[Users] Determination of the final spin of the remnant of a binary neutron star merger

Beyhan Karakaş beyhannkarakas at gmail.com
Wed Mar 4 10:12:29 CST 2020

Dear to whom it may concern,

  I am interested in determining the spin of the remnant which are resulted
from binary neutron star (initially are in irrotational configuration)
merger . How could the method to determine the final spin differ (if it
does) in case of remnant is a black hole or a neutron star. For the former
case, I suppose QuasiLocalMeasures parameter
"begin_qlm_calculations_after"  along with AHFinderDirect parameter
"find_after_individual" should be set to the time/iteration that the black
hole formed. If this is not the case, please clarify how could it be
determined? In addition, is there a way to find the evolution of the spin
and orbital eccentricity of the binary?

Best regards,

-------------- next part --------------
An HTML attachment was scrubbed...
URL: http://lists.einsteintoolkit.org/pipermail/users/attachments/20200304/6024f2eb/attachment-0001.html 

More information about the Users mailing list