Bounded compactness from G(E)UP

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Roberto Casadio , Ilim Irfan Çimdiker , Octavian Micu , Jonas Mureika
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引用次数: 0

Abstract

We analyse how different Generalised Uncertainty Principles could place bounds on the compactness of self-gravitating systems. By considering existing experimental bounds on the relevant parameters, we conclude that the compactness of large astrophysical objects is bounded above by the inverse of the GUP parameter, which would naturally be of order one. Conversely, the existence of black holes imposes stronger bounds on those parameters.
从G(E)向上的有界紧性
我们分析了不同的广义不确定性原理如何给自引力系统的紧性设定界限。通过考虑相关参数的现有实验边界,我们得出结论,大型天体物理物体的紧度由GUP参数的倒数所限定,其自然为1阶。相反,黑洞的存在对这些参数施加了更强的限制。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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