Beta decay and inverse beta decay is different?

In summary, beta decay results in the emission of a neutrino, while neutron stars do not have electron degeneracy and instead electrons combine with protons to form neutrons.
  • #1
CookieSalesman
103
5
So in beta decay I know a neutron can decay into, proton, electron and antineutrino
(Or, neutrino, since they're both the same?)
But anyhow, regardless of the neutrino, in neutron stars electron degeneracy doesn't hold and electrons combine with photons to form neutrons.
But isn't that missing a neutrino?
 
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  • #2
CookieSalesman said:
So in beta decay I know a neutron can decay into, proton, electron and antineutrino
(Or, neutrino, since they're both the same?)
But anyhow, regardless of the neutrino, in neutron stars electron degeneracy doesn't hold and electrons combine with protons to form neutrons.
But isn't that missing a neutrino?
Electron capture occurs with naturally occurring nuclides on earth. It's the same process:

e- + p => n + v
 
  • #3
Yes, that is missing a neutrino. The neutrino, being weakly interacting, typically escapes from the neutron star.

Neutron stars can be formed during core collapse supernovae, where a star ends its life cycle in an enormously bright explosion that typically would outshine the rest of the host galaxy. Yet only 0.01% of the energy released is released in the form of light. About 100 times as much is released in kinetic energy of the mass that is expulsed by the explosion yet this is about 1% of the total energy release. The major part of the energy release, about 99%, is in the form of neutrinos being created as the protoneutron star forms. That is, a supernova sends out 1000 times more energy in neutrinos than in light.

Footnote: The capture of an electron by a proton would typically be referred to as "electron capture". With "inverse beta decay" the process where an anti neutrino is captured and a positron emitted is usually the intended meaning. This was the reaction used in the first experimental discovery of neutrinos.
 
  • #4
CookieSalesman said:
(Or, neutrino, since they're both the same?)
They are not the same.

See the previous posts for the other questions.
 

1. What is the difference between beta decay and inverse beta decay?

Beta decay is a process in which a neutron in an atom's nucleus converts into a proton, releasing an electron and an antineutrino. Inverse beta decay, also known as electron capture, is the opposite process where a proton in an atom's nucleus captures an electron, converting into a neutron and releasing a neutrino.

2. How does beta decay and inverse beta decay affect the stability of an atom?

Beta decay and inverse beta decay both change the number of protons and neutrons in an atom's nucleus, which can affect its stability. If the resulting nucleus is more stable, then the decay process will occur spontaneously. However, if the resulting nucleus is less stable, it may undergo further decay processes to become more stable.

3. Can beta decay and inverse beta decay be observed in everyday life?

Yes, beta decay and inverse beta decay can be observed in everyday life. For example, carbon-14 dating uses the decay of carbon-14 (a beta decay process) to determine the age of organic materials. Inverse beta decay is also used in nuclear power plants to control the rate of nuclear reactions.

4. How does the energy released in beta decay and inverse beta decay differ?

In beta decay, the energy released is in the form of kinetic energy of the electron and antineutrino. In inverse beta decay, the energy released is in the form of a gamma ray photon and the kinetic energy of the resulting nucleus.

5. What are the implications of beta decay and inverse beta decay in particle physics?

Beta decay and inverse beta decay are important processes in understanding the fundamental building blocks of matter. They are used to study the properties of subatomic particles, such as the mass and charge of the neutrino. These processes also play a crucial role in energy production in stars and the creation of heavy elements in supernovas.

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