WISP (quantum mechanics)

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In quantum mechanics, the acronym WISP refers to a largely hypothetical weakly interacting sub-eV particle, or weakly interacting slender particle, or weakly interacting slim particle – low-mass particles which rarely interact with conventional particles, if ever. With the exception of “active” neutrinos, all WISPs are hypothetical particles.

The term is essentially synonymous with axion-like particle (ALP).

Discussion[]

Although left-chiral neutrinos and right-chiral antineutrinos (“active” neutrinos) are known to exist – and active neutrinos do technically satisfy the definition of the term – “WISP” is most often used to refer to a low-mass hypothetical particles which are still dark matter candidates. Examples include:[1]

All WISPs are dark matter candidates, except for conventional, active neutrinos, whose cumulative density could not be sufficient to account for the observed effects of dark matter, based on current estimated limits on their numbers and mass.[1]

Sources[]

The various sources of WISPs could possibly include, hot astrophysical plasma and energy transport in stars.[1] Note however, that since they remain hypothetical (except neutrinos) the means of creation of WISPs depends on the theoretical framework used to propose them.

Massive counterpart[]

WISPs are the low-mass counterpart of weakly interacting massive particles (WIMPs).

See also[]

References[]

  1. ^ a b c Lindner, Axel; Ringwald, Andreas; Majorovits, Béla (4 March 2021). "In search of WISPs". CERN Courier. Searches for New Physics. CERN. Retrieved 7 May 2021.{{cite news}}: CS1 maint: url-status (link)



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