Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events

This work is supported by NSFC No.11773028, 11633001, 11653002, 11603020, 11903030, 12003029, 11903033, the Fundamental Research Funds for the Central Universities under Grant No.WK2030000036, WK3440000004 and WK2030000044, the Strategic Priority Research Program of the Chinese Academy of Sciences Grant No. XDB23010200, Key Research Program of the Chinese Academy of Sciences, Grant No. XDPB15, and the China Manned Space Program through its Space Application System, and the China Postdoctoral Science Foundation grant No.2019M662168. This research has made use of data, software and/or web tools obtained from the Gravitational Wave Open Science Center (https://www.gw-openscience.org/ ), a service of LIGO Laboratory, the LIGO Scientific Collaboration and the Virgo Collaboration. LIGO Laboratory and Advanced LIGO are funded by the United States National Science Foundation (NSF) as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. Virgo is funded, through the European Gravitational Observatory (EGO), by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale di Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by institutions from Belgium, Germany, Greece, Hungary, Ireland, Japan, Monaco, Poland, Portugal, Spain.