Bibliography

ID	Authors	Ref	Year	Title	Journal
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
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
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
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
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
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
91	Andrew W. Steiner, Madappa Prakash, James M. Lattimer, Paul J. Ellis	SPLE_2005	2005	Isospin asymmetry in nuclei and neutron stars	Phys. Rep. 411, 325	Eos
92	L.G. Cao, U. Lombardo, C.W. Shen, Nguyen Van Giai	CLSG_2006	2006	From Brueckner approach to Skyrme-type energy density functional	Phys. Rev. C 73, 014313	Eos
93	F. Tondeur, M. Brack, M. Farine, J.M. Pearson	TBFP_1984	1984	Static nuclear properties and the parametrisation of Skyrme forces	Nucl. Phys. A 420, 297	Eos
94	V. Dexheimer and S. Schramm	VS_2010	2010	A Novel Approach to Model Hybrid Stars	Phys.Rev.C 81, 045201	Eos
95	V. Dexheimer, R.O. Gomes, T. Klähn, S. Han, M. Salinas	VGTHS_2021	2021	GW190814 as a massive rapidly rotating neutron star with exotic degrees of freedom	Phys.Rev.C 103, 2	Eos
79	K. Otto, M. Oertel, B.-J. Schaefer	OOS_2019	2020	Hybrid and quark star matter based on a non-perturbative equation of state	Phys. Rev. D 101, 103021	Eos
96	K. Otto, M. Oertel, B.-J. Schaefer	OOS_2020	2020	Nonperturbative quark matter equations of state with vector interactions	Eur.Phys.J.ST 229, 3629	Eos
88	Andreas Bauswein, Niels-Uwe F. Bastian, David B. Blaschke, Katerina Chatziioannou, 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
97	N. Jokela, M. Jarvinen and J. Remes	JJR_2019	2019	Holographic QCD in the Veneziano limit and neutron stars	JHEP 03, 041	Eos
98	T. Ishii, M. Jarvinen and G. Nijs	IJN_2019	2019	Cool baryon and quark matter in holographic QCD	JHEP 07, 003	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	Euro. Phys. J Special Topics, 230, 561	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	Astrophys.J. 885, 42	Eos
99	C. Ecker, M. Jarvinen, G. Nijs and W. van der Schee	EJNS_2020	2020	Gravitational waves from holographic neutron star mergers	Phys. Rev. D 101, 103006	Eos
100	N. Jokela, M. Jarvinen, G. Nijs and J. Remes	JJNR_2021	2021	Unified weak and strong coupling framework for nuclear matter and neutron stars	Phys. Rev. D 103, 086004	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
101	T. Malik, S. Banik & D. Bandyopadhyay	MBB_2021b	2021	Equation of State table with hyperon and antikaon for supernova and neutron star merger	Astrophysical Journal, 910,96	Eos
102	R. Negreiros, L. Tolos, M. Centelles, A. Ramos, and V. Dexheimer	NTCRD_2018	2018	Cooling of Small and Massive Hyperonic Stars	Astrophys. J. 863, 104	Eos
103	C. Providência, M. Fortin, H. Pais, and A. Rabhi	PFPR_2019	2019	Hyperonic stars and the symmetry energy	Astron. Space Sci. 6, 13	Eos
104	C. J. Horowitz and J. Piekarewicz	HP_2001	2001	Neutron Star Structure and the Neutron Radius of 208Pb	Phys. Rev. Lett. 86, 5647	Eos
105	C. J. Horowitz and J. Piekarewicz	HPb_2001	2001	Neutron radii of 208Pb and neutron stars	Phys. Rev. C 64, 062802	Eos
106	H. Pais and C. Providência	PP_2016	2016	Vlasov formalism for extended relativistic mean field models: The crust-core transition and the stellar matter equation of state	Phys. Rev. C 94, 015808	Eos
107	P.A.M. Guichon	G_1988	1988	A Possible Quark Mechanism for the Saturation of Nuclear Matter	Phys.Lett.B 200, 235	Eos
