Using semi-analytic approach, we present an estimate of the properties of the largest virialized dark halos in the present universe for three different scenarios of structure formation: SCDM, ACDM and OCDM models. The resulting virial mass and temperature increase from the lowest values of 1.6 x 10(15)h(-1)M(circle dot) and 9.8 keV,in OCDM, the mid-range values of 9.0 x 10(15)h(-1)M(circle dot) and 31 keV in LambdaCDM, to the highest values of 20.9 x 10(15)h(-1)M(circle dot), 65 keV in SCDM. As compared with the largest virialized object seen in the universe, the richest clusters of galaxies, we can safely rule out the OCDM model. In addition, the SCDM model is very unlikely because of the unreasonably high virial mass and temperature. Our computation favors the prevailing ACDM model in which superclusters may be marginally regarded as dynamically-virialized systems. [References: 18]
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机译：使用半解析方法，我们针对三种不同的结构形成场景：SCDM，ACDM和OCDM模型，对当前宇宙中最大的虚拟暗光晕的性质进行了估算。所得的病毒质量和温度从OCDM中的最低值1.6 x 10（15）h（-1）M（圆点）和9.8 keV开始增加，中间值是9.0 x 10（15）h（- LambdaCDM中的1）M（圆点）和31 keV，在SCDM中最高值为20.9 x 10（15）h（-1）M（圆点），65 keV。与宇宙中最大的病毒化物体（最丰富的星系团）相比，我们可以安全地排除OCDM模型。另外，由于过高的病毒质量和温度，SCDM模型非常不可能。我们的计算偏向盛行的ACDM模型，在该模型中，超级集群可能被视为动态虚拟化系统。 [参考：18]
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