Fluence rate of gamma source - getting two different answers

Hercuflea
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Homework Statement


A 1 meter long uniform line source of high energy photons emits 10^7 photons /sec. Calculate the particle fluence rate (flux density) at a point P 1m away from the midpoint of the source.

Homework Equations


## dN = number~of~particles ##
## da = differential~area##
##\Phi = fluence = \frac{dN}{da}##
##\phi = fluence~rate = \frac{d\Phi}{dt} = \frac{d}{dt} \frac{dN}{da} = \frac {\frac{dN}{dt}}{da}##

The Attempt at a Solution



I have tried to solve the problem two different ways, and I get 2 different answers.
Define the origin (0,0) to be the location of the point P. Define the rod source such that it's endpoints lie at ##(1,-\frac{1}{2})## and ## (1, \frac{1}{2})##.

1st method: I integrated using the pythagorean theorem and I got

$$ r = \sqrt{y^{2} + 1^{2}}$$
$$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dr $$
$$ = \int_{-\frac{1}{2}}^{\frac{1}{2}} \frac{10^7}{4\pi (\sqrt{y^2+1})^2} dy\ $$
$$ = \frac{10^7}{4\pi} \int_{-\frac{1}{2}}^{\frac{1}{2}} \frac {1}{y^2+1} dy\ $$
$$ = \frac{10^7}{4 \pi} (arctan(y)) $$ from -0.5 to 0.5
$$= \frac{10^7}{4 \pi} (arctan(0.5)-arctan(-0.5)) $$
$$= 7.379 \times 10^5 \frac{photons}{m^2 s} (\frac{1m}{100cm})^2 = 73.79 \frac{photons}{cm^2 s}$$

2nd method:
Since ##rcos(\theta) = 1 ## always, I solved for ##r## in terms of ##\theta## and I got
$$ r = \frac{1}{cos\theta}$$
Also, since ##tan\theta_{max} = \frac{\frac{1}{2}}{1} ## we have ##\theta_{max} = tan^{-1} (0.5)##.

Therefore
$$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dr $$
$$= \int_{-tan^{-1}(0.5)}^{tan^{-1} (0.5)} \frac{10^7}{4\pi {\frac{1}{cos\theta}}^2} d\theta $$
$$ = \frac{10^7}{4\pi} \int_{-tan^{-1}(0.5)}^{tan^{-1} (0.5)} cos^{2}(\theta) d\theta $$
$$ = \frac{10^7}{4\pi} \frac{1}{2} (\theta + \frac{1}{2} sin(2\theta)) $$ from ##-tan^{-1}(0.5)## to ##tan^{-1}(0.5)##
$$=\frac{10^7}{8\pi} (tan^{-1}(0.5)-(-tan^{-1}(0.5)) + \frac{1}{2} (sin(2tan^{-1}(0.5))-sin(-2tan^{-1}(0.5))))$$
$$ = 6.87 \times 10^5 \frac {photons}{m^2 s}(\frac{1m}{100cm})^2 = 68.7\frac {photons}{cm^2 s} $$

Why do the two methods give different answers? I am integrating over the same geometric object...only one way I am using the angle and the other way I am using the vertical component of r. Which method is correct?
 
Last edited:
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I think the substitution in the second method is missing something when you go from ##dr## to ##d\theta##.
 
Thank you for catching that.

Now that I have fixed that, I'm just getting 0.

$$r= \frac 1 {cos\theta} = sec\theta$$
$$dr = sec\theta tan\theta d\theta$$
$$ \phi = \frac {10^7} {4\pi} \int_{-arctan(0.5)}^{arctan(0.5)} \frac {sec\theta tan\theta}{(\frac {1}{cos\theta})^2} d\theta $$
$$=\frac {10^7} {4\pi} \int_{-arctan(0.5)}^{arctan(0.5)} \frac {tan\theta}{sec \theta} d\theta $$
$$=\frac {10^7} {4\pi} \int_{-arctan(0.5)}^{arctan(0.5)} sin\theta d\theta $$
$$=\frac {10^7} {4\pi} (0) = 0 $$

If I divide the bounds of integration by 2 and multiply the integral by 2 i get:
$$ \phi = \frac {10^7} {4\pi} 2\int_{0}^{arctan(0.5)} \frac {sec\theta tan\theta}{(\frac {1}{cos\theta})^2} d\theta $$
$$=\frac {10^7} {2\pi} \int_{0}^{arctan(0.5)} \frac {tan\theta}{sec \theta} d\theta $$
$$=\frac {10^7} {2\pi} \int_{0}^{arctan(0.5)} sin\theta d\theta $$
$$=\frac {10^7} {2\pi} (-cos(arctan(0.5))-(-cos0)) = -1.7 \times 10^5 $$
?
 
