Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-41501
Schneider, A; Krauss, L; Moore, B (2010). Impact of dark matter microhalos on signatures for direct and indirect detection. Physical Review D, 82(6):063525.
PDF (Accepted manuscript, Version 2)
View at publisher
PDF (Accepted manuscript, Version 1)
Detecting dark matter as it streams through detectors on Earth relies on knowledge of its phase space density on a scale comparable to the size of our Solar System. Numerical simulations predict that our galactic halo contains an enormous hierarchy of substructures, streams and caustics, the remnants of the merging hierarchy that began with tiny Earth-mass microhalos. If these bound or coherent structures persist until the present time, they could dramatically alter signatures for the detection of weakly interacting elementary particle dark matter. Using numerical simulations that follow the coarse grained tidal disruption within the Galactic potential and fine grained heating from stellar encounters, we find that microhalos, streams, and caustics have a negligible likelihood of impacting direct detection signatures implying that dark matter constraints derived using simple smooth halo models are relatively robust. We also find that many dense central cusps survive, yielding a small enhancement in the signal for indirect detection experiments.
44 downloads since deposited on 01 Mar 2011
15 downloads since 12 months
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Dewey Decimal Classification:||530 Physics|
|Deposited On:||01 Mar 2011 09:16|
|Last Modified:||21 Jun 2014 04:35|
|Publisher:||American Physical Society|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page