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Smoothly evolving supercritical-string dark energy relaxes supersymmetric-dark-matter constraints

2006/12/31 by A. B. Lahanas, A.B. Lahanas, Nick E. Mavromatos +3 · 2 citations
Physics and Astronomy · #Astrophysics #CMB cold spot #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark fluid #Dark matter #Dilaton #Parameter space #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum gravity #Quantum mechanics #String (physics) #String cosmology #Supercritical fluid #Supersymmetry #Theoretical physics #astro-ph #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1016/j.physletb.2007.03.058

published as Phys.Lett.B649:83-90,2007 · 13 pages revtex, 5 eps figures incorporated. Version to appear in Physics Lett. B, no effects on conclusions

openalex publication_date 2007/04/07 · arxiv created 2007/04/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We show that Supercritical-String-Cosmology (SSC) off-equilibrium and time-dependent-dilaton effects lead to a smoothly evolving dark energy for the last 10 billion years in concordance with all presently available astrophysical data. Such effects dilute by a factor O ( 10 ) the supersymmetric dark matter density (neutralinos), relaxing severe WMAP 1, 3 constraints on the SUSY parameter space. Thus, LHC anticipated searches/discoveries may discriminate between conventional and supercritical-string cosmology.

Citations

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