key term - Electron Capture

Definition

Electron capture is a nuclear process in which a proton-rich atomic nucleus absorbs an inner atomic electron, converting a proton into a neutron and emitting a neutrino. This process is an important mechanism for the radioactive decay of certain unstable isotopes.

5 Must Know Facts For Your Next Test

1. Electron capture is a common decay mode for proton-rich isotopes, where the nucleus has too many protons relative to neutrons.
2. The process of electron capture reduces the atomic number of the nucleus by one, while increasing the number of neutrons by one.
3. Electron capture is often accompanied by the emission of characteristic X-rays or Auger electrons as the atom reorganizes its electron shell.
4. The energy released during electron capture can be used to excite the daughter nucleus, leading to the emission of gamma rays.
5. Electron capture is an important process in the evolution of massive stars, as it can trigger the final stages of stellar collapse and supernova explosions.

Review Questions

• Explain the mechanism of electron capture and how it affects the atomic nucleus.
  • In electron capture, a proton-rich atomic nucleus absorbs an inner atomic electron, typically from the K or L shell. This process converts a proton into a neutron, reducing the atomic number of the nucleus by one and increasing the number of neutrons by one. The energy released during this process can be used to excite the daughter nucleus, leading to the emission of characteristic X-rays or Auger electrons as the atom reorganizes its electron shell.
• Describe the role of electron capture in the evolution of massive stars.
  • Electron capture is an important process in the late stages of the evolution of massive stars. As the core of a massive star becomes more proton-rich, electron capture can occur, converting protons into neutrons. This process can trigger the final stages of stellar collapse, leading to the formation of a neutron star or the core collapse that initiates a supernova explosion. The energy released during electron capture and the subsequent changes in the star's structure and composition play a crucial role in the explosive finish of massive stars.
• Analyze how the emission of neutrinos during electron capture affects the energy balance and stability of the atomic nucleus.
  • During electron capture, the absorbed electron combines with a proton in the nucleus, converting it into a neutron and emitting a neutrino. The emission of the neutrino, which is a weakly interacting particle, carries away a small amount of the energy released in the process. This energy loss can affect the overall energy balance and stability of the atomic nucleus, potentially leading to further radioactive decay or nuclear rearrangement. The neutrinos produced in electron capture also play a role in the energy transport and cooling processes within the star, contributing to the complex dynamics of stellar evolution, particularly in the final stages of a massive star's life cycle.

Related terms

Radioactive Decay:

The process by which an unstable atomic nucleus spontaneously loses energy by emitting radiation in the form of particles or electromagnetic waves.

Neutrino:

An electrically neutral, weakly interacting elementary particle that is emitted during certain types of radioactive decay, such as electron capture.

Proton-Rich Isotopes: Atomic nuclei with an excess of protons compared to neutrons, which can undergo electron capture to become more stable.