Running of the spectral index in deformed matter bounce scenarios with Hubble-rate-dependent dark energy

Abstract As a deformed matter bounce scenario with a dark energy component, we propose a deformed one with running vacuum model (RVM) in which the dark energy density $$\rho _{\Lambda }$$ ρΛ is written as a power series of $$H^2$$ H2 and $$\dot{H}$$ H˙ with a constant equation of state parameter, sa...

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Bibliographic Details
Main Authors: M. Arab, A. Khodam-Mohammadi
Format: Article
Language:English
Published: SpringerOpen 2018-03-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-5733-0