http://arxiv.org/abs/2304.06581
GRB 211211A is a rare burst with a genuinely long duration, yet its prominent kilonova association provides compelling evidence that this peculiar burst was the result of a compact binary merger. However, the exact nature of the merging objects, whether they were neutron star pairs, neutron star-black hole systems, or neutron star-white dwarf systems, remains unsettled. This Letter delves into the rarity of this event and the possibility of using current and next-generation gravitational wave detectors to distinguish between the various types of binary systems. Our research reveals an event rate density of $\gtrsim 5.67^{+13.04}_{-4.69} \times 10^{-3}\ \rm Gpc^{-3} yr^{-1}$ for GRB 211211A-like GRBs, which is significantly smaller than that of typical long and short GRB populations. We further calculated that if the origin of GRB 211211A is a result of a neutron star-black hole merger, it would be detectable with a significant signal-to-noise ratio, given the LIGO-Virgo-KAGRA designed sensitivity. On the other hand, a neutron star-white dwarf binary would also produce a considerable signal-to-noise ratio during the inspiral phase at decihertz and is detectable by next-generation space-borne detectors DECIGO and BBO. However, to detect this type of system with millihertz space-borne detectors like LISA, Taiji, and TianQin, the event must be very close, approximately 3 Mpc in distance or smaller.
Y. Yin, B. Zhang, H. Sun, et. al.
Fri, 14 Apr 23
57/64
Comments: 8 pages, 3 figures, 1 table