NSR Query Results
Output year order : Descending NSR database version of April 24, 2024. Search: Author = W.R.Hix Found 44 matches. 2023JA13 Astrophys.J. 955, 51 (2023) R.Jain, E.F.Brown, H.Schatz, A.V.Afanasjev, M.Beard, L.R.Gasques, S.S.Gupta, G.W.Hitt, W.R.Hix, R.Lau, P.Moller, W.J.Ong, M.Wiescher, Y.Xu Impact of Pycnonuclear Fusion Uncertainties on the Cooling of Accreting Neutron Star Crusts NUCLEAR REACTIONS 40Mg(40Mg, X)80Cr, 44Mg(40Mg, X)84Cr, 44Mg(44Mg, X)88Cr, 44Mg(38Ne, X)82Ti, 40Mg(38Ne, X)78Ti, 32Ne(32Ne, X)64Ca, 32Ne(30Ne, X)62Ca, 30Ne(30Ne, X)60Ca, 40Mg(24O, X), E not given; calculated abundances, pycnonuclear fusion rates using the reaction network with the thermal evolution code dStar. 56Fe; deduced impact of uncertainties on the depth at which nuclear heat is deposited although the total heating remains constant.
doi: 10.3847/1538-4357/acebc4
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
2022SI17 Phys.Rev. C 106, 015803 (2022) A.Sieverding, J.S.Randhawa, D.Zetterberg, R.J.deBoer, T.Ahn, R.Mancino, G.Martinez-Pinedo, W.R.Hix Role of low-lying resonances for the 10Be(p, α)7Li reaction rate and implications for the formation of the Solar System NUCLEAR REACTIONS 10Be(p, α), (α, n), E not given; 10Be(ν, e-), E=2.8-10 MeV; analyzed reaction rates, σ; deduced influence on the content of 10Be in supernovae environment. 10Be(p, α), E<1.5 MeV; analyzed reaction rate, experimental data on resonance in 11B at 193 keV, ; deduced reaction rate, astrophysical S-factor. Showed that, with the new reaction rate, a low-mass corecollapse supernovae is unlikely to produce enough 10Be to explain the observed 10Be/9Be ratio in meteorites. Comparison to data from JINA-REACLIB.
doi: 10.1103/PhysRevC.106.015803
2020CH35 Phys.Rev. C 102, 035806 (2020) K.A.Chipps, P.Adsley, M.Couder, W.R.Hix, Z.Meisel, K.Schmidt Evaluation of experimental constraints on the 44Ti(α, p)47V reaction cross section relevant for supernovae NUCLEAR REACTIONS 44Ti(α, p)47V, E(cm)=4-11 MeV; calculated σ(E) using TALYS with eight alpha optical models, and compared with experimental data, and other theoretical calculations; deduced χ2 fits. 44Ti(α, p)47V, T9=2.0-10.05; evaluated recommended astrophysical reaction rates based on fits and evaluation of the experimental data and theoretical calculations. Relevance to the understanding of observational 44Ti afterglow in core collapse supernovae.
doi: 10.1103/PhysRevC.102.035806
2018LA06 Astrophys.J. 859, 62 (2018) R.Lau, M.Beard, S.S.Gupta, H.Schatz, A.V.Afanasjev, E.F.Brown, A.Deibel, L.R.Gasques, G.W.Hitt, W.R.Hix, L.Keek, P.Moller, P.S.Shternin, A.W.Steiner, M.Wiescher, Y.Xu Nuclear Reactions in the Crusts of Accreting Neutron Stars
doi: 10.3847/1538-4357/aabfe0
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
2016HI10 Acta Phys.Pol. B47, 645 (2016) W.R.Hix, E.J.Lentz, S.W.Bruenn, A.Mezzacappa, O.E.B.Messer, E.Endeve, J.M.Blondin, J.A.Harris, P.Marronetti, K.N.Yakunin The Multi-dimensional Character of Core-collapse Supernovae
doi: 10.5506/APhysPolB.47.645
2014SC01 Nature(London) 505, 62 (2014) H.Schatz, S.Gupta, P.Moller, M.Beard, E.F.Brown, A.T.Deibel, L.R.Gasques, W.R.Hix, L.Keek, R.Lau, A.W.Steiner, M.Wiescher Strong neutrino cooling by cycles of electron capture and β- decay in neutron star crusts NUCLEAR STRUCTURE 105Zr; calculated single-particle energy levels, J, π, hexadecapole deformation parameters.
