The Cosmological Trajectories Method: Modelling cosmic structure formation in the non-linear regime (2021)
Attributed to:
The Detectability of Self-Interacting Dark Matter in Cosmological Structure: The View from Numerical Simulations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2102.01698
Publication URI: http://dx.doi.org/10.48550/arxiv.2102.01698
Type: Journal Article/Review
Parent Publication: arXiv e-prints