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NSR database version of April 11, 2024.

Search: Author = S.Postnikov

Found 2 matches.

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2016SA24      Phys.Rev. C 93, 055801 (2016)

I.Sagert, G.I.Fann, F.J.Fattoyev, S.Postnikov, C.J.Horowitz

Quantum simulations of nuclei and nuclear pasta with the multiresolution adaptive numerical environment for scientific simulations

NUCLEAR STRUCTURE 16O, 208Pb, 238U; calculated nuclear ground states, binding energies, shapes of light and heavy nuclei with different geometries with and without spin-orbit forces via three-dimensional (3D) Skyrme Hartree-Fock (SHF) simulations of nuclear pasta with Multi-resolution ADaptive Numerical Environment for Scientific Simulations (MADNESS); deduced that pasta phase remains in waffle geometry. Relevance to exotic shapes of neutron star and supernova matter.

doi: 10.1103/PhysRevC.93.055801
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2008CA24      Phys.Rev. C 78, 045805 (2008)

O.L.Caballero, S.Postnikov, C.J.Horowitz, M.Prakash

Shear viscosity of the outer crust of neutron stars: Ion contributions

doi: 10.1103/PhysRevC.78.045805
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