Abstract
Recently we presented limits on the deviation of the Universe from a Friedmann-Robertson-Walker form, which are implied directly by anisotropies in the cosmic background radiation, without assuming inflationary or other models of evolution. Here we weaken some of our previous assumptions, ensuring that all assumptions are in principle observational, and obtain improved limits.
Original language | English |
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Pages (from-to) | 5942-5945 |
Number of pages | 4 |
Journal | Physical Review D |
Volume | 51 |
Issue number | 10 |
DOIs | |
Publication status | Published - 15 May 1995 |