What is the Role of Neutrinos in Explaining Beta Decay Energy Loss?

In summary, the discovery of the neutrino in 1930 by Pauli was a result of studying the continuous rather than discrete spectrum of energy from beta decay, which seemed to contradict the energy conservation law. To solve this, it was proposed that another neutral and light particle, the neutrino, was being created alongside the electron in the decay process. This was a more logical explanation than speculating that the nucleus was initially in an unbound state.
  • #1
TrickyDicky
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I'm interested in the history of the discovery of the neutrino suggested in 1930 by Pauli and I read that the first clue came from the fact that beta decay energy from electrons had a continuous rather than discrete spectrum and this seemed to contradict the energy conservation law.
I would like to understand why the fact that the spectrum from beta decay is continuous rather than discrete implies that energy is being lost and how the neutrino solves this situation.
Thanks
 
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  • #2


Well, what's happening? A neutron is decaying into a proton and emitting an electron. The neutron and proton are bound particles in the nucleus, and so you're transitioning between two states of the nucleus, which has discrete energy levels since its a system of bound particles. So the total beta decay energy is quantized.

So if the total energy is: nucleus(undecayed) -> nucleus(decayed) + e-

That means the electron energy is just the difference between the two discrete nuclear levels, and so it must be discrete. But if you measure it, it's not. It doesn't add up. So either conservation of energy is being violated, or something else is going on. The easiest explanation (that preserves thermodynamics) would be that there's another free particle being created alongside the electron:

nucleus(undecayed) -> nucleus(decayed) + e- + neutrino

So, now the electron energy is the difference in nuclear energy minus the neutrino energy. Since a free particle can have any amount of kinetic energy, the electron would then have a continuous energy spectrum.

Since charge is conserved and a charged particle would've been relatively easy to detect alongside an electron, we can also conclude that this particle is neutral. From the energy, you can estimate that it must be very light. And from conservation of spin you can deduce it's a fermion. So either you have a light, uncharged (and thus difficult-to-detect) particle being formed, or a whole bunch of conservation laws are being broken.
 
  • #3


alxm said:
Well, what's happening? A neutron is decaying into a proton and emitting an electron. The neutron and proton are bound particles in the nucleus, and so you're transitioning between two states of the nucleus, which has discrete energy levels since its a system of bound particles. So the total beta decay energy is quantized.

So if the total energy is: nucleus(undecayed) -> nucleus(decayed) + e-

That means the electron energy is just the difference between the two discrete nuclear levels, and so it must be discrete. But if you measure it, it's not. It doesn't add up. So either conservation of energy is being violated, or something else is going on. The easiest explanation (that preserves thermodynamics) would be that there's another free particle being created alongside the electron:

nucleus(undecayed) -> nucleus(decayed) + e- + neutrino

So, now the electron energy is the difference in nuclear energy minus the neutrino energy. Since a free particle can have any amount of kinetic energy, the electron would then have a continuous energy spectrum.

Since charge is conserved and a charged particle would've been relatively easy to detect alongside an electron, we can also conclude that this particle is neutral. From the energy, you can estimate that it must be very light. And from conservation of spin you can deduce it's a fermion. So either you have a light, uncharged (and thus difficult-to-detect) particle being formed, or a whole bunch of conservation laws are being broken.
Ok, thank you, that's a clear explanation. Just to see if I understand it, it was expected that since the transition was between bound states of the nucleus the spectrum of the emitted energy should be discrete,but since it is continuous the natural thing to do was to postulate
the emission of another particle to keep the energy conservation, I guess another way to do it would have been to speculate that the nucleus (undecayed) was initially in an unbound state, being excited by some not yet known influence, but there was no basis to justify this, right?
 
  • #4

What is the neutrino and how was it discovered?

The neutrino is a subatomic particle that has no electric charge and very little mass. It was first theorized by physicist Wolfgang Pauli in 1930. In 1956, physicists Frederick Reines and Clyde Cowan successfully detected the neutrino for the first time through their experiments at the Savannah River Plant in South Carolina.

Why was the discovery of the neutrino significant?

The discovery of the neutrino was significant because it confirmed the existence of a new type of subatomic particle and opened up new possibilities for understanding the fundamental building blocks of the universe. It also provided evidence for the theory of weak interactions, which describes the way particles interact through the weak nuclear force.

How does the neutrino interact with matter?

The neutrino interacts with matter very weakly, making it difficult to detect. It mostly interacts through the weak nuclear force, which is one of the four fundamental forces of nature. Neutrinos can also interact with matter through the gravitational force, but this interaction is extremely small and difficult to observe.

What are the different types of neutrinos?

There are three known types of neutrinos: electron neutrinos, muon neutrinos, and tau neutrinos. Each type is associated with a different charged lepton (electron, muon, or tau) and they can transform into each other through a process known as neutrino oscillation. This phenomenon was first observed in the late 1990s and has led to further insights into the properties of neutrinos.

How is the study of neutrinos relevant to modern science?

The study of neutrinos is relevant to modern science because it helps us understand the fundamental properties of matter and the universe. Neutrinos are the most abundant particles in the universe, and their behavior can provide insights into the Big Bang, the formation of galaxies, and the evolution of stars. They are also being used in various cutting-edge experiments to study topics such as dark matter, nuclear reactions, and the possibility of new physics beyond the Standard Model.

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