Problem 5
Question
Write down the kinetic energy of a particle in cylindrical polar coordinates in a frame rotating with angular velocity \(\omega\) about the \(z\)-axis. Show that the terms proportional to \(\omega\) and \(\omega^{2}\) reproduce the Coriolis force and centrifugal force respectively.
Step-by-Step Solution
Verified Answer
Question: Derive the kinetic energy of a particle in a frame rotating with angular velocity \(\omega\) about the \(z\)-axis using cylindrical polar coordinates, and identify the terms proportional to \(\omega\) and \(\omega^2\). Explain how they correspond to the Coriolis force and the centrifugal force, respectively.
Answer: In cylindrical polar coordinates, the kinetic energy (T) of a particle in a rotating frame is given by \(T = \frac{1}{2}m \left[\left(\frac{d\rho}{dt}\right)^2 + \rho^2\omega^2 + \left(\frac{dz}{dt}\right)^2\right]\). The term proportional to \(\omega^2\) is the centrifugal force, which represents the effective force acting radially outward and is given by \(F_\text{centrifugal} = -m\rho\omega^2\hat{\rho}\). Since there are no terms proportional to \(\omega\) in the expression for kinetic energy, we can infer that the Coriolis force, given by \(F_\text{Coriolis} = -2m(\vec{v} \times \vec{\omega})\), doesn't directly contribute to the kinetic energy expression and is responsible for changing the direction of the particle's velocity within a rotating frame.
1Step 1: 1. Position vector in cylindrical polar coordinates
In cylindrical polar coordinates, the position vector \(\vec{r}\) of a particle can be written as:
\(\vec{r} = \rho \hat{\rho} + z\hat{z}\), where \(\rho\) represents the distance from the \(z\)-axis, and \(z\) represents the distance along the \(z\)-axis.
2Step 2: 2. Velocity vector in cylindrical polar coordinates
To obtain the velocity vector \(\vec{v}\) of the particle, we need to differentiate the position vector with respect to time, considering the frame is rotating with angular velocity \(\omega\) about the \(z\)-axis.
\(\vec{v} = \frac{d\vec{r}}{dt} = \frac{d\rho}{dt}\hat{\rho} + \rho\frac{d\hat{\rho}}{dt} + \frac{dz}{dt}\hat{z} + z\frac{d\hat{z}}{dt}\).
Noting that \(\frac{d\hat{\rho}}{dt} = \omega\hat{\phi}\) and \(\frac{d\hat{z}}{dt} = 0\), we get:
\(\vec{v} = \frac{d\rho}{dt}\hat{\rho} + \rho\omega\hat{\phi} + \frac{dz}{dt}\hat{z}\).
3Step 3: 3. Kinetic energy in cylindrical polar coordinates
The kinetic energy \(T\) of the particle can be written as:
\(T = \frac{1}{2}m \vec{v} \cdot \vec{v}\), where \(m\) is the mass of the particle.
Now, substitute the expression for \(\vec{v}\) from step 2 and calculate the dot product:
\(T = \frac{1}{2}m \left[\left(\frac{d\rho}{dt}\right)^2 + \rho^2\omega^2 + \left(\frac{dz}{dt}\right)^2\right]\).
4Step 4: 4. Identify terms proportional to \(\omega\) and \(\omega^2\)
In the expression for the kinetic energy, we can identify the terms proportional to \(\omega\) and \(\omega^2\):
Terms proportional to \(\omega\): \(\frac{1}{2}m\rho^2\omega^2\).
As for terms proportional to \(\omega\), there are none in the expression.
5Step 5: 5. Coriolis and centrifugal forces
The term proportional to \(\omega^2\) is the centrifugal force, which represents the effective force that acts on a particle within a rotating frame. This force points radially outward and is given by:
\(F_\text{centrifugal} = -m\rho\omega^2\hat{\rho}\).
Since there are no terms proportional to \(\omega\) in the expression for kinetic energy, we can also infer that the Coriolis force, given by:
\(F_\text{Coriolis} = -2m(\vec{v} \times \vec{\omega})\),
doesn't directly contribute to the kinetic energy expression. The Coriolis force is responsible for changing the direction of the particle's velocity within a rotating frame without causing a change in the scalar magnitude of the velocity.
