Pseudo-Complex General Relativity: Schwarzschild, Reissner-Nordström and Kerr Solutions

Abstract

The pseudo-complex General Relativity (pc-GR) is further considered. A new projection method is proposed. It is shown, that the pc-GR introduces automatically terms into the system which can be interpreted as dark energy. The modified pseudo-complex Schwarzschild solution is investigated. The dark energy part is treated as a liquid and possible solutions are discussed. As a consequence, the collapse of a large stellar mass into a singularity at $r=0$ is avoided and no event-horizon is formed. Thus, black holes don't exist. The resulting object can be viewed as a gray star. It contains no singularity which emphasizes, again, that it is not a black hole. The corrections implied by a charged large mass object (Reissner- Nordström) and a rotating gray star (Kerr) are presented. For the latter, a special solution is presented. Finally, we will consider the orbital speed of a mass in a circular orbit and suggest a possible experimental verification.

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• The black hole merger event GW150914 within a modified theory of General Relativity
• Testing pseudo-complex general relativity with gravitational waves
• Vacuum fluctuation inside a star and their consequences for neutron stars, a simple model
• Predictions of the pseudo-complex theory of Gravity for EHT observations- II. Theory and predictions
• Confronting eikonal and post-Kerr methods with numerical evolution of scalar field perturbations in spacetimes beyond Kerr