Brown-York Mass and the Thorne Hoop Conjecture

被引:14
作者
Murchadha, Niall O. [1 ,2 ]
Tung, Roh-Suan [1 ]
Xie, Naqing [3 ]
Malec, Edward [2 ,4 ]
机构
[1] Shanghai Normal Univ, Ctr Astrophys, Shanghai, Peoples R China
[2] Univ Coll Cork, Dept Phys, Cork, Ireland
[3] Fudan Univ, Sch Math Sci, Shanghai 200433, Peoples R China
[4] Jagiellonian Univ, Inst Phys, Krakow, Poland
基金
中国国家自然科学基金;
关键词
QUASI-LOCAL ENERGY; TRAPPED SURFACES; GENERAL-RELATIVITY; VACUUM SPACETIMES; BLACK-HOLE; MATTER;
D O I
10.1103/PhysRevLett.104.041101
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The Thorne hoop conjecture is an attempt to make precise the notion that gravitational collapse occurs if enough energy is compressed into a small enough volume, with the "size" being defined by the circumference. We can make a precise statement of this form, in spherical symmetry, using the Brown-York mass as our measure of the energy. Consider a spherical 2-surface in a spherically symmetric spacetime. If the Brown-York mass M(BY) and the circumference C satisfy C<2 pi M(BY), then the system must either have emerged from a white hole or will collapse into a black hole. We show that no equivalent result can hold true using either the Liu-Yau mass M(LY) or the Wang-Yau mass M(WY). This forms a major obstacle to any attempt to establish a Thorne-type hoop theorem in the general case based on either the Liu-Yau or the Wang-Yau mass.
引用
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页数:4
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