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The sound velocity $v_s$ and dimensionless tidal deformability $\Lambda$ are analyzed using the pseudo-conformal model we developed before.
1908
Earlier work this paper cites.
S. Nadkarni, H. B. Nielsen, and I. Zahed, Bosonization relations as bag boundary conditions, Nucl. Phys. B 253
1994
Earlier work this paper cites.
M. Harada and K. Yamawaki, Wilsonian matching of effective field theory with underlying QCD, Phys. Rev. D 64
2001
Earlier work this paper cites.
M. Harada and K. Yamawaki, Vector manifestation of the chiral symmetry, Phys. Rev. Lett. 86
2001
Earlier work this paper cites.
M. Harada and K. Yamawaki, Fate of vector dominance in the effective field theory, Phys. Rev. Lett. 87
2001
Earlier work this paper cites.
S. K. Bogner, T. T. S. Kuo, and A. Schwenk, Model independent low momentum nucleon interaction from phase shift equivalence, Phys. Rep. 386
2003
Earlier work this paper cites.
P. Demorest, T. Pennucci, S. Ransom, M. Roberts and J. Hessels, Shapiro delay measurement of a two solar mass neutron star, Nature (London) 467
2010
Earlier work this paper cites.
J. Antoniadis et al
2013
Earlier work this paper cites.
M. G. Alford, S. Han, and M. Prakash, Generic conditions for stable hybrid stars, Phys. Rev. D 88
2013
Earlier work this paper cites.
Y. L. Ma, M. Harada, H. K. Lee, Y. Oh, B. Y. Park, and M. Rho, Dense baryonic matter in conformally-compensated hidden local symmetry: Vector manifestation and chiral symmetry restoration, Phys. Rev. D 90
2014
Cited alongside, same era.
P. Bedaque and A. W. Steiner, Sound velocity bound and neutron stars, Phys. Rev. Lett. 114
2015
Cited alongside, same era.
R. J. Crewther and L. C. Tunstall, Δ I = 1 / 2 \Delta I=1/2 rule for kaon decays derived from QCD infrared fixed point, Phys. Rev. D 91
2015
Cited alongside, same era.
B. P. Abbott et al
2017
Cited alongside, same era.
C. C. Moustakidis, T. Gaitanos, C. Margaritis, and G. A. Lalazissis, Bounds on the speed of sound in dense matter, and neutron star structure, Phys. Rev. C 95
2017
Cited alongside, same era.
J. Alsing, H. O. Silva, and E. Berti, Evidence for a maximum mass cut-off in the neutron star mass distribution and constraints on the equation of state, Mon. Not. R. Astron. Soc. 478
2018
Closest in time.
D. M. Podkowka, R. F. P. Mendes, and E. Poisson, Trace of the energy-momentum tensor and macroscopic properties of neutron stars, Phys. Rev. D 98
2018
Closest in time.
Y. L. Li, Y. L. Ma, and M. Rho, Nonquenching of g A g_{A} in nuclei, Landau-Migdal fixed-point theory, and emergence of scale symmetry in dense baryonic matter, Phys. Rev. C 98
2018
Closest in time.
G. Baym, T. Hatsuda, T. Kojo, P. D. Powell, Y. Song, and T. Takatsuka, From hadrons to quarks in neutron stars: A review, Rep. Prog. Phys. 81
2018
Closest in time.
Y.-L. Ma and M. Rho, Effective Field Theories for Nuclei and Compact-Star Matter: Chiral Nuclear Dynamics (CND-III)
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W. G. Paeng, T. T. S. Kuo, H. K. Lee, Y. L. Ma and M. Rho, Scale-invariant hidden local symmetry, topology change, and dense baryonic matter. II., Phys. Rev. D 96
2017
Cited alongside, same era.
B.-Y. Park and V. Vento, Skyrmion approach to finite density and temperatur, in The Multifaceted Skyrmion
2017
Cited alongside, same era.
Y. L. Ma and M. Rho, Recent progress on dense nuclear matter in skyrmion approaches, Sci. China Phys. Mech. Astron. 60
2017
Cited alongside, same era.
I. Tews, J. Carlson, S. Gandolfi, and S. Reddy, Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations, Astrophys. J. 860
2018
Cited alongside, same era.
2018
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Y. L. Ma, H. K. Lee, W. G. Paeng, and M. Rho, A pseudo-conformal equation of state in compact-star matter from topology change and hidden symmetries of QCD, Sci. China Phys. Mech. Astron. 62
2019
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Y. L. Ma and M. Rho, Pseudoconformal structure in dense baryonic matter, Phys. Rev. D 99
2019
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B. P. Abbott et al
2019
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