Exact Solution to Finite Temperature SFDM: Natural Cores without Feedback
Victor H. Robles, T. Matos

TL;DR
This paper presents an exact analytic solution for scalar field dark matter at finite temperature, naturally producing core-like density profiles in galaxies without requiring feedback mechanisms, aligning with observations of low surface brightness galaxies.
Contribution
It introduces a novel exact solution for finite temperature scalar field dark matter, demonstrating its ability to naturally form cores without feedback, unlike traditional models.
Findings
Scalar field dark matter can produce natural cores in galaxies.
The solution shows non-universal rotation curve profiles.
The model aligns with observed low surface brightness galaxy data.
Abstract
Recent high-quality observations of low surface brightness (LSB) galaxies have shown that their dark matter (DM) halos prefer flat central density profiles. On the other hand, the standard cold dark matter model simulations predict a more cuspy behavior. One mechanism to reconcile the simulations with the observed data is the feedback from star formation, this might be successful in isolated dwarf galaxies but its success in LSB galaxies remains unclear. Additionally, including too much feedback in the simulations is a double-edged sword, in order to obtain a cored DM distribution from an initially cuspy one, the feedback recipes usually require to remove a large quantity of baryons from the center of galaxies, however, some feedback recipes produce twice more satellite galaxies of a given luminosity and with much smaller mass to light ratios from those that are observed. Therefore, one…
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