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Equilibrium

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Equilibrium

An object is in equilibrium if the linear momentum of its center of mass is constant and if its angular momentum about its center of mass is constant: P = constant L = constant An object is in static equilibrium if its linear momentum and angular momentum is equal to zero: P = 0 kg m/s L = 0 kg m2/s

Conditions For Equilibrium


We say that a rigid body is in equilibrium when both its linear and angular acceleration are zero relative to an inertial frame of reference.
This means that a body in equilibrium can be moving, but if so, its linear and angular velocities must be constant.
We say that a rigid body is in static equilibrium when it is at rest in our selected frame of reference.
Notice that the distinction between the state of rest and a state of uniform motion is artificial—that is, an object may be at rest in our selected frame of reference, yet to an observer moving at constant velocity relative to our frame, the same object appears to be in uniform motion with constant velocity.
Because the motion is relative, what is in static equilibrium to us is in dynamic equilibrium to the moving observer, and vice versa.
Since the laws of physics are identical for all inertial reference frames, in an inertial frame of reference, there is no distinction between static equilibrium and equilibrium.


According to Newton’s second law of motion, the linear acceleration of a rigid body is caused by a net force acting on it, or


Here, the sum is of all external forces acting on the body, where m is its mass and  a  is the linear acceleration of its center of mass (a concept we discussed in Linear Momentum and Collisions on linear momentum and collisions).
In equilibrium, the linear acceleration is zero. If we set the acceleration to zero in Equation 12.1, we obtain the following equation:




The first equilibrium condition, Equation 12.2, is the equilibrium condition for forces, which we encountered when studying applications of Newton’s laws.


This vector equation is equivalent to the following three scalar equations for the components of the net force:



Second Equilibrium Condition


Analogously to Equation 12.1,
we can state that the rotational acceleration α of a rigid body about a fixed axis of rotation is caused by the net torque acting on the body, or

∑kτ = k=Iα . (12.4)

Here  I  is the rotational inertia of the body in rotation about this axis and the summation is over all torques  τ⃗ k  of external forces in Equation 12.2.

In equilibrium, the rotational acceleration is zero. By setting to zero the right-hand side of Equation 12.4, we obtain the second equilibrium condition:




The second equilibrium condition, Equation 12.5, is the equilibrium condition for torques that we encountered when we studied rotational dynamics.
It is worth noting that this equation for equilibrium is generally valid for rotational equilibrium about any axis of rotation (fixed or otherwise).
Again, this vector equation is equivalent to three scalar equations for the vector components of the net torque:




The second equilibrium condition means that in equilibrium, there is no net external torque to cause rotation about any axis.






Lami’s Theorem

It states if  a particle acted upon by 3 forces remains in equilibrium then each force acting upon the particle bears the same proportionality with the sine of the angle between the other 2 forces.”
So, this law is also called law of sines.




Torque due to Couple


  • A Couple is system of forces that consists of 2 parallel forces that has equal magnitude, oppositely directed and do not act in a straight line but are separated by a perpendicular distance.

  • Couple does not produce any translational but rotational motion.

  • The resultant force of a couple is zero but the resultant moment is not zero.


Principle of Moment


The turning effect of a single force depends not just on the magnitude of force and its direction, it also depends on the distance from the point of application of force to the point about which turning would take place.

The moment of a force about a given axis is the measure of the turning effect of force and is mathematically defined as


   Moment of Force = Force * perpendicular distance from the axis of rotation to the point of application of force.


Principle of Moment states that “if the masses or the distances of masses from axis of rotation are adjusted so as to keep the scale in horizontal position, the scale in horizontal position, the scale is said to be in equilibrium.”


Thus, if a body is in rotational equilibrium, under the action of different forces, the sum of clockwise moments must be equal to sum of anticlockwise moments.
This is known as principle of moments.

        W1r1 = W2r2

  or,  m1gr1 = m2gr2

  or,  m1r1 = m2r2