Format results

Evolving quantum state for black holes
Steve Giddings University of California System

Nonlocal cosmological models from infrared quantum gravity effects
Enis Belgacem Utrecht University

Matterdriven phase transition in lattice quantum gravity
Andrzej Gorlich Jagiellonian University

Getting hot without accelerating: vacuum thermal effects from conformal quantum mechanics
Michele Arzano Università degli Studi di Napoli Federico II

Underground tests of Quantum Mechanics: Gravityrelated and CSL wave function collapse models
Catalina Curceanu National Institute for Nuclear Physics

Debate on Asymptotically Safe Quantum Gravity

John Donoghue University of Massachusetts Amherst

Roberto Percacci SISSA International School for Advanced Studies


Interplay of quantum gravity and matter: Role of symmetries
Astrid Eichhorn University of Southern Denmark

A Generalized HartleHawking State
Stephon Alexander Brown University

Null infinity from quasilocal phase space
Wolfgang Wieland University of ErlangenNuremberg

Deformations of General Relativity, Geometrodynamics and reality conditions
Ermis Mitsou University of Zurich

Galilean and Carrollian relativities in noncommutative spacetime models
Giulia Gubitosi University of Naples Federico II

What happens at the end of Hawking's evaporation?
Carlo Rovelli Centre de Physique Théorique