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NSR database version of April 27, 2024.

Search: Author = B.Ricci

Found 12 matches.

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2004DE20      Phys.Lett. B 590, 13 (2004)

S.Degl'Innocenti, G.Fiorentini, B.Ricci, F.L.Villante

The ¹⁴N(p, γ)¹⁵O reaction, solar neutrinos and the age of the globular clusters

NUCLEAR REACTIONS ¹⁴N(p, γ), E=low; analyzed astrophysical S-factor. Implications for solar models and globular cluster dating discussed.

doi: 10.1016/j.physletb.2004.04.003
Citations: PlumX Metrics

2004FI06      Prog.Theor.Phys.(Kyoto), Suppl. 154, 309 (2004)

G.Fiorentini, B.Ricci, F.L.Villante

Nuclear Fusion in the Sun

doi: 10.1143/PTPS.154.309
Citations: PlumX Metrics

2003FI01      Phys.Rev. C 67, 014603 (2003)

G.Fiorentini, C.Rolfs, F.L.Villante, B.Ricci

Fusion rate enhancement due to energy spread of colliding nuclei

NUCLEAR REACTIONS ²H(d, X), E=low; calculated fusion rate enhancement due to energy spread of colliding nuclei.

doi: 10.1103/PhysRevC.67.014603
Citations: PlumX Metrics

2001FI07      Phys.Lett. 503B, 121 (2001)

G.Fiorentini, B.Ricci, F.L.Villante

Helioseismology and Screening of Nuclear Reactions in the Sun

NUCLEAR REACTIONS ¹H, ⁷Be(p, X), ^3,4He(³He, X), E not given; analyzed reaction screening models, consistency with helioseismic data.

doi: 10.1016/S0370-2693(01)00221-0
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1999AN35      Nucl.Phys. A656, 3 (1999)

C.Angulo, M.Arnould, M.Rayet, P.Descouvemont, D.Baye, C.Leclercq-Willain, A.Coc, S.Barhoumi, P.Aguer, C.Rolfs, R.Kunz, J.W.Hammer, A.Mayer, T.Paradellis, S.Kossionides, C.Chronidou, K.Spyrou, S.Degl'Innocenti, G.Fiorentini, B.Ricci, S.Zavatarelli, C.Providencia, H.Wolters, J.Soares, C.Grama, J.Rahighi, A.Shotter, M.Lamehi-Rachti

A Compilation of Charged-Particle Induced Thermonuclear Reaction Rates

COMPILATION ¹H(p, e⁺ν), ²H, ^6,7Li, ^7,9Be, ^10,11B, ^12,13C, ^13,14,15N, ^16,17,18O, ¹⁹F, ^20,21,22Ne, ^22,23Na, ^24,25,26Mg, ^26,27Al, ²⁸Si(p, γ), ²H(d, γ), (d, p), ^2,3H(d, n), ^2,3H, ³He, ⁷Li, ⁷Be, ¹²C, ^14,15N, ^16,18O, ^20,22Ne(α, γ), ³He(³He, 2p), ^6,7Li, ⁹Be, ^10,11B, ^14,15N, ^17,18O, ¹⁹F, ²⁰Ne, ²³Na, ²⁴Mg, ²⁷Al(p, α), ⁷Li, ⁹Be, ¹³C, ¹⁴N, ^17,18O, ^21,22Ne, ²³Na, ^25,26Mg, ²⁷Al(α, n), ⁹Be, ¹¹B, ¹³C, ^14,15N, ¹⁹F, ²³Na(p, n), ⁹Be(p, d), E < 10 MeV; compiled, analyzed σ, S-factors; calculated astrophysical reaction rates vs T₉. Analytical approximations.

doi: 10.1016/S0375-9474(99)00030-5
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1998DE02      Phys.Lett. 416B, 365 (1998)

S.Degl'Innocenti, G.Fiorentini, B.Ricci

Helioseismology and p + p → d + e⁺ + ν(e) in the Sun

NUCLEAR REACTIONS ¹H(p, e⁺), E not given; analyzed helioseismic data; deduced astrophysical S-factor limits with respect to standard solar model.

doi: 10.1016/S0370-2693(97)01197-0
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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
Citations: PlumX Metrics

1996CA47      Nucl.Phys. B(Proc.Suppl.) S48, 343 (1996)

E.Calabresu, G.Fiorentini, M.Lissia, B.Ricci

Intermediate Energy Solar Neutrinos

doi: 10.1016/0920-5632(96)00270-8
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1996FE04      Phys.Lett. 387B, 427 (1996)

N.Ferrari, G.Fiorentini, B.Ricci

The ⁵¹Cr Neutrino Source and Borexino: A desirable marriage

doi: 10.1016/0370-2693(96)01023-4
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1995RI07      Phys.Rev. C52, 1095 (1995)

B.Ricci, S.Degl'Innocenti, G.Fiorentini

Screening of Nuclear Reactions in the Sun and Solar Neutrinos

NUCLEAR REACTIONS ⁹Be, ¹H(p, X), E=solar; ⁴He(α, X), E=solar; calculated solar neutrino production associated enhancement factor vs solar profile. Different screening models.

doi: 10.1103/PhysRevC.52.1095
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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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1992CI06      Phys.Lett. 297B, 197 (1992)

R.Cimiraglia, G.Fiorentini, B.Ricci

Molecular Trapping of Nuclei Produced in Neutrino Capture Reactions

NUCLEAR REACTIONS ⁷¹Ga(ν, e^-), E=solar; calculated fraction of ⁷¹Ge nuclei trapped in molecular GaGe.

doi: 10.1016/0370-2693(92)91092-N
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