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The Mathematical Analysis of Extremal Black Holes and Gravitational Radiation

Project description

Tackling fundamental questions in general relativity with advanced mathematical tools

Einstein equations, a system of non-linear partial differential equations, are central to understanding gravitational dynamics in general relativity. Recent advances in partial differential equations, differential geometry and microlocal analysis have deepened understanding of gravitational dynamics. The ERC-funded ExBHGravRad project focuses on two key mathematical problems. First, it will examine the stability and instability of extremal Kerr black holes, which are rapidly rotating objects at the boundary between black holes and naked singularities. Resolving this could reveal how these extreme black holes behave when perturbed. Second, it will investigate late-time tails in gravitational radiation by analysing the dynamics of perturbations in both flat space-time and black hole space-times. The proposed research could advance the understanding of the strong cosmic censorship conjecture.

Objective

"The Einstein equations constitute a system of geometric, nonlinear partial differential equations that describe gravitational dynamics in the framework of Einstein's theory of general relativity. The last decade has seen tremendous progress towards understanding dynamical aspects of the Einstein equations. At the mathematical level, great insight has been gained due to recent advances in the study of partial differential equations, differential geometry and microlocal analysis. The present proposal builds upon these advances in the context of the following two mathematical problems.

Stability and instability of extremal black holes: Extremal Kerr black holes describe rapidly rotating solutions to the Einstein equations. They sit at the transition between black holes and ""naked singularities"" and exhibit critical geometric features.

This proposal addresses the stability and instability properties of extremal Kerr black holes and is motivated by recent advances by the PI, which cover linear and nonlinear aspects. A successful resolution would give fundamental, new insights into the fate of perturbed extremal black holes and the transition between black holes and naked singularities.

The late-time analysis of gravitational radiation: Gravitational radiation provides an observational window into deep mathematical aspects of general relativity. In this proposal, we investigate a key feature that is amenable to mathematical analysis: the existence of late-time tails in gravitational radiation.

Recent work by the PI and collaborators has lead to the first proof of the existence of late-time tails in a toy model setting, also known as Price's Law. This proposal considers the full setting of the nonlinear Einstein equations via the analysis of late-time tails in the dynamics of perturbations of both flat spacetime and black hole spacetimes. A successful resolution would have important implications for the Strong Cosmic Censorship conjecture."

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Topic(s)

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HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

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(opens in new window) ERC-2023-STG

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Host institution

UNIVERSITAET LEIPZIG
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 497 500,00
Address
RITTERSTRASSE 26
04109 Leipzig
Germany

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Region
Sachsen Leipzig Leipzig
Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 497 500,00

Beneficiaries (1)

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