NSR Query Results

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NSR database version of April 27, 2024.

Search: Author = J.W.Truran

Found 18 matches.

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2012GL03      J.Phys.:Conf.Ser. 337, 012071 (2012)

S.A.Glasner, J.W.Truran

Novae - The study of the reactive flow

doi: 10.1088/1742-6596/337/1/012071
Citations: PlumX Metrics

2012TR07      J.Phys.:Conf.Ser. 337, 012040 (2012)

J.W.Truran, A.S.Glasner, Y.Kim

56Ni, Explosive Nucleosynthesis, and SNe Ia Diversity

doi: 10.1088/1742-6596/337/1/012040
Citations: PlumX Metrics

2012TR12      J.Phys.:Conf.Ser. 381, 012015 (2012)

J.W.Truran

Nuclear Physics Constraints on the Characteristics of Astrophysical Thermonuclear Flashes

doi: 10.1088/1742-6596/381/1/012015
Citations: PlumX Metrics

2010FA02      Astrophys.J. 712, 1359 (2010)

K.Farouqi, K.-L.Kratz, B.Pfeiffer, T.Rauscher, F.-K.Thielemann, J.W.Truran

Charged-particle and neutron-capture processes in the high-entropy wind of core-collapse supernovae

doi: 10.10///0004-637X/712/2/1359
Citations: PlumX Metrics

2009SE01      At.Data Nucl.Data Tables 95, 96 (2009)

I.R.Seitenzahl, D.M.Townsley, F.Peng, J.W.Truran

Nuclear statistical equilibrium for Type Ia supernova simulations

doi: 10.1016/j.adt.2008.08.001
Citations: PlumX Metrics

2007KR20      Astrophys.J. 662, 39 (2007)

K.-L.Kratz, K.Farouqi, B.Pfeiffer, J.W.Truran, C.Sneden, J.J.Cowan

Explorations of the r-Processes: Comparisons between Calculations and Observations of Low-Metallicity Stars

NUCLEAR REACTIONS 138Ba(n, γ), E ∼ 30 keV; analyzed available data; calculated r-process abundances in low-metallicity stars.

doi: 10.1086/517495
Citations: PlumX Metrics

2001FR16      Nucl.Phys. A688, 172c (2001)

B.Fryxell, M.Zingale, F.X.Timmes, D.Q.Lamb, K.Olson, A.C.Calder, L.J.Dursi, P.Ricker, R.Rosner, J.W.Truran, P.MacNeice, H.Tufo

Numerical Simulations of Thermonuclear Flashes on Neutron Stars

doi: 10.1016/S0375-9474(01)00692-3
Citations: PlumX Metrics

2001ST18      Nucl.Phys. A688, 110c (2001)

S.Starrfield, C.Iliadis, J.W.Truran, M.Wiescher, W.M.Sparks

Nuclear Reaction Rates and the Nova Outburst

NUCLEAR STRUCTURE 12,13C, 14,15N, 22Na, 26,27Al, 32S; analyzed, surveyed astrophysical nuclear reaction rates; deduced nova luminosity, yields.

doi: 10.1016/S0375-9474(01)00679-0
Citations: PlumX Metrics

2001TR15      Nucl.Phys. A688, 330c (2001)

J.W.Truran, J.J.Cowan, B.D.Fields

Halo Star Abundances and r-Process Synthesis

doi: 10.1016/S0375-9474(01)00722-9
Citations: PlumX Metrics

2000ME22      Phys.Rep. 333-334, 1 (2000)

B.S.Meyer, J.W.Truran

Nucleocosmochronology

doi: 10.1016/S0370-1573(00)00012-0
Citations: PlumX Metrics

2000SO01      Phys.Rev.Lett. 84, 1651 (2000)

A.A.Sonzogni, K.E.Rehm, I.Ahmad, F.Borasi, D.L.Bowers, F.Brumwell, J.Caggiano, C.N.Davids, J.P.Greene, B.Harss, A.Heinz, D.Henderson, R.V.F.Janssens, C.L.Jiang, G.McMichael, J.Nolen, R.C.Pardo, M.Paul, J.P.Schiffer, R.E.Segel, D.Seweryniak, R.H.Siemssen, J.W.Truran, J.Uusitalo, I.Wiedenhover, B.Zabransky

The 44Ti(α, p) Reaction and Its Implication on the 44Ti Yield in Supernovae

NUCLEAR REACTIONS 44Ti(α, p), E(cm)=5.7-9 MeV; measured σ, astrophysical reaction rate. Comparison with statistical model calculations. Effects on the production of 44Ti in core-collapsed supernovae discussed.

doi: 10.1103/PhysRevLett.84.1651
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0609.

1999BU10      Phys.Rev.Lett. 82, 4176 (1999)

S.Burles, K.M.Nollett, J.W.Truran, M.S.Turner

Sharpening the Predictions of Big-Bang Nucleosynthesis

NUCLEAR REACTIONS 1H(n, γ), 2H(p, γ), (d, p), (d, n), 3H(α, γ), (d, n), 3He(α, γ), (d, p), (n, p), 7Li(p, α), (p, n), E < 2000 keV; analyzed data. 2H, 3,4He, 7Li; deduced big-bang nucleosynthesis yields, sources of uncertainty.

doi: 10.1103/PhysRevLett.82.4176
Citations: PlumX Metrics

1997CO17      Nucl.Phys. A621, 41c (1997)

J.J.Cowan, C.Sneden, J.W.Truran, D.L.Burris, A.McWilliam, G.W.Preston

R- and S-Process Signatures in Metal-Poor Halo Stars

doi: 10.1016/S0375-9474(97)00209-1
Citations: PlumX Metrics

1997ST20      Nucl.Phys. A621, 495c (1997)

S.Starrfield, J.W.Truran, M.Wiescher, W.M.Sparks

Nova Nucleosynthesis

doi: 10.1016/S0375-9474(97)00296-0
Citations: PlumX Metrics

1997TH02      Nucl.Phys. A621, 485c (1997)

K.Thornton, H.-Th.Janka, J.W.Truran

Supernovae as Thermal and Kinetic Energy Input to Their Environment

doi: 10.1016/S0375-9474(97)00294-7
Citations: PlumX Metrics

1997TR08      Nucl.Phys. A621, 548c (1997)

J.W.Truran, F.X.Timmes

Cosmic Chemical Evolution

doi: 10.1016/S0375-9474(97)00302-3
Citations: PlumX Metrics

1997WA23      Nucl.Phys. A621, 499c (1997)

S.Wanajo, K.Nomoto, M.Hashimoto, J.W.Truran

A Quasi-Analytic Study of Nucleosynthesis in ONeMg Novae

doi: 10.1016/S0375-9474(97)00297-2
Citations: PlumX Metrics

1988KR08      J.Phys.(London) G14, Supplement S331 (1988)

K.-L.Kratz, F.-K.Thielemann, W.Hillebrandt, P.Moller, V.Harms, A.Wohr, J.W.Truran

Constraints on r-Process Conditions from Beta-Decay Properties Far Off Stability and r-Abundances

NUCLEAR STRUCTURE 130Cd, 80Zn; analyzed β-decay data; deduced A ≈ 130, 80 r-abundances. Shell model imput.

doi: 10.1088/0305-4616/14/S/034
Citations: PlumX Metrics

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Note: The following list of authors and aliases matches the search parameter J.W.Truran: , J.W.TRURAN