Abstract.
The present contribution aims to present some general features of the experimental approaches in Nuclear Astrophysics. After a general introduction on light elements nucleosynthesis and on how to determine the reaction rates in a stellar environment, we will focus our attention on underground experiments aimed to directly measure nuclear cross sections of astrophysics interest. We will discuss the 14N(p,\( \gamma\))15O and 12C + 12C reactions, underlying the advantages in approaching these measurements in a deep underground laboratory, as the Laboratori Nazionali del Gran Sasso.
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References
R.J. Deboer et al., Rev. Mod. Phys. 89, 035007 (2017)
R.E. Tribble et al., Rep. Prog. Phys. 77, 106901 (2014)
A. Boeltzig et al., J. Phys. G 45, 025203 (2018)
H. Costantini et al., Rep. Prog. Phys. 72, 086301 (2009)
D.C. Clayton, Principles of Stellar Evolution and Nucleosynthesis (University of Chicago Press, 1968)
G. Gilmore et al., Messenger 147, 25 (2012)
S.W. Stahler, F. Palla, The Formation of Stars (Wiley-VCH, Weinheim, 2004)
E.G. Adelberger et al., Rev. Mod. Phys. 83, 195 (2011)
H.A. Bethe, Phys. Rev. 55, 434 (1939)
C.F. von Weizsacker, Phys. Z 39, 633 (1939)
G. Imbriani et al., Astron. Astrophys. 420, 625 (2004)
C.E. Rolfs, W.S. Rodney, Cauldrons in the Cosmos (University of Chicago Press, 1988)
A. Couture et al., Phys. Rev. C 77, 015802 (2008)
R.C. Runkle et al., Phys. Rev. Lett. 94, 082503 (2005)
D. Schürmann et al., Eur. Phys. J. A 26, 301 (2005)
A. Di Leva et al., Phys. Rev. Lett. 102, 232502 (2009)
C. Matei et al., Phys. Rev. Lett. 97, 242503 (2006)
H. Costantini, A. Formicola, G. Imbriani, M. Junker, C. Rolfs, F. Strieder, Rep. Prog. Phys. 72, 086301 (2009)
H.V. Klapdor-Kleingrothaus et al., Nucl. Instrum. Methods A 522, 371 (2004)
A. Caciolli et al., Eur. Phys. J. A 39, 179 (2009)
G. Audi, A.H. Wapstra et al., Nucl. Phys. A 729, 337 (2003)
U. Schröder et al., Nucl. Phys. A 467, 240 (1987)
A. Formicola et al., Phys. Lett. B 591, 61 (2004)
G. Imbriani et al., Eur. Phys. J. A 25, 455 (2005)
R.C. Runkle et al., Phys. Rev. Lett. 94, 082503 (2005)
R.C. Runkle et al., Phys. Rev. Lett. 94, 082503 (2005)
A. Lemut et al., Phys. Lett. B 634, 483 (2006)
D. Bemmerer et al., Nucl. Phys. A 779, 297 (2006)
M. Marta et al., Phys. Rev. C 78, 022802(R) (2008)
A.M. Mukhamedzhanov et al., Phys. Rev. C 67, 065804 (2003)
D. Schürmann et al., Phys. Rev. C 77, 055803 (2008)
S.O. Nelson et al., Phys. Rev. C 68, 065804 (2003)
P.F. Bertone et al., Phys. Rev. Lett. 87, 152501 (2001)
K. Yamada et al., Phys. Lett. B 579, 265 (2004)
C. Angulo et al., Nucl. Phys. A 656, 3 (1999)
C. Bennett et al., Astrophys. J. 583, 123 (2003)
O. Straniero, L. Piersanti, S. Cristallo, J. Phys.: Conf. Ser. 665, 012008 (2016)
B. Leibundgut, Annu. Rev. Astron. Astrophys. 39, 67 (2001)
H.W. Becker et al., Z. Phys. A 303, 305 (1981)
T. Spillane et al., Phys. Rev. Lett. 98, 122501 (2007)
L.R. Gasques et al., Phys. Rev. C 76, 035802 (2007)
A. Tumino et al., Nature 557, 687 (2018)
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Formicola, A., Imbriani, G. Introduction to experimental nuclear astrophysics. Eur. Phys. J. Plus 134, 89 (2019). https://doi.org/10.1140/epjp/i2019-12497-1
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DOI: https://doi.org/10.1140/epjp/i2019-12497-1