Upper Limits on the Rates of Binary Neutron Star and Neutron Star-Black Hole Mergers from Advanced Ligo's First Observing Run

Abbott, B.P. and Abbott, R. and Abbott, T.D. and Abernathy, M.R. and Acernese, F. and Frei, Zsolt and Gergely, Árpád László and Gondán, László and Raffai, Péter and Tápai, Márton and Vasúth, Mátyás Zsolt (2016) Upper Limits on the Rates of Binary Neutron Star and Neutron Star-Black Hole Mergers from Advanced Ligo's First Observing Run. ASTROPHYSICAL JOURNAL LETTERS, 832 (2). ISSN 2041-8205

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Abstract

We report here the non-detection of gravitational waves from the merger of binary neutron star systems and neutron-star–black-hole systems during the first observing run of Advanced LIGO. In particular we searched for gravitational wave signals from binary neutron star systems with component masses ∈ [1, 3]M and component dimensionless spins < 0.05. We also searched for neutron-star–black-hole systems with the same neutron star parameters, black hole mass ∈ [2, 99]M and no restriction on the black hole spin magnitude. We assess the sensitivity of the two LIGO detectors to these systems, and find that they could have detected the merger of binary neutron star systems with component mass distributions of 1.35±0.13M at a volume-weighted average distance of ∼ 70 Mpc, and for neutron-star–black-hole systems with neutron star masses of 1.4M and black hole masses of at least 5M , a volume-weighted average distance of at least ∼ 110 Mpc. From this we constrain with 90% confidence the merger rate to be less than 12,600 Gpc−3 yr−1 for binary-neutron star systems and less than 3,600 Gpc−3 yr−1 for neutron-star–black-hole systems. We discuss the astrophysical implications of these results, which we find to be in tension with only the most optimistic predictions. However, we find that if no detection of neutron-star binary mergers is made in the next two Advanced LIGO and Advanced Virgo observing runs we would place significant constraints on the merger rates.

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