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Uncertainties in direct dark matter detection in light of Gaia's escape velocity measurements
Univ Michigan, Dept Phys, Leinweber Ctr Theoret Phys, Ann Arbor, MI 48109 USA..ORCID iD: 0000-0002-7399-1306
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA. Leinweber Center for Theoretical Physics, Department of Physics, University of Michigan, Ann Arbor, MI 48109, United States;Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, Stockholm, 10691, Sweden.
Univ North Florida, Dept Phys, Jacksonville, FL 32224 USA..
Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, AlbaNova, S-10691 Stockholm, Sweden..
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2019 (English)In: Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, E-ISSN 1475-7516, no 10, article id 034Article in journal (Refereed) Published
Abstract [en]

Direct detection experiments have set increasingly stringent limits on the cross section for spin-independent dark matter-nucleon interactions. In obtaining such limits, experiments primarily assume the standard halo model (SHM) as the distribution of dark matter in our Milky Way. Three astrophysical parameters are required to define the SHM: the local dark matter escape velocity, the local dark matter density and the circular velocity of the sun around the center of the galaxy. This paper studies the effect of the uncertainties in these three astrophysical parameters on the XENON1T exclusion limits using the publicly available DDCalc code. We compare limits obtained using the widely assumed escape velocity from the RAVE survey and the newly calculated escape velocity by Monari et al. using Gaia data. Our study finds that the astrophysical uncertainties are dominated by the uncertainty in the escape velocity (independent of the best fit value) at dark matter masses below 6 GeV and can lead to a variation of nearly 6 orders of magnitude in the exclusion limits at 4 GeV. Above a WIMP mass of 6GeV, the uncertainty becomes dominated by the local dark matter density, leading to uncertainties of factors of similar to 10 (3) at 6 (15) GeV WIMP mass in the exclusion limits. Additionally, this work finds that the updated best fit value for the escape velocity based on Gaia data leads to only very minor changes to the effects of the astrophysical uncertainties on the XENON1T exclusion limits.

Place, publisher, year, edition, pages
IOP PUBLISHING LTD , 2019. no 10, article id 034
Keywords [en]
dark matter detectors, dark matter experiments, dark matter simulations, dark matter theory
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-266429DOI: 10.1088/1475-7516/2019/10/034ISI: 000503491500002Scopus ID: 2-s2.0-85076043825OAI: oai:DiVA.org:kth-266429DiVA, id: diva2:1386409
Note

QC 20200117

Available from: 2020-01-17 Created: 2020-01-17 Last updated: 2020-01-17Bibliographically approved

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Freese, Katherine

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