| 46 |
Y. Sugahara, H. Toki |
STNP_1994 |
1994 |
Relativistic mean-field theory for unstable nuclei with non-linear σ and ω terms |
Nucl. Phys. A 579, 557
|
Eos |
| 38 |
P.-G. Reinhard et al. |
RPRC_1999 |
1999 |
Shape coexistence and the effective nucleon-nucleon interaction |
Phys. Rev. C 60, 014316
|
Eos |
| 37 |
P.-G. Reinhard and H. Flocard |
RFNP_1995 |
1995 |
Nuclear effective forces and isotope shifts |
Nucl. Phys. A 584, 467
|
Eos |
| 23 |
H. Toki, D. Hirata, Y. Sugahara, K. Sumiyoshi, and I. Tanihata |
THSSN_1995 |
1995 |
Relativistic many body approach for unstable nuclei and supernova |
Nucl. Phys. A 588, 357
|
Eos |
| 22 |
H. S. Köhler |
KNPA_1976 |
1976 |
Skyrme force and the mass formula |
Nucl. Phys. A 258, 301
|
Eos |
| 31 |
M. Hempel and J. Schaffner-Bielich |
HSNP_2010 |
2010 |
Statistical Model for a Complete Supernova Equation of State |
Nucl. Phys. A 837, 210
|
Eos |
| 36 |
P. Danielewicz et J. Lee |
DLNP_2009 |
2009 |
Symmetry Energy I: Semi-Infinite Matter |
Nucl. Phys. A818, 36
|
Eos |
| 15 |
F.J. Fattoyev, C.J. Horowitz, J. Piekarewicz, and G. Shen |
FHPSP_2010 |
2010 |
Relativistic effective interaction for nuclei, giant resonances, and neutron stars |
Phys. Rev. C 82, 055803
|
Eos |
| 45 |
X. Roca-Maza and J. Piekarewicz |
RPPR_2008 |
2008 |
Impact of the symmetry energy on the outer crust of nonaccreting neutron stars |
Phys. Rev. C 78, 025807
|
Eos |
| 44 |
T. Gaitanos et al. |
GNPA_2004 |
2004 |
On the Lorentz structure of the symmetry energy |
Nucl. Phys. A732, 24
|
Eos |
| 42 |
S. Typel, G. Röpke, T. Klähn, D. Blaschke, and H.H. Wolter |
TRKBP_2010 |
2010 |
Composition and thermodynamics of nuclear matter with light clusters |
Phys. Rev. C 81, 015803
|
Eos |
| 41 |
S. Banik, M. Hempel, and D. Bandyopadhyay |
BHB_2014 |
2014 |
New Hyperon Equations of State for Supernovae and Neutron Stars in Density-dependent Hadron Field Theory |
Astrophys.J.Suppl. 214, 22
|
Eos |
| 40 |
S. Balberg and A. Gal |
BGNP_1997 |
1997 |
An effective equation of state for dense matter with strangeness |
Nucl. Phys. A 625, 435
|
Eos |
| 39 |
P. Möller, J.R. Nix, and K.-L. Kratz |
MNKA_1997 |
1997 |
NUCLEAR PROPERTIES FOR ASTROPHYSICAL AND RADIOACTIVE-ION-BEAM APPLICATIONS |
Atomic Data and Nuclear Data Tables 66, 131
|
Eos |
| 35 |
N. K. Glendenning and S. A. Moszkowski |
GMPR_1991 |
1991 |
Reconciliation of neutron star masses and binding of the lambda in hypernuclei |
Phys. Rev. Lett. 67, 2414
|
Eos |
| 34 |
M. Oertel, C. Providencia, F. Gulminelli, A. Raduta |
OPGR_2015 |
2015 |
Hyperons in neutron star matter within relativistic mean-field models |
J. Phys. G 42, 075202
|
Eos |
| 32 |
M. Hempel, T. Fischer, J. Schaffner-Bielich, and M. Liebendörfer |
HFSLA_2012 |
2012 |
New Equations of State in Simulations of Core-Collapse Supernovae |
Astrophys. J. 748, 70
|
Eos |
| 30 |
L. Geng, H. Toki, and J. Meng |
GTMP_2005 |
2005 |
Masses, deformations and charge radii: Nuclear ground-state properties in the relativistic mean field model |
Prog. Theor. Phys. 113, 785
|
Eos |
| 27 |
J. M. Lattimer and F. D. Swesty |
LSNP_1991 |
1991 |
