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Rotational Stability of Linear String Baryon Configuration

1998/12/30 by Valery Petrov, V. P. Petrov, Petrov, V. P. +2
Engineering · Physics and Astronomy · #FOS: Physical sciences #Geotechnical and Geomechanical Engineering #High Energy Physics - Phenomenology (hep-ph) #Pulsars and Gravitational Waves Research #Superconducting Materials and Applications #hep-ph

paper · pdf · doi:10.48550/arxiv.hep-ph/9812527

13 pages, 1 figure, LaTeX

arxiv created 1998/12/30 · openalex publication_date 1998/12/30 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

For the linear baryon string model with three massive points (three quarks) connected sequentially by the relativistic strings the initial-boundary value problem is stated and solved in general. This problem implies defining a classical motion of the system on the base of given initial position and initial velocities of string points. The given solution work reduces the initial-boundary value problem for the considered model to the system of ordinary differential equations that can be integrated numerically in general. The examples of numerical simulation of the system motion are considered, which, in particular, allow to answer to the old question about stability of a flat uniform rotation of the linear string configuration.

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