TL;DR
This paper explores the potential of using gravitational magnetosonic waves (GMSW) in highly magnetized plasma as a novel method for detecting gravitational waves emitted by neutron stars, linking observed pulsar impulses to GMSW phenomena.
Contribution
It introduces GMSW as a new detection mechanism for gravitational waves and suggests that pulsar impulses may be evidence of GMSW activity.
Findings
GMSW can serve as an effective gravitational wave detector.
Giant impulses in pulsar NP 0532 may be caused by GMSW.
The study supports the link between pulsar impulses and gravitational wave activity.
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.
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