2021
DOI: 10.1088/2633-1357/abec9f
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Generalized Poisson distributions for systems with two-particle interactions

Abstract: In a cosmological context, observational best fits for galaxies’ distributions in the Universe have been tackled by recourse to different distribution functions. We provide here arguments favoring the formulation of a rather general distribution function (DF), of Poisson origin, describing galaxy clustering. The DF should be useful irrespective of distances or temperatures. We will be discussing distribution function for gravitational interactions.

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Cited by 3 publications
(4 citation statements)
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“…) ˆ, which is consistent with the definition in equation (12). It is easy to check that 2 z á ñ ˆis also consistently defined in a similar manner.…”
Section: Derivation Via the Path Integralsupporting
confidence: 83%
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“…) ˆ, which is consistent with the definition in equation (12). It is easy to check that 2 z á ñ ˆis also consistently defined in a similar manner.…”
Section: Derivation Via the Path Integralsupporting
confidence: 83%
“…It should be emphasized that the factor of p 2 ℓ in equation (12) was not an ad hoc choice but in fact a physicallysignificant one, which will become apparent in the context of the path-integral derivation presented in the following section (See the comments following equation (42) for more details).…”
Section: Correspondence Of Statistical/spacetime Eventsmentioning
confidence: 99%
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