Abstract
From the point of view of Dark Matter searches, antideuteron are an interesting species of cosmic rays. In the past eighteen years much progress has been done in the understanding of these cosmic rays but this did not translate into experimental efforts to actually detect these particles. In this work, starting from a specific case of dark matter candidate with relatively generic features, we study some sources of theoretical uncertainties and show that the margin of improvement beyond the limits already set by cosmic-ray antiproton are quite narrow and anyway unachievable for the next generation of experiments.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
