2018
DOI: 10.1088/1475-7516/2018/03/020
|View full text |Cite
|
Sign up to set email alerts
|

Unbraiding the bounce: superluminality around the corner

Abstract: We study a particular realization of the cosmological bounce scenario proposed recently by Ijjas and Steinhardt in [1]. First, we find that their bouncing solution starts from a divergent sound speed and ends with its vanishing. Thus, the solution connects two strongly coupled configurations. These pathologies are separated from the bouncing regime by only a few Planck times. We then reveal the exact structure of the Lagrangian, which reproduces this bouncing solution. This reconstruction allowe… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
4
1

Citation Types

0
51
0

Year Published

2018
2018
2024
2024

Publication Types

Select...
8

Relationship

0
8

Authors

Journals

citations
Cited by 64 publications
(51 citation statements)
references
References 75 publications
0
51
0
Order By: Relevance
“…We illustrate that c 2 T is positive during the whole cosmological process, but it will exceed the speed of light squared, i.e., c 2 > 1 for a short time interval near the genesis event, triggering the superluminality problem. The existence of superluminality is a general feature in scalartensor theory beyond Horndeski [67], and here we shall argue that superluminality does not necessarily correspond to acasuality [69,70,[72][73][74]. Still, it is interesting to see whether we can develop a genesis model without the superluminality issue.…”
Section: B Tensor Perturbationsmentioning
confidence: 66%
“…We illustrate that c 2 T is positive during the whole cosmological process, but it will exceed the speed of light squared, i.e., c 2 > 1 for a short time interval near the genesis event, triggering the superluminality problem. The existence of superluminality is a general feature in scalartensor theory beyond Horndeski [67], and here we shall argue that superluminality does not necessarily correspond to acasuality [69,70,[72][73][74]. Still, it is interesting to see whether we can develop a genesis model without the superluminality issue.…”
Section: B Tensor Perturbationsmentioning
confidence: 66%
“…This problem has been addressed from various perspectives, e.g., in Refs. [21,22,23,24,25]. Superluminal propagation was argued to be troublesome, since it indicates that a Lorentz-covariant UV-completion is impossible for such a theory [26].…”
Section: Introductionmentioning
confidence: 99%
“…The stability and superluminal nature of these models has been a subject of interesting debates in literature. Authors in [5,17,22] have argued that it is possible to obtain a healthy bounce using Galilean action while [16,23] argue that when coupling to matter or other regions of phasespace are included, Galilean models have superluminal speed of sound 2 .…”
Section: Introductionmentioning
confidence: 99%