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M. Eichler ∗a, A. Arcones bc, A. Kelic c, O. Korobkin d, K. Langanke bc, G. Martinez-Pinedo bc, I. V. Panov ea, T. Rauscher f a, S. Rosswog d, C. Winteler g, N. T. Zinner h, and F.-K. Thielemann a aDepartment of Physics, University of Basel, Switzerland bInstitut für Kernphysik, Technische Universität Darmstad t, Germany cGSI Helmholtzzentrum für Schwerionenforschung GmbH, Darm stadt, Germany dThe Oskar Klein Centre, Department of Astronomy, Stockholm University, Sweden eSSC RF ITEP of NRC "Kurchatov Institute", Moscow, Russia f Centre for Astrophysics Research, University of Hertfords hire, UK gInstitut Energie am Bau, Fachhochschule Nordwestschweiz, Muttenz, Switzerland hDepartment of Physics and Astronomy, Aarhus University, De nmark E-mail: marius.eichler@unibas.ch

The influence of fission on neutron star merger r-process and the position of the third r-process peak