WarmAndFuzzy: the halo model beyond CDM
David J. E. Marsh

TL;DR
WarmAndFuzzy is a new computational tool that extends the halo model to include warm and fuzzy dark matter, enabling the analysis of their non-linear effects on the matter power spectrum, which was previously unexplored for fuzzy dark matter.
Contribution
This paper introduces the first halo model calculation for fuzzy dark matter and provides a publicly available code incorporating WDM and FDM into the standard halo model framework.
Findings
Differences between WDM, FDM, and CDM persist at low redshifts.
The code models ultralight axions and thermal WDM.
Cores in halo profiles are under development and expected to have minor effects.
Abstract
Cold dark matter (CDM) is a well established paradigm to describe cosmological structure formation, and works extraordinarily well on large, linear, scales. Progressing further in dark matter physics requires being able to understand structure formation in the non-linear regime, both for CDM and its alternatives. This short note describes a calculation, and accompanying code, WarmAndFuzzy, incorporating the popular models of warm and fuzzy dark matter (WDM and FDM) into the standard halo model to compute the non-linear matter power spectrum. The FDM halo model power spectrum has not been computed before. The FDM implementation models ultralight axions and other scalar fields with . The WDM implementation models thermal WDM with mass . The halo model shows that differences between WDM, FDM, and CDM survive at low redshifts in the…
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Code & Models
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Opportunistic and Delay-Tolerant Networks
