Backreaction of linear perturbations and dark energy
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| dc.contributor.author |
Räsänen, Syksy |
|
| dc.date.accessioned |
2020-01-23T11:43:01Z |
|
| dc.date.available |
2020-01-23T11:43:01Z |
|
| dc.date.issued |
2004-08-17 |
|
| dc.identifier.citation |
Räsänen , S 2004 ' Backreaction of linear perturbations and dark energy ' arXiv . < https://arxiv.org/abs/astro-ph/0407317 > |
|
| dc.identifier.other |
PURE: 130559908 |
|
| dc.identifier.other |
PURE UUID: 72a474cb-29f5-46b3-9cf8-03269c103c33 |
|
| dc.identifier.other |
ORCID: /0000-0003-2296-302X/work/68615178 |
|
| dc.identifier.uri |
http://hdl.handle.net/10138/310237 |
|
| dc.description.abstract |
A simple discussion on the backreaction of inhomogeneities in cosmology, focusing on the possibility that it could explain the present acceleration and solve the coincidence problem. |
en |
| dc.format.extent |
4 |
|
| dc.language.iso |
eng |
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| dc.rights |
other |
|
| dc.rights.uri |
info:eu-repo/semantics/openAccess |
|
| dc.subject |
114 Physical sciences |
|
| dc.title |
Backreaction of linear perturbations and dark energy |
en |
| dc.type |
Working paper |
|
| dc.contributor.organization |
Department of Physics |
|
| dc.rights.accesslevel |
openAccess |
|
| dc.type.version |
publishedVersion |
|
| dc.identifier.url |
https://arxiv.org/abs/astro-ph/0407317 |
|
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