Population III star explosions and Planck 2018 data

We investigate the effect of population III (Pop III) stars supernova explosion (SN) on high redshifts reionization history using latest Planck data. It is predicted that massive Pop $(130\text{ }\text{ }{M}_{\ensuremath{\bigodot}}\ensuremath{\le}M\ensuremath{\le}270\text{ }{M}_{\ensuremath{\bigodot}})$ explode energetically at end their stellar life as pair-instability supernovae (PISNe). In explosion, remnants grow hot ionized bubbles and enhance ionization fraction in early stage history. This enhancement affects optical depth cosmic microwave background (CMB) generates additional anisotropy CMB polarization large scales. Therefore, analyzing data allows us to examine star SNe abundance progenitors, stars. order model supernova(SN) contribution reionization, we introduce a new parameter $\ensuremath{\zeta}$, which relates collapse Universe. Using Markov chain Monte Carlo method with data, obtain constraint our parameter, $\ensuremath{\zeta}$. Our tells observed consistent PISNe from formation rate initial mass function recent cosmological simulations. also suggest combining further observations late history, such redshift quasi-stellar object (QSO) observations, can provide tighter constraints important information nature