A Generalized equation of state for hot, dense matter |
Nucl. Phys. A 535, 331
|
Eos |
| 26 |
J. Friedrich and P.-G. Reinhard |
FRPR_1986 |
1986 |
Skyrme-force parametrization: Least-squares fit to nuclear ground-state properties |
Phys. Rev. C 33, 335
|
Eos |
| 21 |
H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi |
STOSP_1998 |
1998 |
Relativistic equation of state of nuclear matter for supernova explosion |
Prog. Theor. Phys. 100, 1013
|
Eos |
| 19 |
H. Shen, F. Yang, H. Toki |
SYTP_2006 |
2006 |
Double-Lambda hypernuclei in the relativistic mean-field theory |
Prog. Theor. Phys. 115, 325
|
Eos |
| 17 |
G.A. Lalazissis, S. Raman, and P. Ring |
LRRA_1999 |
1999 |
Ground-State Properties of Even-Even Nuclei in the Relativistic Mean-Field Theory |
Atomic Data and Nuclear Data Tables 71, 1
|
Eos |
| 13 |
F. Gulminelli, A. .R. Raduta and M. Oertel |
GROP_2012 |
2012 |
Phase transition towards strange matter |
Phys. Rev. C 86 , 025805
|
Eos |
| 11 |
F. Grill, H. Pais, C. Providencia, I. Vidana and S. S. Avancini |
GPPVP_2014 |
2014 |
Equation of state and thickness of the inner crust of neutron stars |
Phys. Rev. C 90, 045803
|
Eos |
| 9 |
E. Chabanat |
C_1995 |
1995 |
Interactions effectives pour des conditions extrêmes d'isospin (in french) |
Ph.D. thesis, University Claude Bernard Lyon-1, Lyon, France
|
Eos |
| 5 |
B. K. Agrawal, S. Shlomo and V. Kim Au |
ASKP_2003 |
2003 |
Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models |
Phys. Rev. C 68 , 031304
|
Eos |
| 2 |
A.W. Steiner, M. Hempel, and T. Fischer |
SHF_2013 |
2013 |
Core-collapse supernova equations of state based on neutron star observations |
Astrophys.J. 774,17
|
Eos |
| 1 |
A. Akmal, V. R. Pandharipande and D. G. Ravenhall |
APRP_1998 |
1998 |
The Equation of state of nucleon matter and neutron star structure |
Phys. Rev. C 58, 1804
|
Eos |
| 6 |
B. Peres, M. Oertel and J. Novak |
PONP_2013 |
2013 |
Influence of pions and hyperons on stellar black hole formation |
Phys. Rev. D 87, 043006
|
Eos |
| 29 |
L. Bennour et al. |
BPRC_1989 |
1989 |
Charge distributions of Pb-208, Pb-206, and Tl-205 and the mean-field approximation |
Phys. Rev. C 40 2834
|
Eos |
| 28 |
K. Sumiyoshi, C. Ishizuka, A. Ohnishi, S. Yamada, H. Suzuki |
SIOYA_2009 |
2009 |
Emergence of hyperons in failed supernovae: trigger of the black hole formation |
Astrophys.J. 690 L43
|
Eos |
| 25 |
I. Sagert, T. Fischer, M. Hempel, G. Pagliara, J. Schaffner-Bielich, F.-K. Thielemann, M. Liebendörfer |
SFHPJ_2010 |
2010 |
Strange quark matter in explosive astrophysical systems |
Journ. of Phys. G 37, 094064
|
Eos |
| 24 |
I. Sagert, T. Fischer, M. Hempel, G. Pagliara, J. Schaffner-Bielich, A. Mezzacappa, F.-K. Thielemann, M. Liebendörfer |
SFHPP_2009 |
2009 |
Signals of the QCD phase transition in core-collapse supernovae |
Phys. Rev. Lett. 102, 081101
|
Eos |
| 20 |
H. Shen, H. Toki, K. Oyamatsu, K. Sumiyoshi |
STOSN_1998 |
1998 |
Relativistic equation of state of nuclear matter for supernova and neutron star |
Nucl. Phys. A 637, 435
|
Eos |
| 18 |
G. Baym, C. Pethick and P. Sutherland |
BPSA_1971 |
1971 |
