11–13 Jul 2023
Amsterdam, NL
Europe/Amsterdam timezone

Neutron star crust deformations, solar system mountains, and gravitational waves

11 Jul 2023, 10:10
20m
Amsterdam, NL

Amsterdam, NL

Science Park 904 1098 XH Amsterdam

Speaker

Mr Jorge Morales (Indiana University - Bloomington and Max Planck Institute for Gravitational Physics)

Description

"Mountains”, or non-axisymmetric deformations of rotating neutron stars, efficiently radiate gravitational waves. We consider analogies between neutron star mountains and surface features of solar system bodies. Both neutron stars and moons, such as Europa or Enceladus, have thin crusts over deep oceans while Mercury has a thin crust over a large metallic core. Thin sheets may wrinkle in universal ways. Europa has linear features, Enceladus has "Tiger" stripes, and Mercury has lobate scarps. Neutron stars may have analogous features. The innermost inner core of the Earth is anisotropic with a shear modulus that depends on direction. Possible anisotropies in the neutron star crust material could produce mountains as the star is spun up or down.

Primary authors

Dr Charles Horowitz (Indiana University - Bloomington) Mr Jorge Morales (Indiana University - Bloomington and Max Planck Institute for Gravitational Physics)

Presentation materials