Total Angular Momentum: Difference between revisions

Revision as of 21:53, 3 December 2023

Daniel O'Connor Fall 2023

The Main Idea

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

We can't have angular momentum without an axis

Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

A Mathematical Model

Single Particle Systems

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

[math]\displaystyle{ \vec{L} = \vec{r}\times\vec{p} }[/math]

Multiparticle Systems

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

[math]\displaystyle{ \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} }[/math]

Continuous Masses

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

[math]\displaystyle{ \vec{L} = I\vec{\omega} }[/math]

Here [math]\displaystyle{ I }[/math] is the rotational inertia of the object (For more info see Rotational Inertia) and [math]\displaystyle{ \omega }[/math] is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

A Computational Model

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

This screenshot shows the code in action but you can check it out with this link: https://trinket.io/glowscript/49129c12fd

Examples

These examples will help to solidify the difference between the different components of total angular momentum.

Simple

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

Middling

This example shows the importance of understanding the difference between rotational and translational angular momentum.

a) Calculate Lrot (both magnitude and direction)

b) Calculate Ltrans,B (both magnitude and direction)

c) Calculate Ltotal,B (both magnitude and direction)

Due to the fact that...

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

Difficult

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

a) Calculate Lrot (both magnitude and direction)

b) Calculate Ltrans,B (both magnitude and direction)

c) Calculate Ltotal,B (both magnitude and direction)

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

Computational Model for this problem

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

[math]\displaystyle{ \theta_{f} = \theta_{i} + \vec{w}\times \Delta t }[/math]

Now, the new position of the mass 1 is just

[math]\displaystyle{ \vec{r} = \lt d/2(cos(\theta), d/2sin(\theta), 0)\gt }[/math]

For Mass 2, it's the same but with an angle that is 180 degrees less than \theta.

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

Connectedness

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

History

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time." However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

Revision as of 21:52, 3 December 2023 (view source) DanOConnor (talk \| contribs) (→‎Computational Model for this problem) ← Older edit		Revision as of 21:53, 3 December 2023 (view source) DanOConnor (talk \| contribs) (→‎Computational Model for this problem) Newer edit →
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	:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>		:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

			For Mass 2, it's the same but with an angle that is 180 degrees less than \theta.

Total Angular Momentum: Difference between revisions

Revision as of 21:53, 3 December 2023

Contents

The Main Idea

We can't have angular momentum without an axis

A Mathematical Model

A Computational Model

Examples

Simple

Middling

Difficult

Computational Model for this problem

Connectedness

History

See also

Further reading

Video Content

External links

References

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