General relativity and the standard model in scale-invariant variables

General Relativity and Standard Model are formulated in terms of scale-invariant variables where the initial data are integrals of motion. In this case, the Hubble law can be explained by a cosmological evolution of particle masses. Supernovae type Ia data and the CMB energy budget in the model are in agreement with the dominance of a scalar field kinetic energy density and an intensive cosmological creation of primordialW, Z, and Higgs bosons from vacuum. Some arguments are discussed testifying to that two-photon processes of primordial particle annihilation and decays form three peaks in the CMB power spectrum, and their values and positions ℓ = 220, 546, 800 are in agreement with the QED coupling constant, Weinberg's angle, and the Higgs particle mass of about 118 GeV. © Pleiades Publishing, Ltd., 2009.

Авторы
Arbuzov A.B.1 , Barbashov B.M.1 , Borowiec A.2 , Pervushin V.N.1 , Shuvalov S.A. 3 , Zakharov A.F.4
Номер выпуска
3
Язык
Английский
Страницы
199-212
Статус
Опубликовано
Том
15
Год
2009
Организации
  • 1 Bogoliubov Laboratory of Theoretical Physics, JINR, Joliot-Curie ul. 6, Dubna 141980, Russian Federation
  • 2 Institute of Theoretical Physics, University of Wrocław, Wrocław, Poland
  • 3 Peoples' Friendship University of Russia, Miklukho-Maklay ul. 6, Moscow 117198, Russian Federation
  • 4 Institute of Theoretical and Experimental Physics, B. Cheryomushkinskaya ul. 25, Moscow 117259, Russian Federation
Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/2940/
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