- Abstract:
-
Measurements of the SNe Ia Hubble diagram which suggest that the universe is accelerating due to the effect of dark energy may be biased because we are located in a 200-300 Mpc underdense "void" which is expanding 20-30% faster than the average rate. With the smaller global Hubble parameter, the WMAP-5 data on cosmic microwave background anisotropies can be fitted without requiring dark energy if there is some excess power in the spectrum of primordial perturbations on 100 Mpc scales. The SDS...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2009.15670.x
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- Journal:
- Mon.Not.Roy.Astron.Soc.
- Volume:
- 401
- Issue:
- 1
- Pages:
- 547
- Publication date:
- 2008-07-28
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:124458d0-4635-4b0a-a80e-c8eb9c2dcd83
- Source identifiers:
-
180080
- Local pid:
- pubs:180080
- Language:
- English
- Keywords:
- Copyright date:
- 2008
- Notes:
- 14 pages, 7 figures; accepted for publication in MNRAS
Journal article
Constraints on large scale inhomogeneities from WMAP-5 and SDSS: confrontation with recent observations
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