Torsional Newton-Cartan gravity and strong gravitational fields

Abstract

We review how the large $c$ expansion of General Relativity leads to an effective theory in the form of Twistless Torsional Newton-Cartan gravity. We show how this is a strong field expansion around the static sector of General Relativity and illustrate this through two examples.

arXiv commentProceedings of talk at Fifteenth Marcel Grossmann Meeting. 6p

Cited by in corpus (2)

• Torsional Newton-Cartan gravity from the large $c$ expansion of General Relativity
• Dynamical de Sitter black holes in a quasi-stationary expansion