Abstract
The cosmic no hair conjecture is tested in the spherically symmetric Einstein-Maxwell-dilaton (EMD) system with a positive cosmological constant Λ. First, we analytically show that once gravitational collapse occurs in the massless dilaton case, the system of field equations breaks down inevitably in outer communicating regions or at the boundary provided that a future null infinity I+ exists. Next, we find numerically the static black hole solutions in the massive dilaton case and investigate their properties for comparison with the massless case. It is shown that their Abbott-Deser (AD) mass is infinite, which implies that a spacetime with finite AD mass does not approach a black hole solution after gravitational collapse. These results suggest that I+ cannot appear in the EMD system once gravitational collapse occurs and hence the cosmic no hair conjecture is violated in both the massless and massive cases, in contrast with general relativity.
| Original language | English |
|---|---|
| Article number | 064012 |
| Pages (from-to) | 1-9 |
| Number of pages | 9 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 61 |
| Issue number | 6 |
| Publication status | Published - 2000 Mar 15 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
- Mathematical Physics
- Physics and Astronomy (miscellaneous)
Cite this
Violation of the cosmic no hair conjecture in the Einstein-Maxwell-dilaton system. / Maeda, Kengo; Torii, Takashi; Narita, Makoto.
In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 61, No. 6, 064012, 15.03.2000, p. 1-9.Research output: Contribution to journal › Article
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TY - JOUR
T1 - Violation of the cosmic no hair conjecture in the Einstein-Maxwell-dilaton system
AU - Maeda, Kengo
AU - Torii, Takashi
AU - Narita, Makoto
PY - 2000/3/15
Y1 - 2000/3/15
N2 - The cosmic no hair conjecture is tested in the spherically symmetric Einstein-Maxwell-dilaton (EMD) system with a positive cosmological constant Λ. First, we analytically show that once gravitational collapse occurs in the massless dilaton case, the system of field equations breaks down inevitably in outer communicating regions or at the boundary provided that a future null infinity I+ exists. Next, we find numerically the static black hole solutions in the massive dilaton case and investigate their properties for comparison with the massless case. It is shown that their Abbott-Deser (AD) mass is infinite, which implies that a spacetime with finite AD mass does not approach a black hole solution after gravitational collapse. These results suggest that I+ cannot appear in the EMD system once gravitational collapse occurs and hence the cosmic no hair conjecture is violated in both the massless and massive cases, in contrast with general relativity.
AB - The cosmic no hair conjecture is tested in the spherically symmetric Einstein-Maxwell-dilaton (EMD) system with a positive cosmological constant Λ. First, we analytically show that once gravitational collapse occurs in the massless dilaton case, the system of field equations breaks down inevitably in outer communicating regions or at the boundary provided that a future null infinity I+ exists. Next, we find numerically the static black hole solutions in the massive dilaton case and investigate their properties for comparison with the massless case. It is shown that their Abbott-Deser (AD) mass is infinite, which implies that a spacetime with finite AD mass does not approach a black hole solution after gravitational collapse. These results suggest that I+ cannot appear in the EMD system once gravitational collapse occurs and hence the cosmic no hair conjecture is violated in both the massless and massive cases, in contrast with general relativity.
UR - http://www.scopus.com/inward/record.url?scp=16644373993&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=16644373993&partnerID=8YFLogxK
M3 - Article
AN - SCOPUS:16644373993
VL - 61
SP - 1
EP - 9
JO - Physical review D: Particles and fields
JF - Physical review D: Particles and fields
SN - 1550-7998
IS - 6
M1 - 064012
ER -