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arXiv · 2301.11619

Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO

Gonzalo Morrás·José Francisco Nuño Siles·Juan García-Bellido·Ester Ruiz Morales·Alexis Menéndez-Vázquez·Christos Karathanasis·Katarina Martinovic·Khun Sang Phukon·Sebastien Clesse·Mario Martí nez·Mairi Sakellariadou
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Abstract

We perform an exhaustive follow-up analysis of a subsolar-mass (SSM) gravitational wave (GW) candidate reported by Phukon et al. from the second observing run of Advanced LIGO. This candidate has a reported signal-to-noise ratio (SNR) of $8.6$ and false alarm rate of $0.41$ yr which are too low to claim a clear gravitational-wave origin. When improving on the search by using more accurate waveforms, extending the frequency range from 45 Hz down to 20 Hz, and removing a prominent blip glitch, we find that the posterior distribution of the network SNR lies mostly below the search value, with the $90\%$ confidence interval being $7.94^{+0.70}_{-1.05}$. Assuming that the origin of the signal is a compact binary coalescence (CBC), the secondary component is $m_2 = \text{$0.76^{+0.50}_{-0.14}$} M_\odot$, with $m_2 < 1 M_\odot$ at $84\%$ confidence level, suggesting an unexpectedly light neutron star or a black hole of primordial or exotic origin. The primary mass would be $m_1 = \text{$4.71^{+1.57}_{-2.18}$} M_\odot$, likely in the hypothesized lower mass gap and the luminosity distance is measured to be $D_{\rm L}=124^{+82}_{-48}$Mpc. We then probe the CBC origin hypothesis by performing the signal coherence tests, obtaining a log Bayes factor of $4.96 \pm 0.13$ for the coherent vs. incoherent hypothesis. We demonstrate the capability of performing a parameter estimation follow-up on real data for an SSM candidate with moderate SNR. The improved sensitivity of O4 and subsequent LIGO-Virgo-KAGRA observing runs could make it possible to observe similar signals, if present, with a higher SNR and a more precise measurement of the parameters of the binary.

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Gonzalo Morrás, José Francisco Nuño Siles, Juan García-Bellido, Ester Ruiz Morales, Alexis Menéndez-Vázquez, Christos Karathanasis, Katarina Martinovic, Khun Sang Phukon, Sebastien Clesse, Mario Martí nez, Mairi Sakellariadou. 2023-01-27. Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO. https://doi.org/10.1016/j.dark.2023.101285

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