Resumen
The Klein-Gordon equation is solved in the curved background spacetime created by a dispersive gravitational wave. Unlike solutions of perturbed Einstein equations in vacuum, dispersive gravitational waves do not travel exactly at the speed of light. As a consequence, the gravitational wave can resonantly exchange energy with scalar massive particles. Some details of the resonant interaction are displayed in a calculation demonstrating how relativistic particles (modeled by the Klein-Gordon equation), feeding on such gravitational waves, may be driven to extreme energies.
Idioma original | Inglés |
---|---|
Número de artículo | 063010 |
Publicación | Physical Review D |
Volumen | 101 |
N.º | 6 |
DOI | |
Estado | Publicada - 15 mar. 2020 |
Publicado de forma externa | Sí |