Self-gravitating neutron star-disks in general relativity
ORAL
Abstract
Binary neutron star mergers or accreting compact objects other than black holes can lead to a self-gravitating neutron star-disk system. Using the COCAL initial value code, we compute self-gravitating neutron star-disk spacetimes for a variety of neutron star equations of state and rotation parameters, as well as for different disk angular velocity profiles. We make direct comparisons with similar self-gravitating disks around black holes.
* This work was supported in part by National Science Foundation Grants No. PHY-2308242 and No. OAC-2310548 to the University of Illinois at Urbana-Champaign.
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Presenters
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Eric Yu
University of Illinois at Urbana-Champaign
Authors
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Eric Yu
University of Illinois at Urbana-Champaign
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Antonios Tsokaros
University of Illinois at Urbana-Champain, University of Illinois at Urbana-Champai
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Milton Ruiz
Universitat de Valéncia
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Koji Uryu
Univ of the Ryukyus