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Large-scale galaxy correlations as a test for dark energy

Abstract:

We have shown earlier that, contrary to popular belief, Einstein--de Sitter (E--deS) models can still fit the {\sl WMAP} data on the cosmic microwave background provided one adopts a low Hubble constant and relaxes the usual assumption that the primordial density perturbation is scale-free. The recent {\sl SDSS} measurement of the large-scale correlation function of luminous red galaxies at $z \sim 0.35$ has however provided a new constraint by detecting a `baryon acoustic peak'. Our best-fit...

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Publication status:
Published

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Publisher copy:
10.1051/0004-6361:20054640

Authors


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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author
Journal:
Astron.Astrophys. More from this journal
Volume:
449
Issue:
3
Pages:
925
Publication date:
2005-12-05
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
Language:
English
Keywords:
Pubs id:
pubs:180105
UUID:
uuid:ebb3a0b2-0b51-4cbe-b0c1-75bdbd03e7fa
Local pid:
pubs:180105
Source identifiers:
180105
Deposit date:
2012-12-19

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