LUNA

(Laboratory for Underground Nuclear Astrophysics)

Other Web pages: INSPIRE

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References

1 - Reviews

[1-1]
LUNA: Status and Prospects, C. Broggini, D. Bemmerer, A. Caciolli, D. Trezzi, Prog.Part.Nucl.Phys. 98 (2018) 55-84, arXiv:1707.07952.
[Broggini:2017cez]
[1-2]
Twenty years of LUNA, C. Broggini (LUNA), Prog.Part.Nucl. Phys. 66 (2011) 293-297.
[Broggini:2011zz]
[1-3]
LUNA: Nuclear Astrophysics Deep Underground, Carlo Broggini, Daniel Bemmerer, Alessandra Guglielmetti, Roberto Menegazzo, Ann. Rev. Nucl. Part. Sci. 60 (2010) 53-73, arXiv:1010.4165.
[Broggini:2010mu]

2 - Articles

[2-1]
Proton-Capture Rates on Carbon Isotopes and Their Impact on the Astrophysical C12/C13 Ratio, J. Skowronski et al. (LUNA), Phys. Rev. Lett. 131 (2023) 162701, arXiv:2308.16098.
[LUNA:2023enu]
[2-2]
Direct Measurement of the $^{13}$C ($\alpha$, n) $^{16}$O Cross Section into the s-Process Gamow Peak, G. F. Ciani et al. (LUNA), Phys. Rev. Lett. 127 (2021) 152701, arXiv:2110.00303.
[LUNA:2021jlt]
[2-3]
The baryon density of the Universe from an improved rate of deuterium burning, V. Mossa et al., Nature 587 (2020) 210-213.
[Mossa:2020gjc]
[2-4]
Underground experimental study finds no evidence of low-energy resonance in the $^{6}$Li(p,$\gamma$)$^{7}$Be reaction, D. Piatti et al., Phys. Rev. C 102 (2020) 052802.
[Piatti:2020gyp]
[2-5]
Cross section of the reaction 18 O(p, $\gamma$ ) 19 F at astrophysical energies: The 90 keV resonance and the direct capture component, A. Best et al., Phys. Lett. B 797 (2019) 134900.
[Best:2019bcb]
[2-6]
Direct measurements of low-energy resonance strengths of the 23 Na(p, $\gamma$ ) 24 Mg reaction for astrophysics, A. Boeltzig et al., Phys. Lett. B 795 (2019) 122-128.
[Boeltzig:2019jmp]
[2-7]
Improved astrophysical rate for the 18 O(p, $\alpha$ ) 15 N reaction by underground measurements, C. G. Bruno et al., Phys. Lett. B 790 (2019) 237-242.
[Bruno:2019dim]
[2-8]
Direct capture cross section and the $E_p$ = 71 and 105 keV resonances in the $^{22}$Ne($p,\gamma$)$^{23}$Na reaction, F. Ferraro et al., Phys. Rev. Lett. 121 (2018) 172701, arXiv:1810.01628.
[Ferraro:2018zun]
[2-9]
Big Bang 6 Li nucleosynthesis studied deep underground (LUNA collaboration), D. Trezzi et al., Astropart. Phys. 89 (2017) 57-65.
[Trezzi:2017omf]
[2-10]
Direct measurement of low-energy $^{22}$Ne(p,$\gamma$)$^{23}$Na resonances, R. Depalo et al., Phys. Rev. C 94 (2016) 055804, arXiv:1610.00925.
[Depalo:2016seq]
[2-11]
Improved Direct Measurement of the 64.5 keV Resonance Strength in the O17(p,$\alpha$)N14 Reaction at LUNA, C. G. Bruno et al. (LUNA), Phys. Rev. Lett. 117 (2016) 142502, arXiv:1610.00483.
