Exploring Lepton Annihilation and Hadron Formation in the Standard Model

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SUMMARY

The discussion centers on the differences in interactions between leptons (electron and positron) and hadrons (electron and proton) within the framework of the Standard Model of particle physics. It is established that while electron-positron pairs can annihilate due to their nature as antiparticles, the electron-proton interaction does not lead to annihilation but rather forms a stable compound, hydrogen. This is attributed to the conservation laws governing quantum numbers, including flavor and color, which prevent the creation of a photon from the electron-proton interaction. The weak force is also mentioned as a possible interaction between electrons and protons, allowing for processes like electron-proton to neutron and neutrino transitions.

PREREQUISITES
  • Understanding of the Standard Model of particle physics
  • Familiarity with quantum numbers such as flavor and color
  • Knowledge of electromagnetic and weak interactions
  • Basic concepts of particle-antiparticle relationships
NEXT STEPS
  • Research the role of conservation laws in particle interactions
  • Study the properties and interactions of quarks and hadrons
  • Explore the implications of the weak force in particle decay processes
  • Investigate the theoretical frameworks for many-body interactions in quantum physics
USEFUL FOR

Physicists, students of particle physics, and anyone interested in the fundamental interactions of particles within the Standard Model.

  • #31
When a positron approaches an electron, it first gets captured into atomic states, just like the states that bind the electron to the proton in hydrogen. The positron then gets captured by the electron and annihilated in several nanoseconds. If the mass of the neutron were slightly less than the mass of the proton, then the electron in the hydrogen atom would eventually get absorbed by the proton to produce a neutron and a neutrino. However, the neutron is heavier than the proton, and the neutron decays into a proton, an electron, and a (nearly) massless neutrino. In nuclei, beta (electron)decay is an example of neutron decay. Beta (positron) decay in nuclei is an example of proton decay in nuclei.
There is one additional effect called K capture, in which a proton in a nucleus "captures" an electron in the atomic K shell and becomes a neutron with the emission of a neutrino. This is also called inverse beta decay.
 
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