The Concept of Gravito-Rotational Acceleration and its Consequences for Compact Stellar Objects

In a previous series of papers related to the Combined Gravitational Action (CGA), we focused on studying orbital motion without spin. In this paper, we extend the application of CGA to self-rotating material bodies, specifically axially spinning massive objects. These objects can be viewed as gravito-rotational sources capable of generating gravito-rotational acceleration, a concept not addressed in existing gravity theories. Consequently, the concept of Gravito-Rotational Acceleration should be primarily understood as the combination of gravitational and rotational forces acting on an object. This phenomenon occurs when an object is both rotating and experiencing the effects of its self-gravity. The interaction between these two forces can result in unique acceleration patterns that are not seen in objects that are only subject to one of these forces. Understanding Gravito-Rotational Acceleration can provide valuable insights into the behavior of rotating objects in gravitational fields. For example, the implications of this acceleration are particularly intriguing for Compact Stellar Objects. Regardless of the equation of state, we have discovered that the maximum internal magnetic field strength of the Sun and magnetar are, respectively, 1.68716 x10⁵G and 5.6x10¹⁸G.

在先前一系列与联合引力作用（Combined Gravitational Action, CGA）相关的研究论文中，我们的研究重点聚焦于无自旋的轨道运动。本文将CGA的应用范畴拓展至自转物质天体，具体为轴向旋转的大质量天体。这类天体可被视为引力旋转源，能够产生引力旋转加速度（Gravito-Rotational Acceleration）——这一概念在现有引力理论中尚未被探讨过。因此，引力旋转加速度的核心内涵应理解为作用于天体的引力与旋转力的复合效应。当天体既处于自转状态，又受自身引力场的作用时，便会出现这一现象。两种力的相互作用可催生独特的加速度模式，这类模式在仅受单一作用力影响的天体中并不存在。对引力旋转加速度的研究，可为理解引力场中自转天体的运动行为提供极具价值的视角。例如，该加速度的物理意义对于致密恒星天体而言尤为引人关注。无论物态方程如何，我们均已发现：太阳与磁星的内部最大磁场强度分别为1.68716×10⁵高斯（G）与5.6×10¹⁸高斯（G）。