Detectability of Cosmic Topology in Almost Flat Universes

Details Detectability of Cosmic Topology in Almost Flat Universes Detectability of Cosmic Topology in Almost Flat Universes

2001-05-02

arxiv.org/abs/gr-qc/0105002v3

Class.Quant.Grav. 18 (2001) 4461-4476

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

18 pages, 3 figures, LaTeX2e. Two references added. Minors corrections in section 4. To appear in Class. Quantum Grav. {\bf 18

Scientific paper

10.1088/0264-9381/18/21/306

Recent observations suggest that the ratio of the total density to the critical density of the universe, $\Omega_0$, is likely to be very close to one, with a significant proportion of this energy being in the form of a dark component with negative pressure. Motivated by this result, we study the question of observational detection of possible non-trivial topologies in universes with $\Omega_0 \sim 1$, which include a cosmological constant. Using a number of indicators we find that as $\Omega_0 \to 1$, increasing families of possible manifolds (topologies) become either undetectable or can be excluded observationally. Furthermore, given a non-zero lower bound on $|\Omega_0 - 1|$, we can rule out families of topologies (manifolds) as possible candidates for the shape of our universe. We demonstrate these findings concretely by considering families of topologies and employing bounds on cosmological parameters from recent observations. We find that given the present bounds on cosmological parameters, there are families of both hyperbolic and spherical manifolds that remain undetectable and families that can be excluded as the shape of our universe. These results are of importance in future search strategies for the detection of the shape of our universe, given that there are an infinite number of theoretically possible topologies and that the future observations are expected to put a non-zero lower bound on $|\Omega_0 - 1|$ which is more accurate and closer to zero.

Affiliated with

Also associated with

No associations

Rating

Detectability of Cosmic Topology in Almost Flat Universes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Detectability of Cosmic Topology in Almost Flat Universes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detectability of Cosmic Topology in Almost Flat Universes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-4785