The nuclear physics of the hydrogen burning in the Sun

[1]  A. Serenelli Alive and well: A short review about standard solar models , 2016, The European Physical Journal A.

[2]  V. Rigato,et al.  Underground nuclear astrophysics: Why and how , 2016, The European Physical Journal A.

[3]  E. Klempt,et al.  Interference phenomena in the JP = 1/2− wave in η photoproduction , 2015 .

[4]  A. Kontos,et al.  Monte Carlo uncertainty of the He 3 ( α , γ ) Be 7 reaction rate , 2014 .

[5]  L. Cadonati,et al.  Neutrinos from the primary proton–proton fusion process in the Sun , 2014, Nature.

[6]  A. Kontos,et al.  Astrophysical S factor of 3 He(α,γ) 7 Be , 2013 .

[7]  Z. Fülöp,et al.  Activation measurement of the He3(α,γ)Be7 reaction cross section at high energies , 2013, 1304.4740.

[8]  A. Serenelli,et al.  Using the standard solar model to constrain solar composition and nuclear reaction S factors , 2012, 1211.6740.

[9]  A. Muñoz-Martín,et al.  New measurement of the 3 He(α,γ) 7 Be cross section at medium energies , 2012 .

[10]  Alessandra Guglielmetti,et al.  LUNA: Nuclear Astrophysics Deep Underground , 2010, 1010.4165.

[11]  H. Costantini,et al.  AZURE: An R-matrix code for nuclear astrophysics , 2010 .

[12]  J. Ferguson,et al.  NEW SOLAR COMPOSITION: THE PROBLEM WITH SOLAR MODELS REVISITED , 2009, 0909.2668.

[13]  F. Terrasi,et al.  Stellar and Primordial Nucleosynthesis ofBe7: Measurement ofHe3(α,γ)Be7 , 2009 .

[14]  H. Costantini,et al.  LUNA: a laboratory for underground nuclear astrophysics , 2009, 0906.1097.

[15]  L. Agostino,et al.  Ultra-sensitive in-beam $ \gamma$ -ray spectroscopy for nuclear astrophysics at LUNA , 2008, 0812.3223.

[16]  F. Terrasi,et al.  The He-3(alpha,gamma)Be-7 S-factor at solar energies: The Prompt gamma experiment at LUNA , 2008, 0809.5269.

[17]  C. Mazzocchi,et al.  Precision study of ground state capture in the 14N(p,γ)15O reaction , 2008, 0807.4919.

[18]  A. Serenelli,et al.  CN Cycle Solar Neutrinos and the Sun's Primordial Core Metallicity , 2008, 0805.2013.

[19]  R. Kunz,et al.  Lifetime measurement of the 6792 keV state in O 15 , important for the astrophysical S factor extrapolation in N 14 ( p , γ ) O 15 , 2008, 0804.1934.

[20]  H. M. Antia,et al.  Helioseismology and Solar Abundances , 2007, 0711.4590.

[21]  T. A. Brown,et al.  The 3He + 4He --> 7Be Astrophysical S-factor , 2007, 0710.1279.

[22]  M. Suhail Zubairy,et al.  Quantum lithography with classical light: Generation of arbitrary patterns , 2007 .

[23]  F. Terrasi,et al.  He3(alpha,gamma)Be7 cross section at low energies , 2007, nucl-ex/0702003.

[24]  G. Imbriani,et al.  Low energy measurement of the 14N(p, γ)15O total cross section at the LUNA underground facility , 2006 .

[25]  F. Terrasi,et al.  Activation measurement of the 3He(alpha,gamma)7Be cross section at low energy. , 2006, Physical review letters.

[26]  F. Terrasi,et al.  First measurement of the 14N(p,γ)15O cross section down to 70 keV , 2006, nucl-ex/0602012.

[27]  C. Rossi-Alvarez,et al.  S-factor of 14N(p,γ)15O at astrophysical energies⋆ , 2005, nucl-ex/0509005.

[28]  Neubauer,et al.  Electron energy spectra, fluxes, and day-night asymmetries of 8B solar neutrinos from measurements with NaCl dissolved in the heavy-water detector at the Sudbury Neutrino Observatory , 2005 .

[29]  S. Basu,et al.  New Solar Opacities, Abundances, Helioseismology, and Neutrino Fluxes , 2004, astro-ph/0412440.

[30]  E. Dudas,et al.  Issues on tadpoles and vacuum redefinitions in String Theory , 2004, hep-th/0503204.

[31]  R. Longland,et al.  Direct measurement of the 14N(p,gamma)15O S factor. , 2004, Physical review letters.

[32]  G. Miele,et al.  Nuclear reaction network for primordial nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields , 2004, astro-ph/0408076.

[33]  G. Haquin,et al.  New precision measurement of the 3He(4He,gamma) 7Be cross section. , 2004, nucl-ex/0407017.

[34]  M. Mendenhall,et al.  An algorithm for computing screened Coulomb scattering in Geant4 , 2004, physics/0406066.

