NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = P.Shternin Found 5 matches. 2022SH12 Eur.Phys.J. A 58, 42 (2022) Transport coefficients of magnetized neutron star cores
doi: 10.1140/epja/s10050-022-00687-w
2018LA06 Astrophys.J. 859, 62 (2018) R.Lau, M.Beard, S.S.Gupta, H.Schatz, A.V.Afanasjev, E.F.Brown, A.Deibel, L.R.Gasques, G.W.Hitt, W.R.Hix, L.Keek, P.Moller, P.S.Shternin, A.W.Steiner, M.Wiescher, Y.Xu Nuclear Reactions in the Crusts of Accreting Neutron Stars
doi: 10.3847/1538-4357/aabfe0
2018ME05 J.Phys.(London) G45, 093001 (2018) Z.Meisel, A.Deibel, L.Keek, P.Shternin, J.Elfritz Nuclear physics of the outer layers of accreting neutron stars
doi: 10.1088/1361-6471/aad171
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
2012SH23 Phys.Rev. C 86, 015808 (2012) P.S.Shternin, M.Beard, M.Wiescher, D.G.Yakovlev Neutron degeneracy and plasma physics effects on radiative neutron captures in neutron star crust NUCLEAR REACTIONS 38Mg(n, γ), E<1.5 MeV; 39Mg(n, γ), E<0.1 MeV; 46Mg(n, γ), E<6 MeV; 62Ca(n, γ), E<10 MeV; calculated astrophysical σ(E), Rn ratios (Fermi-Dirac to Maxwell-Boltzmann cross sections), forward and inverse reaction rates in dense stellar medium with consideration of effects of plasma physics and neutron degeneracy in neutron star crust.
doi: 10.1103/PhysRevC.86.015808
Back to query form Note: The following list of authors and aliases matches the search parameter P.Shternin: , P.S.SHTERNIN |