论文标题
紧凑型二进制合并残余的全息图
Holographic Bound on Area of Compact Binary Merger Remnant
论文作者
论文摘要
同时使用黑洞热力学的综合定律和通过环量子重力校正到量子黑洞熵的限制的全息bekenstein熵，我们表明，在诸如GW150914的gw150914 dys Is Boundections the Practitation Biary Merger形成的邮政隔离区域的边界横截面区域。该下限比在黑洞中使用经典区域定理的限制更一般，因为它不取决于灵感的紧凑型二进制二进制对还是由黑洞或其他外来紧凑型物体组成。界限的推导需要估计二进制合并期间发出的重力波的熵，该二进制合并会适应重力波，这是最初针对粒子集成的现存形式主义。讨论了合并残留的最小横截面区域，这是由于Ligo-Virgo合作最近观察到的二进制紧凑合并而导致的。尽管准确测量BNS合并GW170817的残留物质量仍然是一个挑战，但我们提供了原则的证明，即BNS合并我们的下限在残余物的横截面区域，提供了一种替代方法，可以探究状态星程的有效性，该型号的体重符号，独立于特定型降低符号的数量符号符号符号符号符号符号符号的型号。
Using concomitantly the Generalized Second Law of black hole thermodynamics and the holographic Bekenstein entropy bound embellished by Loop Quantum Gravity corrections to quantum black hole entropy, we show that the boundary cross sectional area of the postmerger remnant formed from the compact binary merger in gravitational wave detection experiments like GW150914, is bounded from below. This lower bound is more general than the bound from application of the classical area theorem for black holes, since it does not depend on whether the inspiralling compact binary pair or the postmerger remnant consists of black holes or other exotic compact objects. The derivation of the bound entails an estimate of the entropy of the gravitational waves emitted during the binary merger which adapts to gravitational waves an extant formalism proposed originally for particle ensembles. The results for the minimal cross-sectional area of the merger remnant due to binary compact mergers observed recently by the LIGO-VIRGO collaboration are discussed. While accurate measurement of the mass of the remnant for the BNS merger GW170817 remains a challenge, we provide a proof of principle that for BNS mergers our lower bound on the cross-sectional area of the remnant provides an alternative approach to probe the validity of neutron star Equations of State, independent of the measurements of the tidal deformabilities of the components.
