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 ...
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...
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 ...
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As an extension of the above model [11], we consider the inclusion of the radiation, baryons, and dark matter: h(φ) = h i +h f qφ 2 1 +qφ 2 , (18) Modified gravity as an alternative for Lambda-CDM cosmology 5
Mpc ΛCDM hy- drodynamic simulation with 10h −1 kpc resolution. The mass correlation function grows with time, but the galaxy correlation function shows little evolution and is well described by a power law. At early times, galaxies
Abstract Bulk viscosity in cold dark matter is an appealing feature that introduces distinctive phenomenological effects in the cosmological setting as compared to theCDM model. Under this view, we propose a general parametrization of the bulk viscosity of the formξ∼H1−2sρms, Some advantages...
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I find bounds on the Brans–Dicke coupling constant \\\(\\\omega _extsc {bd}\\\), which are consistent with well-known results.doi:10.1007/978-3-319-31299-6_7Israel QuirosSpringer International Publishing