Rindler空间中部分电离相对论氢等离子体的Saha方程

Sanchita Das, S. Chakrabarty
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引用次数: 0

摘要

众所周知,传统的洛伦兹变换是两个惯性参照系之间的时空坐标变换[1]。然而,根据等效原理,用与狭义相对论相同的方法获得匀加速系和惯性系之间的时空变换是很容易的[2,3,4,5,6]。在目前的情况下,平坦的时空几何被称为伦德勒空间。为了说明等效原理,我们可以这样说,一个参考系在没有引力场的情况下进行加速运动,等于一个静止的参考系在有引力场的情况下。因此,在这幅图中,均匀加速度的大小正好等于引力场的强度。我们可以假设引力场是由一个强引力物体产生的。我们进一步近似得出引力场在一个特殊区域的小范围内是恒定的。因为它正好等于运动坐标系的均匀加速度,所以它也被称为坐标系的局部加速度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Saha Equation for Partially Ionized Relativistic Hydrogen Plasma in Rindler Space
It is well-known that the conventional Lorentz transformations are the spacetime coordinate transformations between two inertial frames of references [1]. However, following the principle of equivalence, it is trivial to obtain the space-time transformations between a uniformly accelerated frame and an inertial frame and vice-versa in the same manner as it is done in special theory of relativity [2, 3, 4, 5, 6]. In the present scenario the flat spacetime geometry is called the Rindler space. For the sake of illustration of principle of equivalence, one may state, that a reference frame undergoing an accelerated motion in absence of gravitational field is equivalent to a frame at rest in presence of a gravitational field. Therefore, in the present picture, the magnitude of the uniform acceleration is exactly equal to the strength of gravitational field. We may assume that the gravitational field is produced by a strong gravitating object. We further approximate that the gravitational field is constant within a small domain of special region. Since it is exactly equal to the uniform acceleration of the moving frame, this is also called the local acceleration of the frame.
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