Gravimagnetic shock waves and gravitational-wave experiments

TL;DR

This paper proposes a new perspective on gravitational-wave detection by linking pulsar giant pulses to gravimagnetic shock waves, suggesting a novel astrophysical source for gravitational waves.

Contribution

It introduces the idea that pulsar giant pulses may be caused by gravimagnetic shock waves, offering a new approach to gravitational-wave experiments.

Findings

GMSW can be excited in neutron star magnetospheres by gravitational radiation.

Giant pulses in pulsar NP 0532 may be linked to GMSW.

New outlook on gravitational-wave detection methods.

Abstract

Causes of the unsatisfactory condition of the gravitational-wave experiments are discussed and a new outlook at the detection of gravitational waves of astrophysical origin is proposed. It is shown that there are strong grounds for identifying the so-called giant pulses in the pulsar NP 0532 radiation with gravimagnetic shock waves (GMSW) excited in the neutron star magnetosphere by sporadic gravitational radiation of this pulsar.