[LUNA:2016kdc]
[2-12]
Three New Low-Energy Resonances in the $^{22}Ne(p,\gamma)^{23}Na$ Reaction, F. Cavanna et al. (LUNA), Phys. Rev. Lett. 115 (2015) 252501, arXiv:1511.05329. [Erratum: Phys.Rev.Lett. 120, 239901 (2018)].
[LUNA:2015fdq]
[2-13]
First Direct Measurement of the $^2$H($\alpha$,$\gamma$)$^6$Li Cross Section at Big Bang Energies and the Primordial Lithium Problem, M. Anders et al. (LUNA), Phys. Rev. Lett. 113 (2014) 042501.
[LUNA:2014hrn]
[2-14]
The 25Mg(p,g)Al reaction at low astrophysical energies, F. Strieder et al. (LUNA), Phys. Lett. B 707 (2012) 60-65, arXiv:1112.3313.
[LUNA:2011aa]
[2-15]
The 14N(p,gamma)15O reaction studied with a composite germanium detector, M. Marta et al. (LUNA), Phys. Rev. C 83 (2011) 045804, arXiv:1103.5393.
[LUNA:2011duw]
[2-16]
New experimental study of low-energy (p,gamma) resonances in magnesium isotopes, B. Limata et al. (LUNA), Phys. Rev. C 82 (2010) 015801, arXiv:1006.5281.
[LUNA:2010wpm]
[2-17]
Direct measurement of the N-15(p,gamma) O-16 total cross section at novae energies, D Bemmerer et al. (LUNA), J. Phys. G 36 (2009) 045202, arXiv:0902.0783.
[LUNA:2009eez]
[2-18]
Astrophysical S-factor of the He-3(alpha,gamma) Be-7 reaction measured at low energy via prompt and delayed gamma detection, F. Confortola et al. (LUNA), Phys. Rev. C 75 (2007) 065803, arXiv:0705.2151.
[LUNA:2007ffz]
[2-19]
First measurement of the N-14(p,gamma)O-15 cross section down to 70-KeV, A. Lemut et al. (LUNA), Phys. Lett. B 634 (2006) 483-487, arXiv:nucl-ex/0602012.
[LUNA:2006ois]
[2-20]
Low energy measurement of the 14N(p, $\gamma$)15O total cross section at the LUNA underground facility, D. Bemmerer et al. (LUNA), Nucl. Phys. A 779 (2006) 297-317.
[LUNA:2006ltn]
[2-21]
S-factor of N-14 (p, gamma) O-15 at astrophysical energies, G. Imbriani et al. (LUNA), Eur. Phys. J. A 25 (2005) 455-466, arXiv:nucl-ex/0509005.
[LUNA:2005yso]
[2-22]
Astrophysical S-factor of 14N(p,g)15O, A. Formicola et al. (LUNA), Phys. Lett. B591 (2004) 61, arXiv:nucl-ex/0312015.
[LUNA:2003yvu]
[2-23]
First measurement of the d(p,$\gamma$) 3 He cross section down to the solar Gamow peak, C. Casella et al. (LUNA), Nucl. Phys. A 706 (2002) 203-216.
[LUNA:2002eis]
[2-24]
First Measurement of the He3+He3- > He4+2p Cross Section down to the Lower Edge of the Solar Gamow Peak, R. Bonetti et al. (LUNA), Phys. Rev. Lett. 82 (1999) 5205-5208, arXiv:nucl-ex/9902004.
[LUNA:1999enm]
[2-25]
The Cross-section of He-3 (He-3, 2 p) He-4 measured at solar energies, M. Junker et al. (LUNA), Phys. Rev. C 57 (1998) 2700-2710, arXiv:nucl-ex/9707003.
[LUNA:1997roj]

