\({\boldsymbol{a}\text{(}t\text{)}_{j}}\) is the j-th body’s acceleration (\(\frac{\text{m}}{\text{s}^{2}}\))
\(\boldsymbol{g}\) is the gravitational acceleration (\(\frac{\text{m}}{\text{s}^{2}}\))
\({\boldsymbol{F}_{j}}\) is the force applied to the j-th body at time t (\({\text{N}}\))
\(t\) is the time (\({\text{s}}\))
\({m_{j}}\) is the mass of the j-th particle (\({\text{kg}}\))
Notes
The above equation expresses the total acceleration of the rigid body \(j\) as the sum of gravitational acceleration (from GD:accelGravity) and acceleration due to applied force \({\boldsymbol{F}_{j}}\left(t\right)\) (from TM:NewtonSecLawMot). The resultant outputs are then obtained from this equation using DD:linDisp, DD:linVel, and DD:linAcc.
The output of the instance model will be the functions of position and velocity over time that satisfy the ODE for the acceleration, with the given initial conditions for position and velocity. The motion is translational, so the position and velocity functions are for the centre of mass (from DD:ctrOfMass).
\({α_{j}}\) is the j-th body’s angular acceleration (\(\frac{\text{rad}}{\text{s}^{2}}\))
\({\boldsymbol{τ}_{j}}\) is the torque applied to the j-th body (\(\text{N}\text{m}\))
\(t\) is the time (\({\text{s}}\))
\(\boldsymbol{I}\) is the moment of inertia (\(\text{kg}\text{m}^{2}\))
Notes
The above equation for the total angular acceleration of the rigid body \(j\) is derived from TM:NewtonSecLawRotMot, and the resultant outputs are then obtained from this equation using DD:angDisp, DD:angVel, and DD:angAccel.
We may calculate the total angular acceleration of rigid body \(j\) by calculating the derivative of its angular velocity with respect to time (from DD:angAccel).
\({\boldsymbol{v}\text{(}t\text{)}_{\text{A}}}\) is the velocity at point A (\(\frac{\text{m}}{\text{s}}\))
\({t_{\text{c}}}\) is the denotes the time at collision (\({\text{s}}\))
\(t\) is the time (\({\text{s}}\))
\(j\) is the impulse (scalar) (\(\text{N}\text{s}\))
\({m_{\text{A}}}\) is the mass of rigid body A (\({\text{kg}}\))
\(\boldsymbol{n}\) is the collision normal vector (\({\text{m}}\))
Notes
The output of the instance model will be the functions of position, velocity, orientation, and angular acceleration over time that satisfy the equations for the velocity and angular acceleration, with the given initial conditions for position, velocity, orientation, and angular acceleration. The motion is translational, so the position, velocity, orientation, and angular acceleration functions are for the centre of mass (from DD:ctrOfMass).