Speaker
Dr
Massimo Mannarelli
(INFN)
Description
Strange stars are exotic stellar objects, almost entirely consisting of deconfined quark matter. We analyze the possible emission of electromagnetic signals and of gravitational wave echoes from strange stars. In both cases we expect that the typical frequency of the emitted signals are on the order of tens of kHz.
Primary author
Dr
Massimo Mannarelli
(INFN)
