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When two Neutron Stars collide a multi-band electromagnetic emission, knownas Kilonova (KN), follows being powered by the radioactive decay of ejectaproducts. In this contribution we discuss how the equation of state of densematter, impacts the mass and velocity in the KN ejecta and thus its lightcurve. Using this information encoded in the stellar mass-radius relationship,we ellaborate on how the future experimental observations in photon channels,in addition to complementary multimessenger probes, could provide a new andmore detailed insight into the equation of state of nuclear matter.

Neutron Stars Mass-Radius relationship and Electromagnetic follow-up of Kilonovae