eifueo/docs/ce1/ece105.md
2022-11-02 22:56:14 -04:00

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ECE 105: Classical Mechanics

Motion

Please see SL Physics 1#2.1 - Motion for more information.

Kinematics

Please see SL Physics 1#Kinematic equations for more information.

Projectile motion

Please see SL Physics 1#Projectile motion for more information.

Uniform circular motion

Please see SL Physics 1#6.1 - Circular motion for more information.

Forces

Please see SL Physics 1#2.2 - Forces for more information.

Work

Please see SL Physics 1#2.3 - Work, energy, and power for more information.

Momentum and impulse

Please see SL Physics 1#2.4 - Momentum and impulse for more information.

The change of momentum with respect to time is equal to the average force so long as mass is constant.

\[\frac{dp}{dt} = \frac{mdv}{dt} + \frac{vdm}{dt}\]

Impulse is actually the change of momentum over time.

\[\vec J = \int^{p_f}_{p_i}d\vec p\]

Centre of mass

The centre of mass \(x\) of a system is equal to the average of the centre of masses of its components relative to a defined origin.

\[x_{cm} = \frac{m_1x_1 + m_2x_2 + ... + m_nx_n}{m_1 + m_2 + ... + m_n}\]

To determine the centre of mass of a system with a hole, the hole should be treated as negative mass. If the geometry of the system is symmetrical, the centre of mass is also symmetrical in the x and y dimensions.

For each mass, its surface density \(\sigma\) is equal to:

\[ \sigma = \frac{m}{A} \\ m = \sigma A \]

Holes have negative mass, i.e., \(m = -\sigma A\).

For a one-dimensional hole, the linear mass density uses a similar formula:

\[ \lambda =\frac{m}{L} \\ \lambda = \frac{dm}{dx} \]

This means that a hole in a rod can use a different formula: \[x_{cm} = \frac{1}{M}\int^M_0 xdm\]