Mass scales in the RS models: the μ and cosmological constant

2001/03/07 by Jihn E. Kim, Kim, Jihn E.
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Noncommutative and Quantum Gravity Theories #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/0103071

8 pages including 3 eps figures. Talk presented at CICHEP, Cairo, Egypt, Jan. 9--13, 2001

arxiv created 2001/03/07 · openalex publication_date 2001/03/07 · arxiv updated 2009/11/30 · openalex created_date 2024/04/11 · openalex updated_date 2026/07/28

Abstract

There is the scale problem in the Randall-Sundrum models. Regarding this, I review the works done with B. S. Kyae and H. M. Lee. In a supersymmetric generalization in the RSI model, we discuss that the μ parameter can be obtained by an intermediate scale brane. In addition, we also discuss the cosmological constant problem with a self-tuning solution in the RSII model.

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