108	P.A.M. Guichon, J.R. Stone, A.W. Thomas	GST_2018	2018	Quark–Meson-Coupling (QMC) model for finite nuclei, nuclear matter and beyond	Prog.Part.Nucl.Phys. 100, 262	Eos
109	J.R. Stone, V. Dexheimer, P.A.M. Guichon, A.W. Thomas, S. Typel	SDGTT_2021	2021	Equation of state of hot dense hyperonic matter in the Quark–Meson-Coupling (QMC-A) model	Mon.Not.Roy.Astron.Soc. 502, 3476	Eos
110	O. Boukari, H. Pais, S. Antić, and C. Providência	BPAP_2021	2021	Critical properties of calibrated relativistic mean-field models for the transition to warm, nonhomogeneous nuclear and stellar matter	Phys. Rev. C 103, 055804	Eos
111	W.-C. Chen and J. Piekarewicz	CP_2014	2014	Building relativistic mean field models for finite nuclei and neutron stars	Phys. Rev. C 90, 044305	Eos
112	G. A. Lalazissis, T. Niksic, D. Vretenar, and P. Ring	LNVR_2005	2005	New relativistic mean-field interaction with density-dependent meson-nucleon couplings	Phys. Rev. C 71, 024312	Eos
114	T. Kojo, G. Baym, and T. Hatsuda,	KBH_2021	2021	QHC21 equation of state of neutron star matter – in light of 2021 NICER data	arXiv: 2111.11919	Eos
115	C. Drischler, S. Han, J.M. Lattimer, M. Prakash, S. Reddy, and T. Zhao	DHLPR_2021	2021	Limiting masses and radii of neutron stars and their implications	Phys. Rev. C 103, 045808	Eos
116	M. Oertel, M. Hempel, T. Klähn, S. Typel	OHKT_2017	2017	Equations of state for supernovae and compact stars	Rev. Mod. Phys. 89, 015007	Eos
117	S. Typel, M. Oertel, T. Klähn	TOK_2015	2015	CompOSE CompStar online supernova equations of state harmonising the concert of nuclear physics and astrophysics	Phys.Part.Nucl. 46, 633	Eos
118	Ad. R. Raduta, M. Oertel, A. Sedrakian	ROS_2020	2020	Proto-neutron stars with heavy baryons and universal relations	MNRAS 499, 914	Eos
119	A.R. Raduta	R_2022	2022	—	in preparation	Eos
120	X. Vinas, C. Gonzalez-Boquera, M. Centelles, C. Mondal and L. M. Robledo	VGCMR_2021	2021	Unified Equation of State for Neutron Stars Based on the Gogny Interaction	Symmetry 13, 1613	Eos
121	V. Allard and N. Chamel	AC_2021	2021	1S0 Pairing Gaps, Chemical Potentials and Entrainment Matrix in Superfluid Neutron-Star Cores for the Brussels–Montreal Functionals	Universe 7, 470	Eos
122	J. M. Pearson and N. Chamel	PC_2022	2022	Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. III. Inclusion of microscopic corrections to pasta phases	Phys. Rev. C 105, 015803	Eos
123	J. M. Pearson, N. Chamel, and A. Y. Potekhin	PCP_2020	2020	Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. II. Pasta phases in semiclassical approximation	Phys. Rev. C 101, 015802	Eos
124	J. M. Pearson, N. Chamel, A. Y. Potekhin, A. F. Fantina, C. Ducoin, A. K. Dutta, and S. Goriely	PCP_2018	2018	Unified equations of state for cold non-accreting neutron stars with Brussels–Montreal functionals – I. Role of symmetry energy	MNRAS 481, 2994	Eos
125	S. Goriely, N. Chamel, and J. M. Pearson	GCP_2013	2013	Hartree-Fock-Bogoliubov nuclear mass model with 0.50 MeV accuracy based on standard forms of Skyrme and pairing functionals	Phys. Rev. C 88, 024308	Eos
126	L. Perot, N. Chamel, and A. Sourie	PCS_2019	2019	Role of the symmetry energy and the neutron-matter stiffness on the tidal deformability of a neutron star with unified equations of state	Phys. Rev. C 100, 035801	Eos
