K40 Background Simulations for the Seawiet OM

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Effects of simulation parameters

distribution of hits on OM surface remains the same

70mm PC, Nemo water

70mm PC, Antares water

75mm PC, Nemo water

75mm PC, Antares water

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Effects of simulation parameters distribution of hits on OM surface remains the same 70mm PC, Nemo water 70mm PC, Antares water 75mm PC, Nemo water 75mm PC, Antares water

Summary and Outlook most correlated coincidences • originate from within 5 m from the OM, therefore absorption length has little effect • are distributed to two or more PMTs • occur in PMTs next to each other calibration opportunities from K40 coincidences: • s.p.e. response • time calibration (under investigation)

Page 1 and 2: K40 Background Simulations for the
Page 3 and 4: Simulation Using a Geant4 based MC-
Page 5 and 6: Optimisation to get realistic total
Page 7 and 8: Simulation parameters Simulation ha
Page 9: Results: Correlated rates we distin
Page 13: Time difference preview

K40 Background Simulations for the Seawiet OM

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