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NSR database version of April 27, 2024.

Search: Author = V.Castellani

Found 4 matches.

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2003PI13      Nucl.Phys. A718, 496c (2003)

R.G.Pizzone, C.Spitaleri, M.Lattuada, A.Musumarra, M.G.Pellegriti, S.Romano, A.Tumino, S.Cherubini, P.Figuera, D.Miljanic, C.Rolfs, S.Typel, H.H.Wolter, V.Castellani, S.Degl'Innocenti, A.Imperio

Bare astrophysical S(E)-factor for the 6Li(d, α)4He and 7Li(p, α)4He reactions at astrophysical energies

NUCLEAR REACTIONS 6Li(d, α), 7Li(p, α), E(cm) ≈ 10-1000 keV; analyzed astrophysical S-factors, electron screening potential energy.

doi: 10.1016/S0375-9474(03)00868-6
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2003PI14      Nucl.Phys. B(Proc.Supp.) S118, 455 (2003)

R.G.Pizzone, C.Spitaleri, M.Lattuada, A.Musumarra, M.G.Pellegriti, C.Rolfs, D.Miljanic, A.Di Pietro, P.Figuera, S.Romano, S.Tudisco, A.Tumino, S.Typel, H.H.Wolter, V.Castellani, S.Degl'Innocenti, A.Imperio

The 7Li(p, α)4He fusion reaction studied via the Trojan Horse Method and its astrophysical implications

NUCLEAR REACTIONS 7Li(d, 2α), E not given; measured not given. 7Li(p, α), E=low; deduced astrophysical S-factor, electron screening potential.

doi: 10.1016/S0920-5632(03)01356-2
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1996CA17      Z.Phys. A354, 237 (1996)

V.Castellani, G.Fiorentini, B.Ricci, O.Straniero

The Fate of Li and Be in Stars and the Laboratory

NUCLEAR REACTIONS 6,7Li, 9Be(p, X), E not given; calculated reactivity N(A)<σv> vs temperature, other aspects; deduced Li, Be fate in stars and reproducibility in laboratory related futures.

doi: 10.1007/s002180050040
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1994CA19      Phys.Lett. 324B, 425 (1994)

V.Castellani, S.Degl'Innocenti, G.Fiorentini, M.Lissia, B.Ricci

Future Solar Neutrino Spectroscopy and Neutrino Properties

doi: 10.1016/0370-2693(94)90217-8
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