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NSR database version of April 25, 2024.

Search: Author = F.Brachwitz

Found 5 matches.

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2005TH04      Nucl.Phys. A751, 301c (2005)

F.-K.Thielemann, D.Argast, F.Brachwitz, J.L.Fisker, C.Frohlich, R.Hirschi, E.Kolbe, D.Mocelj, T.Rauscher

Nuclear Physics: A Key Ingredient in Astrophysical Modeling

doi: 10.1016/j.nuclphysa.2005.02.111
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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1997NO08      Nucl.Phys. A621, 467c (1997)

K.Nomoto, K.Iwamoto, N.Nakasato, F.-K.Thielemann, F.Brachwitz, T.Tsujimoto, Y.Kubo, N.Kishimoto

Nucleosynthesis in Type Ia Supernovae

NUCLEAR STRUCTURE A=16-70; calculated integrated abundances ratio, normalized to ⁵⁶Fe, relative to solar abundances; deduced synthesized mass. Delayed detonation model.

doi: 10.1016/S0375-9474(97)00291-1
Citations: PlumX Metrics

1997TH01      Nucl.Phys. A621, 477c (1997)

F.-K.Thielemann, F.Brachwitz, K.Nomoto, K.Iwamoto

Nucleosynthesis in SNe Ia as a Function of the Burning Front Propagation

NUCLEAR STRUCTURE ⁴⁸Ca, ^54,56,58Fe, ^56,58,60Ni, ^60,62Zn, ⁵⁰Ti, ⁵⁴Cr; calculated abundance plots; deduced astrophysical models constraints.

doi: 10.1016/S0375-9474(97)00292-3
Citations: PlumX Metrics