Speaker
Prof.
Elena Arbuzova
(Dubna State University and Novosibirsk State University)
Description
The model of vacuum energy compensation due to interaction of a nonlinear function of scalar field $\phi$ with curvature scalar is proposed. The form of the function $f(\phi)$ is adjusted to lead to the canonical cosmological evolution and to the observed value of dark energy.
| Тематическая секция | Гравитация и космология |
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Primary author
Prof.
Elena Arbuzova
(Dubna State University and Novosibirsk State University)
