The Remnant of GW170817: A Trapped Neutron Star with a Massive Incompressible Superfluid Core

Ahmad A. Hujeirat, Ravi Samtaney
2020 Journal of Modern Physics  
Our bimetric spacetime model of glitching pulsars is applied to the remnant of GW170817. Accordingly, pulsars are born with embryonic incompressible superconducting gluon-quark superfluid cores (SuSu-matter) that are embedded in Minkowski spacetime, whereas the ambient compressible and dissipative media (CDM) are imbedded in curved spacetime. As pulsars cool down, the equilibrium between both spacetime is altered, thereby triggering the well-observed glitch phenomena. Based thereon and assuming
more » ... all neutron stars (NSs) to be born with the same initial mass of , but predicted to increase as the CDM and cools down, rendering the remnant an invisible dark energy object, and therefore to an excellent black hole candidate.
doi:10.4236/jmp.2020.1111111 fatcat:d5xkog5llveurdyolk3pdqb3e4