Spherical Black(球形黑色)研究综述
Spherical Black 球形黑色 - Finally, we re-compute the tidal Love numbers of spherical black holes in higher dimensions. [1] In this paper, we study the thermodynamics and geothermodynamics of spherical black hole solutions in dRGT massive gravity in a new extended phase space. [2] We study the quasinormal modes of $p$-form fields in spherical black holes in $D$-dimensions. [3] While we largely focus on the planar black hole limit in this paper, we include some preliminary analysis of the spherical black hole case in an appendix. [4] Photomicrographs of yttrium-90 selective internal radiation therapy–induced chronic (A) and acute cholecystitis with mucosal erosion (B) and the presence of characteristic spherical black microspheres. [5] These encapsulations can provide an approach to control the net charge on the resulting cage-guest complexes and regulate their charge-dominated assembly into hollow spherical blackberry-type assemblies in dilute solutions: encapsulation of neutral guests will hardly influence their self-assembly process, including the blackberry structure size, which is directly related to the intercage distance in the assembly; whereas encapsulating negatively (positively) charged guests resulted in a shorter (longer) intercage distance with larger (smaller) assemblies formed. [6] In both the 2014 and 2016 Maritime RobotX Challenges, it was found that detecting obstacles using LIDAR only and classifying obstacles using vision only can be challenged by environmental conditions, such as glare from the sun or by objects such as the spherical black buoys from the obstacle field that disperses LIDAR rays. [7] To compare with the black hole limit, we obtain a recursion relation for the lowest-twist products of two stress tensors in a spherical black hole background, letting us efficiently compute their OPE coefficients and prove their insensitivity to higher curvature terms. [8] We find for spherical black holes that there are respectively at most two and three physical critical points in five and six dimensions. [9] Spherical black hole (BH) solutions in Einstein-Maxwell-scalar (EMS) models wherein the scalar field is non-minimally coupled to the Maxwell invariant by some coupling function are discussed. [10] In this paper, we focus on angular radius of spherical black hole shadow with respect to freely falling observers. [11]最后，我们重新计算了更高维度球形黑洞的潮汐 Love 数。 [1] 在本文中，我们在一个新的扩展相空间中研究了 dRGT 大质量引力中球形黑洞溶液的热力学和地热力学。 [2] 我们研究了$D$-维度的球形黑洞中$p$-form 场的准正规模式。 [3] 虽然我们在本文中主要关注平面黑洞极限，但我们在附录中包含了对球形黑洞情况的一些初步分析。 [4] 钇90选择性内部放射治疗引起的慢性（A）和急性胆囊炎伴有黏膜糜烂（B）和特征性球形黑色微球的显微照片。 [5] 这些封装可以提供一种方法来控制所产生的笼客体复合物的净电荷，并将其电荷主导的组装体在稀溶液中调节为空心球形黑莓型组装体：中性客体的封装几乎不会影响它们的自组装过程，包括黑莓结构尺寸，与组件中的间距直接相关；而封装带负（正）电的客人会导致更短（更长）的嵌入距离，并形成更大的 （更小）组件。 [6] 在 2014 年和 2016 年的海上 RobotX 挑战赛中，发现仅使用 LIDAR 检测障碍物并仅使用视觉对障碍物进行分类可能会受到环境条件的挑战，例如来自太阳的眩光或物体（例如来自障碍物的球形黑色浮标）分散激光雷达射线的场。 [7] 为了与黑洞极限进行比较，我们获得了球形黑洞背景中两个应力张量的最低扭曲乘积的递归关系，让我们有效地计算了它们的 OPE 系数并证明了它们对更高曲率项的不敏感性。 [8] 我们发现对于球形黑洞，在五维和六维中分别最多有两个和三个物理临界点。 [9] 讨论了爱因斯坦-麦克斯韦标量 (EMS) 模型中的球形黑洞 (BH) 解，其中标量场通过一些耦合函数非最小耦合到麦克斯韦不变量。 [10] 在本文中，我们关注的是球形黑洞阴影相对于自由落体观察者的角半径。 [11]
spherical black hole 球形黑洞
Finally, we re-compute the tidal Love numbers of spherical black holes in higher dimensions. [1] In this paper, we study the thermodynamics and geothermodynamics of spherical black hole solutions in dRGT massive gravity in a new extended phase space. [2] We study the quasinormal modes of $p$-form fields in spherical black holes in $D$-dimensions. [3] While we largely focus on the planar black hole limit in this paper, we include some preliminary analysis of the spherical black hole case in an appendix. [4] To compare with the black hole limit, we obtain a recursion relation for the lowest-twist products of two stress tensors in a spherical black hole background, letting us efficiently compute their OPE coefficients and prove their insensitivity to higher curvature terms. [5] We find for spherical black holes that there are respectively at most two and three physical critical points in five and six dimensions. [6] Spherical black hole (BH) solutions in Einstein-Maxwell-scalar (EMS) models wherein the scalar field is non-minimally coupled to the Maxwell invariant by some coupling function are discussed. [7] In this paper, we focus on angular radius of spherical black hole shadow with respect to freely falling observers. [8]最后，我们重新计算了更高维度球形黑洞的潮汐 Love 数。 [1] 在本文中，我们在一个新的扩展相空间中研究了 dRGT 大质量引力中球形黑洞溶液的热力学和地热力学。 [2] 我们研究了$D$-维度的球形黑洞中$p$-form 场的准正规模式。 [3] 虽然我们在本文中主要关注平面黑洞极限，但我们在附录中包含了对球形黑洞情况的一些初步分析。 [4] 为了与黑洞极限进行比较，我们获得了球形黑洞背景中两个应力张量的最低扭曲乘积的递归关系，让我们有效地计算了它们的 OPE 系数并证明了它们对更高曲率项的不敏感性。 [5] 我们发现对于球形黑洞，在五维和六维中分别最多有两个和三个物理临界点。 [6] 讨论了爱因斯坦-麦克斯韦标量 (EMS) 模型中的球形黑洞 (BH) 解，其中标量场通过一些耦合函数非最小耦合到麦克斯韦不变量。 [7] 在本文中，我们关注的是球形黑洞阴影相对于自由落体观察者的角半径。 [8]