Closed universes can satisfy the holographic principle in three dimensions

被引：3
作者：
Cruz, N
Lepe, S
机构：
[1] Univ Santiago Chile, Fac Ciencia, Dept Fis, Santiago, Chile
[2] Pontificia Univ Catolica Valparaiso, Inst Fis, Valparaiso, Chile
来源：
PHYSICS LETTERS B | 2001年 / 521卷 / 3-4期
关键词：
D O I：
10.1016/S0370-2693(01)01234-5
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We examine in details Friedmann-Robertson-Walk-er models in 2 + 1 dimensions in order to investigate the cosmic holographic principle suggested by Fischler and Susskind. Our results are rigorously derived differing from the previous one found by Wang and Abdalla. We discuss the erroneous assumptions done in this work. The matter content of the models is composed of a perfect fluid, with a gamma -law equation of state. We found that closed universes satisfy the holographic principle only for exotic matter with a negative pressure. We also analyze the case of a collapsing flat universe. (C) 2001 Elsevier Science B.V. All rights reserved.
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页码：343 / 349
页数：7
相关论文
共 32 条
[1]  
BAK D, HEPTH9902173
[2]   M theory as a matrix model: A conjecture [J].
Banks, T ;
Fischler, W ;
Shenker, SH ;
Susskind, L .
PHYSICAL REVIEW D, 1997, 55 (08) :5112-5128
[3]   3-DIMENSIONAL CLASSICAL SPACETIMES [J].
BARROW, JD ;
BURD, AB ;
LANCASTER, D .
CLASSICAL AND QUANTUM GRAVITY, 1986, 3 (04) :551-567
[4]  
BEKENSTEIN J, 1998, PHYS REV D, V9, P3292
[5]   ENTROPY BOUNDS AND BLACK-HOLE REMNANTS [J].
BEKENSTEIN, JD .
PHYSICAL REVIEW D, 1994, 49 (04) :1912-1921
[6]   UNIVERSAL UPPER BOUND ON THE ENTROPY-TO-ENERGY RATIO FOR BOUNDED SYSTEMS [J].
BEKENSTEIN, JD .
PHYSICAL REVIEW D, 1981, 23 (02) :287-298
[7]   ENTROPY CONTENT AND INFORMATION-FLOW IN SYSTEMS WITH LIMITED ENERGY [J].
BEKENSTEIN, JD .
PHYSICAL REVIEW D, 1984, 30 (08) :1669-1679
[8]  
BIGATTI D, HEPTH0002044
[9]  
BOUSSO R, HEPTH9905177
[10]  
BOUSSO R, HEPTH9906022
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