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Marginal evidence for cosmic acceleration from Type Ia supernovae

Abstract:
The ‘standard’ model of cosmology is founded on the basis that the expansion rate of the universe is accelerating at present — as was inferred originally from the Hubble diagram of Type Ia supernovae. There exists now a much bigger database of supernovae so we can perform rigorous statistical tests to check whether these ‘standardisable candles’ indeed indicate cosmic acceleration. Taking account of the empirical procedure by which corrections are made to their absolute magnitudes to allow for the varying shape of the light curve and extinction by dust, we find, rather surprisingly, that the data are still quite consistent with a constant rate of expansion.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1038/srep35596

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author


Publisher:
Springer Nature
Journal:
Scientific Reports More from this journal
Volume:
6
Issue:
1
Article number:
35596
Publication date:
2016-10-21
Acceptance date:
2016-10-03
DOI:
EISSN:
2045-2322


Language:
English
Keywords:
Pubs id:
pubs:656097
UUID:
uuid:c15c4d1a-6b31-4213-81a6-c618ffc501a6
Local pid:
pubs:656097
Source identifiers:
656097
Deposit date:
2016-11-01

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