Big Bang equivalence of $f(R)$ gravity with no cosmological lithium problem

Big Bang equivalence of $f(R)$ gravity with no cosmological lithium problem
Abhijit Talukdar, Sanjeev Kalita
arXiv:2404.12084v1 Announce Type: new
Abstract: $f(R)$ gravity is one of the serious alternatives of general relativity having large range of astronomical consequences. In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. We consider modification to gravity due to the existence of primordial black holes in the radiation era which introduce additional degrees of freedom known as scalarons. We calculate the light element abundances by using the BBN code PArthENoPE. It is found that for a range of scalaron mass $(2.2-3.5) times 10^4$ eV, the abundance of lithium is lowered by $3-4$ times the value predicted by general relativistic BBN which is a level desired to address the cosmological lithium problem. For the above scalaron mass range helium abundance is within observed bound. However, deuterium abundance is found to be increased by $3-6$ times the observed primordial abundance which calls for high efficiency of stellar formation and evolution processes for destruction of the same. A novel relation between scalaron mass and black hole mass has been used to estimate that the above scalaron mass range corresponds to primordial black holes of sub-planetary mass ($sim 10^{19}$ g) serving as one of the potential non-baryonic dark matter candidates. We infer Big Bang equivalence of power law $f(R)$ gravity with primordial black holes.arXiv:2404.12084v1 Announce Type: new
Abstract: $f(R)$ gravity is one of the serious alternatives of general relativity having large range of astronomical consequences. In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. We consider modification to gravity due to the existence of primordial black holes in the radiation era which introduce additional degrees of freedom known as scalarons. We calculate the light element abundances by using the BBN code PArthENoPE. It is found that for a range of scalaron mass $(2.2-3.5) times 10^4$ eV, the abundance of lithium is lowered by $3-4$ times the value predicted by general relativistic BBN which is a level desired to address the cosmological lithium problem. For the above scalaron mass range helium abundance is within observed bound. However, deuterium abundance is found to be increased by $3-6$ times the observed primordial abundance which calls for high efficiency of stellar formation and evolution processes for destruction of the same. A novel relation between scalaron mass and black hole mass has been used to estimate that the above scalaron mass range corresponds to primordial black holes of sub-planetary mass ($sim 10^{19}$ g) serving as one of the potential non-baryonic dark matter candidates. We infer Big Bang equivalence of power law $f(R)$ gravity with primordial black holes.