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| | Cosmolological Implications of Weakly Interacting Massive Particles |
 | | The annihilation of X particles does not continue unabated though, since the annihilation rate is proportional to the X number density, n, times the anti-X number density, which is assumed^7 to be equal to n, so as n decreases, the annihilation rate decreases like n^2. |
 | | It is expected the number of particles per comoving^35 volume, which is proportional to f, remains approximately equal to the number of particles per comoving volume in equilibrium, f_eq, until the chemical equilibrium is destroyed at the freezing temperature. |
 | | Since Majarona particles are their own antiparticles, if X were a Majorana particle, then the number density of anti-X particles would be the number density of X particles. |
| particle.physics.ucdavis.edu /archive/wimps.html (7599 words) |
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