NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.Oertel Found 26 matches. 2023SU13 Phys.Rev. C 108, 035803 (2023) L.Suleiman, M.Oertel, M.Mancini Modified Urca neutrino emissivity at finite temperature
doi: 10.1103/PhysRevC.108.035803
2022AN24 Eur.Phys.J. A 58, 254 (2022) D.Antonopoulou, E.Bozzo, C.Ishizuka, D.I.Jones, M.Oertel, C.Providencia, L.Tolos, S.Typel CompOSE: a repository for neutron star equations of state and transport properties
doi: 10.1140/epja/s10050-022-00908-2
2022TY01 Eur.Phys.J. A 58, 221 (2022) S.Typel, M.Oertel, T.Klahn, D.Chatterjee, V.Dexheimer, C.Ishizuka, M.Mancini, J.Novak, H.Pais, C.Providencia, Ad.R.Raduta, M.Servillat, L.Tolos, for the CompOSE Core Collaboration CompOSE reference manual
doi: 10.1140/epja/s10050-022-00847-y
2021CH49 Eur.Phys.J. A 57, 249 (2021) D.Chatterjee, J.Novak, M.Oertel Structure of ultra-magnetised neutron stars
doi: 10.1140/epja/s10050-021-00525-5
2021KH02 Phys.Rev. C 103, 055811 (2021) S.Khadkikar, A.R.Raduta, M.Oertel, A.Sedrakian Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
doi: 10.1103/PhysRevC.103.055811
2021RA33 Eur.Phys.J. A 57, 329 (2021) Equations of state for hot neutron stars
doi: 10.1140/epja/s10050-021-00628-z
2020OE01 Phys.Rev. C 102, 035802 (2020) M.Oertel, A.Pascal, M.Mancini, J.Novak Improved neutrino-nucleon interactions in dense and hot matter for numerical simulations
doi: 10.1103/PhysRevC.102.035802
2020PA01 Phys.Rev. C 101, 015803 (2020) A.Pascal, S.Giraud, A.F.Fantina, F.Gulminelli, J.Novak, M.Oertel, A.R.Raduta Impact of electron capture rates for nuclei far from stability on core-collapse supernovae NUCLEAR STRUCTURE Z=10-60, N=20-114; Z=15-55, N-16-90; calculated electron-capture (EC) rates for ≈170 different nuclear species around 86Kr using self-consistent numerical simulations of core-collapse supernovae (CCSN), with hydrodynamic codes COCONUT and ACCEPT.
doi: 10.1103/PhysRevC.101.015803
2019CH22 Phys.Rev. C 99, 055811 (2019) D.Chatterjee, J.Novak, M.Oertel Magnetic field distribution in magnetars
doi: 10.1103/PhysRevC.99.055811
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
2017RA02 Phys.Rev. C 95, 025805 (2017) Ad.R.Raduta, F.Gulminelli, M.Oertel Stellar electron capture rates on neutron-rich nuclei and their impact on stellar core collapse
doi: 10.1103/PhysRevC.95.025805
2016OE01 Eur.Phys.J. A 52, 50 (2016) M.Oertel, F.Gulminelli, C.Providencia, A.R.Raduta Hyperons in neutron stars and supernova cores
doi: 10.1140/epja/i2016-16050-1
2016RA05 Phys.Rev. C 93, 025803 (2016) Ad.R.Raduta, F.Gulminelli, M.Oertel Modification of magicity toward the dripline and its impact on electron-capture rates for stellar core collapse NUCLEAR STRUCTURE A=17-80; calculated electron capture rates in stellar environment using extended nuclear statistical equilibrium (NSE) model, possible quenching of N=50 and N=82 shell closures on the electron-capture rates during core collapse. Z=27-68, N=28-98; calculated S(2n) using different mass models and compared with experimental data. Z=10-70, N=10-70; calculated proton and neutron numbers of A≥20 nuclei produced in core-collapsing solar systems as a function of baryonic density. Z<80, N<100; calculated nuclear abundances and compared with experimental mass measurements. Z=22, N=5-65; Z=26, N=10-80; Z=30, N=20-95; Z=36, N=20-100; Z=40, N=20-110; Z=44, N=30-120; calculated LDM-shifted binding energies as function of neutron number for isotopes strongly populated during stellar core collapse. Discussed impact of nuclear binding energies on nuclear abundances, and effect of nuclear structure far from stability on electron-capture probabilities.
doi: 10.1103/PhysRevC.93.025803
2013GU18 Phys.Rev. C 87, 055809 (2013) F.Gulminelli, Ad.R.Raduta, M.Oertel, J.Margueron Strangeness-driven phase transition in (proto-)neutron star matter
doi: 10.1103/PhysRevC.87.055809
2012GU17 Phys.Rev. C 86, 025805 (2012) F.Gulminelli, Ad.R.Raduta, M.Oertel Phase transition toward strange matter
doi: 10.1103/PhysRevC.86.025805
2012OE01 Phys.Rev. C 85, 055806 (2012) M.Oertel, A.F.Fantina, J.Novak Extended equation of state for core-collapse simulations
doi: 10.1103/PhysRevC.85.055806
2011DI14 Phys.Rev. C 84, 045801 (2011) Collective excitations in the neutron star inner crust
doi: 10.1103/PhysRevC.84.045801
2007VA15 Nucl.Phys. A791, 422 (2007) T.Varin, D.Davesne, M.Oertel, M.Urban How to preserve symmetries with cut-off regularized integrals?
doi: 10.1016/j.nuclphysa.2007.05.003
2005BU22 Czech.J.Phys. 55, 521 (2005) Color superconductivity in cold dense quark matter
doi: 10.1007/s10582-005-0058-2
2003CH28 Phys.Lett. B 563, 61 (2003) G.Chanfray, M.Ericson, M.Oertel In-medium modification of the isovector pion-nucleon amplitude
doi: 10.1016/S0370-2693(03)00596-3
2003DA01 Eur.Phys.J. A 16, 35 (2003) A consistent approximation scheme beyond RPA for bosons
doi: 10.1140/epja/i2002-10075-y
2003NE05 Nucl.Phys. A714, 481 (2003) F.Neumann, M.Buballa, M.Oertel Mixed phases of color superconducting quark matter
doi: 10.1016/S0375-9474(02)01371-4
2002BU15 Nucl.Phys. A703, 770 (2002) Color-Flavor Unlocking and Phase Diagram with Self-Consistently Determined Strange-Quark Masses
doi: 10.1016/S0375-9474(01)01674-8
2000OE04 Nucl.Phys. A676, 247 (2000) M.Oertel, M.Buballa, J.Wambach Meson Properties in the 1/Nc-Corrected NJL Model
doi: 10.1016/S0375-9474(00)00198-6
1999BU15 Phys.Lett. 457B, 261 (1999) Strange Quark Matter with Dynamically Generated Quark Masses
doi: 10.1016/S0370-2693(99)00533-X
1998BU24 Nucl.Phys. A642, 39c (1998) Quark Droplets in the NJL Mean Field
doi: 10.1016/S0375-9474(98)00496-5
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