Holography in the Gravitational Wave Era
This project aims to enhance understanding of quantum matter and gravity through holography, focusing on cosmological phase transitions, neutron star mergers, and spacetime singularities.
Projectdetails
Introduction
The revolution unleashed by the discovery of gravitational waves will gradually unfold over the coming decades. The detection of a neutron star merger by LIGO and Virgo opened a new era in multi-messenger astronomy. Future ground-based interferometers, such as the Cosmic Explorer and the Einstein Telescope, will extend the range of detection to the entire Universe, and the frequency to millions of detections per year. Space-based missions like LISA may discover gravitational waves from phase transitions in the early Universe.
Theoretical Understanding
Reaping the benefits of this experimental revolution requires a theoretical understanding of quantum matter coupled to dynamical classical gravity. The fact that the relevant physics is often out-of-equilibrium and/or strongly coupled makes this a challenging regime for conventional approaches.
Project Purpose
The purpose of this project is to use holography, also known as gauge/string duality, to make essential contributions in this direction. I have recently pioneered and provided proof of concept that this line of research is both powerful and feasible.
Research Program
In the next five years, I will turn these initial investigations into a fully-fledged research program to improve our understanding of:
- Cosmological phase transitions, in particular of bubble dynamics and baryogenesis;
- Neutron stars, with a focus on out-of-equilibrium physics in binary mergers;
- Spacetime singularities, specifically in the presence of quantum matter effects.
Interconnected Objectives
These three main objectives are interconnected by two horizontal lines:
- Identification of universal observables, which hold the best potential to make contact with experiment;
- Communication with other fields, which is crucial for the success of an interdisciplinary proposal.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.499.451 |
Totale projectbegroting | € 2.499.451 |
Tijdlijn
Startdatum | 1-1-2025 |
Einddatum | 31-12-2029 |
Subsidiejaar | 2025 |
Partners & Locaties
Projectpartners
- UNIVERSITAT DE BARCELONApenvoerder
Land(en)
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High-Precision Gravitational Wave Physics from a Worldline Quantum Field Theory
This project aims to enhance the precision of gravitational wave predictions from black hole and neutron star mergers using a novel quantum formalism to test Einstein's gravity in extreme conditions.
Black holes: gravitational engines of discovery
The project aims to explore black holes and compact binaries through gravitational-wave and electromagnetic observations to advance understanding of strong gravity and fundamental physics.
From Subatomic to Cosmic Scales: Simulating, Modelling, Analysing Binary Neutron Star Mergers
The project aims to develop theoretical models for binary neutron star mergers to enhance the accuracy of multi-messenger observations, enabling insights into matter at supranuclear densities and the expansion rate of the Universe.
Dynamical Formation of Black Hole Mergers
This ERC research program aims to advance gravitational wave astrophysics by developing tools and methods to investigate binary black hole mergers and their formation in dense stellar environments.
de Sitter Space Holography and Quantum Information
This project aims to explore holography in de Sitter space using quantum information tools to identify a precise quantum mechanical dual, enhancing our understanding of quantum gravity.