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Name: Sungho J.
Status: other
Age: 30s
Location: N/A
Country: N/A
Date: 8/3/2004


Question:
Hi. If an electron with enough energy collides with a proton, then what happens? They just form a hydrogen atom? Or they form a neutron? If both are possible, then which factor controls the process? I am asking because I heard that a neutron can decay to a proton and an electron and the reverse is possible.


Replies:
To form a hydrogen atom, it is required that the electron and proton have almost no energy, almost no velocity relative to each other. A hydrogen atom ionizes at less than 20 electron-volts of energy, so reverse ionization requires energy less than about 20 electron-volts (eV) AND freedom and luck to radiate a photon of the right energy to render the electron "captured". It happens all the time in every electrified gas lamp (fluorescents, neons, mercury-arc, etc), and in the surface layers of the sun.

When a neutron decays into a proton, electron, and neutrino, it also releases energy, 780,000 eV, as the sum of the kinetic energy of the 3 particles. It is unreasonably difficult to get 3 separate particles to collide simultaneously, so the exact reverse of this never happens to a significant extent. It is particularly difficult to get the ghost-like neutrino to react on command with an electron and proton . Neutrinos are the particles that sail all the way through the earth, almost never bumping anything.

However, it is not so difficult for a balanced neutrino / anti-neutrino pair to be accidentally made out of pure excess energy, from the collision between an electron and a proton. Then you have the situation of the electron and proton and neutrino in the same place, merging to form a neutron, and an anti-neutrino flying away free carrying any excess energy (beyond the 780 keV that was needed to make up the neutron). I think this is one of the processes which together make sun-sized masses of neutrons when a neutron star is formed in a supernova explosion. Actually, in that situation the electron and proton are steadily squeezed together by pressure of others around them. Increasing pressure and temperature can smoothly change the energy of repeated collisions until the best energy is found, and the conversion becomes quite rapid and energy-efficient.

If the excess energy of collision is over 1,000 keV, other random particles might be made from the energy too. It only takes 1,020 keV to make an electron-positron pair, for example. I'm not sure what it takes to start emitting excess energy as gamma-ray photons.

That might happen too.



Jim Swenson



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