In cosmology, the relic abundance of a given elementary particle is a measure of the present quantity of that particle remaining from the Big Bang.
Uses
editRelic abundance is modelled for WIMPs (weakly interacting massive particles) in the study of dark matter.[1]
Calculation
editAssuming that an elementary particle was formerly in thermal equilibrium, its relic abundance may be calculated using a Boltzmann equation.[2]
The temperature scaled abundance of a particle is defined[3] by
where is the number density:
that is, number of particles per physical volume (not the comoving volume).
The relic abundance of a particle is shown by indicates the asymptotic value of abundance of a species of a particle which it will reach after its "freeze-out".[4]
References
edit- ^ Kim Griest, "Relic Abundance in More Detail", The Net Advance of Physics: The Nature of Dark Matter, Section 6C, MIT
- ^ J. Thanh Van Tran (1 January 1990). Z0 Physics: Proceedings of the XXVth Rencontre de Moriond, Les Arcs, Savoie, France, March 4-11, 1990. Atlantica Séguier Frontières. p. 306. ISBN 978-2-86332-081-5.
- ^ Scott Dodelson (2003). Modern Cosmology. Academic Press. pp. 74–76. ISBN 978-0-12-219141-1.
- ^ Patrick Petter (28 October 2013). Basic Knowledge of Astrophysic: A New Way. epubli. p. 91. ISBN 978-3-8442-7203-1.
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