Calculating Binding Energy for a Neutron System with Gravitational Forces

In summary, we are considering a system of two neutrons interacting through gravitational forces and want to find the binding energy and characteristic size of the ground state configuration. We can use the formula for the ground state energy of a hydrogen atom, with modifications for the gravity case, and take into account the movement of both neutrons in the "neutron atom". It is uncertain if such a system exists in reality.
  • #1
andre220
75
1

Homework Statement


Consider a system of two neutrons interacting only through gravitational attractive forces. Find the binding energy of this "quantum atom" (in eV) and the characteristic size of the ground state configuration. Is there any chance to find such a system in reality?


Homework Equations



[tex] F = \frac{G m_1 m_2}{r^2} [/tex]

The Attempt at a Solution



Okay so, I am not really sure where to start here. Obviously the force is as written above. My first though was to use [tex]U_G = -\frac{G m_1 m_2}{r}[/tex], but I am not really sure if this is on the right track, or, if so, where to go from there.
 
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  • #2
The first thing that comes to mind is that you can estimate the minimum kinetic energy from the Heisenberg uncertainty principle. For the neutrons to be bound, gravitational binding energy must be bigger than kinetic energy.
 
  • #3
Hello, andre220. Welcome to PF.

The force of gravity between the two neutrons has exactly the same form as the electric force between the electron and the proton in a hydrogen atom. Only certain constants are different. So, recall the formula for the ground state energy of the hydrogen atom and figure out how to modify it for the gravity case.

There is an additional matter to consider. In the hydrogen atom, it is assumed to a good approximation that the proton is at rest and only the electron is moving. In the "neutron atom" both neutrons will be moving.
 
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1. What is the Binding Energy Problem?

The Binding Energy Problem is a concept in nuclear physics that refers to the difference between the mass of a nucleus and the sum of the masses of its individual protons and neutrons. This difference is known as the mass defect, and it represents the energy that is released when a nucleus is formed.

2. Why is the Binding Energy Problem important?

The Binding Energy Problem is important because it helps us understand the stability and structure of atomic nuclei. It also plays a crucial role in nuclear reactions and energy production, such as in nuclear power plants and nuclear weapons.

3. How is the Binding Energy Problem calculated?

The Binding Energy Problem is calculated using Einstein's famous equation, E=mc^2, where E represents the energy released, m is the mass defect, and c is the speed of light. The mass defect can be determined by subtracting the sum of the individual masses of the protons and neutrons from the mass of the nucleus.

4. What factors affect the Binding Energy Problem?

The Binding Energy Problem is affected by the number of protons and neutrons in a nucleus, as well as the particular arrangement of these particles. The stronger the nuclear force between the particles, the greater the binding energy and the more stable the nucleus.

5. How does the Binding Energy Problem relate to nuclear fission and fusion?

The Binding Energy Problem is crucial in understanding and predicting nuclear fission and fusion reactions. In fission, the nucleus splits into smaller fragments, releasing energy due to the loss of binding energy. In fusion, smaller nuclei combine to form a larger nucleus, releasing energy as well. The energy released in these reactions is due to the difference in binding energy between the reactants and products.

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