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Foreword
Authors:Ana Inés Gómez de Castro
Affiliation:(1) Via Fratelli Manfredi 55, Reggio Emilia, 42100, Italy
Abstract:Protons of energy 109 GeV and 104 GeV accelerating by the magnetic field of very strongly magnetized neutron stars and of extreme Kerr-Newmann black holes (respectively) may undergo instantaneous decay.
Keywords:gravitation  thermodynamics  Unruh effect  cosmic rays  neutron stars  black holes  magnetars
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