Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data | Paper Citation Record

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This paper cites Therefore, local bounds do not force the model to become observationally indistinguishable from ΛCDM at cosmological scales.

Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data Therefore, local bounds do not force the model to become observationally indistinguishable from ΛCDM at cosmological scales

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This paper cites Within DESI-DR2+BBN+CMB, the best-fit value of the f(R) model is S8 = 0.8129±0.0086, which is larger than the corresponding ΛCDM value S8 = 0.8076±0.0083.

Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data Within DESI-DR2+BBN+CMB, the best-fit value of the f(R) model is S8 = 0.8129±0.0086, which is larger than the corresponding ΛCDM value S8 = 0.8076±0.0083

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Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data For the Hubble constant, the modified gravity scenario yields values ofH0 that are systematically slightly lower than those obtained in the ΛCDM model for all dataset combinations

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This paper cites The scalaron thereforeadiabatically tracks ϕmin(ρ(t)) throughout the cosmological evolution, justifying the quasi-static approximation used in the background equations (4) and (5).

Testing Exponential $f(R)$ Gravity with CMB, DESI-DR2, and Supernova Data The scalaron thereforeadiabatically tracks ϕmin(ρ(t)) throughout the cosmological evolution, justifying the quasi-static approximation used in the background equations (4) and (5)

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