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The new Minimal Standard Model

2004/05/12 by Hooman Davoudiasl, Ryuichiro Kitano, Tianjun Li +1 · 1 voice · 9 citations
Mathematics · Physics and Astronomy · #Astrophysics #Baryon #Baryon asymmetry #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark energy #Dark matter #Electroweak interaction #Gauge (firearms) #Inflation (cosmology) #Lambda-CDM model #Lepton #Mathematics #Minimal model #Neutrino #Nuclear physics #Particle physics #Particle physics theoretical and experimental studies #Physics #Physics beyond the Standard Model #Proton decay #Standard Model (mathematical formulation) #Theoretical physics #astro-ph #hep-ph #hep-th

paper · pdf · doi:10.1016/j.physletb.2005.01.026

published as Phys.Lett.B609:117-123,2005 · 5 pages, 2 figures. The discussions expanded with clarifications. The version accepted for publication in Phys. Lett. B

arxiv published 2004/05/12 · arxiv created 2005/01/13 · arxiv updated 2005/01/13 · openalex publication_date 2005/01/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

We construct the new Minimal Standard Model that incorporates the new discoveries of physics beyond the Minimal Standard Model (MSM): dark energy, non-baryonic dark matter, neutrino masses, as well as baryon asymmetry and cosmic inflation, adopting the principle of minimal particle content and the most general renormalizable Lagrangian. We base the model purely on empirical facts rather than aesthetics. We need only six new degrees of freedom beyond the MSM. It is free from excessive flavor-changing effects, CP violation, too-rapid proton decay, problems with electroweak precision data, and unwanted cosmological relics. Any model of physics beyond the MSM should be measured against the phenomenological success of this model.

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