Hola,
¿eres nuevo aquí?

Regístrate gratis y conecta tu empresa con financiación pública, partners y proyectos.

Tengo cuenta

Regístrate

Ver video

QBH

Financiado

Cerrado

Quantum Black Holes A macroscopic window into the microstructure of gravity

The thermodynamic behavior of black holes is a precious clue in unravelling the microscopic structure of quantum gravity. High precision computations of quantum black hole entropy provide a new window into the fundamental microsco... ver más

28/02/2023

KINGS COLLEGE LOND...

2M€

Presupuesto del proyecto: 2M€

Líder del proyecto

KINGS COLLEGE LONDON No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Fecha límite participación Sin fecha límite de participación.

Ver 2 Participantes

Financiación concedida El organismo H2020 notifico la concesión del proyecto el día 2023-02-28

ERC-CoG-2015: ERC Consolidator Grant Scope:Objectives

I+D

Cerrada hace 10 años

0% 100% 100%

Características del participante

Este proyecto no cuenta con búsquedas de partenariado abiertas en este momento.

Información adicional privada

No hay información privada compartida para este proyecto. Habla con el coordinador.

2 Participantes

KINGS COLLEGE LONDON

1.76M€ | Lider

SCA GANADERA DEL VALLE DE LO...

195.29K€ | Participante

Conecta tu I+D

¿Tienes un proyecto y buscas un partner? Gracias a nuestro motor inteligente podemos recomendarte los mejores socios y ponerte en contacto con ellos. Te lo explicamos en este video

Duración del proyecto: 84 meses Fecha Inicio: 2016-02-19
Fecha Fin: 2023-02-28

Líder del proyecto

KINGS COLLEGE LONDON No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 2M€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto The thermodynamic behavior of black holes is a precious clue in unravelling the microscopic structure of quantum gravity. High precision computations of quantum black hole entropy provide a new window into the fundamental microscopic theory of gravity and its deviations from classical general relativity. Traditional methods of quantum field theory have proved to be not well-suited to perform these computations. Two breakthroughs in my recent work establish new ground for progress. On one front, a new method to sum up all perturbative quantum contributions to the entropy of a large class of black holes has been developed. This gives rise to the first exactly solvable model of a quantum black hole. On a second front, a longstanding theoretical obstacle called the wall-crossing problem has been cleared in my recent work on the microscopic description of black holes in string theory. The newly-developed field of mock modular forms is shown to be the correct framework to address questions of exact black hole entropy. This makes a large class of microscopic models amenable to analytic control, many of which were previously beyond reach. These developments open up a new line of research that I propose to pursue along two intersecting avenues. First, I aim to extend the computations of exact quantum black hole entropy towards models of realistic black holes. Second, I aim to advance the theoretical understanding of quantum black holes by investigating the deeper origins of mock modular symmetry. As a concrete application, I aim to establish that newfound group-theoretical structures called moonshine symmetries are physically realized in quantum black holes, thus opening up connections between two exciting fields of research previously thought to be distinct. Together, the broad goal is to explain black hole microstructure through systematic computations of exact quantum entropy, and to investigate its consequences on the fundamental microscopic theory of gravity.

Conecta tu I+D

Entra hoy

Forgot your password?

Financiación

Empresas

CTIs/Universidades

Proyectos

Investigadores