Theoretical resonant Auger decay spectra of ammonia with core-hole excited state dynamics simulation were investigated and some specific features of the experiment except for a vibrational structure were reproduced. A power spectral analysis with short-time maximum entropy method has been applied, and an obtained vibrational spacing assigned to NH stretching mode was 340 meV, which was consistent with the experiment of 390 ± 10 meV. Proton dynamics of ammonia on the first core-excited state was discussed. 1. Introduction Auger decay [1, 2] is one of the de-excitation processes in atoms and molecules after core-excitation. The processes are classified based on the excitation energy as "normal" or "resonant" Auger decay for autoionization of a state created through ionization of an inner-shell electron and through resonant excitation of an inner-shell electron to an unoccupied valence orbital. Depending on the potential energy surface of the excited state the molecule may undergo dynamics during the core-hole lifetime, which depends on the specific element and is in the range of femtoseconds for the second-row atoms. Even if the core-excited state is dissociative, the Auger decay transition in most cases takes place before a bond scission. For some special cases, however, the repulsive character of the potential energy surface in the core-excited state can induce bond scissions within the core-hole lifetime; this is usually referred to as ultra-fast dissociation. Ultra-fast dissociation upon resonant core-excitation into dissociative states has indeed been observed by several researchers through effects on the subsequent Auger decay [3-8] and X-ray emission [9-11]. The ammonia molecule is the simplest molecule including an N atom and has been studied for a long time experimentally and theoretically. It is also interested from a viewpoint of periodicity because HF, H 2 O, NH 3 , and CH 4 are isoelectronic with neon. Recent developments of soft X-ray