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NSR database version of May 2, 2024.

Search: Author = O.G.Benvenuto

Found 5 matches.

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2023BA12      Phys.Rev. C 107, 065804 (2023)

E.Bauer, J.Torres Patino, O.G.Benvenuto

Neutrino mean free path for proto--neutron star matter within the Skyrme model

doi: 10.1103/PhysRevC.107.065804
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2023BE12      Eur.Phys.J. A 59, 159 (2023)

O.G.Benvenuto, E.Bauer, I.Vidana

Hot and highly magnetized neutron star matter properties with Skyrme interactions

doi: 10.1140/epja/s10050-023-01070-z
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2021BE22      Phys.Rev. C 104, 025801 (2021)

O.G.Benvenuto, E.Bauer

Contributions from Λ hyperons to nucleosynthesis in kilonovae

NUCLEAR STRUCTURE A=15-240; calculated abundances for the most abundant isotopes resulting from the expansion of matter resulting from the collision of neutron stars or neutron start and a black hole using a network of 3298 isotopes, and weak decays of Λ hyperons, applied to nucleosynthesis in kilonovae, using equation of state (EOS) with the presence of Λ hyperons.

doi: 10.1103/PhysRevC.104.025801
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1998LU13      Phys.Rev. D58, 083001 (1998)

G.Lugones, O.G.Benvenuto

Effect of Trapped Neutrinos in the Hadron Matter to Quark Matter Transition

doi: 10.1103/PhysRevD.58.083001
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1997BE24      Phys.Scr. 55, 550 (1997)

O.G.Benvenuto, O.Civitarese, M.Reboiro

Temperature Dependence of the Nuclear Binding Energy: Effects on the EOS for hot nuclear matter using different models

NUCLEAR STRUCTURE ²⁰⁸Pb, ¹¹⁶Sn, ⁴⁰Ca; calculated binding energy vs temperature. Hot nuclear matter, equation of state, liquid drop model based temperature dependent terms.

doi: 10.1088/0031-8949/55/5/007
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