On the Numerical Influences of Inertia Representation for Rigid Body Dynamics in Terms of Unit Quaternion

2016 ◽  
Vol 83 (6) ◽  
Author(s):  
Xiaoming Xu ◽  
Wanxie Zhong

Inertia plays a crucial role in the quaternion-based rigid body dynamics, the associated mass matrix, however, presents singularity in the traditional representation. Recent researches demonstrated that the singularity can be avoided by adding an extra term into kinetic energy via a multiplier. Here, we propose a modified inertia representation through splitting the kinetic energy into two parts, where a square term of quaternion velocity, governed by an extra inertial parameter, is separated from the original expression. We further derive new numerical integration schemes in both Lagrange and Hamilton framework. Error estimation shows that the extra inertial parameter has a significant influence on the numerical error in discretization, and an iterative scheme of optimizing the extra inertial parameter to reduce the numerical error in simulation is proposed for quaternion-based rigid body dynamics. Numerical results demonstrate that the mean value of the three principal moments of inertia is a reasonable value of the extra inertia parameter which can impressively improve the accuracy in most cases, and the iterative scheme can further reduce the numerical error for numerical integration, taking the implementation in Lagrange's frame as an example.

PAMM ◽  
2008 ◽  
Vol 8 (1) ◽  
pp. 10139-10140 ◽  
Author(s):  
Ralf Siebert ◽  
Peter Betsch

1991 ◽  
Vol 58 (3) ◽  
pp. 754-758 ◽  
Author(s):  
Charles E. Smith

The observation by Thomas Kane a few years ago, that long-used relationships for predicting post-collision motion of a system of rigid bodies can imply a significant increase in kinetic energy during collision, has revived interest in this type of problem. This paper is intended to clarify understanding of the sources of this difficulty, and to suggest an alternative to some of the previously used assumptions for making such predictions. An organization of the pertinent equations of kinetics is presented, which provides a more direct means of examining the aforementioned question and of obtaining rebound predictions.


Author(s):  
Mate Antali ◽  
Gabor Stepan

AbstractIn this paper, the general kinematics and dynamics of a rigid body is analysed, which is in contact with two rigid surfaces in the presence of dry friction. Due to the rolling or slipping state at each contact point, four kinematic scenarios occur. In the two-point rolling case, the contact forces are undetermined; consequently, the condition of the static friction forces cannot be checked from the Coulomb model to decide whether two-point rolling is possible. However, this issue can be resolved within the scope of rigid body dynamics by analysing the nonsmooth vector field of the system at the possible transitions between slipping and rolling. Based on the concept of limit directions of codimension-2 discontinuities, a method is presented to determine the conditions when the two-point rolling is realizable without slipping.


2015 ◽  
Vol 69 ◽  
pp. 40-44
Author(s):  
H.M. Yehia ◽  
E. Saleh ◽  
S.F. Megahid

2014 ◽  
Vol 10 (2) ◽  
pp. e1003456 ◽  
Author(s):  
Pascal Carrivain ◽  
Maria Barbi ◽  
Jean-Marc Victor

1986 ◽  
Vol 54 (7) ◽  
pp. 585-586
Author(s):  
Stephen F. Felszeghy

2020 ◽  
Vol 30 (6) ◽  
pp. 3199-3233 ◽  
Author(s):  
Cristian Guillermo Gebhardt ◽  
Ignacio Romero

Abstract This work proposes and investigates a new model of the rotating rigid body based on the non-twisting frame. Such a frame consists of three mutually orthogonal unit vectors whose rotation rate around one of the three axis remains zero at all times and, thus, is represented by a nonholonomic restriction. Then, the corresponding Lagrange–D’Alembert equations are formulated by employing two descriptions, the first one relying on rotations and a splitting approach, and the second one relying on constrained directors. For vanishing external moments, we prove that the new model possesses conservation laws, i.e., the kinetic energy and two nonholonomic momenta that substantially differ from the holonomic momenta preserved by the standard rigid body model. Additionally, we propose a new specialization of a class of energy–momentum integration schemes that exactly preserves the kinetic energy and the nonholonomic momenta replicating the continuous counterpart. Finally, we present numerical results that show the excellent conservation properties as well as the accuracy for the time-discretized governing equations.


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