ARGUS distribution

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search
ARGUS
Probability density function

c = 1.
Cumulative distribution function

c = 1.
Parameters c>0 cut-off (real)
χ>0 curvature (real)
Support x(0,c)
PDF see text
CDF see text
Mean μ=cπ/8χeχ24I1(χ24)Ψ(χ)

where I1 is the Modified Bessel function of the first kind of order 1, and Ψ(x) is given in the text.
Mode c2χ(χ22)+χ4+4
Variance c2(13χ2+χϕ(χ)Ψ(χ))μ2

In physics, the ARGUS distribution, named after the particle physics experiment ARGUS,[1] is the probability distribution of the reconstructed invariant mass of a decayed particle candidate in continuum background[clarification needed].

Definition

[edit | edit source]

The probability density function (pdf) of the ARGUS distribution is:

f(x;χ,c)=χ32πΨ(χ)xc21x2c2exp{12χ2(1x2c2)},

for 0x<c. Here χ and c are parameters of the distribution and

Ψ(χ)=Φ(χ)χϕ(χ)12,

where Φ(x) and ϕ(x) are the cumulative distribution and probability density functions of the standard normal distribution, respectively.

Cumulative distribution function

[edit | edit source]

The cumulative distribution function (cdf) of the ARGUS distribution is

F(x)=1Ψ(χ1x2/c2)Ψ(χ).

Parameter estimation

[edit | edit source]

Parameter c is assumed to be known (the kinematic limit of the invariant mass distribution), whereas χ can be estimated from the sample X1, ..., Xn using the maximum likelihood approach. The estimator is a function of sample second moment, and is given as a solution to the non-linear equation

13χ2+χϕ(χ)Ψ(χ)=1ni=1nxi2c2.

The solution exists and is unique, provided that the right-hand side is greater than 0.4; the resulting estimator χ^ is consistent and asymptotically normal.

Generalized ARGUS distribution

[edit | edit source]

Sometimes a more general form is used to describe a more peaking-like distribution:

f(x)=2pχ2(p+1)Γ(p+1)Γ(p+1,12χ2)xc2(1x2c2)pexp{12χ2(1x2c2)},0xc,c>0,χ>0,p>1
F(x)=Γ(p+1,12χ2(1x2c2))Γ(p+1,12χ2)Γ(p+1)Γ(p+1,12χ2),0xc,c>0,χ>0,p>1

where Γ(·) is the gamma function, and Γ(·,·) is the upper incomplete gamma function.

Here parameters c, χ, p represent the cutoff, curvature, and power respectively.

The mode is:

c2χ(χ22p1)+χ2(χ24p+2)+(1+2p)2

The mean is:

μ=cpπΓ(p)Γ(52+p)χ2p+22p+2M(p+1,52+p,χ22)Γ(p+1)Γ(p+1,12χ2)

where M(·,·,·) is the Kummer's confluent hypergeometric function.[2][circular reference]

The variance is:

σ2=c2(χ2)p+1χp+3eχ22+(χ22(p+1)){Γ(p+2)Γ(p+2,12χ2)}χ2(p+1)(Γ(p+1)Γ(p+1,12χ2))μ2

p = 0.5 gives a regular ARGUS, listed above.

References

[edit | edit source]
  1. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). (More formally by the ARGUS Collaboration, H. Albrecht et al.) In this paper, the function has been defined with parameter c representing the beam energy and parameter p set to 0.5. The normalization and the parameter χ have been obtained from data.
  2. ^ Confluent hypergeometric function

Further reading

[edit | edit source]
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).