3 - Detector

[3-1]
Setup commissioning for an improved measurement of the D(p,$\gamma $)$^3$He cross section at Big Bang Nucleosynthesis energies: LUNA collaboration, V. Mossa et al., Eur. Phys. J. A 56 (2020) 144, arXiv:2005.00002.
[Mossa:2020qgj]
[3-2]
A new approach to monitor $^{13}\hbox {C}$-targets degradation in situ for $^{13}\hbox {C}(\alpha,\hbox {n})^{16}\hbox {O}$ cross-section measurements at LUNA, G. F. Ciani et al., Eur. Phys. J. A 56 (2020) 75, arXiv:2001.08744.
[Ciani:2020xdi]
[3-3]
Effect of beam energy straggling on resonant yield in thin gas targets: The cases $^{22}$Ne(p,{\textbackslash{}gamma})$^{23}$Na and $^{14}$N(p,{\textbackslash{}gamma})$^{15}$O, D. Bemmerer et al. (LUNA), EPL 122 (2018) 52001, arXiv:1806.11501.
[LUNA:2018wjn]
[3-4]
A high-efficiency gas target setup for underground experiments, and redetermination of the branching ratio of the 189.5 keV$^{22}$Ne(p, $\gamma$ )$^{23}$Na resonance, F. Ferraro et al., Eur. Phys. J. A 54 (2018) 44, arXiv:1802.04164.
[Ferraro:2018yny]
[3-5]
Improved background suppression for radiative capture reactions at LUNA with HPGe and BGO detectors, A. Boeltzig et al., J. Phys. G 45 (2018) 025203.
[Boeltzig:2018ufp]
[3-6]
A new study of the $^{22}$Ne(p,$\gamma$)$^{23}$Na reaction deep underground: Feasibility, setup, and first observation of the 186 keV resonance, F. Cavanna et al. (LUNA), Eur. Phys. J. A 50 (2014) 179, arXiv:1411.2888.
[LUNA:2014vex]
[3-7]
Neutron-induced background by an alpha-beam incident on a deuterium gas target and its implications for the study of the 2H(alpha,gamma)6Li reaction at LUNA, M. Anders et al. (LUNA), Eur. Phys. J. A 49 (2013) 28, arXiv:1301.7185.
[LUNA:2013kpr]
[3-8]
Preparation and characterisation of isotopically enriched Ta$_2$O$_5$ targets for nuclear astrophysics studies, A. Caciolli et al. (LUNA), Eur. Phys. J. A 48 (2012) 144, arXiv:1210.0327.
[LUNA:2012xmc]
[3-9]
An actively vetoed Clover gamma-detector for nuclear astrophysics at LUNA, T. Szucs et al. (LUNA), Eur. Phys. J. A 44 (2010) 513-519, arXiv:1003.6072.
[LUNA:2010rtd]
[3-10]
Ultra-sensitive in-beam gamma-ray spectroscopy for nuclear astrophysics at LUNA, A. Caciolli et al. (LUNA), Eur. Phys. J. A 39 (2009) 179-186, arXiv:0812.3223.
[LUNA:2008yib]
[3-11]
Electron screening in d(d, p)t for deuterated metals: Temperature effects, F. Raiola et al. (LUNA), J. Phys. G 31 (2005) 1141-1149.
[LUNA:2005byg]
[3-12]
Electron screening in 7 Li (p,$\alpha$)$\alpha$ and 6 Li (p,$\alpha$)3 He for different environments, J. Cruz et al. (LUNA), Phys. Lett. B 624 (2005) 181-185.
[LUNA:2005jer]
[3-13]
Target stability and beam-induced background studies at the LUNA underground facility, F. Strieder et al. (LUNA), Nucl. Phys. A 718 (2003) 135-138.
[Strieder:2003ztu]

4 - Talks

[4-1]
Results from LUNA, C. Broggini (LUNA), Nucl. Phys. Proc. Suppl. 87 (2000) 177-179.
[Broggini:2000dx]
[4-2]
Status of the LUNA experiment, C. Arpesella et al., Nucl. Phys. Proc. Suppl. 48 (1996) 375-377.
[Arpesella:1996wb]
[4-3]
The LUNA experiment, C. Broggini (LUNA), Nucl. Phys. Proc. Suppl. 43 (1995) 58-61.
[Broggini:1995in]

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Authors:
Stefano Gariazzo / gariazzo@to.infn.it
Carlo Giunti / giunti@to.infn.it
Marco Laveder / marco.laveder@pd.infn.it
Last Update: Thu 28 Mar 2024, 15:06:49 CET