论文标题
长臂猿辐射和通货膨胀会因时空量子而产生吗？
Can Gibbons-Hawking Radiation and Inflation Arise Due to Spacetime Quanta?
论文作者
论文摘要
在这项研究中，我们提供了对长臂猿辐射和通货膨胀的反重新制定解释。通过使用L.C.最近提出的时空量化程序Céleri等人，在抗DE保姆空间中，我们表明，长臂猿的辐射是相关空间的内在特性，由于存在标量场的存在，其量子的量子“载有“长度” $ l $（即双骨曲率的半径）。此外，在Tsallis Q-Framework的背景下，我们提出了一个依赖非扩展参数$ Q $的通货膨胀模型。这种通货膨胀的主要来源是前面提到的标量领域。受观察数据的约束，Q参数以及模型参数的其余部分被用来估计通胀结束的时间以及重新加热的温度。后者发现与长臂猿温度有关。因此，本模型提供了有关宇宙背景辐射（CMB）的性质的另一种观点。
In this study, we provide an alternatively reformulated interpretation of Gibbons-Hawking radiation as well as inflation. By using a spacetime quantization procedure, proposed recently by L.C. Céleri et al., in anti-de Sitter space we show that Gibbons-Hawking radiation is an intrinsic property of the concerned space, that arises due to the existence of a scalar field whose quanta "carry" a length $l$ (i.e. the radius of the hyperboloid curvature). Furthermore, within the context of Tsallis q-framework, we propose an inflationary model that depends on the non-extensive parameter $q$. The main source of such an inflation is the same scalar field mentioned before. Being constrained by the observational data, the q-parameter along with the rest of the model's parameters has been used to estimate the time at which inflation ends as well as the reheating temperature. The latter is found to be related to Gibbons-Hawking temperature. Thus, the present model offers an alternative perspective regarding the nature of the cosmic background radiation (CMB).
