Authors: Yu.G. Ignatyev
Date: 17 Jan 2011
Abstract: The effect of an excitation of a gravitational wave (GW) on shock waves in a highly magnetized plasma, GMSW, is studied as an effective means for the detection of GW radiated by neutron stars. It is shown that there is every reason to identify the giant impulses of the pulsar NP 0532 with GMSW.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis