Global and local horizon quantum mechanics

被引:23
|
作者
Casadio, Roberto [1 ,2 ]
Giugno, Andrea [3 ]
Giusti, Andrea [1 ,2 ]
机构
[1] Univ Bologna, Dipartimento Fis & Astron, Via Irnerio 46, I-40126 Bologna, Italy
[2] Ist Nazl Fis Nucl, 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
关键词
Horizon; Gravitational radius; Quantum gravity; BLACK-HOLES; WAVE-FUNCTION; PORTRAIT; GRAVITY; MATTER; TIME;
D O I
10.1007/s10714-017-2198-7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Horizons are classical causal structures that arise in systems with sharply defined energy and corresponding gravitational radius. A global gravitational radius operator can be introduced for a static and spherically symmetric quantum mechanical matter state by lifting the classical "Hamiltonian" constraint that relates the gravitational radius to the ADM mass, thus giving rise to a "horizon wave-function". This minisuperspace-like formalism is shown here to be able to consistently describe also the local gravitational radius related to the Misner-Sharp mass function of the quantum source, provided its energy spectrum is determined by spatially localised modes.
引用
收藏
页数:13
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