Simulating the collapse of rotating primordial gas clouds to study the survival possibility of Pop III protostars

Shubham Raghuvanshi, Jayanta Dutta

It has been argued that the low-mass primordial stars ($m_{\mathrm{PopIII}}\le 0.8M_{\odot }$) are likely to enter the main sequence and hence possibly be found in the present-day Ga…