Horizon quantum mechanics for spheroidal sources

被引:8
|
作者
Casadio, Roberto [1 ,2 ]
Giusti, Andrea [1 ,2 ,3 ]
Rahim, Rehana [1 ,4 ]
机构
[1] Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[2] INFN, Sez Bologna, IS FLAG, Via B Pichat 6-2, I-40127 Bologna, Italy
[3] Ludwig Maximilians Univ Munchen, Arnold Sommerfeld Ctr, Theresienstr 37, D-80333 Munich, Germany
[4] Quaid I Azam Univ, Dept Math, Islamabad, Pakistan
关键词
BLACK-HOLE; WAVE-FUNCTION;
D O I
10.1209/0295-5075/121/60004
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We start investigating the extension of the horizon quantum mechanics to the case of non-spherical sources. We first study the location of trapping surfaces in space-times resulting from an axial deformation of static isotropic systems, and show that the Misner-Sharp mass evaluated on the corresponding undeformed spherically symmetric space provides the correct gravitational radius to locate the horizon. We finally propose a way to determine the deformation parameter in the quantum theory. Copyright (C) EPLA, 2018
引用
收藏
页数:7
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