Process
for Finding Energy Peaks for Cosmic Rays
In our set-up, the geometry of the device allows
the maximum path length to lie close to the PMT. This is ideal because
we can first find the maximum path length and then use this to find the
theoretical value for the maximum amount of energy reaching the PMT from
a cosmic ray.
-
Find the maximum path length
from measurements and geometry. Using
trigonometry, q =16°
. Using similar triangles and more trig, d/x = cos q
. This yields a value of 11.2 cm for x.

-
Find the maximum energy emitted
as photons over this path length. We know that x is 11.2
cm. From The Particle Physics Booklet, dE/dx = 1.936 MeV/(g cm2)
and D = 1.032 g/cm3 for polystyrene scintillator. Therefore,
-
Find the fraction of the photons
reaching the PMT. As the ray passes
through the scintillator, the photons are emitted radially. Only a cone
of photons will reach the PMT. To simplify calculations, we assume all
of the energy is emmited at the midpoint of the path in the scintillator.
The fraction reaching the PMT is approximately equal to the area of the
base of the cone (i.e. the end of the scintillator) divided by the surface
area of the sphere.
-
Calculate the energy deposited
by the fraction of photons reaching the PMT. Assuming our path
found is the path of the maximum energy, the peak should be given by
To
compare with our results . . .