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.

Proceedings of talk at Fifteenth Marcel Grossmann Meeting. 6p

Cited by in corpus (1)

• Dynamical de Sitter black holes in a quasi-stationary expansion