, S.Wang, S.Wu, C.Xie, Y.Yang, T.Zhang, L.Zhao, S.Aune, Y.Bedfer, E.Berthoumieux, D.Calvet, N.d'Hose, E.Ferrer-Ribas, F.Kunne, B.Manier, D.Neyret, T.Papaevangelou, L.Chen, S.Hu, P.Li, X.Li, H.Zhang, M.Zhao, J.Zhou, Y.Mao, H.Qiao, S.Wang, Y.Yuan, M.Wang, Y.Chen, A.N.Khan, J.Tang, W.Wang, H.Chen, C.Feng, J.Liu, S.Liu, X.Wang, D.Zhu, J.F.Castel, S.Cebrian, T.Dafni, I.G.Irastorza, G.Luzon, H.Mirallas, X.Sun, A.Tan, W.Haxton, Y.Mei, C.Kobdaj, Y.Yan

Topological background discrimination in the PandaX-III neutrinoless double beta decay experiment

doi: 10.1088/1361-6471/ab4dbe
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2015BE02      Phys.Lett. B 741, 128 (2015)

J.Beller, C.Stumpf, M.Scheck, N.Pietralla, D.Deleanu, D.M.Filipescu, T.Glodariu, W.Haxton, A.Idini, J.H.Kelley, E.Kwan, G.Martinez-Pinedo, R.Raut, C.Romig, R.Roth, G.Rusev, D.Savran, A.P.Tonchev, W.Tornow, J.Wagner, H.R.Weller, N.-V.Zamfir, M.Zweidinger

Separation of the 1+/1- parity doublet in 20Ne

NUCLEAR REACTIONS 20Ne, 28Si(polarized γ, γ'), E=11.26 MeV; measured reaction products, Eγ, Iγ; deduced the energy difference of the parity doublet, the ratio of their integrated σ. Comparison with shell model calculations.

doi: 10.1016/j.physletb.2014.12.018
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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
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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
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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
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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
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2009HA24      Nucl.Phys. A827, 42c (2009)


Fundamental Symmetries and Conservation Laws

doi: 10.1016/j.nuclphysa.2009.05.017
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2008HA06      Phys.Rev. C 77, 034005 (2008)


Form of the effective interaction in harmonic-oscillator-based effective theory

doi: 10.1103/PhysRevC.77.034005
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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
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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
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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
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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
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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
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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
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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
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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
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2002HA40      Phys.Rev.Lett. 89, 182503 (2002)

W.C.Haxton, T.Luu

Perturbative Effective Theory in an Oscillator Basis?

doi: 10.1103/PhysRevLett.89.182503
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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
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2001HA43      Nucl.Phys. A690, 15c (2001)

W.C.Haxton, T.Luu

The Canonical Nuclear Many-Body Problem as an Effective Theory

doi: 10.1016/S0375-9474(01)00927-7
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2001HA64      Ann.Rev.Nucl.Part.Sci. 51, 261 (2001)

W.C.Haxton, C.E.Wieman

Atomic Parity Nonconservation and Nuclear Anapole Moments

doi: 10.1146/annurev.nucl.51.101701.132458
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2000HA29      Phys.Rev.Lett. 84, 5484 (2000)

W.C.Haxton, C.-L.Song

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
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1999HA01      Phys.Rev. C59, 515 (1999)

W.C.Haxton, R.G.H.Robertson

Solar Neutrino Interactions with 18O in the SuperKamiokande Water Cerenkov Detector

doi: 10.1103/PhysRevC.59.515
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1999HA47      Nucl.Phys. A654, 315c (1999)


Fundamental Symmetries and Theory

doi: 10.1016/S0375-9474(99)00261-4
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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
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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
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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
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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
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1996CU06      Phys.Rev.Lett. 77, 4286 (1996)

A.Cumming, W.C.Haxton

3He Transport in the Sun and the Solar Neutrino Problem

doi: 10.1103/PhysRevLett.77.4286
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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
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1996HA55      Phys.Rev.Lett. 76, 1562 (1996)


Salty Water Cerenkov Detectors for Solar Neutrinos

doi: 10.1103/PhysRevLett.76.1562
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1995HA33      Phys.Lett. 353B, 422 (1995)

N.Hata, W.Haxton

Implications of the GALLEX Source Experiment for the Solar Neutron Problem

NUCLEAR STRUCTURE 13,14C, 14N, 17,18O, 19F, 26Mg, 32S, 39K, 71Ga; compiled, reviewed Gamow-Teller transition strength data, estimates; deduced implications to σ for 71Ga(ν, γ), ν from 51Cr, 7Be.

doi: 10.1016/0370-2693(95)00598-F
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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
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1994HA08      Nucl.Phys. A570, 125c (1994)


Solar Neutrino Oscillations

doi: 10.1016/0375-9474(94)90276-3
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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
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1993HA48      Nucl.Phys. A553, 397c (1993)


Nuclear Astrophysics

doi: 10.1016/0375-9474(93)90638-E
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1992EN06      Phys.Rev. C46, R2153 (1992)

J.Engel, W.C.Haxton, P.Vogel

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
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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
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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
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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
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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
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1989BA95      Phys.Rev. D40, 931 (1989)

J.N.Bahcall, W.C.Haxton

Matter-Enchanced Neutrino Oscillations in the Standard Solar Model

doi: 10.1103/PhysRevD.40.931
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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
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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
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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
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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
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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
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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
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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
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1987AD05      Phys.Rev. C36, 879 (1987)

E.G.Adelberger, W.C.Haxton

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
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1985FR08      Phys.Rev. C31, 2027 (1985)

J.L.Friar, W.C.Haxton

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
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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
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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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1294.

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
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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
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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
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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
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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
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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
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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
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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
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1979DO16      At.Data Nucl.Data Tables 23, 103 (1979)

T.W.Donnelly, W.C.Haxton

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
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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
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1978DU12      Phys.Rev.Lett. 41, 1453 (1978)

J.Dubach, W.C.Haxton

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
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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
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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
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1977BO05      Phys.Rev.Lett. 38, 742 (1977)

F.Borkowski, C.Schmitt, G.G.Simon, V.Walther, D.Drechsel, W.Haxton, R.Rosenfelder

Threshold Electroproduction of Charged Pions from Light Nuclei

NUCLEAR REACTIONS 12C, Be, 16O(e, π-), (e, π+), E=280 MeV; measured σ.

doi: 10.1103/PhysRevLett.38.742
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1977DO12      Nucl.Phys. A287, 506 (1977)

T.W.Donnelly, W.C.Haxton

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
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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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Note: The following list of authors and aliases matches the search parameter W.Haxton: , W.C.HAXTON