Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 39, Issue 14, Pages -Publisher
IOP Publishing Ltd
DOI: 10.1088/1361-6382/ac776e
Keywords
exact solutions; spacetime singularities; causal structure; cosmology
Categories
Funding
- JSPS KAKENHI [JP19K03876, JP19H01895, JP20H05853, JP19K14715]
Ask authors/readers for more resources
In this paper, we classify the Friedmann-Lemaitre-Robertson-Walker solutions with spatial curvature K = 0, +/- 1 for perfect fluids with linear equation of state p = w rho without assuming any energy conditions. We extend our previous work to include all geodesics and parallelly propagated (p.p.) curvature singularities. Our study reveals that there are no non-null geodesics emanating from or terminating at the null portion of conformal infinity, and that the initial singularity for certain parameter ranges is a null non-scalar polynomial curvature singularity.
We completely classify the Friedmann-Lemaitre-Robertson-Walker solutions with spatial curvature K = 0, +/- 1 for perfect fluids with linear equation of state p = w rho, where rho and p are the energy density and pressure, without assuming any energy conditions. We extend our previous work to include all geodesics and parallelly propagated (p.p.) curvature singularities, showing that no non-null geodesic emanates from or terminates at the null portion of conformal infinity and that the initial singularity for K = 0, -1 and -5/3 < w < -1 is a null non-scalar polynomial curvature singularity. We thus obtain the Penrose diagrams for all possible cases and identify w = -5/3 as a critical value for both the future big-rip singularity and the past null conformal boundary.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available