Gravity, Geometry and the Quantum
Abhay Ashtekar
Abstract
Open-access reader
Abhay Ashtekar
Abstract
Open-access reader
After a brief introduction, basic ideas of the quantum Riemannian geometry underlying loop quantum gravity are summarized. To illustrate physical ramifications of quantum geometry, the framework is then applied to homogeneous isotropic cosmology. Quantum geometry effects are shown to replace the big bang by a big bounce. Thus, quantum physics does not stop at the big‐bang singularity. Rather there is a pre‐big‐bang branch joined to the current post‐big‐bang branch by a ‘quantum bridge’. Furthermore, thanks to the background independence of loop quantum gravity, evolution is deterministic across the bridge.
OpenAlex reports 38 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
After a brief introduction, basic ideas of the quantum Riemannian geometry underlying loop quantum gravity are summarized. To illustrate physical ramifications of quantum geometry, the framework is then applied to homogeneous isotropic cosmology. Quantum geometry effects are shown to replace the big bang by a big bounce. Thus, quantum physics does not stop at the big‐bang singularity. Rather there is a pre‐big‐bang branch joined to the current post‐big‐bang branch by a ‘quantum bridge’. Furthermore, thanks to the background independence of loop quantum gravity, evolution is deterministic across the bridge.
Key concepts: Loop quantum cosmology, Quantum geometry, Loop quantum gravity, Big Bounce, Quantum gravity, Quantum cosmology, Initial singularity, Physics