Model-Independent Measurement of the Matter-Radiation Equality Scale in DESI 2024
arXiv:2505.16153 · doi:10.1103/yqm1-ybbv
Abstract
The peak of the matter power spectrum, known as the turnover (TO) scale, is determined by the horizon size at the time of matter-radiation equality. This scale can serve as a standard ruler, independent of other features in the matter power spectrum, such as baryon acoustic oscillations (BAO). Here, we present the first detection of the turnover in the galaxy auto-power spectrum, utilising the distribution of quasars (QSO) and luminous red galaxies (LRG) measured by the Dark Energy Spectroscopic Instrument (DESI) during its first year of survey operations in a model-independent manner. To avoid confirmation bias, we first analyse the data using data blinding methods designed for the DESI baryon acoustic oscillation, redshift space distortion and scale-dependent bias signals. We measure the angle-averaged dilation distance from the quasars and from the LRG sample in units of the horizon at the matter-radiation-equality epoch. Combining these two constraints and assuming a flat CDM model with three standard neutrino species, we can translate this into a constraint of . We can break the - degeneracy with low-redshift distance measurements from type-Ia supernova (SN) data from Pantheon+, we obtain a sound-horizon free estimate of the Hubble-Lemaître parameter of km/s/Mpc, consistent with sound-horizon dependent DESI measurements. On the other hand, combining the DESI BAO and TO, we find a truly DESI-only measurement of km/s/Mpc, in line with DESI-only full-shape results where the sound-horizon scale is marginalised out. This discrepancy in can be reconciled in a CDM cosmology, where the combination of DESI BAO and TO data yields .
21 pages, 13 figures, 2 tables. Version updated to match version accepted by the journal
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