IS DARK ENERGY FROM COSMIC HAWKING RADIATION?

被引：8
作者：
Lee, Jae-Weon [1 ,2 ]
Kim, Hyeong-Chan [3 ]
Lee, Jungjai [4 ]
机构：
[1] Korea Inst Adv Study, Sch Computat Sci, 207-43 Cheongnyangni 2 Dong, Seoul 130012, South Korea
[2] Jungwon Univ, Dept Energy Resources Dev, Chungbuk 367805, South Korea
[3] Chungju Natl Univ, Div Liberal Arts, Chungju 380702, South Korea
[4] Daejin Univ, Dept Phys, Pochon 487711, Gyeonggi, South Korea
来源：
MODERN PHYSICS LETTERS A | 2010年 / 25卷 / 04期
关键词：
Dark energy; Hawking radiation; COSMOLOGICAL CONSEQUENCES; FIELD THEORY; THERMODYNAMICS; ENTROPY; MODEL; EQUATION; UNIVERSE; FLUCTUATIONS; CONSTRAINTS; COMPONENT;
D O I：
10.1142/S0217732310032469
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
It is suggested that dark energy is the energy of the Hawking radiation from a cosmic horizon. Despite its extremely low Gibbons-Hawking temperature, this radiation could have the appropriate magnitude O((MPH2)-H-2) and the equation of state to explain the observed cosmological data if there is a Planck scale UV-cutoff, where H is the Hubble parameter.
引用
收藏
页码：257 / 267
页数：11
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