Diversity of Fuzzy Dark Matter Solitons

Fuente: arXiv
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Autores principales: Tan, Chen, Delliou, M. Le, Wang, Ke
Formato: Preprint
Publicado: 2024
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author Tan, Chen
Delliou, M. Le
Wang, Ke
author_facet Tan, Chen
Delliou, M. Le
Wang, Ke
contents According to the Schrödinger-Poisson equations, fuzzy dark matter (FDM) can form a stable equilibrium configuration, the so-called FDM soliton. In principle, given the FDM particle mass, the profile of the FDM soliton is fixed. In practice, however, there is a great diversity of structures in the Universe. Possible causes of such diversity can lie in such sources as the gravitoelectric field due to a central supermassive black hole, the gravitomagnetic field due to the system angular momentum, an extra denser and compact FDM soliton and an ellipsoidal baryon background. We find that the effects of the gravitomagnetic field due to the soliton's self-angular momentum are very weak while those of the other sources are considerable.
format Preprint
id arxiv_https___arxiv_org_abs_2411_16114
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Diversity of Fuzzy Dark Matter Solitons
Tan, Chen
Delliou, M. Le
Wang, Ke
High Energy Physics - Phenomenology
Astrophysics of Galaxies
According to the Schrödinger-Poisson equations, fuzzy dark matter (FDM) can form a stable equilibrium configuration, the so-called FDM soliton. In principle, given the FDM particle mass, the profile of the FDM soliton is fixed. In practice, however, there is a great diversity of structures in the Universe. Possible causes of such diversity can lie in such sources as the gravitoelectric field due to a central supermassive black hole, the gravitomagnetic field due to the system angular momentum, an extra denser and compact FDM soliton and an ellipsoidal baryon background. We find that the effects of the gravitomagnetic field due to the soliton's self-angular momentum are very weak while those of the other sources are considerable.
title Diversity of Fuzzy Dark Matter Solitons
topic High Energy Physics - Phenomenology
Astrophysics of Galaxies
url https://arxiv.org/abs/2411.16114