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Space-like singularities beyond general relativity

Project description

Quantum gravity theories to understand space-like singularities

Recent studies of space-like singularities (where spacetime curvature is infinite) have highlighted challenges for modern physics and the limitations of general relativity. To address these, several quantum gravity frameworks have emerged, with string theory being the most notable. These frameworks enhance the Einstein-Hilbert Lagrangian by incorporating higher-order curvature terms. With the support of the Marie Skłodowska-Curie Actions programme, the SpSBeyondGR project will expand our understanding of space-like singularities in the context of these theories. Additionally, the project will reformulate the Belinski-Khalatnikov-Lifshitz conjecture within generalised quasi-topological gravities to understand chaotic dynamics near space-like singularities, such as black holes and the early universe. It will also pursue additional activities, including developing key computationally efficient numerical methods and exploring holographic implications of singularities.

Objective

Space-like singularities, where space-time curvature becomes infinite, pose a profound challenge in modern physics, highlighting the limitations of general relativity and necessitating a quantum gravity framework. Several potential candidates for quantum gravity have been proposed and developed, with String Theory standing out as the most prominent one. At the level of low-energy effective actions, these theories refine the Einstein–Hilbert Lagrangian by introducing specific higher-order terms in spacetime curvature. This proposal seeks to understand space-like singularities in this context. Particularly, I will reformulate the Belinski-Khalatnikov-Lifshitz (BKL) conjecture within generalised quasi-topological gravities. This approach aims to deepen our understanding of the chaotic dynamics near space-like singularities, particularly in black holes and the early universe.

The motivation for this research stems from the need to understand space-like singularities, particularly the spacetime dynamics close to it, in an effective theory of quantum gravity. The project involves developing computationally efficient numerical methods to solve the complex equations of motion in generalised quasi-topological gravity coupled with massive tensor fields, focusing on spherically symmetric spacetimes to maintain tractability. We will explore the holographic implications of singularities through the AdS/CFT correspondence, analyzing boundary conformal field theory observables to gain insights into black hole interiors. This dual approach will enhance our understanding of how singularities encode themselves in these observables and provide fresh perspectives on the holographic nature of black hole interiors.

The project will be conducted under the supervision of Professor Simon Ross at Durham University. The expected outcomes include significant advancements in theoretical physics, resulting in high-impact publications and the development of new computational techniques.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

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Funding Scheme

HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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Call for proposal

(opens in new window) HORIZON-MSCA-2024-PF-01

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Coordinator

UNIVERSITY OF DURHAM
Net EU contribution
€ 276 187,92
Address
STOCKTON ROAD THE PALATINE CENTRE
DH1 3LE DURHAM
United Kingdom
Region
North East (England) Tees Valley and Durham Durham CC
Activity type
Higher or Secondary Education Establishments
Links
Total cost
No data