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NSR database version of May 24, 2024.

Search: Author = W.R.Hix

Found 44 matches.

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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
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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
Citations: PlumX Metrics


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1953. Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics


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
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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
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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
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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
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Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1582. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1567.


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1509. Data from this article have been entered in the XUNDL database. For more information, click here.


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
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2006HI17      Nucl.Phys. A777, 188 (2006)

W.R.Hix, B.S.Meyer

Thermonuclear kinetics in astrophysics

doi: 10.1016/j.nuclphysa.2004.10.009
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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
Citations: PlumX Metrics


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
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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
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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
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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
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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
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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
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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1141.


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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1138.


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
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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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
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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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0902.


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
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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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