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NSR database version of May 2, 2024.

Search: Author = D.Logoteta

Found 19 matches.

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2023VI02      Phys.Rev.Lett. 130, 122501 (2023)

M.Viviani, L.Girlanda, A.Kievsky, D.Logoteta, L.E.Marcucci

Theoretical Study of the d(d, p)3H and d(d, n)3H Processes at Low Energies

NUCLEAR REACTIONS 2H(d, p), (d, n), E(cm)<1 MeV; analyzed available data; deduced astrophysical S factor, the quintet suppression factor, single and double polarized observables, first estimate of the theoretical uncertainty for all these quantities.

doi: 10.1103/PhysRevLett.130.122501
Citations: PlumX Metrics

2022CU06      Eur.Phys.J. A 58, 99 (2022)

M.Cusinato, F.M.Guercilena, A.Perego, D.Logoteta, D.Radice, S.Bernuzzi, S.Ansoldi

Neutrino emission from binary neutron star mergers: characterising light curves and mean energies

doi: 10.1140/epja/s10050-022-00743-5
Citations: PlumX Metrics

2022LO04      Eur.Phys.J. A 58, 55 (2022)

D.Logoteta, I.Bombaci, A.Perego

Isoentropic equations of state of β-stable hadronic matter with a quark phase transition

doi: 10.1140/epja/s10050-022-00708-8
Citations: PlumX Metrics

2022LO07      Phys.Rev. C 105, 055808 (2022)

A.Lovato, I.Bombaci, D.Logoteta, M.Piarulli, R.B.Wiringa

Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials

doi: 10.1103/PhysRevC.105.055808
Citations: PlumX Metrics

2022PE10      Phys.Rev.Lett. 129, 032701 (2022)

A.Perego, D.Logoteta, D.Radice, S.Bernuzzi, R.Kashyap, A.Das, S.Padamata, A.Prakash

Probing the Incompressibility of Nuclear Matter at Ultrahigh Density through the Prompt Collapse of Asymmetric Neutron Star Binaries

doi: 10.1103/PhysRevLett.129.032701
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2022VI05      Phys.Rev. C 106, 035804 (2022)

I.Vidana, D.Logoteta, I.Bombaci

Effect of chiral nuclear forces on the neutrino mean free path in hot neutron matter

doi: 10.1103/PhysRevC.106.035804
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2021BO11      Phys.Rev.Lett. 126, 162702 (2021)

I.Bombaci, A.Drago, D.Logoteta, G.Pagliara, I.Vidana

Was GW190814 a Black Hole-Strange Quark Star System?

doi: 10.1103/PhysRevLett.126.162702
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2020PI05      Phys.Rev. C 101, 045801 (2020)

M.Piarulli, I.Bombaci, D.Logoteta, A.Lovato, R.B.Wiringa

Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions

doi: 10.1103/PhysRevC.101.045801
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2019LO10      Eur.Phys.J. A 55, 133 (2019)

D.Logoteta

Constraints on hybrid neutron stars equation of state from neutron stars merging

doi: 10.1140/epja/i2019-12819-x
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2019LO13      Phys.Rev. C 100, 045803 (2019)

D.Logoteta

Consistent nuclear matter calculations with local three-nucleon interactions

NUCLEAR STRUCTURE 3H; calculated binding energy and the Gamow-Teller matrix element in 3H β- decay. Microscopic Brueckner-Hartree-Fock approach using interactions in chiral perturbation theory at next-to-next-to-next-to-leading order (N3LO) for the nucleon-nucleon (NN) force, and next-to-next-to leading order (N2LO) for the nucleon-nucleon-nucleon (NNN) force. Comparison with pure neutron matter (PNM) and symmetric neutron matter (SNM) calculations.

doi: 10.1103/PhysRevC.100.045803
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2019LO15      Eur.Phys.J. A 55, 207 (2019)

D.Logoteta, I.Vidana, I.Bombaci

Impact of chiral hyperonic three-body forces on neutron stars

doi: 10.1140/epja/i2019-12909-9
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2018KI09      Phys.Rev.Lett. 121, 072701 (2018)

A.Kievsky, M.Viviani, D.Logoteta, I.Bombaci, L.Girlanda

Correlations imposed by the unitary limit between few-nucleon systems, nuclear matter, and neutron stars

doi: 10.1103/PhysRevLett.121.072701
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2018LO15      Eur.Phys.J. A 54, 111 (2018)

D.Logoteta

Optimized chiral N2LO interactions in nuclear matter

doi: 10.1140/epja/i2018-12547-9
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2016BO07      Eur.Phys.J. A 52, 58 (2016)

I.Bombaci, D.Logoteta, I.Vidana, C.Providencia

Quark matter nucleation in neutron stars and astrophysical implications

doi: 10.1140/epja/i2016-16058-5
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2016LO17      Phys.Rev. C 94, 064001 (2016)

D.Logoteta, I.Bombaci, A.Kievsky

Nuclear matter properties from local chiral interactions with Δ isobar intermediate states

doi: 10.1103/PhysRevC.94.064001
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2015LO06      Phys.Rev. C 91, 064001 (2015)

D.Logoteta, I.Vidana, I.Bombaci, A.Kievsky

Comparative study of three-nucleon force models in nuclear matter

NUCLEAR STRUCTURE 3H, 3,4He; calculated Energy per particle E/A of nuclear and pure neutron matter, binding energies of 3H, 3,4He, neutron-deuteron doublet scattering length, and symmetry energy. Microscopic many-body Brueckner-Hartree-Fock (BHF) approach with Argonne V18 (AV18) nucleon-nucleon (NN) potential using two three-nucleon force models.

doi: 10.1103/PhysRevC.91.064001
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2013LO11      Nucl.Phys. A914, 433c (2013)

D.Logoteta, I.Vidana, C.Providencia

Two-meson exchange hyperonic three-body forces and consequences for neutron stars

doi: 10.1016/j.nuclphysa.2013.01.022
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2013LO14      Phys.Rev. C 88, 055802 (2013)

D.Logoteta, C.Providencia, I.Vidana

Formation of hybrid stars from metastable hadronic stars

doi: 10.1103/PhysRevC.88.055802
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2012LO06      Phys.Rev. C 85, 055807 (2012)

D.Logoteta, C.Providencia, I.Vidana, I.Bombaci

Quark matter nucleation with a microscopic hadronic equation of state

doi: 10.1103/PhysRevC.85.055807
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