NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = I.Sagert Found 6 matches. 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
2014FI04 Eur.Phys.J. A 50, 46 (2014) T.Fischer, M.Hempel, I.Sagert, Y.Suwa, J.Schaffner-Bielich Symmetry energy impact in simulations of core-collapse supernovae
doi: 10.1140/epja/i2014-14046-5
2012SA48 Phys.Rev. C 86, 045802 (2012) I.Sagert, L.Tolos, D.Chatterjee, J.Schaffner-Bielich, C.Sturm Soft nuclear equation-of-state from heavy-ion data and implications for compact stars
doi: 10.1103/PhysRevC.86.045802
2009LI69 Nucl.Phys. A827, 573c (2009) M.Liebendorfer, T.Fischer, M.Hempel, A.Mezzacappa, G.Pagliara, I.Sagert, J.Schaffner-Bielich, S.Scheidegger, F.-K.Thielemann, S.C.Whitehouse Supernovae as Nuclear and Particle Physics Laboratories
doi: 10.1016/j.nuclphysa.2009.05.126
2008SA10 J.Phys.(London) G35, 014053 (2008) I.Sagert, M.Wietoska, J.Schaffner-Bielich, C.Sturm Is a soft nuclear equation of state extracted from heavy-ion data incompatible with pulsar data?
doi: 10.1088/0954-3899/35/1/014053
2008SA11 J.Phys.(London) G35, 014062 (2008) Pulsar kicks by anisotropic neutrino emission from quark matter
doi: 10.1088/0954-3899/35/1/014062
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