Talk detail

MG13 - Talk detail

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 Participant

Pinto-Neto, Nelson

Institution

Centro Brasileiro de Pesquisas Físicas  - Rua das laranjeiras, 83, 1103 - Rio de Janeiro - Rio de Janeiro - Brazil

Session

CM3

Accepted

Yes

Order

6

Time

16:30 - 16:50

Talk

Oral abstract

Title

Bouncing Models and the Cosmological Constant
Co-authors Rodrigo Maier, Stella Pereira and Beatriz B. Siffert

Abstract

Most bouncing models contain a contracting phase from a very large and rarefied state, where dark energy might have had an important role as it has today in accelerating our large Universe. In this talk, we will assume the simplest and most appealing candidate for dark energy, the cosmological constant, and evaluate its influence on the evolution of cosmological perturbations during the contracting phase of a bouncing model, which also contains a scalar field satisfying $p=w\epsilon$, $w$ being a constant. An almost scale invariant spectrum of perturbations is obtained for $w\approx 0$, which is the usual result for bouncing models. However, the presence of the cosmological constant induces oscillations and a running towards a tiny red-tilted spectrum for long wavelength perturbations.

Session

CM3

Accepted

Yes

Order

1

Time

14:00 - 14:40

Talk

Oral abstract

Title

Revision talk on bouncing models
Co-authors

Abstract

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