The Ground state of matter at high densities: Equation of state and stellar models |
Astrophys. J. 170, 299
|
Eos |
| 16 |
G.A. Lalazissis, J. König, and P. Ring |
LKRP_1997 |
1997 |
A New parametrization for the Lagrangian density of relativistic mean field theory |
Phys. Rev. C 55, 540
|
Eos |
| 14 |
F. Gulminelli, A. .R. Raduta, M. Oertel and J. Margueron |
GROMP_2013 |
2013 |
Strangeness-driven phase transition in (proto-)neutron star matter |
Phys. Rev. C 87, 05580
|
Eos |
| 12 |
F. Gulminelli and Ad. R. Raduta |
GR_2015 |
2015 |
Unified treatment of subsaturation stellar matter at zero and finite temperature |
Phys. Rev. C 92, 055803
|
Eos |
| 10 |
F. Douchin, P. Haensel |
DHA_2001 |
2001 |
A unified equation of state of dense matter and neutron star structure |
Astronomy and Astrophysics 380, 151
|
Eos |
| 8 |
E. Chabanat et al. |
CNPA_1997 |
1997 |
A Skyrme parametrization from subnuclear to neutron star densities |
Nucl. Phys. A 627, 710
|
Eos |
| 7 |
C. Ishizuka, A. Ohnishi, K. Tsubakihara, K. Sumiyoshi, S. Yamada |
IOTSJ_2008 |
2008 |
Tables of Hyperonic Matter Equation of State for Core-Collapse Supernovae |
Journ. of Phys. G 35 085201
|
Eos |
| 4 |
B. K. Agrawal, S. Shlomo and V. Kim Au |
ASKP_2005 |
2005 |
Determination of the parameters of a Skyrme type effective interaction using the simulated annealing approach |
Phys. Rev. C 72 , 014310
|
Eos |
| 3 |
B.G. Todd-Rutel and J. Piekarewicz |
TPPR_2005 |
2005 |
Neutron-Rich Nuclei and Neutron Stars: A New Accurately Calibrated Interaction for the Study of Neutron-Rich Matter |
Phys. Rev. Lett. 95 , 122501
|
Eos |
| 43 |
T. Fischer, I. Sagert, G. Pagliara, M. Hempel, J. Scahaffner-Bielich, T. Rauscher, F.-K. Thielemann, R. Kappeli, G. Martinez-Pinedo, M. Liebendörfer |
FSPHA_2011 |
2011 |
Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase |
ApJ Suppl. 194, 39
|
Eos |
| 48 |
G. Shen, C.J. Horowitz, S. Teige |
SHT_2011 |
2011 |
A New Equation of State for Astrophysical Simulations |
Phys.Rev. C83, 035802
|
Eos |
| 47 |
G. Shen, C.J. Horowitz, E. O'Connor |
SHO_2011 |
2011 |
A Second Relativistic Mean Field and Virial Equation of State for Astrophysical Simulations |
Phys.Rev. C83, 065808
|
Eos |
| 33 |
M. Oertel, A. F. Fantina and J. Novak |
OFNP_2012 |
2012 |
An extended equation of state for core-collapse simulations |
Phys. Rev. C 85, 055806
|
Eos |
| 60 |
H. Shen, H. Toki, K. Oyamatsu , K. Sumiyoshi |
STOS_2011 |
2011 |
Relativistic Equation of State for Core-Collapse Supernova Simulations |
Astrophys.J.Suppl. 197, 20
|
Eos |
| 51 |
H. Togashi, K. Nakazato, Y. Takehara, S. Yamamuro, H. Suzuki and M. Takano |
TNTYST_17 |
2017 |
Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces |
Nucl. Phys. A 961, 78
|
Eos |
| 52 |
S. Furusawa, H. Togashi, H. Nagakura, K. Sumiyoshi, S. Yamada, H. Suzuki & M. Takano |
FTNS_2017 |
2017 |
A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble |
J. Phys. G 44,9
|
Eos |
| 53 |
Shun Furusawa, Kohsuke Sumiyoshi, Shoichi Yamada, Hideyuki Suzuki. |
FYSS_2017 |
2017 |
Supernova equations of state including full nuclear ensemble with in-medium effects |
Nucl. Phys. A 957, 188.