127	Y. Xu, S. Goriely, A. Jorissen, G. L. Chen, and M. Arnould	XGJCA_2013	2013	Databases and tools for nuclear astrophysics applications BRUSsels Nuclear LIBrary (BRUSLIB), Nuclear Astrophysics Compilation of REactions II (NACRE II) and Nuclear NETwork GENerator (NETGEN)	Astronomy & Astrophysics 549, A106	Eos
128	A. Welker, et al	W_2017	2017	Binding Energy of 79Cu: Probing the Structure of the Doubly Magic 78Ni from Only One Proton Away	Phys. Rev. Lett. 119, 192502	Eos
129	C. Mondal, X. Vinas, M. Centelles and J. N. De	MVCD_2020	2020	Structure and composition of the inner crust of neutron stars from Gogny interactions	Phys. Rev. C 102,015802	Eos
130	C. Gonzalez-Boquera, M. Centelles, X. Vinas, L. M. Robledo	GCVR_2018	2018	New Gogny interaction suitable for astrophysical applications	Phys. Lett. B 779, 195.	Eos
131	S. Typel , M. Oertel, T. Klähn, D. Chatterjee, V. Dexheimer et al.	TOK_2022	2022	CompOSE Reference Manual	arxiv: 2203.03209	Eos
132	A. Clevinger, J. Corkish, K. Aryal, V. Dexheimer	CCAD_2022	2022	Hybrid equations of state for neutron stars with hyperons and deltas	Eur.Phys.J.A 58, 96	Eos
133	V. Dexheimer, R. O. Gomes, S. Schramm, H. Pais	DGSP_2019	2019	What do we learn about vector interactions from GW170817?	J. Phys. G 46, 034002	Eos
134	L. Suleiman, M. Fortin, J. L. Zdunik, P. Haensel	SFZH_2021	2021	Influence of the crust on the neutron star macrophysical quantities and universal relations	Phys.Rev.C 104, 015801	Eos
136	C.-J. Xia, T. Maruyama, A. Li, B. Y. Sun, W.-H. Long, and Y.-X. Zhang	XMLSL_2022	2022	Unified neutron star EOSs and neutron star structures in RMF models	Commun.Theor. Phys. 74, 095303	Eos
137	C.-J. Xia, B. Y. Sun, T. Maruyama, W.-H. Long, and A. Li	XSMLL_2022	2022	Unified nuclear matter equations of state constrained by the in-medium balance in density-dependent covariant density functionals	Phys. Rev. C 105, 045803	Eos
138	B. Wei, Q. Zhao, Z.-H. Wang, J. Geng, B.-Y. Sun, Y.-F. Niu, and W.-H. Long	WZWG_2020	2020	Novel relativistic mean field Lagrangian guided by pseudo-spin symmetry restoration	Chin. Phys. C 44, 074107	Eos
139	A. Taninah, S. Agbemava, A. Afanasjev, and P. Ring	TAAR_2020	2020	Parametric correlations in energy density functionals	Phys. Lett. B 800, 135065	Eos
140	T. Maruyama, T. Tatsumi, D. N. Voskresensky, T. Tanigawa, and S. Chiba	MTVTC_2005	2005	Nuclear pasta structures and the charge screening effect	Phys. Rev. C 72, 015802	Eos
141	W.-H. Long, J. Meng, N. V. Giai, and S.-G. Zhou	LMGZ_2004	2004	New effective interactions in RMF theory with nonlinear terms and density dependent meson nucleon coupling	Phys. Rev. C 69, 034319	Eos
144	Nadine Hornick, Laura Tolos, Andreas Zacchi, Jan-Erik Christian, and Jürgen Schaffner-Bielich	HTZCS_2018	2018	Relativistic parameterizations of neutron matter and implications for neutron stars	Phys.Rev.C 98 (2018) 6, 065804	Eos
113	G. Grams, J. Margueron, R. Somasundaram and S. Reddy	GMSR_2021	2022	Confronting a set of Skyrme and χEFTχEFT predictions for the crust of neutron stars: On the origin of uncertainties in model predictions	Eur.Phys.J.A 58 (2022) 56	Eos
145	Domenico Logoteta , Albino Perego , Ignazio Bombaci	LPB_2021	2021	Microscopic equation of state of hot nuclear matter for numerical relativity simulations	Astron.Astrophys. 646, A55	Eos
146	Maria Piarulli , Luca Girlanda , Rocco Schiavilla , Alejandro Kievsky , Alessandro Lovato	PGSKL_2016	2016	Local chiral potentials with Δ-intermediate states and the structure of light nuclei	Phys.Rev.C 94, 054007	Eos
