A Finite Relaxation Timescale for Mass–Gas Offsets in Dissociative Galaxy Cluster Mergers
Abstract
This paper presents an empirical analysis of mass–gas offsets in dissociative galaxy cluster mergers using a uniform system-level separation observable and interval-sampled merger ages. The results are consistent with a finite relaxation timescale of order 10^8 years. This work is intended as an observational and phenomenological complement to Viscoelastic General Relativity (VGR) v2 and does not depend on accepting the underlying theoretical framework.
Fields of Study & Subjects
Galaxies: Formation
Evolution
Phenomena
Cosmology and Gravitation Theories
Astrophysical Phenomena and Observations
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 9 February 2026
- Language
- EN
- Document type
- Preprint