.png){kind=icon}
.png){kind=icon}
Return
A simple harmonic universe
.png){kind=icon}
OA
AI
DOI：10.1007/JHEP02(2014)029.png)
.png){kind=icon}
Original request for help.png){kind=icon}
Share.png){kind=icon}
Save
Abstract
En 中文
We explore simple but novel bouncing solutions of general relativity that avoid singularities. These solutions require curvature k = +1, and are supported by a negative cosmological term and matter with -1 < w < -1/3. In the case of moderate bounces (where the ratio of the maximal scale factor a (+) to the minimal scale factor a (-) is ), the solutions are shown to be classically stable and cycle through an infinite set of bounces. For more extreme cases with large a (+) /a (-), the solutions can still oscillate many times before classical instabilities take them out of the regime of validity of our approximations. In this regime, quantum particle production also leads eventually to a departure from the realm of validity of semiclassical general relativity, likely yielding a singular crunch. We briefly discuss possible applications of these models to realistic cosmology.
Keywords:
Classical Theories of Gravity
Spacetime Singularities
Journal
IF:
5.5
Papers:
3.9W
Citations:
13.7W