147	Domenico Logoteta , Ignazio Bombaci , Alejandro Kievsky	LBK_2016	2016	Nuclear matter properties from local chiral interactions with Δ isobar intermediate states	Phys.Rev.C 94, 064001	Eos
148	Albino Perego , Domenico Logoteta , David Radice , Sebastiano Bernuzzi , Rahul Kashyap	PLRBK_2022	2022	Probing the Incompressibility of Nuclear Matter at Ultrahigh Density through the Prompt Collapse of Asymmetric Neutron Star Binaries	Phys.Rev.Lett. 129, 032701	Eos
149	Aviral Prakash , David Radice , Domenico Logoteta , Albino Perego , Vsevolod Nedora	PRLPN_2021	2021	Signatures of deconfined quark phases in binary neutron star mergers	Phys. Rev. D 104, 083029	Eos
150	Sebastiano Bernuzzi , Matteo Breschi , Boris Daszuta , Andrea Endrizzi , Domenico Logoteta et al.	BBDEL_2020	2020	Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signals	Mon. Not. R. Astron. Soc. 497, 1488	Eos
151	Rahul Kashyap , Abhishek Das , David Radice , Surendra Padamata , Aviral Prakash et al.	KDRPP_2022	2022	Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817	Phys. Rev. D 105, 103022	Eos
143	Bikram Keshari Pradhan , Debarati Chatterjee , Radhika Gandhi , Jürgen Schaffner-Bielich	PCGS_2022	2022	Role of vector self-interaction in Neutron Star properties	Nucl.Phys.A 1030 (2023) 122578	Eos
153	M. G. Alford, L. Brodie, A. Haber, and I. Tews	ABHT_2023	2023	Tabulated Equations of State From Models Informed by Chiral Effective Field Theory	arXiv:2304.07836	Eos
135	M. G. Alford, L. Brodie, A. Haber, and I. Tews	ABHT_2022	2022	Relativistic mean-field theories for neutron-star physics based on chiral effective field theory	Phys. Rev. C 106, 055804	Eos
142	T. Demircik, C. Ecker, and M. Jarvinen	DEJ_2022	2022	Dense and Hot QCD at Strong Coupling	Phys.Rev.X 12, 041012	Eos
154	C. Hoyos, N. Jokela, M. Järvinen, J. G. Subils, J. Tarrı́o, and A. Vuorinen	HJJST_2020	2020	Transport in strongly coupled quark matter	Phys.Rev. Lett. 125, 241601	Eos
155	P. M. Chesler, N. Jokela, A. Loeb, and A. Vuorinen	CJLV_2019	2019	Finite-temperature Equations of State for Neutron Star Mergers	Phys. Rev. D 100, 066027	Eos
156	Thomas Carreau , Francesca Gulminelli , Jérôme Margueron	CGM_2019	2019	Bayesian analysis of the crust-core transition with a compressible liquid-drop model	Eur.Phys.J.A 55, 188	Eos
157	P. Char, C. Mondal, F. Gulminelli, M. Oertel	CMGO_2023	2023	Relativistic metamodel for NS EoS	to be submitted	Eos
158	P. Gögelein, E. N. E. van Dalen, C. Fuchs, and H. Müther	GDFM_2008	2008	Nuclear matter in the crust of neutron stars derived from realistic NN interactions	Phys. Rev. C 77, 025802	Eos
159	Hristijan Kochankovski, Angels Ramos, Laura Tolos	KRT_2022	2022	Equation of state for hot hyperonic neutron star matter	MNRAS 517, 507	Eos
160	Laura Tolos, Mario Centelles, Angels Ramos	TCR_2017	2017	Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints	Astrophys. J 834,1	Eos
161	Luigi Scurto , Helena Pais, Francesca Gulminelli	SPG_2024	2024	General predictions of neutron star properties using unified relativistic mean-field equations of state	arxiv:2402.15548	Eos
163	Jia Jie Li, Armen Sedrakian	LS_2023	2023	New Covariant Density Functionals of Nuclear Matter for Compact Star Simulations	Astrophysical Journal 957:41	Eos
162	Stefanos Tsiopelas, Armen Sedrakian, Micaela Oertel	TSO_2024	2024	Finite-temperature equations of state of compact stars with hyperons: three-dimensional tables	Eur.Phys.J.A 60, 127	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