The Destiny of Universes After the Big Trip
| dc.creator | Yurov, A. V. | |
| dc.date | 2007-09-29 | |
| dc.date.accessioned | 2026-07-07T08:33:09Z | |
| dc.date.available | 2026-07-07T08:33:09Z | |
| dc.description | The big trip can be describe with the help of the Wheeler-DeWitt wave equation ${\hat H}ψ(w,a)=0$. The probability to find the universe after big trip in the state with $w=w_0$ will be maximal if $\partialψ(w,a)/\partial w|_{w=w_0}=0$ for any values of the scale factor $a$. It is shown that this will be the case if and only if $w_0=-1/3$. This fact allows one to suggest that vast majority of universes in multiverse must be in this state after their big trips. | |
| dc.description | RevTex, 4 pages, 1 figure | |
| dc.identifier | https://arxiv.org/abs/0710.0094 | |
| dc.identifier | http://arxiv.org/abs/0710.0094 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/139027 | |
| dc.subject | Astrophysics | |
| dc.title | The Destiny of Universes After the Big Trip | |
| dc.type | text |