How Does Beta Minus Decay Affect the Kinetic Energy of a Tin Nucleus?

In summary, a first year student asked about a radioactive isotope of Tin undergoing beta minus decay. The resulting electron has a speed of 0.999c and the new nucleus is able to bind the electron into one of its orbits. The equation for potential and kinetic energy with two varying speeds was discussed, along with the possibility of taking the finite size of the nucleus into account. The student is not familiar with models for the size of nuclei but mentioned that it is small, with a length of 10-15m.
  • #1
omiros
30
0
Hello everybody, I am a first year student and I have a question that I am not sure if I can answer.

A radioactive isotope of Tin(50), with 85 neutrons in its nucleus and without any electrons bound to it, undergoes a beta minus decay. The electron pops into existence, 10-15m from the center of the nucleus (consider that the nucleus is uniformly charged), and it leaves with a speed of 0.999c.

(We consider Mn=Mp=1.6x10-27)

1. What is the final speed of, both the electron and the nucleus?

2. Will the the new nucleus, be able to bind the electron, into one of its orbits?

Tips: The new nucleus will have 51 protons and 84 neutrons.

The atom is a hydrogen like one, so we can find the probable bound energies through the Bohr model. (We don't care about its angular distribution)

The kinetic energy of the electron has to be calculated through the K = (γ-1)mc2
and the potential energy from the Coulomb law U = -Ze2/(4πε0r).

I assume that the energy levels will be 51x13.6/n2eV.

So the hard part, is the equation of potential-kinetic energy with two varying speeds, that can give us the result.
 
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  • #2
"two varying speeds"?
Did you compare the kinetic energy of the electron to its potential energy?

(consider that the nucleus is uniformly charged)
That could indicate that you have to take the finite size of the nucleus into account. Do you know models about the size of nuclei?
 
  • #3
mfb said:
"two varying speeds"?
Did you compare the kinetic energy of the electron to its potential energy?

No. I am just saying that, as the electron is travelling, it is 'pulling' the nucleus with it. A positive and a negative charge, that are getting separated (cause of the moving electron and the stationary, at the beginning nucleus.)

mfb said:
That could indicate that you have to take the finite size of the nucleus into account. Do you know models about the size of nuclei?

Personally I do not. However I am thinking of it as : It is of a finite size and quite small. 10-15m, is its whole length.
 
  • #4
omiros said:
No.
Well that would be interesting!

Personally I do not. However I am thinking of it as : It is of a finite size and quite small. 10-15m, is its whole length.
In that case, the electron would "appear" (directly) outside the nucleus, and the given uniform charge distribution in the nucleus would not matter.
 
  • #5


First, let's calculate the initial kinetic energy of the electron. We can use the formula K = (γ-1)mc2, where γ is the Lorentz factor given by γ = 1/√(1-v2/c2). Since the electron's speed is given as 0.999c, we can calculate the Lorentz factor as γ = 1/√(1-0.9992) = 22.36. Plugging this into the formula, we get K = (22.36-1)(9.11x10^-31)(3x10^8)^2 = 2.46x10^-13 J.

Now, let's calculate the potential energy of the electron at a distance of 10^-15 m from the nucleus. We can use the Coulomb's law formula U = -Ze2/(4πε0r), where Z is the atomic number of the nucleus (in this case, 51), e is the elementary charge, ε0 is the permittivity of vacuum and r is the distance from the nucleus. Plugging in the values, we get U = -(51)(1.6x10^-19)^2/(4πx8.85x10^-12x10^-15) = -4.56x10^-12 J.

Now, we can use conservation of energy to calculate the final kinetic energy of the electron. The total energy (kinetic + potential) remains constant during the decay process. So, we can write the equation as Kinitial + Uinitial = Kfinal + Ufinal. Plugging in the values, we get Kfinal = Kinitial + Uinitial - Ufinal = 2.46x10^-13 + (-4.56x10^-12) - (-2.04x10^-13) = -4.72x10^-12 J.

Since the final kinetic energy is negative, we can conclude that the final velocity of the electron will be less than 0.999c. To calculate the exact velocity, we can use the formula K = (γ-1)mc2 and solve for v. This gives us v = √(1-(1-K/mc2)^2) = 0.998c.

Now, let's calculate the final speed of the nucleus. We can use conservation of momentum to write the equation as mvinitial = mvfinal. Since the mass of
 

Related to How Does Beta Minus Decay Affect the Kinetic Energy of a Tin Nucleus?

1. What is kinetic energy of a nucleus?

Kinetic energy of a nucleus refers to the energy that a nucleus possesses due to its motion or movement. This energy is a result of the repulsive forces between positively charged protons and is responsible for holding the nucleus together.

2. How is the kinetic energy of a nucleus calculated?

The kinetic energy of a nucleus can be calculated using the formula KE = 1/2mv2, where m is the mass of the nucleus and v is its velocity. This formula is based on the classical mechanics approach and is applicable for larger nuclei.

3. What factors affect the kinetic energy of a nucleus?

The kinetic energy of a nucleus is affected by its mass and velocity. The higher the mass and velocity of a nucleus, the greater its kinetic energy will be. Additionally, the number of protons and neutrons in the nucleus also play a role in determining its kinetic energy.

4. How does the kinetic energy of a nucleus contribute to nuclear reactions?

The kinetic energy of a nucleus plays a crucial role in nuclear reactions. In fusion reactions, the kinetic energy of nuclei is converted into thermal energy, which is responsible for the release of large amounts of energy. In fission reactions, the release of kinetic energy is what causes the splitting of the nucleus and the release of energy.

5. Can the kinetic energy of a nucleus be measured?

Yes, the kinetic energy of a nucleus can be measured using various techniques such as particle accelerators and spectroscopy methods. These methods allow scientists to study the properties of nuclei and measure their kinetic energy in different states.

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