论文标题
重力（MOG）和质量差距中的重中子恒星
Modified Gravity (MOG) and Heavy Neutron Star in Mass Gap
论文作者
论文摘要
修饰的重力（MOG）理论适用于重力波二进制合并GW190814，以证明中子星的修改的Tolman -Oppenheimer -Volkoff方程将产生质量$ M = 2.6 -2.7 m_ \ odot $，可以使biary septim septim $ 2. 5. hypoth $ 2. m_ \ odot $。
The modified gravity (MOG) theory is applied to the gravitational wave binary merger GW190814 to demonstrate that the modified Tolman-Oppenheimer-Volkoff equation for a neutron star can produce a mass $M=2.6 -2.7 M_\odot$, allowing for the binary secondary component to be identified as a heavy neutron star in the hypothesized mass gap $2.5 - 5 M_\odot$.
