Bounds on 2m/R for static spherical objects
dc.contributor.author | Guven, Jemal | |
dc.contributor.author | Ó Murchadha, Niall | |
dc.date.accessioned | 2017-08-29T09:14:25Z | |
dc.date.available | 2017-08-29T09:14:25Z | |
dc.date.issued | 1999 | |
dc.description.abstract | It is well known that a spherically symmetric constant density static star, modeled as a perfect fluid, possesses a bound on its mass m by its radial size R given by 2m/R less than or equal to 8/9 and that this bound continues to hold when the energy density decreases monotonically. The existence of such a bound is intriguing because it occurs well before the appearance of an apparent horizon at m = R/2. However, the assumptions made are extremely restrictive. They do not hold in a simple soap bubble and they certainly do not approximate any known topologically stable field configuration. In addition, Such configurations will not generally be compact. We show that the 8/9 bound is robust by relaxing these assumptions. If the density is monotonically decreasing and the tangential stress is less than or equal to the radial stress we show that the 8/9 bound continues to hold through the entire bulk if m is replaced by the quasi-local mass. If the tangential stress is allowed to exceed the radial stress and/or the density is not monotonic we cannot recover the 8/9 bound. However, we can show that 2m/R remains strictly bounded away from unity by constructing an explicit upper bound which depends only on the ratio of the stresses and the variation of the density. (S0556-2821(99)09818-5). | en |
dc.description.status | Peer reviewed | en |
dc.description.version | Published Version | en |
dc.format.mimetype | application/pdf | en |
dc.identifier.articleid | 84020 | |
dc.identifier.citation | Guven, J. and Ó Murchadha, N. (1999) 'Bounds on 2m/R for static spherical objects', Physical Review D, 60(8), 084020 (8pp). doi: 10.1103/PhysRevD.60.084020 | en |
dc.identifier.doi | 10.1103/PhysRevD.60.084020 | |
dc.identifier.issn | 0556-2821 | |
dc.identifier.issued | 8 | |
dc.identifier.journaltitle | Physical Review D | en |
dc.identifier.uri | https://hdl.handle.net/10468/4580 | |
dc.identifier.volume | 60 | |
dc.language.iso | en | en |
dc.publisher | American Physical Society | en |
dc.relation.uri | https://journals.aps.org/prd/abstract/10.1103/PhysRevD.60.084020 | |
dc.rights | © 1999, American Physical Society | en |
dc.subject | Classical general-relativity | en |
dc.subject | Stellar models | en |
dc.subject | Configuration-space | en |
dc.subject | Symmetry | en |
dc.subject | Constraints | en |
dc.title | Bounds on 2m/R for static spherical objects | en |
dc.type | Article (peer-reviewed) | en |
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