SFDM: A new formation mechanism of tidal debris
Victor H. Robles, L.A. Martinez-Medina, T. Matos

TL;DR
This paper proposes a novel formation mechanism for tidal debris, such as shells and rings, driven by the wave-like properties of ultra-light scalar field dark matter, independent of merger events.
Contribution
It introduces the SFDM model's ability to naturally produce tidal features through halo density ripples, offering an alternative to merger-based explanations.
Findings
Tidal structures can form due to scalar field dark matter wave interference.
Stable multistate halos exhibit ripples that lead to tidal features.
The model explains observed tidal debris without requiring recent mergers.
Abstract
Recent observations of tidal debris around galaxies have revealed that the structural properties of the spheroidal components of tidally disturbed galaxies are similar to those found in non-interacting early-type galaxies(ETGs), likely due to minor merging events that do not strongly affect the bulge region or to major mergers that happened a long time ago. We show that independently of merger events, tidal features like shells or rings can also arise if the the dark matter is an ultra light scalar field of mass ~10eV/c. In the scalar field dark matter (SFDM) model the small mass precludes halo formation below ~10 M reducing the number of small galaxies today, it produces shallow density profiles due to the uncertainty principle in contrast to the steep profiles found in the standard cold dark matter (CDM) paradigm, in addition to the usual soliton solution…
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Taxonomy
TopicsTropical and Extratropical Cyclones Research · Underwater Acoustics Research
