Bibliographic Details
| Title: |
The 10B(p,α)7Be S(E)-factor from 5 keV to 1.5 MeV using the Trojan Horse Method |
| Authors: |
Puglia Sebastiana Maria Regina, Spitaleri Claudio, La Cognata Marco, Lamia Livio, Broggini Carlo, Caciolli Antonio, Carlin Nelson, Cherubini Silvio, Cvetinovic Alexandra, D’Agata Giuseppe, Dell’aquila Daniele, Depalo Rosanna, Gulino Marisa, Guardo Giovanni Luca, Indelicato Iolanda, Lombardo Ivano, Menegazzo Roberto, Munhoz Marcelo Gimenez, Pizzone Rosario Gianluca, Rapisarda Giuseppe Gabriele, Rigato Valentino, Romano Stefano, Sergi Maria Letizia, Souza Francisco, Sparta Roberta, Tudisco Salvo, Tumino Aurora |
| Source: |
EPJ Web of Conferences, Vol 165, p 01042 (2017) |
| Publisher Information: |
EDP Sciences, 2017. |
| Publication Year: |
2017 |
| Collection: |
LCC:Physics |
| Subject Terms: |
Physics, QC1-999 |
| More Details: |
The 10B(p,α)7Be reaction is the main responsible for the 10B destruction in stellar interior [1]. In such environments this p-capture process occurs at a Gamow energy of 10 keV and takes places mainly through a resonant state (Ex = 8.701 MeV) of the compound 11C nucleus. Thus a resonance right in the region of the Gamow peak is expected to significantly influence the behavior of the astrophysical S(E)-factor. The 10B(p,α)7Be reaction was studied via the Trojan Horse Method (THM) applied to the 2H(10B,α7Be)n in order to extract the astrophysical S(E)-factor in a wide energy range from 5 keV to 1.5 MeV. |
| Document Type: |
article |
| File Description: |
electronic resource |
| Language: |
English |
| ISSN: |
2100-014X |
| Relation: |
https://doaj.org/toc/2100-014X |
| DOI: |
10.1051/epjconf/201716501042 |
| Access URL: |
https://doaj.org/article/ce191a1694f34197b0c3a2d71dec6277 |
| Accession Number: |
edsdoj.191a1694f34197b0c3a2d71dec6277 |
| Database: |
Directory of Open Access Journals |
