Palestrante: Cecília Chirenti (UFABC)
Título: When neutron stars shake: theory and observations
Resumo: Neutron stars hold many puzzles about their composition and phenomenology. Some observations may be explained as signals resulting from oscillations of the neutron star, caused by a starquake or another catastrophic event. The theoretical study of these oscillations can help us learn more about neutron stars in different guises, including pulsars, magnetars, short gamma ray bursts and fast radio bursts.
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