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@INPROCEEDINGS{Broggini:308158,
author = {Broggini, Carlo},
title = {{N}uclear processes at solar energy},
reportid = {PUBDB-2016-03509, astro-ph/0308537. PIC-2003-THAT03},
pages = {21-30},
year = {2003},
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.},
month = {Jun},
date = {2003-06-26},
organization = {23rd International Conference on
Physics in Collision, Zeuthen
(Germany), 26 Jun 2003 - 28 Jun 2003},
cin = {L},
cid = {I:(DE-H253)L-20120731},
pnm = {899 - ohne Topic (POF3-899)},
pid = {G:(DE-HGF)POF3-899},
experiment = {EXP:(DE-H253)HERA(machine)-20150101},
typ = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8},
url = {https://bib-pubdb1.desy.de/record/308158},
}