Electromagnetic luminosity function of superconducting cosmic string loops

Physics

Scientific paper

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Scientific paper

The luminosity function (LF) of electromagnetically radiating closed loops of superconducting cosmic strings (SCS) is calculated in a cosmological context. The LF has a peak as a function of luminosity and a cutoff at the low-luminosity end, and increases with increasing redshift. Some questions concerning a hypothetical model of quasars in which SCS loops act as the ``central engines'' are discussed.

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