WIMPonium and boost factors for indirect dark matter detection

March-Russell, John and West, Stephen M.

(2009)

March-Russell, John and West, Stephen M. (2009) WIMPonium and boost factors for indirect dark matter detection. Physics Letters B, 676 (4-5).

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Abstract

We argue that WIMP dark matter can annihilate via long-lived "WIMPonium" bound states in reasonable particle physics models of dark matter (DM). WIMPonium bound states call occur at or near threshold leading to substantial enhancements in the DM annihilation rate, closely related to the Sommerfeld effect. Large "boost factor" amplifications in the annihilation rate call thus occur without large density enhancements. possibly preferring colder less dense objects such as dwarf galaxies as locations for indirect DM searches. The radiative capture to and transitions among the WIMPonium states generically lead to a rich energy spectrum of annihilation products, With many distinct lines possible in the case of 2-body decays to gamma gamma or gamma Z final states. The existence of multiple radiative capture modes further enhances the total annihilation rate, and the detection of the lines would give direct over-determined information on the nature and self-interactions of the DM particles. (C) 2009 Elsevier B.V. All rights reserved.

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This is a Approved version
This version's date is: 8/6/2009
This item is not peer reviewed

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https://repository.royalholloway.ac.uk/items/f4903e00-36f5-cea1-b2cc-8fdb1ec4f795/6/

Item TypeJournal Article
TitleWIMPonium and boost factors for indirect dark matter detection
AuthorsMarch-Russell, John
West, Stephen M.
Uncontrolled KeywordsDark matter, Indirect detection, Bound-state, RAY POSITRON FRACTION, GAMMA-RAYS, NEUTRALINO ANNIHILATION, PHOTINO ANNIHILATION, 2 PHOTONS, ELECTRONS
DepartmentsFaculty of Science\Physics
Research Groups and Centres\Physics\Low Temperature Physics

Identifiers

doihttp://dx.doi.org/10.1016/j.physletb.2009.04.010

Deposited by Research Information System (atira) on 20-Mar-2014 in Royal Holloway Research Online.Last modified on 20-Mar-2014


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