doi: 10.1038/nature12757
2012KO36 Phys.Rev.Lett. 109, 172501 (2012) R.L.Kozub, G.Arbanas, A.S.Adekola, D.W.Bardayan, J.C.Blackmon, K.Y.Chae, K.A.Chipps, J.A.Cizewski, L.Erikson, R.Hatarik, W.R.Hix, K.L.Jones, W.Krolas, J.F.Liang, Z.Ma, C.Matei, B.H.Moazen, C.D.Nesaraja, S.D.Pain, D.Shapira, J.F.Shriner, Jr., M.S.Smith, T.P.Swan Neutron Single Particle Structure in 131Sn and Direct Neutron Capture Cross Sections NUCLEAR REACTIONS 2H(130Sn, p), E=630 MeV; 130Sn(n, γ), E<5 MeV;measured reaction products, Ep, Ip; deduced σ(θ), energy levels, J, π, properties of single-particle states, direct-semidirect σ. Comparison with available data.
doi: 10.1103/PhysRevLett.109.172501
2011ES06 Phys.Rev.Lett. 107, 172503 (2011) A.Estrade, M.Matos, H.Schatz, A.M.Amthor, D.Bazin, M.Beard, A.Becerril, E.F.Brown, R.Cyburt, T.Elliot, A.Gade, D.Galaviz, S.George, S.S.Gupta, W.R.Hix, R.Lau, G.Lorusso, P.Moller, J.Pereira, M.Portillo, A.M.Rogers, D.Shapira, E.Smith, A.Stolz, M.Wallace, M.Wiescher Time-of-Flight Mass Measurements for Nuclear Processes in Neutron Star Crusts ATOMIC MASSES 53,54,55Sc, 57Ti, 60,61V, 63Cr, 65,66Mn, 67,68Fe, 68,69,70,71Co, 74Ni; measured time of flight; deduced masses. Stellar nucleosynthesis implications.
doi: 10.1103/PhysRevLett.107.172503
2010HI05 Nucl.Phys. A834, 602c (2010) W.R.Hix, E.J.Lentz, M.Baird, O.E.B.Messer, A.Mezzacappa, C.-T.Lee, S.W.Bruenn, J.M.Blondin, P.Marronetti Understanding Core-Collapse Supernovae
doi: 10.1016/j.nuclphysa.2010.01.104
2010JU04 Nucl.Phys. A848, 454 (2010) A.Juodagalvis, K.Langanke, W.R.Hix, G.Martinez-Pinedo, J.M.Sampaio Improved estimate of electron capture rates on nuclei during stellar core collapse
doi: 10.1016/j.nuclphysa.2010.09.012
2010PE18 J.Phys.:Conf.Ser. 202, 012008 (2010) I.Petermann, G.Martinez-Pinedo, A.Arcones, W.R.Hix, A.Kelic, K.Langanke, I.Panov, T.Rauscher, K.-H.Schmidt, F.-K.Thielemann, N.Zinner Network calculations for r-process nucleosynthesis
doi: 10.1088/1742-6596/202/1/012008
2009BE01 J.Phys.(London) G36, 025201 (2009) J.Beun, J.C.Blackmon, W.R.Hix, G.C.McLaughlin, M.S.Smith, R.Surman Neutron capture on 130Sn during r-process freeze-out
doi: 10.1088/0954-3899/36/2/025201
2009SU07 Phys.Rev. C 79, 045809 (2009) R.Surman, J.Beun, G.C.McLaughlin, W.R.Hix Neutron capture rates near A=130 that effect a global change to the r-process abundance distribution NUCLEAR REACTIONS Sn, In, Cd(n, γ); calculated σ for A=105-155, neutron capture rates, separation energies. Implications for r-process model.
doi: 10.1103/PhysRevC.79.045809
2008BE07 Phys.Rev. C 77, 035804 (2008) J.Beun, G.C.McLaughlin, R.Surman, W.R.Hix Fission cycling in a supernova r process
doi: 10.1103/PhysRevC.77.035804
2008JU03 J.Phys.(London) G35, 014031 (2008) A.Juodagalvis, J.M.Sampaio, K.Langanke, W.R.Hix Extended pool of electron-capture rates for core-collapse supernovae simulations
doi: 10.1088/0954-3899/35/1/014031
2008SU04 J.Phys.(London) G35, 014059 (2008) R.Surman, J.Beun, G.C.McLaughlin, S.Kane, W.R.Hix The role of neutrinos in r-process nucleosynthesis in supernovae and gamma-ray bursts
doi: 10.1088/0954-3899/35/1/014059
2007BA69 Phys.Rev. C 76, 045803 (2007) D.W.Bardayan, J.C.Blackmon, R.P.Fitzgerald, W.R.Hix, K.L.Jones, R.L.Kozub, J.F.Liang, R.J.Livesay, Z.Ma, L.F.Roberts, M.S.Smith, J.S.Thomas, D.W.Visser 30S studied with the 32S(p, t)30S reaction and the 29P(p, γ)30S reaction rate NUCLEAR REACTIONS 32S(p, t), E=37 MeV; measured triton energies, angular distributions. 30S deduced levels, J, π. 29P(p, γ)30S; deduced reaction rates of astrophysical significance.
doi: 10.1103/PhysRevC.76.045803
2007MA48 Phys.Rev. C 76, 015803 (2007); Erratum Phys.Rev. C 76, 039901 (2007) Z.Ma, D.W.Bardayan, J.C.Blackmon, R.P.Fitzgerald, M.W.Guidry, W.R.Hix, K.L.Jones, R.L.Kozub, R.J.Livesay, M.S.Smith, J.S.Thomas, D.W.Visser Astrophysically important 31S states studied with the 32S(p, d)31S reaction NUCLEAR REACTIONS 32S(p, d), E=32 MeV; measured Ed, σ and angular distributions. 31S deduced level energies and spectroscopic factors.
doi: 10.1103/PhysRevC.76.015803
2007MO20 Phys.Rev. C 75, 065801 (2007) B.H.Moazen, D.W.Bardayan, J.C.Blackmon, K.Y.Chae, K.Chipps, C.P.Domizioli, R.Fitzgerald, U.Greife, W.R.Hix, K.L.Jones, R.L.Kozub, E.J.Lingerfelt, R.J.Livesay, C.D.Nesaraja, S.D.Pain, L.F.Roberts, J.F.Shriner, Jr., M.S.Smith, J.S.Thomas Measurement of the 183 keV resonance in 17O(p, α)14N using a novel technique NUCLEAR REACTIONS 1H(17O, α)14N, E=3.3 MeV; measured resonance energy and strength. Discussed astrophysical implications.
doi: 10.1103/PhysRevC.75.065801
2007TH05 Prog.Part.Nucl.Phys. 59, 74 (2007) F.-K.Thielemann, C.Frohlich, R.Hirschi, M.Liebendorfer, I.Dillmann, D.Mocelj, T.Rauscher, G.Martinez-Pinedo, K.Langanke, K.Farouqi, K.-L.Kratz, B.Pfeiffer, I.Panov, D.K.Nadyozhin, S.Blinnikov, E.Bravo, W.R.Hix, P.Hoflich, N.T.Zinner Production of intermediate-mass and heavy nuclei
doi: 10.1016/j.ppnp.2006.12.019
2006BA65 Phys.Rev. C 74, 045804 (2006) D.W.Bardayan, J.A.Howard, J.C.Blackmon, C.R.Brune, K.Y.Chae, W.R.Hix, M.S.Johnson, K.L.Jones, R.L.Kozub, J.F.Liang, E.J.Lingerfelt, R.J.Livesay, S.D.Pain, J.P.Scott, M.S.Smith, J.S.Thomas, D.W.Visser Astrophysically important 26Si states studied with the 28Si(p, t)26Si reaction. II. Spin of the 5.914-MeV 26Si level and galactic 26Al production NUCLEAR REACTIONS 28Si(p, t), (p, d), E=40 MeV; measured particle spectra, angular distributions. 26Si level deduced J, π. 25Al(p, γ), E=low; deduced astrophysical reaction rate.
