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Probing Micro-quasars with TeV Neutrinos

Amir Levinson·Eli Waxman
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Abstract

The jets associated with Galactic micro-quasars are believed to be ejected by accreting stellar mass black-holes or neutron stars. We show that if the energy content of the jets in the transient sources is dominated by electron-proton plasma, then a several hour outburst of 1--100 TeV neutrinos produced by photo- meson interactions should precede the radio flares associated with major ejection events. Several neutrinos may be detected during a single outburst by a 1km^2 detector, thereby providing a powerful probe of micro-quasars jet physics.

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Amir Levinson, Eli Waxman. 2001-08-19. Probing Micro-quasars with TeV Neutrinos. https://doi.org/10.1103/physrevlett.87.171101

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