Background Independent Quantum Field Theory and the Cosmological Constant Problem
Olaf Dreyer
Abstract
We introduce the notion of background independent quantum field theory. The distinguishing feature of this theory is that the dynamics can be formulated without recourse to a background metric structure. We show in a simple model how the metric properties of spacetime can be recovered from the dynamics. Background independence is not only conceptually desirable but allows for the resolution of a problem haunting ordinary quantum field theory: the cosmological constant problem.
Create a lesson
Related papers
Horizon exchange and the universal all-spin response of Kerr
Pierre Vanhove
Hecke Relations from Self-Duality
Justin Kaidi
Weyl Rescalings: A First Order Approach
L. Andrianopoli, J. Zanelli
Interpolating between 4d N= 1 SCFT supercurrent multiplet anomalies
Pantelis Panopoulos, Ioannis Papadimitriou
Crossover from Schwarzian dynamics to rotational soft modes in near-extremal Lovelock black holes
Ankit Anand, Aditya Singh, Kimet Jusufi
Fortuitous BMN Operators from Multiple Cores
Robert de Mello Koch, Sarthak Duary, Minkyoo Kim et al.