Intensity mapping of post-reionization 21-cm signal and its cross-correlations as a probe of $f(R)$ gravity
CHANDRACHUD B. V. DASH TAPOMOY GUHA SARKAR ANJAN KUMAR SARKAR
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We propose the intensity mapping of the redshifted Hi 21-cm signal from the post-reionization epoch as a cosmological probe of $f(R)$ gravity. We consider the Hu–Sawicki family of $f(R)$ gravity models characterized by a single parameter $f_{,R0}$. The $f(R)$ modification to gravity affects the post-reionization 21-cm power spectrum through the change in the growth rate of density fluctuations. We find that a radio interferometric observation with a SKA1-mid-like radio telescope in both auto-correlation and cross-correlation with galaxy weak-lensing and Lyman-$\alpha$ forest may distinguish $f(R)$ models from $\Lambda$CDM cosmology at a precision, whichis competitive with other probes of $f(R)$ gravity.
CHANDRACHUD B. V. DASH1 TAPOMOY GUHA SARKAR1 ANJAN KUMAR SARKAR2 3
Volume 44, 2023
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