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This paper investigates the magnetic fields of coalescing neutron star binaries and their role as progenitors of short gamma-ray bursts. Using population synthesis methods, the authors model the distribution of neutron star magnetic fields and find that a log-normal distribution aligns well with the observed luminosity function of gamma-ray bursts. The study emphasizes the importance of magnetic fields in shaping gravitational wave signals and the potential electromagnetic phenomena preceding coalescence.

Author

riki paisal

Language

EN