Explaining Central Force of inverse r^3

In summary, the central force of inverse r^3 is a type of force that is inversely proportional to the cube of the distance between two objects. It is caused by the interaction between two objects with mass and is a direct consequence of Newton's law of universal gravitation. Examples of this force can be seen in the gravitational force between the Earth and the Moon and the electrostatic force between an electron and a proton in an atom. This force is different from other central forces, such as the central force of inverse r^2, in terms of its strength and how it varies with distance.
  • #1
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Homework Statement



Consider the central force F=-k/(r^3) u(hat in r direction). This is an attractive force. For various values of k, explain what the orbit of a particle about a force center looks like.

Homework Equations



Included within question.

The Attempt at a Solution



I am not quite sure where to begin. I know this is like modelling the tidal force separate of gravitation, or I think so. Looking for a starting point if anyone can help. (This is for a classical dynamics course.)
 
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Hello, thank you for your post! The central force F=-k/(r^3) u(hat in r direction) is a type of inverse-square force, which means that the strength of the force decreases with the square of the distance from the force center. In this case, the force is also attractive, meaning that it pulls objects towards the force center.

The value of k determines the strength of the force. If k is small, then the force will be weak and the orbit of a particle will be close to a circular shape around the force center. As k increases, the force becomes stronger and the orbit becomes more elliptical.

When k reaches a critical value, the orbit becomes a parabola, meaning that the particle will approach the force center once and then escape. This is known as a parabolic orbit.

If k continues to increase, the orbit becomes a hyperbola, meaning that the particle will approach the force center twice and then escape to infinity. This is known as a hyperbolic orbit.

In summary, for smaller values of k, the orbit will be more circular, and as k increases, the orbit becomes more elliptical, parabolic, and finally hyperbolic. This behavior can be seen in many real-world systems, such as the orbits of planets around the sun.

I hope this helps to answer your question and provide a starting point for your solution. If you have any further questions, please don't hesitate to ask. Good luck with your classical dynamics course!
 

Related to Explaining Central Force of inverse r^3

What is the central force of inverse r^3?

The central force of inverse r^3 is a type of force that is inversely proportional to the cube of the distance between two objects. It is a central force because it acts in a radial direction towards or away from the center of the objects.

What causes the central force of inverse r^3?

The central force of inverse r^3 is caused by the interaction between two objects with mass. This force is a result of the gravitational or electrostatic forces between the objects, depending on the context in which it is being studied.

How is the central force of inverse r^3 related to Newton's law of universal gravitation?

The central force of inverse r^3 is a direct consequence of Newton's law of universal gravitation. According to this law, the force of gravity between two objects is proportional to the product of their masses and inversely proportional to the square of the distance between them.

What are some examples of central force of inverse r^3 in nature?

One example of the central force of inverse r^3 is the gravitational force between the Earth and the Moon. Another example is the electrostatic force between an electron and a proton in an atom. These forces follow an inverse square law, which can be transformed into an inverse r^3 law by considering the objects as point masses.

How is the central force of inverse r^3 different from other central forces?

The central force of inverse r^3 is different from other central forces, such as the central force of inverse r^2, in terms of its strength and how it varies with distance. The force of inverse r^3 decreases faster with distance compared to the force of inverse r^2, resulting in a stronger force at closer distances and a weaker force at larger distances.

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