Abstract
Following the recent observations of gravitational waves by the LIGO-Virgo science team [Phys. Rev. Lett. 116, 061102 (2016)] resulting from the collision of two black holes in the framework of general relativity theory whose practical studies have listed different types of energy due to the propagation of these massive bodies, we investigate an underlying approach of constructing impulse waves in the form of explosion and implosion excitations, where we use the exact solutions of the field equations derived from the Pomeransky inverse scattering method. In this approach, we assimilate the gravitational soliton to the impulse wave whose propagation allows to unveiling the physical meanings of the different energy densities within the Einstein and Rosen structure while discussing the numerical approach from Piran and Stark to such a problem.
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ACKNOWLEDGMENTS
The authors would like to express their sincere thanks to the anonymous referees for their critical comments and appropriate suggestions which made this paper more precise and readable. They also appreciate the contributions of Mr. Joe Wabo and Ms. Zang Sedena Christine for the improvement of the English language in the text.
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Defo, J.J., Kuetche, V.K. Cylindrical Gravitational Pulse Waveguide Excitations. J. Exp. Theor. Phys. 135, 324–332 (2022). https://doi.org/10.1134/S1063776122090035
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DOI: https://doi.org/10.1134/S1063776122090035