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The 44Ti(alpha,p) reaction and its implication on the 44Ti yield in supernovae

Sonzogni AA; Rehm KE; Ahmad I; Borasi F; Bowers DL; Brumwell F; Caggiano J; Davids CN; Greene JP; Harss B; Heinz A; Henderson D; Janssens RV; Jiang CL; McMichael G; Nolen J; Pardo RC; Paul M; Schiffer JP; Segel RE; Seweryniak D; Siemssen RH; Truran JW; Uusitalo J; Wiedenhover I; Zabransky B.

Phys Rev Lett ; 84(8): 1651-4, 2000 Feb 21.

Artigo em Inglês | MEDLINE | ID: mdl-11017592

RESUMO

Cross sections for the 44Ti(alpha,p)47V reaction which significantly affects the yield of 44Ti in supernovae were measured in the energy range 5.7 MeV

Constraints on the strength of primordial magnetic fields from big bang nucleosynthesis reexamined.

Cheng B; Olinto AV; Schramm DN; Truran JW.

Phys Rev D Part Fields ; 54(8): 4714-4718, 1996 Oct 15.

Artigo em Inglês | MEDLINE | ID: mdl-10021158

Constraints on the strength of a primordial magnetic field from big bang nucleosynthesis.

Cheng B; Schramm DN; Truran JW.

Phys Rev D Part Fields ; 49(10): 5006-5018, 1994 May 15.

Artigo em Inglês | MEDLINE | ID: mdl-10016811

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