NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.Hempel Found 15 matches. 2018EI01 J.Phys.(London) G45, 014001 (2018) M.Eichler, K.Nakamura, T.Takiwaki, T.Kuroda, K.Kotake, M.Hempel, R.Cabezon, M.Liebendorfer, F.-K.Thielemann Nucleosynthesis in 2D core-collapse supernovae of 11.2 and 17.0 M(.) progenitors: implications for Mo and Ru production ATOMIC MASSES 92,94Mo, 96,98Ru; calculated abundances of p-process nuclei.
doi: 10.1088/1361-6471/aa8891
2017DE28 Nucl.Phys. A967, 780 (2017) V.Dexheimer, M.Hempel, I.Iosilevskiy, S.Schramm Phase transitions in dense matter
doi: 10.1016/j.nuclphysa.2017.04.031
2017MA65 Phys.Rev. C 96, 045806 (2017) M.Marques, M.Oertel, M.Hempel, J.Novak New temperature dependent hyperonic equation of state: Application to rotating neutron star models and I-Q relations
doi: 10.1103/PhysRevC.96.045806
2016FI10 Eur.Phys.J. A 52, 225 (2016) Consequences of simultaneous chiral symmetry breaking and deconfinement for the isospin symmetric phase diagram
doi: 10.1140/epja/i2016-16225-8
2015HE13 Phys.Rev. C 91, 045805 (2015) M.Hempel, K.Hagel, J.Natowitz, G.Ropke, S.Typel Constraining supernova equations of state with equilibrium constants from heavy-ion collisions NUCLEAR REACTIONS 112,124Sn(40Ar, X), (64Zn, X), E=47 MeV/nucleon; analyzed experimental data obtained using NIMROD 4π multidetector at Texas A and M University for yields of light particles; deduced temperature and densities, equilibrium constants (ECs) for α, d, t, 3He, mass fraction of heavy nuclei. Cluster formation in heavy-ion collisions, and equation of state (EOS) of warm and dense nuclear matter. Quantum statistical (QS) approach.
doi: 10.1103/PhysRevC.91.045805
2015HE16 Phys.Rev. C 91, 055807 (2015) Nucleon self-energies for supernova equations of state
doi: 10.1103/PhysRevC.91.055807
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
2013BU08 Nucl.Phys. A907, 13 (2013) N.Buyukcizmeci, A.S.Botvina, I.N.Mishustin, R.Ogul, M.Hempel, J.Schaffner-Bielich, F.-K.Thielemann, S.Furusawa, K.Sumiyoshi, S.Yamada, H.Suzuki A comparative study of statistical models for nuclear equation of state of stellar matter
doi: 10.1016/j.nuclphysa.2013.03.010
2013HE17 Phys.Rev. C 88, 014906 (2013) M.Hempel, V.Dexheimer, S.Schramm, I.Iosilevskiy Noncongruence of the nuclear liquid-gas and deconfinement phase transitions
doi: 10.1103/PhysRevC.88.014906
2011HE20 Phys.Rev. C 84, 055804 (2011) M.Hempel, J.Schaffner-Bielich, S.Typel, G.Ropke Light clusters in nuclear matter: Excluded volume versus quantum many-body approaches
doi: 10.1103/PhysRevC.84.055804
2010HE06 Nucl.Phys. A837, 210 (2010) A statistical model for a complete supernova equation of state
doi: 10.1016/j.nuclphysa.2010.02.010
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
2008HE03 J.Phys.(London) G35, 014043 (2008) Mass, radius and composition of the outer crust of nonaccreting cold neutron stars
doi: 10.1088/0954-3899/35/1/014043
2007GU28 Phys.Rev. C 76, 065801 (2007) L.Guo, M.Hempel, J.Schaffner-Bielich, J.A.Maruhn Triaxial nuclear models and the outer crust of nonaccreting cold neutron stars NUCLEAR STRUCTURE Z=20-48, N=24-110; calculated masses, binding energies, deformations. Comparison with experimental values.
doi: 10.1103/PhysRevC.76.065801
2006RU05 Phys.Rev. C 73, 035804 (2006) S.B.Ruster, M.Hempel, J.Schaffner-Bielich Outer crust of nonaccreting cold neutron stars
doi: 10.1103/PhysRevC.73.035804
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