Skip to main content
Go to the home page of the European Commission (opens in new window)
English en
CORDIS - EU research results
CORDIS

Transcending the Boundaries of Holography

Project description

Gravity, chaos and the holographic heart of black holes

Black holes are much more than cosmic mysteries. They also reveal links between gravity and quantum physics. The ERC-funded TraBHolo project aims to explore the physics near black hole singularities and their possible holographic descriptions, where a dual quantum theory could capture the full gravitational behaviour. Existing models rely on a negative cosmological constant, making them unrealistic for the study of our universe. TraBHolo introduces new methods to approximate the complicated near-singularity dynamics of gravity using dynamical Carroll geometry. The project also works towards holographic models for flat spacetime, aiming to quantise dual field theories and illuminate the hidden structure of black holes, gravity and the holographic universe.

Objective

In this project, I will develop new and timely methods for studying gravity in asymptotically flat spacetime and in the region near black hole singularities, along with their possible holographic interpretations. The thermodynamics associated to black hole event horizons suggests a holographic description in terms of a quantum theory without gravity in fewer dimensions. From string theory, such holographic dualities have been constructed and were tested to amazing precision, but all currently-known examples rely crucially on a negative cosmological constant, which prevents us from using them to make predictions for black holes in our universe. On the other hand, approximating gravity near spacelike singularities has long been known to lead to rich and chaotic dynamics, which therefore appears to be a fundamental property of black holes. However, its relation to known holographic descriptions of black holes is still mysterious.

Very recently, I established a new and systematic method of approximating gravity near singularities using dynamical Carroll geometry. By implementing the ultra-local limit of such approximations off shell, my method leads to tractable models in settings previously only accessible with supercomputer simulations, including spatial inhomogeneity and subleading corrections. It is also connected to several recent developments identifying near-singularity chaotic dynamics in AdS/CFT holography. Additionally, using related techniques, I will work towards more realistic holographic models with zero cosmological constant. Here, I will address key roadblocks by establishing how asymptotically flat spacetime metrics are determined by a general null boundary metric, energy-momentum tensor and radiation, which will also allow me to derive consistent ways of quantizing dual Carroll field theories. Through this project I will therefore make key advances in our understanding of black holes and their singularities in gravity and holography.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

HORIZON-ERC - HORIZON ERC Grants

See all projects funded under this funding scheme

Call for proposal

(opens in new window) ERC-2025-STG

See all projects funded under this call

Host institution

TECHNISCHE UNIVERSITAET WIEN
Net EU contribution
€ 1 491 072,00
Address
KARLSPLATZ 13
1040 Wien
Austria
Region
Ostösterreich Wien Wien
Activity type
Higher or Secondary Education Establishments
Links
Total cost
€ 1 491 072,00

Beneficiaries (1)