Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies between collisionless cold DM and galactic structure observations. However, $gamma$-ray searches and the CMB strongly constrain such scenarios. To ease the tension, we consider asymmetric DM. We show that, contrary to the common lore, detectable annihilations occur even for large asymmetries, and derive bounds from the CMB, $gamma$-ray, neutrino and antiproton searches. We then identify the viable space for self-interacting DM. Direct detection does not exclude this scenario, but provides a way to test it
Dark matter (DM) with sizeable self-interactions mediated by a light species offers a compelling exp...
Abstract. Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymme-try, similar to ...
I will discuss some phenomenological consequences of extensions of the Standard Model containing a m...
Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies ...
The putative discrepancies between observations of the small scale galactic structure and the predic...
Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one obs...
We explore the phenomenology of having a second epoch of dark matter annihilation into dark radiatio...
In the simplest models of asymmetric dark matter (ADM) annihilation signals are not expected, since ...
Assuming the existence of a primordial asymmetry in the dark sector, a scenario usually dubbed Asymm...
Assuming the existence of a primordial asymmetry in the dark sector, a scenario usually dubbed Asymm...
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large sel...
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large sel...
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large sel...
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 I...
© 2011 Dr. Thomas David JacquesIt is now well established that some form of Dark Matter (DM) makes a...
Dark matter (DM) with sizeable self-interactions mediated by a light species offers a compelling exp...
Abstract. Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymme-try, similar to ...
I will discuss some phenomenological consequences of extensions of the Standard Model containing a m...
Dark matter (DM) coupled to light mediators has been invoked to resolve the putative discrepancies ...
The putative discrepancies between observations of the small scale galactic structure and the predic...
Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one obs...
We explore the phenomenology of having a second epoch of dark matter annihilation into dark radiatio...
In the simplest models of asymmetric dark matter (ADM) annihilation signals are not expected, since ...
Assuming the existence of a primordial asymmetry in the dark sector, a scenario usually dubbed Asymm...
Assuming the existence of a primordial asymmetry in the dark sector, a scenario usually dubbed Asymm...
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large sel...
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large sel...
Dark matter particles interacting via the exchange of very light spin-0 mediators can have large sel...
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 I...
© 2011 Dr. Thomas David JacquesIt is now well established that some form of Dark Matter (DM) makes a...
Dark matter (DM) with sizeable self-interactions mediated by a light species offers a compelling exp...
Abstract. Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymme-try, similar to ...
I will discuss some phenomenological consequences of extensions of the Standard Model containing a m...