pith. sign in

arxiv: nucl-ex/0209017 · v1 · pith:5IYAJWV4new · submitted 2002-09-24 · ⚛️ nucl-ex · astro-ph

Study of the ¹8F(p, alpha)¹5O reaction for application to nova gamma-ray emission

N. de Sereville , A. Coc , C. Angulo , M. Assuncao , D. Beaumel , B. Bouzid , S. Cherubini , M. Couder
show 17 more authors
P. Demaret F. de Oliveira Santos P. Figuera S. Fortier M. Gaelens F. Hammache J. Kiener D. Labar A. Lefebvre P. Leleux M. Loiselet A. Ninane S. Ouichaoui G. Ryckewaert N. Smirnova V. Tatischeff J.-P. Thibaud
This is my paper
classification ⚛️ nucl-ex astro-ph
keywords reactionalphanovaemissiongamma-rayrateapplicationastronomy
0
0 comments X
read the original abstract

The ^18F(p, alpha)^15O reaction is recognized as one of the most important reaction for nova gamma-ray astronomy as it governs the early =< 511 keV emission. However, its rate remains largely uncertain at nova temperatures due to unknown low-energy resonance strengths. In order to better constrain this reaction rate, we have studied the one-nucleon transfer reaction, D(^18F,p alpha)^15N, at the CRC-RIB facility at Louvain La Neuve.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.