NSR Query Results
Output year order : Descending NSR database version of May 2, 2024. Search: Author = M.Fortin Found 8 matches. 2022SU24 Phys.Rev. C 106, 035805 (2022) L.Suleiman, M.Fortin, J.L.Zdunik, C.Providencia Polytropic fits of modern and unified equations of state
doi: 10.1103/PhysRevC.106.035805
2021SU16 Phys.Rev. C 104, 015801 (2021) L.Suleiman, M.Fortin, J.L.Zdunik, P.Haensel Influence of the crust on the neutron star macrophysical quantities and universal relations
doi: 10.1103/PhysRevC.104.015801
2018MA58 Phys.Rev. C 98, 035804 (2018) T.Malik, N.Alam, M.Fortin, C.Providencia, B.K.Agrawal, T.K.Jha, B.Kumar, S.K.Patra GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability
doi: 10.1103/PhysRevC.98.035804
2017FO12 Phys.Rev. C 95, 065803 (2017) M.Fortin, S.S.Avancini, C.Providencia, I.Vidana Hypernuclei and massive neutron stars NUCLEAR STRUCTURE 6He; calculated binding energy of double-Λ 6He hypernucleus as a calibrant using several different models, and compared to experimental data. Construction of unified hyperonic EoS for massive neutron stars with limited number of constraints set by phenomenological models.
doi: 10.1103/PhysRevC.95.065803
2016AL25 Phys.Rev. C 94, 052801 (2016) N.Alam, B.K.Agrawal, M.Fortin, H.Pais, C.Providencia, Ad.R.Raduta, A.Sulaksono Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation
doi: 10.1103/PhysRevC.94.052801
2016FO18 Phys.Rev. C 94, 035804 (2016) M.Fortin, C.Providencia, Ad.R.Raduta, F.Gulminelli, J.L.Zdunik, P.Haensel, M.Bejger Neutron star radii and crusts: Uncertainties and unified equations of state
doi: 10.1103/PhysRevC.94.035804
2016HA09 Eur.Phys.J. A 52, 59 (2016) P.Haensel, M.Bejger, M.Fortin, L.Zdunik Rotating neutron stars with exotic cores: masses, radii, stability
doi: 10.1140/epja/i2016-16059-4
2010FO12 Phys.Rev. C 82, 065804 (2010) M.Fortin, F.Grill, J.Margueron, D.Page, N.Sandulescu Thermalization time and specific heat of the neutron stars crust
doi: 10.1103/PhysRevC.82.065804
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