Published 1998 | Version v1
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Measurement of reaction rates of interest in stellar structure and evolution

  • 1. INFN, Napoli (Italy)
  • 2. Dipt. di Scienze Ambientali, Seconda Univ. di Napoli, Caserta (Italy)
  • 3. Dipt. di Scienze Fisiche, Univ. Federico II, Napoli (Italy)
  • 4. Inst. fuer Experimentalphysik III, Ruhr-Univ. Bochum, Bochum (Germany)
  • 5. Osservatorio Astronomico di Collurania, Teramo (Italy)

Description

Accurate determinations of reaction rates at astrophysical energies are very important in stellar structure and evolution studies. The cases of two key reactions, namely 7Be(p,γ)8B and 12C(α,γ)16O are discussed, both from the point of view of their astrophysical interest and of the experimental difficulties in the measurement of their cross section. (orig.)

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Part of:
Nuclear astrophysics.Proceedings of the International workshop XXVI on gross properties of nuclei and nuclear excitations

Additional details

Publishing Information

Imprint Title
Nuclear astrophysics.Proceedings of the International workshop XXVI on gross properties of nuclei and nuclear excitations
Imprint Pagination
442 p.
Journal Page Range
p. 378-387.
Report number
INIS-DE--0012

Conference

Title
Nuclear astrophysics (Hirschegg '98).
Acronym
26. international workshop on gross properties of nuclei and nuclear excitations
Dates
11-17 Jan 1998.
Place
Hirschegg (Austria).

Optional Information