Stability of transparent spherically symmetric thin shells and wormholes

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 65, Issue 4, 2002, Pages 6-

  Ishak, Mustapha ^a   Lake, Kayll ^a  

^a QUEEN S UNIVERSITY   (Canada)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; EQUILIBRIUM CONSTANT; MATHEMATICAL ANALYSIS; MOLECULAR DYNAMICS; MOLECULAR STABILITY; MOTION;

EID: 0037084663     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.65.044011     Document Type: Article

References (15)

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5. Indeed, a simple search on “domain AND wall” in “astro-ph + gr-qc + hep-th” at arXiv. org returns over 100 results for the “Last year” and over 500 results over “All years.”
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8. By “domain wall” here we mean a hypersurface with an intrinsics equation of state of the form (Formula presented), where (Formula presented) is the surface density and P is the surface pressure. See, e.g. 3.
9. We write (Formula presented) and (Formula presented) with (Formula presented) denoting the limiting values of X on (Formula presented), and use geometrical units except in Appendix B. We use the letter “m” as follows: M is the surface mass of (Formula presented) defined by Eq. (2), m is the effective gravitational mass of the enveloping spacetimes “+” and “-” [see 9 and Eq. (10)], (Formula presented) and (Formula presented) (Formula presented) is not the effective gravitational mass but is related to it for the cases considered here by Eq. (23).
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15. This is a package which runs within MAPLE. It is entirely distinct from packages distributed with MAPLE and must be obtained independently. The GRTENSORII software and documentation is distributed freely on the world wide web from the address http://grtensor. org