强黑洞(原生黑洞)的物理性质  

The physical characters of strong black hole(primordial black hole)

作　　者：周勋秀[1,2] 焦善庆[1] 

机构地区：[1]西南交通大学应用物理系 [2]四川师范学院物理系,四川南充637002

出　　处：《云南大学学报（自然科学版）》2002年第5期358-360,369,共4页Journal of Yunnan University(Natural Sciences Edition)

基　　金：国家自然科学基金重点资助项目 (1963 5 0 10 );对外交流与合作项目 (10 0 11618)

摘　　要：讨论了早期宇宙暴胀、相变中产生的“强黑洞 (即原生黑洞 )”的能量密度和温度等物理性质 ,认为它是由核子发生连续相变后由大量超微夸克组成的具有统计热平衡性质的高温、超高密物态 .对“强黑洞”的寿命、爆炸持续时间和能量发射率的计算结果表明 ,它可能是超高能宇宙γ暴的最佳对应天体 .文中也指出了现时核子与宇宙早期核子物理性质的显著区别 ,从而解释了宇观天体 -微观粒子的质量、半径统一计算公式中出现的不相容性规律 .The strong black hole (primordial black hole) created from the Early Universe has been discussed about its temperature and energy density and considered to be composed of a large number of micro quarks in super high dense state with high temperature and statistical thermal equilibrium.The calculation about its lifetime,duration time of explosion and energy emission rate shows that the strong black hole is probably the best candidate to ultra high energy gamma ray bursts.The obvious difference of physical property between the nucleons of the early universe and the current stage has been discussed and the non consistent pattern in mass and radius formula of Astro Particle has been explained in this paper.

关 键 词：强黑洞 物理性质 宇宙暴胀 原生黑洞 高温超高密物态 统计热平衡 超高能宇宙γ暴 能量密度 温度 

分 类 号：P145.8[天文地球—天体物理]