Input Energy of Radioactive Decays

In summary, radioactive decays, such as α, SF, CD, need to overcome an energy barrier in order to occur. This is achieved through quantum mechanical tunneling, where a particle can pass through an energy barrier that it would not be able to in classical mechanics. This is different from fusion, where particles need to meet and have a single chance of tunneling through the barrier. The energy released in a decay is not directly the same as the energy barrier, but they are closely linked. Even in a situation where there is not enough energy available, the decay can still occur due to quantum tunnelling.
  • #1
A M
83
16
TL;DR Summary
We know that nuclear fusion doesn't occur under normal conditions (e.g. in a helium balloon).
Because for the fusion of even the lightest elements (like hydrogen isotopes), fairly high energy is needed to 'break' the electrostatic repulsion barrier; although the released energy might be much higher.
But how about some radioactive decays? (α, SF, CD, ...)
Don't we need energy to to separate some nucleons of a radioactive nucleus?
 
Physics news on Phys.org
  • #2
Yes, decays also need to overcome an energy barrier. This is done through quantum mechanical tunneling through the energy barrier. The difference in relation to fusion is that you only have a single radioactive particle and even a small probability per time of decaying will eventually lead to a decay. For fusion, the particles also need to meet up and when they do they have a single chance of tunneling through the energy barrier with very low proability.
 
  • Like
  • Skeptical
Likes vanhees71 and A M
  • #3
Orodruin said:
Yes, decays also need to overcome an energy barrier.
Would you please explain a little more?
 
  • #4
For example of tunnelling where it is electrons that tunnel: we can observe both field emission and photoelectric effect. There is a definite energy barrier (as demonstrated by photoelectric effect) and yet electrons do have a small chance of getting through without any additional energy (as shown by field emission).
 
  • #5
Orodruin said:
Yes, decays also need to overcome an energy barrier. This is done through quantum mechanical tunneling through the energy barrier. The difference in relation to fusion is that you only have a single radioactive particle and even a small probability per time of decaying will eventually lead to a decay.
What does this probability come from? The higher energy they need to overcome that barrier or sth more complicated?
 
  • #6
Yes. We had this discussion and even a graph for alpha decays in the previous thread. The energy released is not directly the same as the energy barrier but the two are closely linked.
 
  • #7
Thank you for the reply, but I haven't quite understood.
What if the nuclei were in a situation without that amount of energy available? The decay wouldn't occur?
 
  • #8
A M said:
Thank you for the reply, but I haven't quite understood.
What if the nuclei were in a situation without that amount of energy available? The decay wouldn't occur?
Yes it would. It is quantum tunnelling. In quantum mechanics a particle can pass an energy barrier that it classically would not be able to.
 
  • Like
Likes vanhees71 and A M

1. What is input energy in radioactive decays?

Input energy in radioactive decays refers to the amount of energy required to initiate the decay process. This energy is usually in the form of an external force, such as heat or radiation, that causes the unstable nucleus to break down and release radiation.

2. How is input energy related to the half-life of a radioactive substance?

The input energy required for a radioactive decay is directly related to the half-life of the substance. The shorter the half-life, the more input energy is needed to initiate the decay process. This is because substances with shorter half-lives are more unstable and require more energy to break down.

3. Can input energy be controlled in radioactive decays?

Yes, input energy can be controlled in radioactive decays. Scientists can manipulate the amount and type of input energy to control the rate of decay and the amount of radiation released. This is important in applications such as nuclear power plants, where the rate of radioactive decay needs to be carefully controlled.

4. How is input energy measured in radioactive decays?

Input energy in radioactive decays is typically measured in electron volts (eV). This unit of measurement represents the amount of energy gained by an electron when it is accelerated through a potential difference of one volt. Other units, such as joules (J) or kilojoules (kJ), can also be used to measure input energy.

5. What happens to the input energy after a radioactive decay occurs?

After a radioactive decay occurs, the input energy is converted into different forms of energy, such as heat, light, or radiation. This energy is then released from the nucleus as the unstable atom becomes more stable. The amount and type of energy released depends on the specific type of decay and the elements involved.

Similar threads

  • High Energy, Nuclear, Particle Physics
Replies
13
Views
2K
  • High Energy, Nuclear, Particle Physics
Replies
7
Views
1K
  • High Energy, Nuclear, Particle Physics
Replies
6
Views
1K
  • High Energy, Nuclear, Particle Physics
Replies
20
Views
1K
  • High Energy, Nuclear, Particle Physics
2
Replies
35
Views
3K
  • High Energy, Nuclear, Particle Physics
2
Replies
44
Views
4K
  • High Energy, Nuclear, Particle Physics
Replies
1
Views
914
  • High Energy, Nuclear, Particle Physics
Replies
2
Views
2K
  • High Energy, Nuclear, Particle Physics
Replies
5
Views
2K
  • High Energy, Nuclear, Particle Physics
Replies
4
Views
2K
Back
Top