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ISSN 2753-3239
CCC: 1
PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON RAILWAY TECHNOLOGY: RESEARCH, DEVELOPMENT AND MAINTENANCE
Edited by: J. Pombo
Paper 12.1

Reduced Models of Railway Track: Critical Velocity and Instability of Moving Inertial Objects

Z. Dimitrovová1,2

1Department of Civil Engineering, NOVA School of Science and Technology, NOVA University of Lisbon, Caparica, Portugal
2IDMEC, Instituto Superior Técnico, Universidade de Lisboa, Lisboa, Portugal

Full Bibliographic Reference for this paper
Z. Dimitrovová, "Reduced Models of Railway Track: Critical Velocity and Instability of Moving Inertial Objects", in J. Pombo, (Editor), "Proceedings of the Fifth International Conference on Railway Technology: Research, Development and Maintenance", Civil-Comp Press, Edinburgh, UK, Online volume: CCC 1, Paper 12.1, 2022, doi:10.4203/ccc.1.12.1
Keywords: moving proximate masses, dynamic interaction, contour integration, semianalytical solution, critical velocity, instability.

Abstract
In this contribution, a new form of semianalytical results related to inertial objects that are traversing homogeneous infinite structures, introduced in previous author’s work, is used to analyse one-, two- and three-layer models of the railway track. The aim of these analyses is determination of the critical velocity of a moving force and of the onset of instability of moving masses or oscillators. First of all, the possible range of dimensional parameters is identified. Within these ranges, there are significant differences between the models. While for the one- and two- layer models the critical velocities are well-defined and their number is 1 or 3, respectively, in the three-layer model their number depends on parameter values and can be 1, 3 or 5. Regarding the onset of instability, there are also significant differences, not only between the models but also between the cases with one or more moving masses or oscillators. For one-layer model, which is in fact the model of an infinite beam on the classical Winkler-Pasternak foundation, instability of one moving mass has regular behaviour and occurs always in the supercritical velocity range when damping is present and at the critical velocity in case of no damping. Two moving proximate masses already introduce severe alterations, because in damped case the dynamic interaction can shift the onset of instability deeply into the subcritical velocity range. The other models introduce other irregularities, even for one moving mass. This contribution will summarize all the differences and common features that exist between these models and within the full range of possible parameter combinations.

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