【第二季】155｜【终结之问】极端物质——中子星与夸克星

参考文献：1. Lattimer， J. M.， & Prakash， M. (2007). Neutron star observations： Prognosis for equation of state constraints. Physics Reports， 442(1–6)， 109–165.2. Ozel， F.， & Freire， P. (2016). Masses， Radii， and the Equation of State of Neutron Stars. Annual Review of Astronomy and Astrophysics， 54， 401–440.3. Witten， E. (1984). Cosmic separation of phases. Physical Review D， 30(2)， 272–285.4. Alford， M. G.， et al. (2008). Hybrid stars that masquerade as neutron stars. Nature， 445(7125)， E7–E8.5. Annala， E.， et al. (2018). Gravitational-wave constraints on the neutron-star-matter equation of state. Physical Review Letters， 120(17)， 172703.6. Fonseca， E.， et al. (2021). Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620. The Astrophysical Journal Letters， 915(1)， L12.7. Baym， G.， et al. (2018). From hadrons to quarks in neutron stars： a review. Reports on Progress in Physics， 81(5)， 056902.8. Hewish， A.， et al. (1968). Observation of a Rapidly Pulsating Radio Source. Nature， 217(5130)， 709–713.9. Demorest， P. B.， et al. (2010). A two-solar-mass neutron star measured using Shapiro delay. Nature， 467(7319)， 1081–1083.10. Shapiro， S. L.， & Teukolsky， S. A. (1983). Black Holes， White Dwarfs， and Neutron Stars： The Physics of Compact Objects. Wiley. Chapters 9–10.