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General Relativistic Simulations of Binary Neutron Star Mergers - Abstract
2 junho 2015, 11:18 - Ana Maria Cidade Mourão
Speaker: Bruno Giacomazzo (University of Trento)
Date: Thursday, June 4, 2015 – 14:30
Place: Physics Dept. Meeting Room, 2nd floor, IST
Contact: vincenzo.vitagliano@ist.utl.pt
Abstract:
Binary
neutron stars (BNSs) are one of the most promising sources for the first
detections of gravitational waves (GWs) by ground-based detectors (such as,
advanced LIGO and Virgo). They may also emit powerful electromagnetic (EM)
signal and they are thought to be behind the central engine that powers short
gamma-ray bursts (SGRBs). In this talk I will review the results of fully
general relativistic simulations of binary neutron star mergers performed with
the Whisky code. I will describe both their GW and EM emission and what we can
learn from their detection. I will in particular describe how BNS mergers can
be used to infer the equation of state of neutron star matter and how they can
be related to SGRBs.