|
Eos |
| 54 |
S. Furusawa, K. Sumiyoshi, S. Yamada, and H. Suzuki |
FYSS_2013 |
2013 |
New equations of state based on the liquid drop model of heavy nuclei and quantum approach to light nuclei for core-collapse supernova simulations |
Astrophys. J. 772,95
|
Eos |
| 55 |
S. Furusawa, S. Yamada, K. Sumiyoshi, and H. Suzuki |
FYSS_2011 |
2011 |
A new baryonic equation of state at sub-nuclear densities for core-collapse simulations |
Astrophys. J 738,178
|
Eos |
| 56 |
V. Dexheimer and S. Schramm |
DS_2008 |
2008 |
Proto-Neutron and Neutron Stars in a Chiral SU(3) Model |
Astrophys. J. 683, 943
|
Eos |
| 57 |
T. Schurhoff, S. Schramm, V. Dexheimer |
SSD_2010 |
2010 |
Neutron stars with small radii - the role of Delta resonances |
Astrophys. J. 724, L74
|
Eos |
| 58 |
V. Dexheimer, R. Negreiros , S. Schramm |
DNS_2015 |
2015 |
Reconciling Nuclear and Astrophysical Constraints |
Phys. Rev. C 92, no. 1, 012801
|
Eos |
| 49 |
M. Marques, M. Oertel, M. Hempel, J. Novak |
MOHN_17 |
2017 |
A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations |
Phys.Rev. C96, 045806
|
Eos |
| 61 |
M. Baldo, I. Bombaci and F. Burgio |
BBB_1997 |
1997 |
Microscopic nuclear equation of state with three-body forces and neutron star structure |
Astron.Astrophys. 328, 274
|
Eos |
| 62 |
V. Dexheimer |
DEX_2017 |
2017 |
Tabulated Neutron Star Equations of State Modelled within the Chiral Mean Field Model |
Publications of the Astronomical Society of Australia 34
|
Eos |
| 63 |
I. Bombaci and D. Logoteta |
BL_2018 |
2018 |
Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions |
Astron. and Astrophys. 609, A128
|
Eos |
| 65 |
E. Chabanat, P. Bonche, P. Haensel, J. Meyer, and R. Schaeffer |
CBHMS_1998 |
1998 |
A Skyrme parametrization from subnuclear to
neutron star densities Part II. Nuclei far from stabilities |
Nucl. Phys. A 635, 231
|
Eos |
| 66 |
J. Duflo and A. P. Zuker |
DZ_1995 |
1995 |
Microscopic mass formulas |
Phys. Rev. C 52, R23
|
Eos |
| 67 |
D. Vautherin |
V_1996 |
1996 |
Many-body methods at finite temperature |
Adv. Nucl. Phys. 22, 123
|
Eos |
| 68 |
M. Wang, G. Audi, A. H. Wapstra, F. G. Kondev, M. MacCormick, X. Xu, and B. Pfeiffer, |
AME_2012 |
2012 |
The Ame2012 atomic mass evaluation |
Chin. Phys. C 36, 1603
|
Eos |
| 69 |
Typel, S. |
T_2018 |
2018 |
Equations of state for astrophysical simulations from generalized relativistic density functionals |
J. Phys. G 45, 11400.
|
Eos |
| 70 |
Pais, H. and Typel, S. |
PT_2017 |
2017 |
Comparison of equation of state models with different cluster dissolution mechanisms |
Nuclear Particle Correlations and Cluster Physics, World Scientific, Singapore, pp. 95-132
|
Eos |
| 71 |
Typel, S., Wolter, H.H., Röpke, G., Blaschke, D. |
TWRB_2014 |
2014 |
Effects of the liquid-gas phase transition and cluster formation on the symmetry energy |
Eur. Phys. J. A50, 17
|
Eos |
| 72 |
Typel, S. and Wolter, H.H. |
TW_1999 |
1999 |
Relativistic mean field calculations with density dependent meson nucleon coupling |
Nucl. Phys. A656 ,331
|
Eos |
| 73 |
Voskresenskaya, M.D. and Typel, S. |
VT_2012 |
2012 |
Constraining mean-field models of the nuclear matter equation of state at low densities |
Nucl. Phys. A887, 42
|
Eos |
| 74 |
M. Wang, G. Audi, F. G. Kondev, W. J. Huang, S. Naimi, and X. Xu |
WGKH_2016 |
2017 |
The NUBASE2016 evaluation of nuclear properties |
Chinese Physics C41, 030003
|
Eos |
| 75 |
G. Baym, T. Hatsuda, T. Kojo, P.D. Powell, Y. Song, T. Takatsuka |
BHK_2018 |
2018 |
From hadrons to quarks in neutron stars: a review |
Rept.Prog.Phys. 81, 056902
|
Eos |
| 76 |