doi: 10.1103/PhysRevC.74.045804
2006FR05 Phys.Rev.Lett. 96, 142502 (2006) C.Frohlich, G.Martinez-Pinedo, M.Liebendorfer, F.-K.Thielemann, E.Bravo, W.R.Hix, K.Langanke, N.T.Zinner Neutrino-Induced Nucleosynthesis of A > 64 Nuclei: The νp Process
doi: 10.1103/PhysRevLett.96.142502
2006HI17 Nucl.Phys. A777, 188 (2006) Thermonuclear kinetics in astrophysics
doi: 10.1016/j.nuclphysa.2004.10.009
2005FR25 Nucl.Phys. A758, 27c (2005) C.Frohlich, P.Hauser, M.Liebendorfer, G.Martinez-Pinedo, E.Bravo, W.R.Hix, N.T.Zinner, F.-K.Thielemann The Innermost Ejecta of Core Collapse Supernovae
doi: 10.1016/j.nuclphysa.2005.05.009
2005HI18 Nucl.Phys. A758, 31c (2005) W.R.Hix, O.E.B.Messer, A.Mezzacappa, J.Sampaio, K.Langanke, G.Martinez-Pinedo, M.Liebendorfer, D.J.Dean Nuclear electron capture in core collapse supernovae
doi: 10.1016/j.nuclphysa.2005.05.010
2005JU02 Nucl.Phys. A747, 87 (2005) A.Juodagalvis, K.Langanke, G.Martinez-Pinedo, W.R.Hix, D.J.Dean, J.M.Sampaio Neutral-current neutrino-nucleus cross sections for A ∼ 50-65 nuclei NUCLEAR REACTIONS 50,51,52,53,54,55,56,57,58,59,60Mn, 52,53,54,55,56,57,58,59,60,61Fe, 54,55,56,57,58,59,60,61,62,63Co, 56,57,58,59,60,61,62,63,64Ni(ν, ν'), E=0-50 MeV; calculated neutral-current inelastic σ, neutrino spectra. NUCLEAR STRUCTURE 50,51,52,53,54,55,56,57,58,59,60Mn, 52,53,54,55,56,57,58,59,60,61Fe, 54,55,56,57,58,59,60,61,62,63Co, 56,57,58,59,60,61,62,63,64Ni; calculated Gamow-Teller strength distributions.
doi: 10.1016/j.nuclphysa.2004.09.005
2005LE30 Nucl.Phys. A758, 84c (2005) R.Lewis, J.Caggiano, A.Parikh, C.Deibel, D.Visser, K.Fear, P.Parker, W.R.Hix 26Alg, m + p resonances studied via proton decays of 27Si NUCLEAR REACTIONS 27Al(3He, t), E=25 MeV; measured Ep following residual nucleus decay to ground and metastable states. 27Si deduced resonance energy. Astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2005.05.166
2005NE12 Nucl.Phys. A758, 174c (2005) C.D.Nesaraja, E.L.Lingerfelt, J.P.Scott, M.S.Smith, W.R.Hix, D.W.Bardayan, J.C.Blackmon, K.Chae, M.W.Guidry, R.A.Meyer A New Computational Infrastructure For Nuclear Astrophysics
doi: 10.1016/j.nuclphysa.2005.05.173
2005ST25 Nucl.Phys. A758, 455c (2005) S.Starrfield, W.R.Hix, F.X.Timmes, E.M.Sion, W.M.Sparks, S.J.Dwyer Studies of Accretion onto Hot, Massive White Dwarfs: The Growth to the Chandrasekhar Limit?
doi: 10.1016/j.nuclphysa.2005.05.084
2004SM08 Nucl.Phys. A746, 565c (2004) M.S.Smith, W.R.Hix, S.Parete-Koon, L.Dessieux, Z.Ma, S.Starrfield, D.W.Bardayan, M.W.Guidry, D.L.Smith, J.C.Blackmon, A.Mezzacappa Element synthesis calculations for stellar explosions: robust uncertainties, sensitivities, and radioactive ion beam measurements
doi: 10.1016/j.nuclphysa.2004.09.091
2004SM09 Nucl.Phys. A746, 569c (2004) M.S.Smith, R.A.Meyer, D.W.Bardayan, J.C.Blackmon, K.Chae, M.W.Guidry, W.R.Hix, R.L.Kozub, E.J.Lingerfelt, Z.Ma, J.P.Scott Nuclear data on unstable nuclei for astrophysics
doi: 10.1016/j.nuclphysa.2004.09.092
2003BA86 Nucl.Phys. A718, 590c (2003) D.W.Bardayan, J.C.Batchelder, J.C.Blackmon, A.E.Champagne, T.Davinson, R.Fitzgerald, W.R.Hix, C.Iliadis, R.L.Kozub, Z.Ma, S.Parete-Koon, P.D.Parker, N.Shu, M.S.Smith, P.J.Woods Measurement of the 18F(p, α)15O Cross Section at Nova Energies NUCLEAR REACTIONS 1H(18F, α), E(cm) ≈ 0.3-0.8 MeV; measured σ; deduced resonance parameters. 18F(p, α), E(cm) ≈ 0.2-1.0 MeV; deduced σ.
