New agegraphic dark energy model with generalized uncertainty principle

Abstract

We investigate the new agegraphic dark energy models with generalized uncertainty principle (GUP). It turns out that although the GUP affects the early universe, it does not change the current and future dark energy-dominated universe significantly. Furthermore, this model could describe the matter-dominated universe in the past only when the parameter $n$ is chosen to be $n>n_c$, where the critical value determined to be $n_c=2.799531478$.

9 pages, 1 figure, version to appear in MPLA

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Cited by in corpus (5)

• Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
• Interacting agegraphic dark energy models in non-flat universe
• Entropy-Corrected Holographic Dark Energy
• Origin of holographic dark energy models
• Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future