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S. Valero,E. del Val,J. Alemany,V. Bottiunderstand the cosmic structure formation in the pre-virialized phase, or quasilinear règime. The emphasis is on the dynamical scaling of the multiresolution coarse-grained mass fields, which are traced by the multiscale identified clusters.丛林 发表于 2025-3-29 01:48:37
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https://doi.org/10.1007/978-94-010-0748-1Accretion; Cosmology; Dark matter; EFE; Gravity; Redshift; Renormalization group; Universe; astronomy; astrop博识 发表于 2025-3-29 09:47:30
978-0-7923-6856-4Kluwer Academic Publishers 2001Bravado 发表于 2025-3-29 13:21:20
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Structure Formation of Galaxy Clusters and Beyondunderstand the cosmic structure formation in the pre-virialized phase, or quasilinear règime. The emphasis is on the dynamical scaling of the multiresolution coarse-grained mass fields, which are traced by the multiscale identified clusters.平息 发表于 2025-3-29 22:00:34
Current Topics in Astrofundamental Physics: The Cosmic Microwave Background978-94-010-0748-1Series ISSN 1389-2185HALO 发表于 2025-3-30 00:43:49
S. Valero,E. del Val,J. Alemany,V. Bottiunderstand the cosmic structure formation in the pre-virialized phase, or quasilinear règime. The emphasis is on the dynamical scaling of the multiresolution coarse-grained mass fields, which are traced by the multiscale identified clusters.CHURL 发表于 2025-3-30 07:53:58
29th International Symposiumon Shock Waves 2There are many familiar situations when the properties of some substance change abruptly with temperature .. For example, a liquid may be converted into a vapor or into a solid state. Phase transitions are associated with non-analyticities of the partition function of the system.