UNDERSTANDING THE ‘FEEBLE GIANT’ CRATER II WITH TIDALLY STRETCHED WAVE DARK MATTER
| dc.contributor.author | Pozo, Alvaro | |
| dc.contributor.author | Broadhurst, Tom | |
| dc.contributor.author | Emami, Razieh | |
| dc.contributor.author | Smoot, George | |
| dc.date.accessioned | 2023-03-29T08:04:09Z | |
| dc.date.available | 2023-03-29T08:04:09Z | |
| dc.date.issued | 2022 | |
| dc.description.abstract | The unusually large ‘dwarf’ galaxy Crater II, with its small velocity dispersion, ≃3 km s−1, defies expectations that low-mass galaxies should be small and dense. We combine the latest stellar and velocity dispersion profiles finding Crater II has a prominent dark core of radius ≃0.71+0.09−0.08 kpc, surrounded by a low density halo, with a transition visible between the core and the halo. We show that this profile matches the distinctive core-halo profile predicted by ‘Wave Dark Matter’ as a Bose-Einstein condensate, ψDM, where the ground state soliton core is surrounded by a tenuous halo of interfering waves, with a marked density transition predicted between the core and halo. Similar core-halo structure is seen in most dwarf spheroidal galaxies (dSphs), but with smaller cores, ≃0.25 kpc and higher velocity dispersions, ≃9 km s−1, and we argue here that Crater II may have been a typical dSph that has lost most of its halo mass to tidal stripping, so its velocity dispersion is lower by a factor of 3 and the soliton is wider by a factor of 3, following the inverse scaling required by the Uncertainty Principle. This tidal solution for Crater II in the context of ψDM is supported by its small pericenter of ≃20 kpc established by Gaia, implying significant tidal stripping of Crater II by the Milky Way is expected. | en_US |
| dc.identifier.citation | Pozo, A., Broadhurst, T., Emami, R., & Smoot, G. F. (2022). Understanding the ‘feeble giant’ Crater II with tidally stretched wave dark matter. Monthly Notices of the Royal Astronomical Society, 515(2), 2624–2632. https://doi.org/10.1093/mnras/stac1862 | en_US |
| dc.identifier.uri | http://nur.nu.edu.kz/handle/123456789/7000 | |
| dc.language.iso | en | en_US |
| dc.publisher | Monthly Notices of the Royal Astronomical Society | en_US |
| dc.rights | Attribution-NonCommercial-ShareAlike 3.0 United States | * |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/3.0/us/ | * |
| dc.subject | Type of access: Open Access | en_US |
| dc.subject | Dark Matter | en_US |
| dc.subject | Galaxy: kinematics and dynamics | en_US |
| dc.title | UNDERSTANDING THE ‘FEEBLE GIANT’ CRATER II WITH TIDALLY STRETCHED WAVE DARK MATTER | en_US |
| dc.type | Article | en_US |
| workflow.import.source | science |