VirgoA M87 Heat Transfer

The research continued from the white hole observation experiment with data analysis. The math- ematical method derived before the observation is supplemented with the heat transfer method. The research took an empirical boundary approach on heat flux for the heat transfer between a black hole and white hole, without considering the Big Bang theory. The heat transfer in the system material boundary is seen as a gravitational indicator from asymptotic decay. Albeit the numerical results are instrumentation specific, the conceptualization of the method can be applied to other data imaging apparatus. However, this method is material dependent, and the estimation of the imaginary time di- mension depends on the chemical components of incident light and detection plate. It puts the cosmic microwave background to the account of instrumentation noise, and conceptualized cosmic background radiation for asymptotic safety. The convergence and divergence can be further corrected by different bias factors.

本研究延续自一项结合数据分析的白洞（white hole）观测实验。研究在观测前推导的数学方法基础上，补充了热传递方法。针对黑洞（black hole）与白洞间热传递的热通量，本研究采用经验边界方法，且未考虑大爆炸理论。系统物质边界处的热传递被视为基于渐近衰减的引力指示指标。尽管数值结果仅适用于特定仪器，但该方法的概念框架可推广至其他数据成像设备。不过，该方法具有材料依赖性，虚时间维度（imaginary time dimension）的估算结果取决于入射光与探测板的化学成分。本研究将宇宙微波背景（cosmic microwave background）纳入仪器噪声的考量范畴，并为渐近安全（asymptotic safety）构建了宇宙背景辐射的概念化模型。该方法的收敛与发散特性可通过不同偏置因子进一步修正。