Bouncing Cosmologies with Dark Matter and Dark Energy
We review matter bounce scenarios where the matter content is dark matter and dark energy. These cosmologies predict a nearly scale-invariant power spectrum with a slightly red tilt for scalar perturbations and a small tensor-to-scalar ratio. Importantly, these models predict a positive running of t...
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doaj-08b2d174ddfe4919ae29b54af98607b42020-11-25T01:11:43ZengMDPI AGUniverse2218-19972016-12-0131110.3390/universe3010001universe3010001Bouncing Cosmologies with Dark Matter and Dark EnergyYi-Fu Cai0Antonino Marcianò1Dong-Gang Wang2Edward Wilson-Ewing3CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, 230026 Hefei, ChinaDepartment of Physics & Center for Field Theory and Particle Physics, Fudan University, 200433 Shanghai, ChinaCAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Chinese Academy of Sciences, 230026 Hefei, ChinaMax Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, 14476 Golm, GermanyWe review matter bounce scenarios where the matter content is dark matter and dark energy. These cosmologies predict a nearly scale-invariant power spectrum with a slightly red tilt for scalar perturbations and a small tensor-to-scalar ratio. Importantly, these models predict a positive running of the scalar index, contrary to the predictions of the simplest inflationary and ekpyrotic models, and hence, could potentially be falsified by future observations. We also review how bouncing cosmological space-times can arise in theories where either the Einstein equations are modified or where matter fields that violate the null energy condition are included.http://www.mdpi.com/2218-1997/3/1/1Matter bounce scenariointeracting dark energyalternatives to inflation |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Yi-Fu Cai Antonino Marcianò Dong-Gang Wang Edward Wilson-Ewing |
spellingShingle |
Yi-Fu Cai Antonino Marcianò Dong-Gang Wang Edward Wilson-Ewing Bouncing Cosmologies with Dark Matter and Dark Energy Universe Matter bounce scenario interacting dark energy alternatives to inflation |
author_facet |
Yi-Fu Cai Antonino Marcianò Dong-Gang Wang Edward Wilson-Ewing |
author_sort |
Yi-Fu Cai |
title |
Bouncing Cosmologies with Dark Matter and Dark Energy |
title_short |
Bouncing Cosmologies with Dark Matter and Dark Energy |
title_full |
Bouncing Cosmologies with Dark Matter and Dark Energy |
title_fullStr |
Bouncing Cosmologies with Dark Matter and Dark Energy |
title_full_unstemmed |
Bouncing Cosmologies with Dark Matter and Dark Energy |
title_sort |
bouncing cosmologies with dark matter and dark energy |
publisher |
MDPI AG |
series |
Universe |
issn |
2218-1997 |
publishDate |
2016-12-01 |
description |
We review matter bounce scenarios where the matter content is dark matter and dark energy. These cosmologies predict a nearly scale-invariant power spectrum with a slightly red tilt for scalar perturbations and a small tensor-to-scalar ratio. Importantly, these models predict a positive running of the scalar index, contrary to the predictions of the simplest inflationary and ekpyrotic models, and hence, could potentially be falsified by future observations. We also review how bouncing cosmological space-times can arise in theories where either the Einstein equations are modified or where matter fields that violate the null energy condition are included. |
topic |
Matter bounce scenario interacting dark energy alternatives to inflation |
url |
http://www.mdpi.com/2218-1997/3/1/1 |
work_keys_str_mv |
AT yifucai bouncingcosmologieswithdarkmatteranddarkenergy AT antoninomarciano bouncingcosmologieswithdarkmatteranddarkenergy AT donggangwang bouncingcosmologieswithdarkmatteranddarkenergy AT edwardwilsonewing bouncingcosmologieswithdarkmatteranddarkenergy |
_version_ |
1725170170407682048 |