论文标题
修饰的引力理论（MOG）和Aligo GW190521重力波事件
Modified Gravitation Theory (MOG) and the aLIGO GW190521 Gravitational Wave Event
论文作者
论文摘要
A consequence of adopting a modified gravitational theory (MOG) for the aLIGO GW190521 gravitational wave detection involving binary black hole sources is to fit the aLIGO strain and chirp data with lower mass, compact coalescing binary systems such as neutron star-neutron star (NS-NS), black hole - neutron star (BH-NS), and black hole-black hole (BH-BH) systems.在MOG BH -BH -BH组件质量可能小于组件质量$ M_1 = 85M_ \ ODOT $和$ M_2 = 66M_ \ ODOT $从Aligo GW190521重力波动事件中推论。这减少了最终残余质量$ m_f = 150m_ \ odot $的质量，并允许黑洞的主要，次级和最终残余质量由常规恒星倒塌模型形成。
A consequence of adopting a modified gravitational theory (MOG) for the aLIGO GW190521 gravitational wave detection involving binary black hole sources is to fit the aLIGO strain and chirp data with lower mass, compact coalescing binary systems such as neutron star-neutron star (NS-NS), black hole - neutron star (BH-NS), and black hole-black hole (BH-BH) systems. In MOG BH - BH component masses can be smaller than the component masses $m_1=85M_\odot$ and $m_2=66M_\odot$ inferred from the aLIGO GW190521 gravitational wave event. This reduces the mass of the final remnant mass $M_f=150M_\odot$ and allows the primary, secondary and final remnant masses of the black holes to be formed by conventional stellar collapse models.