[35]  F. Terrasi,et al.  The bottleneck of CNO burning and the age of Globular Clusters , 2004, astro-ph/0403071.

[36]  M. Pinsonneault,et al.  What do we (not) know theoretically about solar neutrino fluxes? , 2004, Physical review letters.

[37]  H. Kobayashi,et al.  E1 strength of the subthreshold 3/2+ state in 15O studied by Coulomb excitation , 2004 .

[38]  M. Spraker,et al.  Analyzing power measurement for the 14 N ( p→ ,γ) 15 O reaction at astrophysically relevant energies , 2003 .

[39]  H. Costantini,et al.  Astrophysical S-factor of 14N( p, ?) 15O , 2003, nucl-ex/0312015.

[40]  F. Terrasi,et al.  The LUNA II 400 kV accelerator , 2003 .

[41]  H. Toki,et al.  Cross section of 3He(3He,2p)4He measured near the Gamow energy , 2003 .

[42]  Alessandra Guglielmetti,et al.  A new setup for the underground study of capture reactions , 2002 .

[43]  C. Iliadis,et al.  Lifetime of the 6793-keV state in 15O. , 2001, Physical review letters.

[44]  C. Angulo,et al.  The 14 N(p, γ ) 15 O low-energy S -factor , 2001 .

[45]  F. Terrasi,et al.  First Measurement of the 3 He ( 3 He , 2 p ) 4 He Cross Section down to the Lower Edge of the Solar Gamow Peak , 1999, nucl-ex/9902004.

[46]  S. Burles,et al.  SHARPENING THE PREDICTIONS OF BIG-BANG NUCLEOSYNTHESIS , 1999, astro-ph/9901157.

[47]  E. Henley,et al.  Solar fusion cross sections , 1998, astro-ph/9805121.

[48]  E. Bellotti,et al.  Cross section of He-3(He-3,2p)He-4 measured at solar energies , 1997, nucl-ex/9707003.

[49]  E. Bellotti,et al.  Measurement of the 3He(3He,2p)4He cross section within the solar Gamow peak , 1996 .

[50]  C. Arpesella A low background counting facility at laboratori nazionali del Gran Sasso , 1996 .

[51]  A. Lanza,et al.  Laboratory for Underground Nuclear Astrophysics (LUNA) , 1994 .

[52]  John N. Bahcall,et al.  Standard solar models, with and without helium diffusion and the solar neutrino problem , 1992 .

[53]  R. Webb,et al.  Study of penetrating cosmic ray muons and search for large scale anisotropies at the Gran Sasso Laboratory , 1990 .

[54]  H. Becker,et al.  Astrophysical S(E) factor of 3He(3He, 2p)4He at solar energies , 1987 .

[55]  G. Bogaert,et al.  Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars☆ , 1987 .

[56]  H. Mak,et al.  Measurement of the absolute cross section of the 3He(4He, γ)7Be reaction at Ec.m. = 525 keV , 1984 .

[57]  F. Ajzenberg-Selove,et al.  Energy Levels of Light Nuclei A = 9 , 1984 .

[58]  R. Santo,et al.  Activation measurement of the3He(4He,γ)7Be reaction , 1983 .

[59]  P. Schmalbrock,et al.  The3He(α,γ)7Be reaction and the solar neutrino problem , 1982 .

[60]  J. Zyskind,et al.  Low-Energy He-3 (alpha, gamma) Be-7 Cross-Section Measurements , 1982 .

[61]  V. N. Fetisov,et al.  Solar neutrinos and experiments to search for the hypothetical level in 6Be , 1975 .

[62]  M. R. Dwarakanath He-3 (He-3, He-2p) He-4 and the termination of the proton-proton chain , 1974 .

[63]  W. Fowler What Cooks with Solar Neutrinos ? , 1972, Nature.

[64]  M. R. Dwarakanath,et al.  He 3 ( He 3 , 2 p ) He 4 Total Cross-Section Measurements Below the Coulomb Barrier , 1971 .

[65]  M. R. Dwarakanath,et al.  The 3He(α, γ)7Be reaction at very low energy , 1969 .

[66]  P. Parker,et al.  He 3 ( α , γ ) Be 7 Reaction , 1963 .

[67]  T. H. Kruse,et al.  Nuclear Electric Monopole Transitions in O16, Ca40, Ge72, and Zr90 , 1962 .

[68]  A. Dell'Acqua,et al.  Geant4 - A simulation toolkit , 2003 .

[69]  B. A. Brown,et al.  Asymptotic normalization coefficients for 14 N ¿ p \ 15 O and the astrophysical S factor for 14 N „ p , g ... 15 , 2003 .

[70]  Scilla Degl'Innocenti,et al.  Solar neutrinos and nuclear reactions in the solar interior , 1992 .

[71]  C. Maggiore,et al.  Cross section of the capture reaction /sup 3/He(. cap alpha. ,. gamma. ) /sup 7/Be , 1983 .