Hercuflea said:
$$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dr $$
Should ##dr## actually be ##dy##?
 
TSny said:
Should ##dr## actually be ##dy##?
In the pythagorean theorem method, yes. But I'm trying to do it by integrating over the angle and get the same result as that.
 
For the method of integrating over the angle, you will need to decide which of the following is the correct expression to start with:
$$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dr $$ $$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dy $$
 
TSny said:
For the method of integrating over the angle, you will need to decide which of the following is the correct expression to start with:
$$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dr $$ $$ \phi = \int {\frac{10^7}{4\pi r^{2}}} dy $$

##r## is a function of ##y##

$$y = rsin\theta$$
$$r = \frac {y}{sin\theta}$$
$$dr = d(\frac{y}{sin\theta})$$ = ?

If I choose the second integral I just get a circular argument when I try to get the whole thing in terms of ##\theta##...
$$ \phi = \int_{-.5}^{.5} \frac{10^7}{4\pi (\frac{y}{sin\theta})^2} dy$$
$$=\frac{10^7}{4\pi} \int_{-.5}^{.5} (\frac{sin^2 \theta}{y^2}) dy$$

but since ##y=rsin\theta##
$$=\frac{10^7}{4\pi} \int_{-.5}^{.5} (\frac{sin^2 \theta}{(rsin\theta)^2}) dy$$
$$=\frac{10^7}{4\pi} \int_{-.5}^{.5} (\frac{1}{r^2}) dy$$
 
Have you decided which of the two integrals is the correct starting integral? ## \phi = \int {\frac{10^7}{4\pi r^{2}}} dr ## or ## \phi = \int {\frac{10^7}{4\pi r^{2}}} dy ##?

If the second integral is the correct integral, then you need to express ##r## and ##dy## in terms of ##\theta## and ##d\theta## if you want to integrate over ##\theta##.

To relate ##dy## to ##d\theta##, then ##y = rsin\theta## is not a good relation to use. That's because ##y = rsin\theta## relates three variables. Can you relate ##y## to ##\theta## without using a third variable. (Try a different trig function.)

(You already found a nice way to relate ##r## to ##\theta## in your first attempt at integrating over ##\theta##.)
 
TSny said:
Have you decided which of the two integrals is the correct starting integral? ## \phi = \int {\frac{10^7}{4\pi r^{2}}} dr ## or ## \phi = \int {\frac{10^7}{4\pi r^{2}}} dy ##?

If the second integral is the correct integral, then you need to express ##r## and ##dy## in terms of ##\theta## and ##d\theta## if you want to integrate over ##\theta##.

To relate ##dy## to ##d\theta##, then ##y = rsin\theta## is not a good relation to use. That's because ##y = rsin\theta## relates three variables. Can you relate ##y## to ##\theta## without using a third variable. (Try a different trig function.)

(You already found a nice way to relate ##r## to ##\theta## in your first attempt at integrating over ##\theta##.)
I see what you mean now. Yes, I think the integral with dy is correct because the differential length we are integrating over is along the rod, not along the radius.

$$\frac{y}{1} = tan\theta$$
$$dy = sec^2 \theta d\theta$$
$$\phi = \frac{10^7}{4\pi} \int_{-.5}^{.5} \frac{1}{r^2} dy$$
$$= \frac{10^7}{4\pi} \int_{-arctan(.5)}^{arctan(.5)} \frac{sec^2\theta}{(\frac{1}{cos\theta})^2} d\theta$$
$$=\frac{10^7}{4\pi} \int_{-arctan(.5)}^{arctan(.5)} cos^2 \theta sec^2 \theta d\theta$$

wolfram alpha...
$$=7.3792 \times10^5 \frac{photons}{m^2 s} (\frac{1m}{100cm})^2 = 73.79 \frac{photons}{cm^2 s}$$
 
  • #10
Hercuflea said:
$$= \frac{10^7}{4\pi} \int_{-arctan(.5)}^{arctan(.5)} \frac{sec^2\theta}{(\frac{1}{cos\theta})^2} d\theta$$
$$=\frac{10^7}{4\pi} \int_{-arctan(.5)}^{arctan(.5)} sec^4 \theta d\theta$$
Check your work in going from the first line above to the second line.
 
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  • #11
TSny said:
Check your work in going from the first line above to the second line.
Yes! Thank you! I edited the post.
 
  • #12
OK, good work. ##\; \; \cos^2\theta \sec^2\theta = 1##.

Yes, as you say, it should be ##dy## instead of ##dr## in the original integral.
 
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