A Dark Energy Hypothesis V  

作　　者：James Togeas James Togeas(University of Minnesota, Morris Campus, Morris, USA)

机构地区：[1]University of Minnesota, Morris Campus, Morris, USA

出　　处：《Journal of High Energy Physics, Gravitation and Cosmology》2025年第1期56-60,共5页高能物理(英文)

摘　　要：The subject is the mass of the three dominant, equilibrium cosmological objects: the irregular galaxy (dwarf), the regular galaxy (Hubble’s “tuning fork”), and the galactic cluster. The standard ΛCDM theory and a DEH offer contrasting views on the origin of these masses. The latter suggests that they are relics of the early universe.The subject is the mass of the three dominant, equilibrium cosmological objects: the irregular galaxy (dwarf), the regular galaxy (Hubble’s “tuning fork”), and the galactic cluster. The standard ΛCDM theory and a DEH offer contrasting views on the origin of these masses. The latter suggests that they are relics of the early universe.

关 键 词：Cosmic Structure IRREGULAR Regular Galaxies Galactic Clusters 

分 类 号：P15[天文地球—天文学]