Speaker
Debajit Bose
(IIT Kharagpur, India)
Description
Particulate dark matter captured by a population of neutron stars distributed around the galactic center while annihilating through long-lived mediators can give rise to an observable neutrino flux. We examine the prospect of an idealised gigaton detector like IceCube/KM3NeT in probing such scenarios. Within this framework, we report an improved reach in spin-dependent and spin-independent dark matter nucleon cross-section below the current limits for dark matter masses in the TeV-PeV range.
| In-person participation | Yes |
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Primary author
Debajit Bose
(IIT Kharagpur, India)
Co-authors
Tarak Nath Maity
(Centre for High Energy Physics, Indian Institute of Science, Bangalore 560012, India)
Tirtha Sankar Ray
(Department of Physics, Indian Institute of Technology Kharagpur)
