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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 .
The number of particles
N
(
X
)
{\displaystyle N(X)}
as a function of traversed atmospheric depth
X
{\displaystyle X}
is expressed as
N
(
X
)
=
N
max
(
X
−
X
0
X
max
−
X
0
)
X
max
−
X
0
λ
exp
(
X
max
−
X
λ
)
,
{\displaystyle N(X)=N_{\text{max}}\left({\frac {X-X_{0}}{X_{\text{max}}-X_{0}}}\right)^{\frac {X_{\text{max}}-X_{0}}{\lambda }}\exp \left({\frac {X_{\text{max}}-X}{\lambda }}\right),}
where
N
max
{\displaystyle N_{\text{max}}}
is maximum number of particles observed at depth
X
max
{\displaystyle X_{\text{max}}}
, and
X
0
{\displaystyle X_{0}}
and
λ
{\displaystyle \lambda }
are primary mass and energy dependent parameters.
Using substitutions
n
=
N
N
max
{\displaystyle n={\frac {N}{N_{\text{max}}}}}
,
x
=
X
−
X
0
λ
{\displaystyle x={\frac {X-X_{0}}{\lambda }}}
and
m
=
X
max
−
X
0
λ
{\displaystyle m={\frac {X_{\text{max}}-X_{0}}{\lambda }}}
the function can be written in an alternative one-parametric (m ) form as
n
(
x
)
=
(
x
m
)
m
exp
(
m
−
x
)
=
x
m
e
−
x
m
m
e
−
m
=
exp
(
m
(
ln
x
−
ln
m
)
−
(
x
−
m
)
)
.
{\displaystyle n(x)=\left({\frac {x}{m}}\right)^{m}\exp(m-x)={\frac {x^{m}\,e^{-x}}{m^{m}\,e^{-m}}}=\exp \left(m\,(\ln x-\ln m)-(x-m)\right)\,.}
References
Hillas, A. M. (1972). Cosmic rays . New York: Pergamon Press . ISBN 978-0-08-016724-4 . 2013 edition
Darko Veberič (2012). "Lambert W Function for Applications in Physics". Computer Physics Communications . 183 (12): 2622–2628. arXiv :1209.0735 . Bibcode :2012CoPhC.183.2622V . doi :10.1016/j.cpc.2012.07.008 . S2CID 315088 .
Gaisser, T.K.; Hillas, A.M. (1977). "Reliability of the method of constant intensity cuts for reconstructing the average development of vertical showers". Proc. of 15th Int. Cosmic Ray Conf., 13–26 Aug 1977 . Vol. 8. Plovdiv, Bulgaria. p. 353. Bibcode :1977ICRC....8..353G .
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Gaisser–Hillas function
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