Modeling charged particles around dual jets from coalescing binary black holes

Details Modeling charged particles around dual jets from coalescing binary black holes Modeling charged particles around dual jets from coalescing binary black holes

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.j8002k&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #J8.002

Astronomy and Astrophysics

Astrophysics

Scientific paper

Electromagnetic emission produced during the in-spiral and merger of supermassive black holes could provide, together with gravitational waves, the smoking gun to identify these astrophysical events. To gain further insight on the mechanisms responsible for the electromagnetic emission, we present results from simulations of pressure-less charged matter in the vicinity of merging black holes immersed in a magnetic field. In particular, we discuss the effect that the dual jets from coalescing binary black holes have on the dynamics of the charged particles.

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