Conformal Einstein equation and symplectic flux with a positive cosmological constant

Fuente: arXiv
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Main Authors: Hoque, Sk Jahanur, Krtouš, Pavel, Peón-Nieto, Carlos
Format: Preprint
Published: 2025
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author Hoque, Sk Jahanur
Krtouš, Pavel
Peón-Nieto, Carlos
author_facet Hoque, Sk Jahanur
Krtouš, Pavel
Peón-Nieto, Carlos
contents We analyze the conformal Einstein equation with a positive cosmological constant to extract fall-off conditions of the gravitational fields. The fall-off conditions are consistent with a finite, non-trivial presymplectic current on the future boundary of de Sitter. Hence our result allows a non-zero gravitational flux across the boundary of the de Sitter. We present an explicit gauge-free computation to show that the Gibbons-Hawking boundary term, counterterm in the action, and fall-off condition of gravitational field in conformal Einstein equation are crucial to reproduce the finite symplectic flux.
format Preprint
id arxiv_https___arxiv_org_abs_2504_20845
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Conformal Einstein equation and symplectic flux with a positive cosmological constant
Hoque, Sk Jahanur
Krtouš, Pavel
Peón-Nieto, Carlos
General Relativity and Quantum Cosmology
High Energy Physics - Theory
We analyze the conformal Einstein equation with a positive cosmological constant to extract fall-off conditions of the gravitational fields. The fall-off conditions are consistent with a finite, non-trivial presymplectic current on the future boundary of de Sitter. Hence our result allows a non-zero gravitational flux across the boundary of the de Sitter. We present an explicit gauge-free computation to show that the Gibbons-Hawking boundary term, counterterm in the action, and fall-off condition of gravitational field in conformal Einstein equation are crucial to reproduce the finite symplectic flux.
title Conformal Einstein equation and symplectic flux with a positive cosmological constant
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2504.20845