Reconstructing the Cosmic Expansion History with a Monotonicity Prior
Youhua Xu, Hu Zhan, Yeuk-Kwan Edna Cheung

TL;DR
This paper introduces a method to reconstruct the cosmic expansion history by enforcing a monotonicity prior on the Hubble parameter, reducing errors and improving consistency with other cosmological measurements.
Contribution
It proposes a monotonicity prior for reconstructing the Hubble parameter, enhancing accuracy and reducing bias in cosmological data analysis.
Findings
Monotonicity prior does not bias results in mock data tests.
Errors on the Hubble parameter are significantly reduced with the prior.
Results from real SN Ia data agree with galaxy age measurements.
Abstract
The cosmic expansion history, mapped by the Hubble parameter as a function of redshift, offers the most direct probe of the dark energy equation of state. One way to determine the Hubble parameter at different redshifts is essentially differentiating the cosmic age or distance with respect to redshift, which may incur large numerical errors with observational data. Taking the scenario that the Hubble parameter increases monotonically with redshift as a reasonable prior, we propose to enforce the monotonicity when reconstructing the Hubble parameter at a series of redshifts. Tests with mock type Ia supernova (SN Ia) data show that the monotonicity prior does not introduce significant biases and that errors on the Hubble parameter are greatly reduced compared to those determined with a flat prior at each redshift. Results from real SN Ia data are in good agreement with those based on ages…
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