Anthropic principle favours the holographic dark energy

2004/10/31 by Qing-Guo Huang, Miao Li · 8 citations
Physics and Astronomy · #Anthropic principle #Astronomy #Astrophysics #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Galaxies: Formation, Evolution, Phenomena #Holography #Optics #Physics #Theoretical physics #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1088/1475-7516/2005/03/001

published as JCAP 0503 (2005) 001 · 10 Pages; added some clarificaions; Accepted for publicaion in JCAP

arxiv created 2005/03/01 · openalex publication_date 2005/03/10 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We discuss the anthropic principle when applied to holographic dark energy. We find that if the amplitude of the density fluctuation is variable, the holographic dark energy fares better than the cosmological constant. More generally, the anthropic predictions agree better with observation for dark energy with w Λ = p Λ /ρ Λ decreasing over time.

Citations

• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Universal upper bound on the entropy-to-energy ratio for bounded systems
• Black holes and thermodynamics
• Supernova constraints on a holographic dark energy model
• Anthropic Bound on the Cosmological Constant
• Entropy bounds and black hole remnants
• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results
• Generalized second law of thermodynamics in black-hole physics
• The world as a hologram
• Black Holes and Entropy

Cited by

• Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure
• Interacting Ricci dark energy with logarithmic correction
• Holographic dark energy with varying gravitational constant in Hořava-Lifshitz cosmology
• Revisit of cosmic age problem
• A modified holographic dark energy model with infrared infinite extra dimension(s)
• Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
• The three-loop Yang–Mills condensate dark energy model and its cosmological constraints
• Holographic dark energy in a cyclic universe