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NSR database version of April 11, 2024.

Search: Author = G.Mangano

Found 10 matches.

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2017GR16      Phys.Rev. C 96, 045807 (2017)

A.Grassi, G.Mangano, L.E.Marcucci, O.Pisanti

α + d → 6Li + γ astrophysical S factor and its implications for Big Bang nucleosynthesis

NUCLEAR REACTIONS 2H(α, 6Li), E(cm)<7 MeV; calculated phase shifts for every partial wave, partial astrophysical S(E) factors, total astrophysical S(E) factors for five potential models. Comparison with available experimental data.

NUCLEAR STRUCTURE 6Li; calculated binding energy, s-state ANC, magnetic dipole moment, electric quadrupole moment using five different potential models, and compared with available experimental data. 6Li; deduced effect of S-factor prediction on the primordial abundance of 6Li using the code PArthENoPE. Two-body framework for α+d radiative capture, with the α particle and the deuteron treated as structureless constituent of 6Li.

doi: 10.1103/PhysRevC.96.045807
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2016MA14      Phys.Rev.Lett. 116, 102501 (2016)

L.E.Marcucci, G.Mangano, A.Kievsky, M.Viviani

Implication of the Proton-Deuteron Radiative Capture for Big Bang Nucleosynthesis

NUCLEAR REACTIONS 2H(p, γ), E<1 MeV; calculated S-factor using ab initio approach. Comparison with available data.

doi: 10.1103/PhysRevLett.116.102501
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2009DI03      Phys.Rev.Lett. 102, 232502 (2009)

A.Di Leva, L.Gialanella, R.Kunz, D.Rogalla, D.Schurmann, F.Strieder, M.De Cesare, N.De Cesare, A.D'Onofrio, Z.Fulop, G.Gyurky, G.Imbriani, G.Mangano, A.Ordine, V.Roca, C.Rolfs, M.Romano, E.Somorjai, F.Terrasi

Stellar and Primordial Nucleosynthesis of 7Be: Measurement of 3He(αγ)7Be

NUCLEAR REACTIONS 3He(α, γ), E=700-3000 keV: measured cross sections; deduced astrophysical S-factor.

doi: 10.1103/PhysRevLett.102.232502
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1729. Data from this article have been entered in the XUNDL database. For more information, click here.

2007BE13      Nucl.Instrum.Methods Phys.Res. A574, 83 (2007)

P.Benetti, F.Calaprice, E.Calligarich, M.Cambiaghi, F.Carbonara, F.Cavanna, A.G.Cocco, F.Di Pompeo, N.Ferrari, G.Fiorillo, C.Galbiati, L.Grandi, G.Mangano, C.Montanari, L.Pandola, A.Rappoldi, G.L.Raselli, M.Roncadelli, M.Rossella, C.Rubbia, R.Santorelli, A.M.Szelc, C.Vignoli, Y.Zhao

Measurement of the specific activity of 39Ar in natural argon

RADIOACTIVITY 39Ar(β-); measured specific activity in natural argon.

doi: 10.1016/j.nima.2007.01.106
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2006DE42      Phys.Rev. D 74, 103005 (2006)

A.De Felice, G.Mangano, P.D.Serpico, M.Trodden

Relaxing nucleosynthesis constraints on Brans-Dicke theories

doi: 10.1103/PhysRevD.74.103005
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2005MA27      Nucl.Phys. B(Proc.Supp.) S145, 351 (2005)

G.Mangano, P.D.Serpico

Neutrinos and Primordial Nucleosynthesis

doi: 10.1016/j.nuclphysbps.2005.04.038
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2000ES02      Nucl.Phys. B568, 421 (2000)

S.Esposito, G.Mangano, G.Miele, O.Pisanti

Big Bang Nucleosynthesis: An accurate determination of light element yields

doi: 10.1016/S0550-3213(99)00725-7
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2000ES05      Nucl.Phys. B(Proc.Supp.) S81, 59 (2000)

S.Esposito, G.Mangano, G.Miele, O.Pisanti

Primordial Nucleosynthesis: Accurate predictions

doi: 10.1016/S0920-5632(99)00859-2
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1999ES02      Nucl.Phys. B540, 3 (1999)

S.Esposito, G.Mangano, G.Miele, O.Pisanti

Precision Rates for Nucleon Weak Interactions in Primordial Nucleosynthesis and 4He Abundance

NUCLEAR REACTIONS 1n(ν, e), (e+, ν), 1H(e, ν), (ν, e+), E not given; calculated radiative corrections, thermal effects, weak interactions related features; deduced correction to primordial 4He mass fraction.

doi: 10.1016/S0550-3213(98)00757-3
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1996MA68      Nucl.Phys. B(Proc.Suppl.) S48, 272 (1996)

G.Mangano, L.Rosa

Cosmological Implications of a Class of SO(10) Models

doi: 10.1016/0920-5632(96)00260-5
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