Intrinsic problems of the gravitational baryogenesis

E. V. Arbuzova, A. D. Dolgov

Результат исследования: Научные публикации в периодических изданияхстатьярецензирование

11 Цитирования (Scopus)


Modification of gravity due to the curvature dependent term in the gravitational baryogenesis scenario is considered. It is shown that this term leads to the fourth order differential equation of motion for the curvature scalar instead of the algebraic one of General Relativity (GR). The fourth order gravitational equations are generically unstable with respect to small perturbations. Non-linear in curvature terms may stabilize the solution but the magnitude of the stabilized curvature scalar would be much larger than that dictated by GR, so the standard cosmology would be strongly distorted.

Язык оригиналаанглийский
Страницы (с-по)171-175
Число страниц5
ЖурналPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
СостояниеОпубликовано - 10 июн 2017


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