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NSR database version of April 27, 2024.

Search: Author = P.S.Shternin

Found 5 matches.

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2022SH12      Eur.Phys.J. A 58, 42 (2022)

P.Shternin, D.Ofengeim

Transport coefficients of magnetized neutron star cores

doi: 10.1140/epja/s10050-022-00687-w
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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), R_n 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
Citations: PlumX Metrics

Note: The following list of authors and aliases matches the search parameter P.S.Shternin: , P.S.SHTERNIN