Report/Contribution to a conference proceedings

PUBDB-2016-03509

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Nuclear processes at solar energy

Broggini, C. (Corresponding author)

2003

Report No.: PIC-2003-THAT03; astro-ph/0308537

Abstract: LUNA, Laboratory for Underground Nuclear Astrophysics at Gran Sasso, is measuring fusion cross sections down to the energy of the nucleosynthesis inside stars. Outstanding results obtained up to now are the cross-section measurements within the Gamow peak of the Sun of $^{3}He(^{3}He,2p)^{4}He$ and the $D(p,\gamma)^{3}He$. The former plays a big role in the proton-proton chain, largely affecting the calculated solar neutrino luminosity, whereas the latter is the reaction that rules the proto-star life during the pre-main sequence phase. The implications of such measurements will be discussed. Preliminary results obtained last year on the study of $^{14}N(p,\gamma)^{15}O$, the slowest reaction of the CNO cycle, will also be shown.

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Contributing Institute(s):

1. Bibliothek und Dokumentation (L)

Research Program(s):

1. 899 - ohne Topic (POF3-899) (POF3-899)

Experiment(s):

1. Facility (machine) HERA

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Database coverage:

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Proceedings Riemann, S. (Editor)DESY* ; Lohmann, W. (Editor)DESY*
Physics in collisions. Proceedings, 23rd International Conference, PIC 2003, Zeuthen, Germany, June 26-28, 2003
200323rd International Conference on Physics in Collision, PIC 2003, ZeuthenZeuthen, Germany, 26 Jun 2003 - 28 Jun 20032003-06-262003-06-28   BibTeX | EndNote: XML, Text | RIS

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