From Schwinger Balls to Curved Space

TL;DR

This paper demonstrates that Reissner-Nordstrom black holes can be viewed as gravitational Schwinger balls and explores their thermodynamic properties, proposing a new metric aligned with microscopic black hole models.

Contribution

It introduces the concept of black holes as gravitational Schwinger balls and proposes a new metric consistent with microscopic black hole descriptions.

Findings

Reissner-Nordstrom black holes are gravitational Schwinger balls.

Both massless and massive gravitational Schwinger balls are thermodynamic systems.

A new metric is proposed that aligns better with microscopic black hole models.

Abstract

It is shown that the Reissner-Nordstrom black hole is also a gravitational Schwinger ball. It is also shown that both massless and massive-particle gravitational Schwinger balls are thermodynamic systems by deriving the first law of thermodynamics for them. Inconsistency between classical geometrical and microscopic definitions of the horizon is discussed. We propose a new metric, more consistent with microscopic picture of black hole, as gravitational Schwinger ball, by speculations. It has some interesting features.