Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx
Alejandro Mata Rom\'an, Indira Ocampo, Savvas Nesseris

TL;DR
This paper evaluates how well the upcoming SPHEREx survey can test the $ ext{Lambda}$CDM model and its assumptions by forecasting measurement precisions and exploring model dependence effects using neural networks.
Contribution
It introduces a Fisher matrix forecasting approach combined with neural network analysis to assess SPHEREx's potential in testing cosmological models and highlights the importance of considering covariance matrix model dependence.
Findings
SPHEREx can precisely measure BAO observables like $D_A(z)$ and $H(z)$.
Neural networks can detect the underlying cosmological model from covariance matrices with 98% accuracy.
Covariance matrix dependence on the cosmological model is significant and often neglected.
Abstract
In this work we quantify the ability of the upcoming SPHEREx survey to constrain cosmological observables and test the internal consistency of the cosmological constant and cold dark matter (CDM) model. Using Fisher matrix forecasting, we assess the expected precision on Baryon Acoustic Oscillations (BAO) observables, such as the angular diameter distance and the Hubble parameter . We further explore SPHEREx's potential to probe some of the fundamental assumptions of large-scale spatial homogeneity and isotropy, through model-independent reconstructions of several consistency tests of the CDM model. In addition, we also examine the effect of the model dependence of the resulting Fisher and covariance matrices, using a neural network (NN) classification approach. We find that, while it is commonly assumed the covariance matrix depends weakly on…
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