Asymptotics with a positive cosmological constant: I. Basic framework
Abhay Ashtekar, Beatrice Bonga, Aruna Kesavan

TL;DR
This paper reviews the well-established asymptotic structure of gravitational fields when the cosmological constant is zero and highlights the challenges and lack of useful frameworks when extending these concepts to a positive cosmological constant, emphasizing the need for new approaches.
Contribution
It demonstrates that the standard asymptotic framework for gravitational fields does not extend straightforwardly to the case of a positive cosmological constant, identifying key conceptual gaps.
Findings
Standard framework fails for positive cosmological constant
Lack of positive energy theorems in this context
No invariant gravitational wave notion for Λ > 0
Abstract
The asymptotic structure of the gravitational field of isolated systems has been analyzed in great detail in the case when the cosmological constant is zero. The resulting framework lies at the foundation of research in diverse areas in gravitational science. Examples include: i) positive energy theorems in geometric analysis; ii) the coordinate invariant characterization of gravitational waves in full, non-linear general relativity; iii) computations of the energy-momentum emission in gravitational collapse and binary mergers in numerical relativity and relativistic astrophysics; and iv) constructions of asymptotic Hilbert spaces to calculate -matrices and analyze the issue of information loss in the quantum evaporation of black holes. However, by now observations have established that is positive in our universe. In this paper we show that, unfortunately, the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
