(Laboratory for Underground Nuclear Astrophysics)

Other Web pages: INSPIRE

Filter this page

(Note: The process can take some time.)



1 - Reviews

LUNA: Status and Prospects, C. Broggini, D. Bemmerer, A. Caciolli, D. Trezzi, Prog.Part.Nucl.Phys. 98 (2018) 55-84, arXiv:1707.07952.
Twenty years of LUNA, C. Broggini (LUNA), Prog.Part.Nucl. Phys. 66 (2011) 293-297.
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.

2 - Articles

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.
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.
The baryon density of the Universe from an improved rate of deuterium burning, V. Mossa et al., Nature 587 (2020) 210-213.
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.
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.
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.
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.
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.
Big Bang 6 Li nucleosynthesis studied deep underground (LUNA collaboration), D. Trezzi et al., Astropart. Phys. 89 (2017) 57-65.
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.
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.
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)].
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.
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.
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.
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.
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.
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.
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.
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.
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.
Astrophysical S-factor of 14N(p,g)15O, A. Formicola et al. (LUNA), Phys. Lett. B591 (2004) 61, arXiv:nucl-ex/0312015.
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.
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.
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.

3 - Detector

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.
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.
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.
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.
Improved background suppression for radiative capture reactions at LUNA with HPGe and BGO detectors, A. Boeltzig et al., J. Phys. G 45 (2018) 025203.
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.
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.
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.
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.
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.
Electron screening in d(d, p)t for deuterated metals: Temperature effects, F. Raiola et al. (LUNA), J. Phys. G 31 (2005) 1141-1149.
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.
Target stability and beam-induced background studies at the LUNA underground facility, F. Strieder et al. (LUNA), Nucl. Phys. A 718 (2003) 135-138.

4 - Talks

Results from LUNA, C. Broggini (LUNA), Nucl. Phys. Proc. Suppl. 87 (2000) 177-179.
Status of the LUNA experiment, C. Arpesella et al., Nucl. Phys. Proc. Suppl. 48 (1996) 375-377.
The LUNA experiment, C. Broggini (LUNA), Nucl. Phys. Proc. Suppl. 43 (1995) 58-61.

Search Neutrino Unbound

Cross search NU

It is possible to perform a cross search between the various pages of Neutrino Unbound.
This is useful if you want to show the common elements that appear in the listings of two (or more) different topics or experiments.

Go to the search form.

[Go to ...]

Neutrino Unbound Home

Stefano Gariazzo /
Carlo Giunti /
Marco Laveder /
Last Update: Fri 1 Dec 2023, 15:43:29 CET