The ΛCDM model is also known as the standard model of cosmology, but is not related to theStandard Modelof particle physics. 9 参考 Maeder, Andre (2017). "An Alternative to the ΛCDM Model: The Case of Scale Invariance".The Astrophysical Journal.834(2): 194.arXiv:1701.03964.Bibcode:201...
Then, I discuss fundamental modifications of the Lambda-CDM model, through the inclusion of self-interacting dark matter (SIDM). I argue that a simple model of SIDM, with (warm) self-interacting right-handed neutrinos (RHN), that exist in minimal extensions of the Standard model of particle ...
Lambda-CDM-model网络冷暗物质模型 网络释义 1. 冷暗物质模型 ...r (FLRW) metric) ,可以导出 Λ-冷暗物质模型 (Lambda-CDM model),成为因与观测结果的精确吻合而被称为宇宙「标准模 …aeea.nmns.edu.tw|基于1 个网页您要找的是不是 linear model lambda calculus ...
LAMBDA-CDM_MODEL 主站 番剧 游戏中心 直播 会员购 漫画 赛事 下载客户端 登录 开通大会员 大会员 消息 动态 收藏 历史记录 创作中心 投稿 大母鹅 18 这个人懒死了,什么都没有写(￢д￢。) 关注发消息 主页动态投稿39合集和列表0收藏1追番追剧 关注数...
Reproducing the observed properties of disk galaxies thus appears to demand substantial revision to the currently most successful model of structure formation.doi:10.1086/308225Julio F. NavarroMatthias SteinmetzarXivAstrophysical JournalJ. F. Navarro and M. Steinmetz, [arXiv:astro-ph/9908114.]...
Cosmological free-free emission from dark matter halos in the ΛCDM modelKatsuya T. Abe ∗ and Hiroyuki TashiroDivision of Particle and Astrophysical Science, Graduate School of Science,Nagoya University, Chikusa, Nagoya 464-8602, JapanWe study the dif f use background free-free emission induced...
We show that OHD is not only able to play almost the same role in constraining cosmological parameters as SNe Ia does but also provides the effective measurement of the deviation of the DE models from standard \Lambda \Lambda CDM model. In the holographic and agegraphic scenarios, the ...
We find well-defined, real-valued analytical forms for the f(R) f(R) model to describe the universe both in the early epoch from the radiation to matter dominated eras and the late time acceleration period. We further examine the viability of the derived f(R) f(R) model and find that...
case of large bulk viscosity values, which is achieved for large negative values ofs, the presence of dark energy is not required to accelerate the expansion. This physical situation corresponds indeed to an unified dark fluid scenario, and it is another natural convergence of this viscous model....
This parameter-fixed $\Lambda$CDM is awarded distinguished status as separate model, "flat $\Lambda$CDM.'' Ipso facto this places the onus on proponents of "curved $\Lambda$CDM'' to present sufficient evidence that $\Omega_Keq0$, and is needed as a parameter. While certain inflationary ...