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    The Structure and Signals of Neutron Stars, from Birth to Death

    Mar 24 – 28, 2014
    Europe/Rome timezone

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    Session

    Plenary session 11

    Mar 28, 2014, 9:00 AM

    Conveners

    Plenary session 11

    • Deepto Chakrabarty (M)

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    1. 11. Review talk on numerical modelling of neutron star coalesence and their remnants.
      Dr Hans Thomas Janka (MPI Garching)
      3/28/14, 9:00 AM
      Review talk on numerical modelling of neutron star coalesence and their remnants.
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    2. 135. Continuous gravitational waves and neutron star microphysics
      Prof. Benjamin Owen (Penn State, USA)
      3/28/14, 9:40 AM
      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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