Paradox of soft singularity crossing and its resolution by distributional cosmological quantities
A cosmological model of a flat Friedmann universe filled with a mixture of anti-Chaplygin gas and dustlike matter exhibits a future soft singularity, where the pressure of the anti-Chaplygin gas diverges (while its energy density is finite). Despite infinite tidal forces the geodesics pass through t...
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| Dokumentumtípus: | Cikk |
| Megjelent: |
American Physical Society
2012
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| Sorozat: | PHYSICAL REVIEW D
86 No. 6 |
| doi: | 10.1103/PhysRevD.86.063522 |
| mtmt: | 2135292 |
| Online Access: | http://publicatio.bibl.u-szeged.hu/7959 |
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| 024 | 7 | |a 10.1103/PhysRevD.86.063522 |2 doi | |
| 024 | 7 | |a 2135292 |2 mtmt | |
| 040 | |a SZTE Publicatio Repozitórium |b hun | ||
| 041 | |a zxx | ||
| 100 | 1 | |a Keresztes Zoltán | |
| 245 | 1 | 0 | |a Paradox of soft singularity crossing and its resolution by distributional cosmological quantities |h [elektronikus dokumentum] / |c Keresztes Zoltán |
| 260 | |a American Physical Society |c 2012 | ||
| 300 | |a Terjedelem: 12 p.-Azonosító: 063522 | ||
| 490 | 0 | |a PHYSICAL REVIEW D |v 86 No. 6 | |
| 520 | 3 | |a A cosmological model of a flat Friedmann universe filled with a mixture of anti-Chaplygin gas and dustlike matter exhibits a future soft singularity, where the pressure of the anti-Chaplygin gas diverges (while its energy density is finite). Despite infinite tidal forces the geodesics pass through the singularity. Because of the dust component, the Hubble parameter has a nonzero value at the encounter with the singularity, therefore the dust implies further expansion. With continued expansion however, the energy density and the pressure of the anti-Chaplygin gas would become ill-defined hence from the point of view of the anti-Chaplygin gas only a contraction is allowed. Paradoxically, the universe in this cosmological model would have to expand and contract simultaneously. This obviously could not happen. We solve the paradox by redefining the anti-Chaplygin gas in a distributional sense. Then a contraction could follow the expansion phase at the singularity at the price of a jump in the Hubble parameter. Although such an abrupt change is not common in any cosmological evolution, we explicitly show that the set of Friedmann, Raychaudhuri and continuity equations are all obeyed both at the singularity and in its vicinity. We also prove that the Israel junction conditions are obeyed through the singular spatial hypersurface. In particular we enounce and prove a more general form of the Lanczos equation. | |
| 700 | 0 | 1 | |a Gergely Árpád László |e aut |
| 700 | 0 | 1 | |a Kamenshchik A. Yu. |e aut |
| 856 | 4 | 0 | |u http://publicatio.bibl.u-szeged.hu/7959/1/28_cikk_keresztesetal2012.pdf |z Dokumentum-elérés |
| 856 | 4 | 0 | |u http://publicatio.bibl.u-szeged.hu/7959/2/28_cikk_preprint_1204.1199v2.pdf |z Dokumentum-elérés |