Gaisser–Hillas function
{{Short description|Function in physics to determine particle density}}
The Gaisser–Hillas function is used in astroparticle physics. It parameterizes the longitudinal particle density in a cosmic ray air shower. The function was proposed in 1977 by Thomas K. Gaisser and Anthony Michael Hillas.{{cite book |author=Hillas, A. M. |title=Cosmic rays |publisher=Pergamon Press |location=New York |date=1972 |isbn=978-0-08-016724-4 |url=https://archive.org/details/cosmicrays0000hill|url-access=registration }} [https://books.google.com/books?id=1j8fAwAAQBAJ 2013 edition]
The number of particles as a function of traversed atmospheric depth is expressed as
:
where is maximum number of particles observed at depth , and and are primary mass and energy dependent parameters.
Using substitutions
, {{spaces|5}} {{spaces|5}} and {{spaces|5}}
the function can be written in an alternative one-parametric (m) form{{cite journal |title= Lambert W Function for Applications in Physics|date= 2012|author1= Darko Veberič |doi= 10.1016/j.cpc.2012.07.008 |journal= Computer Physics Communications |volume= 183 |issue= 12 |pages= 2622–2628|arxiv=1209.0735 |bibcode= 2012CoPhC.183.2622V|s2cid= 315088}} as
:
References
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{{refbegin}}
{{cite conference
| last = Gaisser
| first = T.K.
| author2 = Hillas, A.M.
| title = Reliability of the method of constant intensity cuts for reconstructing the average development of vertical showers
| journal =
| book-title = Proc. of 15th Int. Cosmic Ray Conf., 13–26 Aug 1977
| place = Plovdiv, Bulgaria
| date = 1977
| volume = 8
| pages = 353
| bibcode = 1977ICRC....8..353G
}}
{{refend}}
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