Phase transitions and the mass-radius curves of relativistic stars

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 58, Issue 2, 1998, Pages 8-

  Lindblom, Lee ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0542442715     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.024008     Document Type: Article

References (13)

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3. Necessary conditions on the equation of state to guarantee that stellar models have finite mass and radius are discussed by L. Lindblom and A. K. M. Masood-ul-Alam, in Directions in General Relativity II: Papers in Honor of Dieter Brill, edited by B. L. Hu and T. A. Jacobson (Cambridge University Press, Cambridge, England, 1993), p. 172.
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13. See for example E. A. Coddington, and N. Levinson, Theory of Ordinary Differential Equations (McGraw-Hill, New York, 1955), Sec. 1.7.