Effect of loop quantization prescriptions on the physics of non-singular gravitational collapse

Giesel K, Li BF, Singh P (2023)


Publication Type: Conference contribution

Publication year: 2023

Original Authors: Kristina Giesel, Bao-Fei Li, Parampreet Singh

Series: The Sixteenth Marcel Grossmann Meeting, pp. 4267-4271 (2023)

Event location: Rome IT

DOI: 10.1142/9789811269776_0357

Abstract

We review recent developments in the physical implications of two loop quantization strategies for the interior of a homogeneous dust cloud. The first is the loop quantization with holonomies and the triads while the second is with holonomies and the gauge covariant fluxes. Although both of the quantization schemes resolve the classical central singularity regardless of the initial conditions, they also lead to a distinct phenomenology. For the first loop quantization, we find that when the dust mass is larger than a threshold value, both black hole and white hole would form and their evolution is symmetric with respect to the bounce point, leading to black hole-white hole twins. In contrast, in the second quantization, the evolution of the outermost dust shell is asymmetric with respect to the bounce point, and as a result the black hole-white hole twins can never form. Even in the situation when both black hole and white hole can form, the mass of the latter is only 2/π of the mass of the former.

Authors with CRIS profile

Involved external institutions

How to cite

APA:

Giesel, K., Li, B.-F., & Singh, P. (2023). Effect of loop quantization prescriptions on the physics of non-singular gravitational collapse. In Proceedings of the The Sixteenth Marcel Grossmann Meeting, pp. 4267-4271 (2023). Rome, IT.

MLA:

Giesel, Kristina, Bao-Fei Li, and Parampreet Singh. "Effect of loop quantization prescriptions on the physics of non-singular gravitational collapse." Proceedings of the The Sixteenth Marcel Grossmann Meeting, pp. 4267-4271 (2023), Rome 2023.

BibTeX: Download