Multifield ultralight dark matter

نویسندگان

چکیده

Ultralight dark matter (ULDM) is usually taken to be a single scalar field. Here we explore the possibility that ULDM consists of $N$ light fields with only gravitational interactions. This configuration more consistent underlying particle physics motivations for these scenarios than ultralight halos have characteristic granular structure increases stellar velocity dispersion and can used as observational constraints on models. In multifield simulations, find inside halo amplitude total density fluctuations decreases $1/\sqrt{N}$ do not become significantly correlated over cosmological timescales. Smoother heat orbits less efficiently, reducing relative field case thus weakening mass. Analytically, show equal-mass mass $m$ contribution scales $1/(N m^3)$. Lighter most efficiently if smallest $m_L$ below other masses $1/(N^2 m_L^3)$.

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ژورنال

عنوان ژورنال: Physical review

سال: 2023

ISSN: ['0556-2813', '1538-4497', '1089-490X']

DOI: https://doi.org/10.1103/physrevd.107.083014