skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Simulated Milky Way analogues: implications for dark matter direct searches

Journal Article · · Journal of Cosmology and Astroparticle Physics
; ; ;  [1]; ; ;  [2];  [3];  [4];  [5]
  1. GRAPPA, University of Amsterdam, Science Park 904, 1090 GL Amsterdam (Netherlands)
  2. Institute for Computational Cosmology, Durham University, South Road, Durham DH1 3LE (United Kingdom)
  3. Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF (United Kingdom)
  4. Department of Physics and Astronomy, University of Victoria, Victoria, BC, V8P 5C2 (Canada)
  5. Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden (Netherlands)

We study the implications of galaxy formation on dark matter direct detection using high resolution hydrodynamic simulations of Milky Way-like galaxies simulated within the EAGLE and APOSTLE projects. We identify Milky Way analogues that satisfy observational constraints on the Milky Way rotation curve and total stellar mass. We then extract the dark matter density and velocity distribution in the Solar neighbourhood for this set of Milky Way analogues, and use them to analyse the results of current direct detection experiments. For most Milky Way analogues, the event rates in direct detection experiments obtained from the best fit Maxwellian distribution (with peak speed of 223–289 km/s) are similar to those obtained directly from the simulations. As a consequence, the allowed regions and exclusion limits set by direct detection experiments in the dark matter mass and spin-independent cross section plane shift by a few GeV compared to the Standard Halo Model, at low dark matter masses. For each dark matter mass, the halo-to-halo variation of the local dark matter density results in an overall shift of the allowed regions and exclusion limits for the cross section. However, the compatibility of the possible hints for a dark matter signal from DAMA and CDMS-Si and null results from LUX and SuperCDMS is not improved.

OSTI ID:
22667570
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 05; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

Simulated Milky Way analogues: implications for dark matter indirect searches
Journal Article · Tue Dec 01 00:00:00 EST 2015 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22667570

The distribution of dark matter in the Milky Way's disk
Journal Article · Tue Apr 01 00:00:00 EDT 2014 · Astrophysical Journal · OSTI ID:22667570

Dark matter direct detection signals inferred from a cosmological N-body simulation with baryons
Journal Article · Mon Feb 01 00:00:00 EST 2010 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22667570