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Gravitational Radiation Coupled to a real massive scalar Field
Abstract
We study the asymptotic behavior of small-data global solutions to the Einstein--Klein--Gordon system with a positive-mass real scalar field in wave gauge. We show that the linearized trace component of the metric perturbation admits a t̂−1≃ t−1 optimal decreasing rate. Moreover, a quantitative one-point observability estimate is established: the initial Klein-Gordon energy is controlled by this leading order coefficient.
Related
- Reconsidering the Vacuum Energy of a Massive Scalar Field in a Spherical Cavity
- Interior gravitational perturbations to naked singularities of a scalar field
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- Exact scalarization thresholds and onset laws for a nonminimally coupled scalar field on the Ellis wormhole
- Hilbert Expansion of the coupled radiation-Euler in the equilibrium regime
BibTeX
@misc{ma2026gravitational,
title = {{Gravitational Radiation Coupled to a real massive scalar Field}},
author = {Yue Ma and Xianghao Wu and Weidong Zhang},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.33928},
eprint = {2610.33928},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.33928},
}
RIS
TY - UNPB
TI - Gravitational Radiation Coupled to a real massive scalar Field
AU - Yue Ma
AU - Xianghao Wu
AU - Weidong Zhang
PY - 2026
DA - 2026/10/24
PB - arXiv
DO - 10.48550/arxiv.2610.33928
UR - https://arxiv.org/abs/2610.33928
AB - We study the asymptotic behavior of small-data global solutions to the Einstein--Klein--Gordon system with a positive-mass real scalar field in wave gauge. We show that the linearized trace component of the metric perturbation admits a t̂^−1≃ t^−1 optimal decreasing rate. Moreover, a quantitative one-point observability estimate is established: the initial Klein-Gordon energy is controlled by this leading order coefficient.
ER -