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非微扰的极早期宇宙现象学:共振的原初扰动与非高斯尾巴
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作者 蔡一夫 何鑫宸 马潇汉 《天文学报》 CAS CSCD 北大核心 2024年第3期1-27,共27页
在精确宇宙学的时代,多信使、高精度、小尺度的宇宙学观测在帮助人们从更加深刻的层面理解宇宙极早期的同时,也给基于线性近似和微扰展开宇宙学扰动理论带来了新的挑战.近年来,对原初引力波和原初黑洞的搜寻使得研究人员们对早期宇宙在... 在精确宇宙学的时代,多信使、高精度、小尺度的宇宙学观测在帮助人们从更加深刻的层面理解宇宙极早期的同时,也给基于线性近似和微扰展开宇宙学扰动理论带来了新的挑战.近年来,对原初引力波和原初黑洞的搜寻使得研究人员们对早期宇宙在小尺度上的非线性非微扰过程产生了浓厚的研究兴趣.综述了在宇宙学小尺度上关于原初黑洞产生以及引力波研究取得的诸多进展,重点关注了使用Mathieu方程的共振效应来研究小尺度功率谱放大以及诱导产生可观测的原初引力波的方法.此外,还尝试探讨了非高斯尾巴对原初黑洞形成的影响.发现Mathieu方程所具备的共振效应可以提供一种有效的方法来刻画原初宇宙中小尺度的非微扰动力学过程,从而能够更好地理解原初黑洞的形成以及相关的引力波产生机制.同时,非微扰的非高斯性在原初黑洞形成中可能会产生不可忽视的影响. 展开更多
关键词 宇宙学:暴胀理论 早期宇宙 原初引力波 非高斯性 原初黑洞
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含αR^2+γR_(μν)R^(μν)项的宇宙暴涨
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作者 李元杰 《天体物理学报》 CSCD 1992年第3期207-209,共3页
我们利用含αR^2+γR_(μv)R^(μv)项的宇宙理论同带有一个标量场φ的Einstein理论之间的等价性,讨论了该宇宙的暴涨行为.结果表明,在D维空时(D>2)中,存在指数型的暴涨解.
关键词 宇宙学 暴涨 宇宙
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A Cosmological Model without Singularity Based on RW Metric (1)
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作者 Shihao Chen 《International Journal of Astronomy and Astrophysics》 2014年第1期264-293,共30页
A new conjecture is proposed that there are two sorts of matter called s-matter and v-matter which are symmetric, whose masses are positive, but whose gravitational masses are opposite to each other. Based on the conj... A new conjecture is proposed that there are two sorts of matter called s-matter and v-matter which are symmetric, whose masses are positive, but whose gravitational masses are opposite to each other. Based on the conjecture and the SUS(5) × SUV(5) gauge group, a cosmological model has been constructed and the following inferences have been derived. There are two sorts of symmetry breaking called V-breaking and S-breaking. In theV-breaking, SUV(5) breaks finally to SUV(3) × UV(1) so that v-particles get their masses and form v-atoms andv-galaxies etc., while SUS(5) still holds so that s-fermions and s-gauge bosons are massless and form SUS(5)color-singlets. There is no interaction among the SUS(5) color-singlets except gravitation so that they distribute loosely in space, cannot be observed, and cause space to expand with an acceleration. Evolution of the universe is explained. There is no space-time singularity. There are the highest temperature and the least scale in the universe. It is impossible that the Plank temperature and length are arrived. A formula is obtained which describes the relation between a luminous distance and its redshift. A huge void is not empty, and is equivalent to a huge concave lens. The densities of hydrogen in the huge voids must be much less than that predicted by the conventional theory. The gravitation between two galaxies whose distance is long enough will be less than that predicted by the conventional theory. A black hole with its big enough mass will transform into a white hole. 展开更多
关键词 cosmology: Theories (cosmology:) Early UNIVERSE (cosmology:) inflation (cosmology:) COSMOLOGICAL Parameters Galaxies: DISTANCES and Reshifts
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