Session

Plenary session 11

28 Mar 2014, 09:00

Conveners

Plenary session 11

  • Deepto Chakrabarty (M)

Presentation materials

There are no materials yet.

  1. Dr Hans Thomas Janka (MPI Garching)
    28/03/2014, 09:00
    Review talk on numerical modelling of neutron star coalesence and their remnants.
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  2. 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...
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