In this work, we study the first order corrections of Hawking temperature and entropy for modified Schwarzschild–Rindler black hole. To do so, we use the modified Lagrangian equation for vector particles in the background of quantum correction parameter \(\delta \). We examine the graphical interpretation of the corrected Hawking temperature with respect to horizon under the effects of correction parameter in order to verify the gravitational effects on the geometry of the modified Schwarzschild–Rindler black hole. We perform a graphic analysis of the modified Schwarzschild–Rindler black hole’s physical state as a function of the mass and Rindler acceleration under the effects of correction parameter. Moreover, we derive the corrected entropy and study the effects of mass and Rindler acceleration parameter on entropy under different variations of correction parameter.

在这项工作中，我们研究了修正史瓦西-林德勒黑洞的霍金温度和熵的一阶修正。为此，我们在量子校正参数\(\delta \)的背景下使用矢量粒子的修正拉格朗日方程。我们检查了在校正参数的影响下校正后的霍金温度相对于视界的图形解释，以验证引力对修正后的史瓦西-林德勒黑洞几何结构的影响。我们对修正后的 Schwarzschild-Rindler 黑洞的物理状态进行了图形分析，作为修正参数影响下质量和 Rindler 加速度的函数。此外，我们推导了校正熵，并研究了校正参数不同变化下质量和 Rindler 加速度参数对熵的影响。