Alumnae and Alumni

Lluis Marti Magro
Project Researcher (from 2013/04/01 to 2016/04/30)
Current Affiliation
Institute for Cosmic Ray Research, The University of Tokyo
Assistant Professor


Last Update 2021/04/14

Since I joined the Super-Kamiokande (SK) collaboration in 2009, my main motivation has been the detection of core collapse supernova (ccSN) neutrinos. This includes those from all the past ccSNe, the diffuse supernova neutrino background (DSNB). Currently having the best world limit, some SK collaborators have been working on EGADS, a project to realise GADZOOKS!. By loading the SK water with gadolinium, we will be able to detect DSNB, our main motivation, and improve SN detection and other studies.

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