Conveners
Plenary session 11
- Deepto Chakrabarty (M)
Dr
Hans Thomas Janka
(MPI Garching)
28/03/2014, 09:00
Review talk on numerical modelling of neutron star coalesence and their remnants.
Prof.
Benjamin Owen
(Penn State, USA)
28/03/2014, 09:40
Mechanisms of continuous gravitational-wave emission from neutron stars include long-lived r-mode oscillations and rotations of static deformations (“mountains”). Emission depends on the equation of state and transport coefficients of matter above nuclear density. Therefore gravitational-wave searches may be guided by, and reveal information on, the equation of state and other properties of...
