Gravitational radiation at infinity with non-negative cosmological constant
Jos\'e M. M. Senovilla

TL;DR
This paper develops a new framework for understanding gravitational radiation at infinity in spacetimes with non-negative cosmological constant, extending the classical News tensor approach to cases where >0.
Contribution
It introduces a novel characterization of gravitational radiation using the asymptotic super-momentum, applicable for , and proposes methods to construct news tensors and analyze asymptotic symmetries.
Findings
New characterization of gravitational radiation for .
Equivalent formulation to the standard News approach when =0.
Example of conserved charge detecting gravitational radiation.
Abstract
The existence of gravitational radiation arriving at null infinity -- i.e. escaping from the physical system -- is addressed in the presence of a non-negative cosmological constant . The case with vanishing is well understood and relies on the properties of the News tensor field (or the News function) defined at infinity. The situation is drastically different when where there is no known notion of `News' with similar good properties. In this paper both situations are considered jointly from a {\em tidal} point of view, that is, taking into account the strength (or energy) of the curvature tensors. The fundamental object used for that purposes in the {\em asymptotic (radiant) super-momentum}, a causal vector defined at infinity with remarkable properties. This leads to a novel characterization of gravitational radiation valid for the general case…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
