Issue |
A&A
Volume 398, Number 2, February I 2003
|
|
---|---|---|
Page(s) | 423 - 427 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361:20021700 | |
Published online | 21 January 2003 |
Proton-induced lithium destruction cross-section and its astrophysical implications
1
Dipartimento di Metodologie Fisiche e Chimiche per l'Ingegneria, Università di Catania, Catania, Italy
2
Laboratori Nazionali del Sud-INFN, Catania, Italy
3
Centro Siciliano Fisica Nucleare e Struttura della Materia, Catania, Italy
4
Dipartimento di Fisica e Astronomia, Università di Catania, Catania, Italy
5
Ruhr Universität Bochum, Bochum, Germany
6
Dipartimento di Fisica, Università di Pisa, Pisa, Italy
Corresponding author: C. Spitaleri, spitaleri@lns.infn.it
Received:
18
July
2002
Accepted:
29
October
2002
Knowledge of the primordial nucleosynthesis offers a powerful tool
to retrieve information on the baryon density of the Universe. In this context
lithium isotopes play a crucial role and in particular we stress how
important the bare nucleus cross-section for the 7Li(p, He
reaction is. Recent application of the Trojan Horse Method led to an indirect
measurement of that cross-section. In the present paper its astrophysical
implications are examined in the case of the Solar lithium problem and of the
primordial nucleosynthesis.
Key words: nuclear reactions, nucleosynthesis, abundances / Sun: abundances / cosmology: cosmological parameters
© ESO, 2003
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