TY  - CONF
AU  - Cavanna, Francesca
TI  - Latest results from LUNA experiment
CY  - Hamburg
PB  - Verlag Deutsches Elektronen-Synchrotron
M1  - PUBDB-2016-05620
SN  - 978-3-945931-08-0
T2  - DESY-PROC
SP  - 129-134
PY  - 2016
AB  - Nuclear processes are responsible for energy generation that makes stars shine, and for the synthesis of the elements in stars and also play a decisive role in explaining the chemical composition of the interstellar medium. Thermonuclear fusion reactions convert protons into heavier elements from He to Fe. Deep underground in the Gran Sasso Laboratory the key reactions of the proton-proton chain, the carbon-nitrogen-oxygen cycle and the neon-sodium cycle have been studied down to the energies of astrophysical interest. The latest results are reviewed, together with future developments of underground nuclear astrophysics.
T2  - Magellan Workshop
CY  - 17 Mar 2016 - 18 Mar 2016, Hamburg (Germany)
Y2  - 17 Mar 2016 - 18 Mar 2016
M2  - Hamburg, Germany
LB  - PUB:(DE-HGF)8 ; PUB:(DE-HGF)7
DO  - DOI:10.3204/DESY-PROC-2016-05/10
UR  - https://bib-pubdb1.desy.de/record/315085
ER  -