NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = P.Haensel Found 25 matches. 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
2020CH24 Phys.Rev. C 102, 015804 (2020) N.Chamel, A.F.Fantina, J.L.Zdunik, P.Haensel Experimental constraints on shallow heating in accreting neutron-star crusts NUCLEAR REACTIONS 12C(12C, X)24Ne*,16O(16O, X)32Si*, E not given; calculated maximum possible heat released from electron captures and pycnonuclear fusion reactions triggered by the burial of x-ray burst ashes of pure 56Fe or 106Pd, and released heat deposited in the outer crust of accreting neutron star crusts.
doi: 10.1103/PhysRevC.102.015804
2018DE29 Phys.Rev. C 98, 025803 (2018) A.Dehghan Niri, H.R.Moshfegh, P.Haensel Role of nuclear correlations and kinematic effects on neutrino emission from the modified Urca processes
doi: 10.1103/PhysRevC.98.025803
2018GO01 Nucl.Phys. A969, 206 (2018) S.Goudarzi, H.R.Moshfegh, P.Haensel The role of three-body forces in nuclear symmetry energy and symmetry free energy
doi: 10.1016/j.nuclphysa.2017.10.007
2017KH05 Acta Phys.Pol. B48, 661 (2017) A.Khodaie, A.Dehghan Niri, H.R.Moshfegh, P.Haensel Emissivity and Mean-free Paths of Neutrinos in Neutron Star Matter via Modified Urca Processes
doi: 10.5506/APhysPolB.48.661
2016DE13 Phys.Rev. C 93, 045806 (2016) A.Dehghan Niri, H.R.Moshfegh, P.Haensel Nuclear correlations and neutrino emissivity from the neutron branch of the modified Urca process
doi: 10.1103/PhysRevC.93.045806
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
2015CH35 Phys.Rev. C 91, 055803 (2015) N.Chamel, A.F.Fantina, J.L.Zdunik, P.Haensel Neutron drip transition in accreting and nonaccreting neutron star crusts NUCLEAR STRUCTURE 56Ar, 60,64Ca, 66,68Ti, 76Cr, 98,104,106Ge, 105As, 106Se, 121,124,126Sr; calculated neutron drip transition in the dense matter between the outer and inner crusts of accreting neutron stars using three different microscopic Hartree-Fock-Bogoliubov (HFB) nuclear mass models.
doi: 10.1103/PhysRevC.91.055803
2013CH35 Int.J.Mod.Phys. E22, 1330018 (2013); Erratum Int.J.Mod.Phys. E22, 1392004 (2013) N.Chamel, P.Haensel, J.L.Zdunik, A.F.Fantina On the maximum mass of neutron stars
doi: 10.1142/S021830131330018X
2013SH49 Phys.Rev. C 88, 065803 (2013) P.S.Shternin, M.Baldo, P.Haensel Transport coefficients of nuclear matter in neutron star cores
doi: 10.1103/PhysRevC.88.065803
2009GU14 Phys.Rev. C 79, 055806 (2009) M.E.Gusakov, E.M.Kantor, P.Haensel Relativistic entrainment matrix of a superfluid nucleon-hyperon mixture: The zero temperature limit
doi: 10.1103/PhysRevC.79.055806
2009GU19 Phys.Rev. C 80, 015803 (2009) M.E.Gusakov, E.M.Kantor, P.Haensel Relativistic entrainment matrix of a superfluid nucleon-hyperon mixture. II. Effect of finite temperatures
doi: 10.1103/PhysRevC.80.015803
2006CH19 Phys.Rev. C 73, 045802 (2006) Entrainment parameters in a cold superfluid neutron star core
doi: 10.1103/PhysRevC.73.045802
2005CA05 Nucl.Phys. A748, 675 (2005) Entrainment coefficient and effective mass for conduction neutrons in neutron star crust: simple microscopic models
doi: 10.1016/j.nuclphysa.2004.11.006
2005CA36 Nucl.Phys. A759, 441 (2005) Effect of BCS pairing on entrainment in neutron superfluid current in neutron star crust
doi: 10.1016/j.nuclphysa.2005.05.151
2005GU31 Nucl.Phys. A761, 333 (2005) The entrainment matrix of a superfluid neutron-proton mixture at a finite temperature
doi: 10.1016/j.nuclphysa.2005.07.005
2004OL08 Phys.Rev. C 70, 025804 (2004) E.Olsson, P.Haensel, C.J.Pethick Static response of Fermi liquids with tensor interactions
doi: 10.1103/PhysRevC.70.025804
2000DO02 Nucl.Phys. A665, 419 (2000) Nuclear Surface and Curvature Properties for SLy Skyrme Forces and Nuclei in the Inner Neutron-Star Crust
doi: 10.1016/S0375-9474(99)00397-8
1998CH17 Nucl.Phys. A635, 231 (1998); Erratum Nucl.Phys. A643, 441 (1998) E.Chabanat, P.Bonche, P.Haensel, J.Meyer, R.Schaeffer A Skyrme Parametrization from Subnuclear to Neutron Star Densities Part II. Nuclei Far from Stabilities NUCLEAR STRUCTURE Ni, Sn, Pb; calculated binding energies, two-neutron separation energies. Pb; calculated isotopic shifts. 208Pb; calculated single-particle levels. Several Skyrme parametrizations compared.
doi: 10.1016/S0375-9474(98)00180-8
1997CH49 Nucl.Phys. A627, 710 (1997) E.Chabanat, P.Bonche, P.Haensel, J.Meyer, R.Schaeffer A Skyrme Parametrization from Subnuclear to Neutron Star Densities NUCLEAR STRUCTURE 16O, 40,48Ca, 56,78Ni, 100,132Sn, 208Pb; calculated binding energies, radii; deduced parameters. Skyrme parametrization.
doi: 10.1016/S0375-9474(97)00596-4
1995CH57 Phys.Scr. T56, 231 (1995) E.Chabanat, P.Bonche, P.Haensel, J.Meyer, R.Schaeffer New Skyrme Effective Forces for Supernovae and Neutron Rich Nuclei NUCLEAR STRUCTURE 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140Sn; calculated two neutron separation energies. Z=32-78; calculated two proton separation energies. Hartree-Fock plus BCS formalism, new Skyrme-like effective interactions.
doi: 10.1088/0031-8949/1995/T56/034
1975HA16 Nucl.Phys. A245, 29 (1975) The Spin and Isospin Dependence of the Imaginary Part of the Nuclear Optical Model Potential NUCLEAR REACTIONS 120Sn, 59Co(n, n), (p, p), E=40, 100 MeV; calculated spin, isospin dependent terms of optical potential.
doi: 10.1016/0375-9474(75)90080-9
1972DA27 Phys.Lett. 42B, 163 (1972) Spin and Isospin Dependence of the Single-Particle Potential in Nuclear Matter
doi: 10.1016/0370-2693(72)90050-0
1971DA25 Phys.Rev. C4, 1985 (1971) J.Dabrowski, E.Fedorynska, P.Haensel, M.Y.M.Hassan Binding Energy of 3H and n-d-Doublet Scattering Length with Charge-Dependent Forces NUCLEAR STRUCTURE 3H; calculated binding energy, n-d doublet scattering length. Charge-dependent forces.
doi: 10.1103/PhysRevC.4.1985
Back to query form |