Abstract
We present a precise measurement of cosmological time dilation using the light curves of 1504 Type Ia supernovae from the Dark Energy Survey spanning a redshift range 0.1 z 1.2. We find that the width of supernova light curves is proportional to (1 + z), as expected for time dilation due to the expansion of the Universe. Assuming Type Ia supernovae light curves are emitted with a consistent duration Δtem, and parametrizing the observed duration as Δtobs = Δtem(1 + z)b, we fit for the form of time dilation using two methods. First, we find that a power of b ≈ 1 minimizes the flux scatter in stacked subsamples of light curves across different redshifts. Secondly, we fit each target supernova to a stacked light curve (stacking all supernovae with observed bandpasses matching that of the target light curve) and find b = 1.003 ± 0.005 (stat) ± 0.010 (sys). Thanks to the large number of supernovae and large redshift-range of the sample, this analysis gives the most precise measurement of cosmological time dilation to date, ruling out any non-time-dilating cosmological models at very high significance.
Original language | English |
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Pages (from-to) | 3365-3378 |
Number of pages | 14 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 533 |
Issue number | 3 |
DOIs | |
State | Published - Sep 1 2024 |
Keywords
- cosmology: observations
- transients: supernovae