Published October 28, 2011 | Version v1
Journal article

Proton-capture Nucleosynthesis In Low Mass Stars: Effects of New Reaction Rates

  • 1. Dipartimento di Fisica, Universita degli Studi di Perugia and INFN Sezione di Perugia (Italy)
  • 2. DMFCI - Universita di Catania and Laboratori Nazionali del Sud - INFN, Catania (Italy)
  • 3. INAF Osservatorio Astronomico di Collurania, Teramo (Italy)
  • 4. Departamento de Fisica Teorica y del Cosmos, Universidad de Granada (Spain)

Description

We present computations of nucleosynthesis in low-mass asymptotic-giant-branch stars of solar metallicity experiencing deep mixing. In this framework, we discuss the effects of recent improvements in relevant reaction rates for proton captures on intermediate-mass nuclei. The calculations are then performed on the basis of a parameterized circulation, where the effects of the new nuclear inputs are best compared to previous works. We find that especially the new reaction rate for the 14N(p,γ)15O reaction implies considerable modifications in the composition of low mass red giant stars.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1377
Journal Issue
1
Journal Page Range
p. 414-416
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
FINUSTAR 3 Conference on frontiers in nuclear structure, astrophysics, and reactions
Dates
23-27 Aug 2010
Place
Rhodes (Greece)

Optional Information

Notes
(c) 2011 American Institute of Physics