A simple ghost free and caustic free mimetic scalar field dark matter model
Emmanuel Kanambaye

TL;DR
This paper introduces a simple scalar field dark matter model that is free from ghost and caustic instabilities, potentially outperforming the standard $ ext{Lambda}$CDM model.
Contribution
It presents a novel, minimal extension of mimetic dark matter that eliminates key instabilities, enhancing its viability as an alternative to $ ext{Lambda}$CDM.
Findings
Model is ghost free and caustic free
Potential to challenge or surpass $ ext{Lambda}$CDM
Provides a stable scalar field dark matter candidate
Abstract
Chamseddine and Mukhanov have promoted the concept of mimetic dark matter as alternative dark matter candidate coming from gravitation. Unfortunately although being very interesting, their proposition turned out to have weakness among which ghost and caustic instabilities. In this paper I propose among the simplest ghost free and caustic free scalar field dark matter extension of their model; a proposition capable of challenging CDM model or even capable of doing better.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
