Cosmological implications of the minimum viscosity principle

TL;DR

This paper explores how black holes in a quark-gluon plasma with minimum viscosity bounds relate to early universe conditions, suggesting long-lived remnants and implications for quantum structures and cosmology.

Contribution

It introduces a novel connection between minimum viscosity black holes, early universe quark asymmetries, and quantum coherent structures, proposing new cosmological and quantum computing implications.

Findings

Black holes obeying minimum viscosity bounds match the strong force range.

Estimated black hole evaporation time exceeds the quark-gluon plasma era.

Possible survival of quark-antiquark asymmetries as antiquark nuggets.

Abstract

It is shown that black holes in a quark gluon plasma (QGP) obeying minimum viscosity bounds, exhibit a Schwarzschild radius in close match with the range of the strong force. For such black holes, an evaporation time of about 1016 secs is estimated, indicating that they would survive by far the quark-gluon plasma era, namely between 10^-10 and 10^-6 seconds after the big bang. On the assumption that the big-bang generated unequal amounts of quark and antiquarks, this suggests that such unbalance might have survived to this day in the form of excess antiquark nuggets hidden to all but gravitational interactions. A connection with the saturon picture, whereby minimum viscosity regimes would associate with the onset coherent quantum field structures with maximum storage properties, is also established, along with potential implication for quantum computing of classical systems.