Titlebook: Cosmological Pattern of Microphysics in the Inflationary Universe; Maxim Yu. Khlopov,Sergei G. Rubin Book 2004 Springer Science+Business M

国家明智

978-90-481-6695-4Springer Science+Business Media Dordrecht 2004

dialect

chondromalacia

Strong Primordial Inhomogeneities and Galaxy Formation,rav­itational instability from small initial perturbations of density or gravitational potential. As a rule, these perturbations are Gaussian, but some versions of non-Gaussian perturbations are also discussed.

合乎习俗

DRAFT

Maxim Yu. Khlopov,Sergei G. RubinAn introduction into the inflationary scenario of, and the crucial role of quantum fluctuations in the evolution of the Universe - clarifying the interactions between different cosmological phenomena

容易懂得

Fundamental Theories of Physicshttp://image.papertrans.cn/c/image/238920.jpg

观点

Cosmological Pattern of Microphysics in the Inflationary Universe978-1-4020-2650-8Series ISSN 0168-1222 Series E-ISSN 2365-6425

迅速成长

言外之意

Tremor

https://doi.org/10.1007/978-3-322-80645-1 a very interesting and important period of the evolution of our Universe. A lot of observational data can find new nontrivial explanation in this framework. In addition, new phenomena are predicted, some of them having been discussed in this book.