NSR Query Results


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NSR database version of May 2, 2024.

Search: Author = M.Fortin

Found 8 matches.

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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
Citations: PlumX Metrics


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
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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
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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
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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
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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
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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
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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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