Abstract
It has long been known that the sharpened tension between the observed and inferred values of the Hubble constant ${H}_{0}$ can be alleviated if a fraction of dark-matter particles of type $\ensuremath{\chi}$ were produced nonthermally in association with photons $\ensuremath{\gamma}$ through the decays of a heavy and relatively long-lived state, viz., $X\ensuremath{\rightarrow}\ensuremath{\chi}\ensuremath{\gamma}$. It was recently proposed that this model can also resolve the long-standing lithium (also known as $^{7}\mathrm{Li}$) problem if $M=4\text{ }\text{ }\mathrm{MeV}$ and $m=0.04\text{ }\text{ }\mathrm{keV}$, where $M$ and $m$ are, respectively, the masses of $X$ and $\ensuremath{\chi}$. We confront this proposal with experiment and demonstrate that cold dark matter decaying before recombination cannot resolve the ${H}_{0}$ problem. Moreover, we show that the best-case scenario for alleviating the ${H}_{0}$ tension within the context of cold dark matter decaying before recombination arises when the particles decay exclusively into dark radiation, while leaving completely unmodified the production of light elements. To this end, we calculate the general functional form describing the number of equivalent light neutrino species $\mathrm{\ensuremath{\Delta}}{N}_{\mathrm{eff}}$ carried by $\ensuremath{\chi}$. We show that to resolve the ${H}_{0}$ tension at the $1\ensuremath{\sigma}$ level, a 55% correction in $m$ is needed and that the required $\mathrm{\ensuremath{\Delta}}{N}_{\mathrm{eff}}$ is excluded at 95% C.L. by Planck data. We argue in favor of a more complex model of dynamical dark matter to relax the ${H}_{0}$ tension.
Highlights
Over the past decade, cosmological parameters have been measured to unprecedented precision
We confront this proposal with experiment and demonstrate that cold dark matter decaying before recombination cannot resolve the H0 problem
We show that the best-case scenario for alleviating the H0 tension within the context of cold dark matter decaying before recombination arises when the particles decay exclusively into dark radiation, while leaving completely unmodified the production of light elements
Summary
Cosmological parameters have been measured to unprecedented precision. Both short-lived (τ ≪ tLS) and long-lived (τ ≫ tLS) darkmatter particles decaying into dark radiation provide promising scenarios to tackle the tension on the expansion rate (where τ is the particle’s lifetime and tLS denotes the time of last scattering) [6,7,8,9,10] To understand why this is so, we begin by noting that the CMB anisotropy power spectrum tightly constrains the angular size of the sound horizon at recombination θÃ, which in a flat universe is given by the ratio of the comoving sound horizon to the comoving angular diameter distance to last-scattering surface: θà 1⁄4 rsðzLSÞ=DMðzLSÞ.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.