Revisiting big bang nucleosynthesis with a new particle species : effect of co-annihilation with nucleons

Abstract

In big bang nucleosynthesis (BBN), the light matter abundance is dictated by the neutron-to-proton ($n/p$) ratio which is controlled by the standard weak processes in the early universe. Here, we study the effect of an extra particle species ($\chi$) which \textit{co-annihilates} with neutron (proton), thereby potentially changing the ($n/p$) ratio in addition to the former processes. We find a novel interplay between the co-annihilation and the weak interaction in deciding the ($n/p$) ratio and the yield of $\chi$. Large co-annihilation strength ($G_D$) in comparison to the weak coupling ($G_F$), potentially can alter the number of nucleons in the thermal bath modifying the ($n/p$) ratio from its standard evolution. We find that the standard BBN prediction is restored for $G_D/G_F\lesssim 10^{-2}$, while the mass of $\chi$ being much smaller than the neutron mass. When the mass of $\chi$ is comparable to the neutron mass, we can allow large $G_D/G_F(\gtrsim 10^2)$ values, as the thermal abundance of $\chi$ becomes Boltzmann-suppressed. Therefore, the ($n/p$) ratio is restored to its standard value via dominant weak processes in later epochs. We also discuss the stability of the new particle in an effective theroy framework for co-annihilation. Further, the co-annihilation interaction generates elastic scattering of $\chi$ and nucleons at the next-to-leading order. This provides a way to probe the scenario in direct detection experiments, if $\chi$ is accidentally stable over cosmological timescale.

arXiv comment18 pages, 7 figures, v4: comments added, typos fixed, version as published in EPJC

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