doi: 10.1016/S0375-9474(03)00873-X
2003BL11 Nucl.Phys. A718, 127c (2003) J.C.Blackmon, D.W.Bardayan, W.Bradfield-Smith, R.Brummitt, A.E.Champagne, A.A.Chen, T.Davinson, L.Dessieux, M.W.Guidry, K.I.Hahn, G.M.Hale, W.R.Hix, R.L.Kozub, Z.Ma, P.D.Parker, G.Rajbaidya, R.C.Runkle, C.M.Rowland, A.C.Shotter, M.S.Smith, L.A.Van Wormer, D.W.Visser, P.J.Woods The 14O(α, p)17F Reaction Rate NUCLEAR REACTIONS 1H(17F, 17F), (17F, 17F'), (17F, 14O), E(cm) ≈ 1-4 MeV; measured particle spectra. 17F(p, p'), E(cm)=2-2.5 MeV; deduced σ. 14O(α, p), E=low; deduced astrophysical reaction rate. R-matrix analysis.
doi: 10.1016/S0375-9474(03)00689-4
2003FI11 Nucl.Phys. A718, 614c (2003) J.L.Fisker, W.R.Hix, M.Liebendorfer, F.-K.Thielemann The transition to stable burning on an accreting neutron star
doi: 10.1016/S0375-9474(03)00902-3
2003HI14 Nucl.Phys. A718, 620c (2003) W.R.Hix, M.S.Smith, S.Starrfield, A.Mezzacappa, D.L.Smith Impact of Nuclear Reaction Rate Uncertainties on Nova Models
doi: 10.1016/S0375-9474(03)00904-7
2003LI43 Nucl.Phys. A719, 144c (2003) M.Liebendorfer, A.Mezzacappa, O.E.B.Messer, G.Martinez-Pinedo, W.R.Hix, F.-K.Thielemann The neutrino signal in stellar core collapse and postbounce evolution
doi: 10.1016/S0375-9474(03)00984-9
2003ME17 Nucl.Phys. A718, 449c (2003) O.E.B.Messer, W.R.Hix, M.Liebendorfer, A.Mezzacappa Electron capture and shock formation in core-collapse supernovae
doi: 10.1016/S0375-9474(03)00846-7
2003PA54 Astrophys.J. 598, 1239 (2003) S.Parete-Koon, W.R.Hix, M.S.Smith, S.Starrfield, D.W.Bardayan, M.W.Guidry, A.Mezzacappa A new 17F(p, γ)18Ne reaction rate and its implications for nova nucleosynthesis NUCLEAR REACTIONS 17F(p, γ), E=low; analyzed data; deduced reaction rates, implications for nucleosynthesis in novae.
doi: 10.1086/378979
2003TH05 Nucl.Phys. A718, 139c (2003) F.-K.Thielemann, D.Argast, F.Brachwitz, W.R.Hix, P.Hoflich, M.Liebendorfer, G.Martinez-Pinedo, A.Mezzacappa, I.Panov, T.Rauscher Nuclear cross sections, nuclear structure and stellar nucleosynthesis
doi: 10.1016/S0375-9474(03)00704-8
2002BB02 Phys.Rev.Lett. 89, 262501 (2002) D.W.Bardayan, J.C.Batchelder, J.C.Blackmon, A.E.Champagne, T.Davinson, R.Fitzgerald, W.R.Hix, C.Iliadis, R.L.Kozub, Z.Ma, S.Parete-Koon, P.D.Parker, N.Shu, M.S.Smith, P.J.Woods Strength of the 18F(p, α)15O Resonance at Ec.m.=330 keV NUCLEAR REACTIONS 1H(18F, α), E(cm)=330 keV; measured Eα, Iα(θ), σ; deduced resonance parameters. 18F(p, α), E=astrophysical; calculated reaction rates.
doi: 10.1103/PhysRevLett.89.262501
2001NA37 Astrophys.J. 555, 880 (2001) T.Nakamura, H.Umeda, K.Iwamoto, K.Nomoto, M.-A.Hashimoto, W.R.Hix, F.-K.Thielemann Explosive Nucleosynthesis in Hypernovae
doi: 10.1086/321495
2001TH08 Prog.Part.Nucl.Phys. 46, 5 (2001) F.-K.Thielemann, F.Brachwitz, C.Freiburghaus, E.Kolbe, G.Martinez-Pinedo, T.Rauscher, F.Rembges, W.R.Hix, M.Liebendorfer, A.Mezzacappa, K.-L.Kratz, B.Pfeiffer, K.Langanke, K.Nomoto, S.Rosswog, H.Schatz, M.Wiescher Element Synthesis in Stars
doi: 10.1016/S0146-6410(01)00103-X
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