Wave-fronts of gravitational waves partially trapped in ultra-compact stars
Marek Abramowicz, Ji\v{r}\'i Hor\'ak, Kate\v{r}ina, Klimovi\v{c}ov\'a
TL;DR
This paper analytically investigates how gravitational wavefronts are partially trapped within ultra-compact stars, exploring implications for quantum gravity and gravitational wave detection.
Contribution
It provides an analytic treatment of gravitational wave damping in ultra-compact stars and discusses potential links to quantum gravity and gravitational wave observations.
Findings
Analytic model of wave damping in ultra-compact stars
Potential connection to quantum gravity effects
Implications for LIGO-Virgo gravitational wave measurements
Abstract
We dedicate this work to Dr Omer Blaes, professor of physics at UCSB, on the occasion of his sixtieth birthday. We have been collaborating now and then with Dr. Blaes on problems involving oscillations, waves and stability. Happy birthday, Omer. Enjoy the analytic treatment of damping of the gravitational waves trapped inside ultra compact stars and its possible connection to Quantum Gravity in the context of the LIGO-Virgo efforts in accurately measuring ringdowns and echoes.
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements