Abstract
We study T3 Gowdy spacetimes in the Einstein-Maxwell-dilaton-axion system and show by the Fuchsian algorithm that they have, in general, asymptotically velocity-term-dominated singularities. The families of the corresponding solutions depend on the maximum number of arbitrary functions. Although coupling of the dilaton field with the Maxwell and/or the axion fields corresponds to the 'potential' which appears in the Hamiltonian of vacuum Bianchi IX spacetimes, our result means that the spacetimes do not become Mixmaster necessarily.
| Original language | English |
|---|---|
| Pages (from-to) | 4597-4613 |
| Number of pages | 17 |
| Journal | Classical and Quantum Gravity |
| Volume | 17 |
| Issue number | 22 |
| DOIs | |
| Publication status | Published - 2000 Nov 21 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
Asymptotic singular behaviour of Gowdy spacetimes in string theory. / Narita, Makoto; Torii, Takashi; Maeda, Kengo.
In: Classical and Quantum Gravity, Vol. 17, No. 22, 21.11.2000, p. 4597-4613.Research output: Contribution to journal › Article
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TY - JOUR
T1 - Asymptotic singular behaviour of Gowdy spacetimes in string theory
AU - Narita, Makoto
AU - Torii, Takashi
AU - Maeda, Kengo
PY - 2000/11/21
Y1 - 2000/11/21
N2 - We study T3 Gowdy spacetimes in the Einstein-Maxwell-dilaton-axion system and show by the Fuchsian algorithm that they have, in general, asymptotically velocity-term-dominated singularities. The families of the corresponding solutions depend on the maximum number of arbitrary functions. Although coupling of the dilaton field with the Maxwell and/or the axion fields corresponds to the 'potential' which appears in the Hamiltonian of vacuum Bianchi IX spacetimes, our result means that the spacetimes do not become Mixmaster necessarily.
AB - We study T3 Gowdy spacetimes in the Einstein-Maxwell-dilaton-axion system and show by the Fuchsian algorithm that they have, in general, asymptotically velocity-term-dominated singularities. The families of the corresponding solutions depend on the maximum number of arbitrary functions. Although coupling of the dilaton field with the Maxwell and/or the axion fields corresponds to the 'potential' which appears in the Hamiltonian of vacuum Bianchi IX spacetimes, our result means that the spacetimes do not become Mixmaster necessarily.
UR - http://www.scopus.com/inward/record.url?scp=0034700064&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0034700064&partnerID=8YFLogxK
U2 - 10.1088/0264-9381/17/22/301
DO - 10.1088/0264-9381/17/22/301
M3 - Article
AN - SCOPUS:0034700064
VL - 17
SP - 4597
EP - 4613
JO - Classical and Quantum Gravity
JF - Classical and Quantum Gravity
SN - 0264-9381
IS - 22
ER -