Quantization of Emergent Gravity
arXiv:1312.0580 · doi:10.1142/S0217751X15500165
Abstract
Emergent gravity is based on a novel form of the equivalence principle known as the Darboux theorem or the Moser lemma in symplectic geometry stating that the electromagnetic force can always be eliminated by a local coordinate transformation as far as spacetime admits a symplectic structure, in other words, a microscopic spacetime becomes noncommutative (NC). If gravity emerges from U(1) gauge theory on NC spacetime, this picture of emergent gravity suggests a completely new quantization scheme where quantum gravity is defined by quantizing spacetime itself, leading to a dynamical NC spacetime. Therefore the quantization of emergent gravity is radically different from the conventional approach trying to quantize a phase space of metric fields. This approach for quantum gravity allows a background independent formulation where spacetime as well as matter fields is equally emergent from a universal vacuum of quantum gravity.
113 pages (We touch only a tip of the iceberg!); to be published in Int. J. Mod. Phys. A
References in corpus (8)
Cited by in corpus (13)
- Mirror Symmetry in Emergent Gravity
- Calabi-Yau manifolds from noncommutative Hermitian U(1) instantons
- Background independent noncommutative gravity from Fedosov quantization of endomorphism bundle
- Dark Energy and Dark Matter in Emergent Gravity
- A note on graviton exchange in emergent gravity scenario
- Emergent Spacetime for Quantum Gravity
- Quantized Kähler Geometry and Quantum Gravity
- Contravariant geometry and emergent gravity from noncommutative gauge theories
- Emergent Spacetime and Cosmic Inflation
- Hermitian-Einstein metrics from noncommutative instantons
- Towards a T-dual Emergent Gravity
- Schwarzschild Instanton in Emergent Gravity
- Matrix models from localization of five-dimensional supersymmetric noncommutative U(1) gauge theory