In a large class of models we show that the light scalar field responsible for the Sommerfeld enhancement in the annihilation of dark matter leads to observable direct detection rates, due to its mixing with the standard model Higgs. As a result the large annihilation cross-section of dark matter at present epoch, required to explain the observed cosmic ray anomalies, can be strongly constrained by direct searches. In particular Sommerfeld boost factors of order of a few hundred are already out of the CDMS-II upper bound at 90% confidence level for reasonable values of the model parameters. © 2010 Elsevier B.V.SCOPUS: ar.jinfo:eu-repo/semantics/publishe
This is the Accepted Manuscript version of an article accepted for publication in Journal of Cosmolo...
Coupling dark matter to light new particles is an attractive way to combine thermal production with ...
AbstractWe argue that WIMP dark matter can annihilate via long-lived “WIMPonium” bound states in rea...
AbstractIn a large class of models we show that the light scalar field responsible for the Sommerfel...
Boost factors of dark matter annihilation into antiprotons and electrons/positrons due to the clumpi...
We demonstrate that the Sommerfeld correction to cold dark matter (CDM) annihilations can be appreci...
We argue that WIMP dark matter can annihilate via long-lived "WIMPonium" bound states in reasonable ...
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matte...
International audienceIndirect searches with gamma rays set strong constraints on the properties of ...
The annihilation cross section of thermal relic dark matter determines both its relic density and in...
Coupling dark matter to light new particles is an attractive way to combine thermal production with ...
We study two models of scalar dark matter from "large" electroweak multiplets with isospin 5/2 (n=6 ...
20 pages, 12 figures; v2: Corrected branching ratio for ground state DM annihilations into leptons, ...
As searches for thermal and self-annihilating dark matter (DM) intensify, it becomes crucial to incl...
This is the Accepted Manuscript version of an article accepted for publication in Journal of Cosmolo...
Coupling dark matter to light new particles is an attractive way to combine thermal production with ...
AbstractWe argue that WIMP dark matter can annihilate via long-lived “WIMPonium” bound states in rea...
AbstractIn a large class of models we show that the light scalar field responsible for the Sommerfel...
Boost factors of dark matter annihilation into antiprotons and electrons/positrons due to the clumpi...
We demonstrate that the Sommerfeld correction to cold dark matter (CDM) annihilations can be appreci...
We argue that WIMP dark matter can annihilate via long-lived "WIMPonium" bound states in reasonable ...
The existence of a dark matter model with a rich dark sector could be the reason why WIMP dark matte...
International audienceIndirect searches with gamma rays set strong constraints on the properties of ...
The annihilation cross section of thermal relic dark matter determines both its relic density and in...
Coupling dark matter to light new particles is an attractive way to combine thermal production with ...
We study two models of scalar dark matter from "large" electroweak multiplets with isospin 5/2 (n=6 ...
20 pages, 12 figures; v2: Corrected branching ratio for ground state DM annihilations into leptons, ...
As searches for thermal and self-annihilating dark matter (DM) intensify, it becomes crucial to incl...
This is the Accepted Manuscript version of an article accepted for publication in Journal of Cosmolo...
Coupling dark matter to light new particles is an attractive way to combine thermal production with ...
AbstractWe argue that WIMP dark matter can annihilate via long-lived “WIMPonium” bound states in rea...