Д. Костюнин Progress of radio detection of ultra-high energy cosmic rays and neutrinos.
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Wednesday 05 September 2018, 11:00 - 13:00
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Ultra-high energy cosmic-rays and neutrinos produce secondary particle cascades in atmosphere and other natural media (water, ice, etc) and thus can be detected by large-scale ground or in-ice/underwater setups. Since the fluxes of these cosmic messengers are falling steeply with the energy, it is necessary to have full duty-cycle detector with full-sky coverage and effective areas and volumes of thousands of square kilometers and gigatons, respectively. Relatively new technique exploiting MHz radio antennas installed on/under the ground allows one to achieve such large areas and volumes. In this talk I will give an introduction to the radio technique and present an overview of the latest achievements of modern radio instruments focused on this topic.

Location DLNP conference hall
Дубна
Московская область
Россия