MG13 - Talk detail |
Participant |
Wan, Mew-Bing | |||||||
Institution |
Asia-Pacific Center for Theoretical Physics - #503 Hogil Kim Memorial Bldg, POSTECH, San 31, Hyoja-dong, Namgu - Pohang - Gyeongbuk - South Korea | |||||||
Session |
EG4 |
Accepted |
Yes |
Order |
99 |
Time |
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Talk |
Poster abstract |
Title |
A class of self-gravitating objects from neutron star type I critical collapses | |||||
Co-authors | ||||||||
Abstract |
We study the neutron star axisymmetric critical solution previously found in the numerical studies of neutron star mergers. Using neutron star-like initial data and performing similar merger simulations, we demonstrate that the solution is indeed a semi-attractor on the threshold plane separating the basin of a neutron star and the basin of a black hole in the solution space of the Einstein equations. The properties of the critical index of the solution, in particular, its dependence on conserved quantities, are then studied. From the study, it is found that a family of neutron star semi-attractors exist that can be classified by both their rest masses and ADM masses. |
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