1994/05/23 by Gordon Kane, G. L. Kane, Kane, G. L. +6
Mathematics · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Mathematical Approximation and Integration #astro-ph #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/9405364
talk given by LR at the 2nd IFT Workshop ``Yukawa Couplings and the Origin of Mass'', Gainesville, Florida, February 11--13, 1994; 7 pages of text in Latex plus 1 figure (included); University of Michigan preprint UM-TH-94-18 (April 1994)
arxiv created 1994/05/23 · openalex publication_date 1994/05/23 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
In the constrained MSSM one is typically able to restrict the supersymmetric mass spectra below roughly 1-2\tev \em without resorting to the ambiguous fine-tuning constraint.