This analysis connects lensing observables to projected accumulation geometry in dynamically disturbed clusters, suggesting a broader interpretive framework.
Key Points
The paper aims to clarify how weak-field lensing in the HγC framework can be understood in terms of projected accumulation geometry rather than local baryonic distribution.
Extended the HγC framework to include weak-field lensing observables.
Established the relationship between geometric descriptors and gravitational responses.
Analyzed cases such as the Bullet Cluster to illustrate the framework's implications.
Weak-field lensing signals reveal information about projected accumulation profiles.
Profile dependence affects perceived gravitational response in accumulation sectors.
Spatial offsets between baryonic mass and lensing geometry can occur, especially in cluster mergers.