Key Concepts
Rotating Reference FrameCoriolis ForceCentrifugal ForceAngular Velocity
Rotating Reference Frame
A rotating reference frame is a viewpoint that moves with a rotating system, providing a unique perspective on the dynamics of particles or bodies within. Imagine you're on a merry-go-round; to you, the world outside seems to be revolving. This is analogous to what happens in a rotating reference frame.
In physics, when we analyze the motion of an object from such a frame, we must account for fictitious forces—forces that appear to exist from the frame's viewpoint, but aren't experienced by an observer in an inertial (non-accelerating) frame. When we calculate kinetic energy within this frame, like in our exercise, it's crucial to consider these forces to understand the object's motion accurately.
In physics, when we analyze the motion of an object from such a frame, we must account for fictitious forces—forces that appear to exist from the frame's viewpoint, but aren't experienced by an observer in an inertial (non-accelerating) frame. When we calculate kinetic energy within this frame, like in our exercise, it's crucial to consider these forces to understand the object's motion accurately.
Coriolis Force
The Coriolis force emerges when dealing with objects in motion within a rotating reference frame. It's a fictitious force that acts perpendicular to the direction of motion and the axis of rotation. This force is essential for explaining phenomena like the deflection of winds on Earth.
For example, as air moves high above the Earth's surface, the planet rotates beneath it, causing the path of the wind to curve—a principle critical for meteorology. While it doesn't show up directly in the expression of kinetic energy, the Coriolis force affects an object's trajectory and must be factored in when predicting its path in rotating systems.
For example, as air moves high above the Earth's surface, the planet rotates beneath it, causing the path of the wind to curve—a principle critical for meteorology. While it doesn't show up directly in the expression of kinetic energy, the Coriolis force affects an object's trajectory and must be factored in when predicting its path in rotating systems.
Centrifugal Force
Centrifugal force is another fictitious force felt in a rotating reference frame. It appears to act radially outward on a body in motion, away from the center of rotation. You've perhaps experienced it while taking a sharp turn in a car; you're pushed against the door, as if a force is pulling you outwards.
This force is represented by the term with \(\omega^2\) in the kinetic energy expression from our problem. As an object spins with the frame, it feels as though it's being flung outward, which is captured by this term in the energy equation. It's important to note that this force is not real in the sense that it doesn't arise from any physical interaction—it's simply a consequence of analyzing motion in a non-inertial frame.
This force is represented by the term with \(\omega^2\) in the kinetic energy expression from our problem. As an object spins with the frame, it feels as though it's being flung outward, which is captured by this term in the energy equation. It's important to note that this force is not real in the sense that it doesn't arise from any physical interaction—it's simply a consequence of analyzing motion in a non-inertial frame.
Angular Velocity
Angular velocity, denoted by \(\omega\), measures how fast something spins or rotates. It is a vector quantity, indicating the rate of rotation as well as the axis about which the rotation occurs. If you're looking at a clock, the angular velocity of the second hand is constant, describing how many radians it sweeps per second.
In our context, the angular velocity defines how quickly our reference frame is rotating, particularly around the z-axis. It plays a pivotal role in determining both the centrifugal and Coriolis forces and thus directly affects the kinetic energy of particles within the rotating frame.
In our context, the angular velocity defines how quickly our reference frame is rotating, particularly around the z-axis. It plays a pivotal role in determining both the centrifugal and Coriolis forces and thus directly affects the kinetic energy of particles within the rotating frame.
Other exercises in this chapter
Problem 1
Masses \(m\) and \(2 m\) are joined by a light inextensible string which runs without slipping over a uniform circular pulley of mass \(2 m\) and radius \(a\).
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A light inextensible string passes over a light smooth pulley, and carries a mass \(4 m\) on one end. The other end supports a second pulley with a string over
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A simple pendulum of mass \(m\) and length \(l\) hangs from a trolley of mass \(M\) running on smooth horizontal rails. The pendulum swings in a plane parallel
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