Ponente
Camilo Garcia Cely
(IFIC, CSIC-UV)
Descripción
The solar plasma is a natural source of gravitational waves at high frequencies, a spectral range that is attracting increasing interest due to its potential to reveal new physical phenomena. Motivated by this, in this talk, I will present the first comprenhensive calculation of the gravitational-wave power spectrum emitted by the Sun. This includes both microscopic processes—such as bremsstrahlung and photoproduction—and macroscopic contributions from hydrodynamic fluctuations, each computed using methods adapted from axion physics.
Based on arXiv:2407.18297 (accepted for publication in PRL)
Autor primario
Camilo Garcia Cely
(IFIC, CSIC-UV)
