Report/Contribution to a conference proceedings/Contribution to a book

PUBDB-2018-01758

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Terrestrial WIMP/Axion astronomy

O'Hare, C. A. J. (Corresponding author)

2018
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-945931-17-2

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2017-02/ohare_ciaran

Report No.: DESY-PROC-2017-02

Abstract: Predicting signals in direct dark matter (DM) detection experiments requires an understanding of the astrophysical structure of the local halo. Any uncertainty in this understanding will feed directly into all experimental results. However our terrestrial experiments are in a position to study this same astrophysical dependence, and in fact represent our only probe of the local halo on sub-milliparsec scales. This is best achieved in the case of WIMP dark matter if directionally sensitive experiments are feasible, but requires novel parameterizations of the velocity distribution to make model independent claims. For axions the prospects are much greater, haloscopes would be able to make better measurements of the local DM distribution than astrometric probes.

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Contributing Institute(s):

1. Bibliothek und Dokumentation (L)

Research Program(s):

1. 899 - ohne Topic (POF3-899) (POF3-899)

Experiment(s):

1. No specific instrument

Appears in the scientific report 2018

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Book/Proceedings/Report Maroudas, M. (Editor)
13th "Patras" Workshop on Axions, WIMPs and WISPs, PATRAS 2017
201813th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2017, ThessalonikiThessaloniki, Greece, 15 May 2017 - 19 May 20172017-05-152017-05-19 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC (2018) [10.3204/DESY-PROC-2017-02]2018     Files BibTeX | EndNote: XML, Text | RIS

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