G. Baym, S. Furusawa, T. Hatsuda, T. Kojo, and H. Togashi |
BFH_2019 |
2019 |
New neutron star equation of state with quark-hadron crossover |
arxiv:1903.08963
|
Eos |
| 77 |
A.S. Schneider, L. Roberts, C.D. Ott |
SRO_17 |
2017 |
Open-source nuclear equation of state framework based on the liquid-drop model with Skyrme interaction |
Phys.Rev. C96, 065802
|
Eos |
| 78 |
A.S. Schneider, C. Constantinou, B. Muccioli, M. Prakash |
SCMP_2019 |
2019 |
The APR equation of state for simulations of supernovae, neutron stars and binary mergers |
arXiv:1901.09652
|
Eos |
| 81 |
S. S. Bao, J. N. Hu, Z. W. Zhang, and H. Shen |
BHZS_2014 |
2014 |
Effects of the symmetry energy on properties of neutron star crusts near the neutron drip density |
Phys. Rev. C 90, 045802
|
Eos |
| 82 |
H. Shen, F. Ji, J. Hu, K. Sumiyoshi |
SJHS_2020 |
2020 |
Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers |
arXiv:2001.10143
|
Eos |
| 80 |
K. Sumiyoshi, K. Nakazato, H. Suzuki, J. Hu, H. Shen |
SNSHS_2019 |
2019 |
Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations |
Astrophys. J 887, 110
|
Eos |
| 64 |
Ad. R. Raduta, F. Gulminelli |
RG_2018 |
2019 |
Nuclear Statistical Equilibrium Equation of State for Core Collapse |
Nucl.Phys. A983, 252
|
Eos |
| 59 |
M. Fortin, M. Oertel, C. Providência |
FOP_17 |
2018 |
Hyperons in hot dense matter: what do the constraints tell us for equation of state? |
Publ.Astron.Soc.Austral. 35, 44
|
Eos |
| 79 |
K. Otto, M. Oertel, B.-J. Schaefer |
OOS_2019 |
2019 |
Hybrid and quark star matter based on a non-perturbative equation of state |
arxiv:1910.11929
|
Eos |
| 84 |
T. Malik, S. Banik and Debades Bandyopadyay |
MBB_2021 |
2021 |
New equation of state involving Bose-Einstein condensate of antikaon for supernova and neutron star merger simulations |
arxiv
|
Eos |
| 85 |
Niels-Uwe Friedrich Bastian |
B_2021 |
2021 |
Phenomenological quark-hadron equations of state with first-order phase transitions for astrophysical applications |
Phys. Rev. D 103, 023001
|
Eos |
| 86 |
M. A. R. Kaltenborn, N.-U. F. Bastian, and D. B. Blaschke |
KBB_2017 |
2017 |
Quark-nuclear hybrid star equation of state with excluded volume effects |
Phys. Rev. D 96, 056024.
|
Eos |
| 87 |
T. Fischer, N.-U. F. Bastian, M.-R. Wu, P. Baklanov, E. Sorokina, S. Blinnikov,
S. Typel, T. Klähn, D. B. Blaschke |
FBW_2018 |
2018 |
Quark deconfinement as a supernova explosion engine for massive blue supergiant stars |
Nature Astronomy 2, 980
|
Eos |
| 88 |
Andreas Bauswein, Niels-Uwe F. Bastian, David B. Blaschke, Katerina Chatzi-
ioannou, James A. Clark, Tobias Fischer, and Micaela Oertel |
BBB_2019 |
2019 |
Identifying a first-order phase transition in neutron star mergers through gravitational waves |
Phys. Rev. Lett. 122, 061102
|
Eos |
| 89 |
Andreas Bauswein, Sebastian Blacker, Vimal Vijayan, Nikolaos Stergioulas, Katerina Chatziioannou, James A. Clark, Niels-Uwe F. Bastian, David B. Blaschke, Mateusz Cierniak, and Tobias Fischer |
BBV_2020 |
2020 |
Equation of state constraints from the threshold binary mass for prompt collapse of neutron star mergers |
Phys. Rev. Lett. 125, 141103
|
Eos |
| 90 |
Sebastian Blacker, Niels-Uwe F. Bastian, Andreas Bauswein, David B. Blaschke, Tobias Fischer, Micaela Oertel, Theodoros Soultanis, and Stefan Typel |
BBB_2020 |
2020 |
Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations |
Phys. Rev. D 102, 123023
|
Eos |
| 83 |
M. Oertel, A. Pascal, M. Mancini, J. Novak |
OPMN_2020 |
2020 |
Improved neutrino-nucleon interactions in dense and hot matter
for numerical simulations |
Phys Rev. C102, 035802
|
Eos |