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Title: Galactoseismology and the local density of dark matter

Journal Article · · Monthly Notices of the Royal Astronomical Society
 [1];  [2];  [3]
  1. Univ. of Florida, Gainesville, FL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
  2. Queen's Univ., Kingston, ON (Canada)
  3. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)

Here, we model vertical breathing mode perturbations in the Milky Way's stellar disc and study their effects on estimates of the local dark matter density, surface density, and vertical force. Evidence for these perturbations, which involve compression and expansion of the Galactic disc perpendicular to its midplane, come from the SEGUE, RAVE, and LAMOST surveys. We show that their existence may lead to systematic errors of $$10\%$$ or greater in the vertical force $$K_z(z)$$ at $$|z|=1.1\,{\rm kpc}$$. These errors translate to $$\gtrsim 25\%$$ errors in estimates of the local dark matter density. Using different mono-abundant subpopulations as tracers offers a way out: if the inferences from all tracers in the Gaia era agree, then the dark matter determination will be robust. Disagreement in the inferences from different tracers will signal the breakdown of the unperturbed model and perhaps provide the means for determining the nature of the perturbation.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1331120
Report Number(s):
FERMILAB-PUB-16-315-A-AE-PPD-T; arXiv:1608.03338; 1480936
Journal Information:
Monthly Notices of the Royal Astronomical Society, Vol. 464, Issue 4; ISSN 0035-8711
Publisher:
Royal Astronomical SocietyCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 32 works
Citation information provided by
Web of Science

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Cited By (13)

The vertical force in the solar neighbourhood using red clump stars in TGAS and RAVE: Constraints on the local dark matter density journal July 2018
Measuring the local matter density using Gaia DR2 journal February 2019
Using Gaia DR2 to constrain local dark matter density and thin dark disk journal April 2019
On the estimation of the local dark matter density using the rotation curve of the Milky Way journal October 2019
The dynamical matter density in the solar neighbourhood inferred from Gaia DR1 journal September 2018
3D Asymmetrical motions of the Galactic outer disc with LAMOST K giant stars journal March 2018
The localdark matter density from SDSS-SEGUE G-dwarfs journal April 2018
Milky Way Tomography with K and M Dwarf Stars: The Vertical Structure of the Galactic Disk journal July 2017
Milky Way Tomography with K and M Dwarf Stars: the Vertical Structure of the Galactic Disk text January 2017
The dynamical matter density in the solar neighbourhood inferred from Gaia DR1 text January 2017
The vertical force in the Solar Neighbourhood using red clump stars in TGASxRAVE - Constraints on the local dark matter density text January 2018
Using Gaia DR2 to Constrain Local Dark Matter Density and Thin Dark Disk text January 2018
On the estimation of the Local Dark Matter Density using the rotation curve of the Milky Way text January 2019

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