In this paper, we have investigated accreting millisecond X-ray pulsars, which are rapidly rotating neutron stars in low-mass X-ray binaries. These systems exhibit coherent X-ray pulsations that arise when the accretion flow is magnetically channeled to the stellar surface. Here, we have developed the fundamental equations for an accretion disk around accreting millisecond X-ray pulsars in the presence of a dynamo generated magnetic field in the inner part of the disk. We have also formulated the numerical method for the structure equations in the inner region of the disk and the highest accretion rate is enough to form the inner region of the disk, which is overpowered by radiation pressure and electron scattering. Finally, we have examined our results with the effects of dynamo magnetic fields on accreting millisecond X-ray pulsars.

在本文中，我们研究了吸积毫秒 X 射线脉冲星，它们是低质量 X 射线双星中快速旋转的中子星。当吸积流被磁性引导到恒星表面时，这些系统表现出相干的 X 射线脉动。在这里，我们开发了在吸积盘内部存在发电机产生的磁场的情况下围绕吸积毫秒 X 射线脉冲星的吸积盘的基本方程。我们还制定了盘内部区域结构方程的数值方法，最高吸积率足以形成盘内部区域，辐射压力和电子散射压倒了盘内部区域。最后，我们用发电机磁场对吸积毫秒 X 射线脉冲星的影响检验了我们的结果。