Emergence of Spacetime from Fluctuations
Preprint
Abstract
We use a result of Hawking and Gilkey to define a Euclidean path integral of gravity and matter which has the special property of being independent of the choice of basis in the space of fields. This property allows the path integral to describe also physical regimes that do not admit position bases. These physical regimes are pre-geometric in the sense that they do not admit a mathematical representation of the physical degrees of freedom in terms of fields that live on a spacetime. In regimes in which a spacetime representation does emerge, the geometric properties of the emergent spacetime, such as its dimension and volume, depend on the balance of fermionic pressure and bosonic and gravitational pull. That balance depends, at any given energy scale, on the number of bosonic and fermionic species that contribute, which in turn depends on their masses. This yields an explicit mechanism by which the effective spacetime dimension can depend on the energy scale.Keywords
All Related Versions
This publication has 29 references indexed in Scilit:
- Gravitational-wave luminosity distance in quantum gravityPhysics Letters B, 2019
- The causal set approach to quantum gravityLiving Reviews in Relativity, 2019
- Quantum Gravity and the Functional Renormalization Group2018
- Dimension and dimensional reduction in quantum gravityClassical and Quantum Gravity, 2017
- What every physicist should know about string theoryPhysics Today, 2015
- Gauge/Gravity Duality2015
- A lower bound for the first eigenvalue in the Laplacian operator on compact Riemannian manifoldsJournal of Geometry and Physics, 2013
- Nonperturbative quantum gravityPhysics Reports, 2012
- Introduction to Quantum Effects in Gravity2007
- String Theory and M-Theory2006