NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of May 2, 2024.

Search: Author = O.Pisanti

Found 7 matches.

Back to query form


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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1998BO25      Prog.Theor.Phys.(Kyoto) 99, 1017 (1998)

C.Bourrely, F.Buccella, O.Pisanti, P.Santorelli, J.Soffer

Polarized Quarks, Gluons and Sea in Nucleon Structure Functions

NUCLEAR REACTIONS 1H(e, e'X), E not given; analyzed data; deduced structure function parameters, relative merits of spin crisis solutions.

doi: 10.1143/PTP.99.1017
Citations: PlumX Metrics

1996BU28      Nuovo Cim. 109A, 159 (1996)

F.Buccella, O.Pisanti, P.Santorelli, J.Soffer

Does One Need the Anomaly to Describe the Polarized Structure Functions ( Question )

NUCLEAR STRUCTURE 1n, 2,1H; calculated polarized structure functions.

doi: 10.1007/BF02730943
Citations: PlumX Metrics

1995AC03      Nuovo Cim. 108A, 375 (1995)

F.Acampora, G.Amelino-Camelia, F.Buccella, O.Pisanti, L.Rosa, T.Tuzi

Proton Decay and Neutrino Masses in SO(10)

doi: 10.1007/BF02787063
Citations: PlumX Metrics

Back to query form