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                                     “Binary neutron star mergers and numerical relativity “





 Thursday, 20. Aug. 2015

Audio-only-Recording as MP3-File (smallest possible size):

       -   Audio.mp3   (ca.25 Mb)


Video-Recording for any system with MP4-support:

       -   Video.mp4   (ca.177 Mb)


 15:15 – 16:10


Abstract :

Compact binary neutron star, a system composed of two neutron stars in close orbits, is one of the most promising sources

for the gravitational-wave detectors such as advanced LIGO, VIRGO, and KAGRA. The merger of this system is also

the most promising candidate for short-duration gamma-ray bursts for which we do not still know the progenitor, and a

promising site for the production of heavy elements such as gold which have been produced by the rapid neutron

capture process in the universe. Gravitational-wave detection and associated observation of the electromagnetic counterparts

from binary neutron star mergers will test these hypotheses in the next decade and hopefully solve many unsolved issues.

I will talk on these aspects on the neutron-star mergers emphasizing that the accurate prediction of the merger events by

numerical studies is quite important.


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