Nuclear physics - solar neutrinos interacting

In summary, the conversation discussed the first part of a question involving a neutrino detector and the probability of interaction with a 37Cl nucleus. The second part of the question involved determining the number of Cl atoms in a pipe with a 1m2 cross section and the fraction of the cross section they cover. A guide was provided to help with the steps needed to solve the problem.
  • #1
Benlaww
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3
Homework Statement
A tank of 12C2 37Cl4, with density 1622 kg m−3, is used as a neutrino detector to measure the flux of neutrinos produced in the Sun. A neutrino has a cross-section of interacting with a 37Cl nucleus of approximately 12 fb (1 femtobarn equals 10−43 m^2).

Write down the nuclear decay that occurs when a solar neutrino interacts with a 37Cl nucleus (try rearranging beta-decay equations).

What is the probability that the neutrino will interact when travelling through 10m of detector? (think of the definition of cross-section).
Relevant Equations
beta plus : p -> n + e- + v
beta minus: n -> p + e+ + anti-v
For the first part I thought you'd have either, p + anti-v -> n + e+ and n + v -> p + e-, but I thought it'd probably be the latter as it's a 'normal' neutrino not an anti neutrino? But do I need to include the actual elements in the equation?

For the second part I have multiplied the density by the cross section to get 1.9*10^-39 kgm-1 but I don't know if this is right or where to go next.
 
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  • #2
Can't help with the first part, but for the second...
Consider a pipe through the tank with a 1m2 cross section.
How many Cl atoms are in the pipe?
If you look along the pipe from one end, and assume you can see all the Cl atoms without overlap, what fraction of the cross section do they cover?
 
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  • #3
Benlaww said:
Homework Statement:: A tank of 12C2 37Cl4, with density 1622 kg m−3, is used as a neutrino detector to measure the flux of neutrinos produced in the Sun. A neutrino has a cross-section of interacting with a 37Cl nucleus of approximately 12 fb (1 femtobarn equals 10−43 m^2).

Write down the nuclear decay that occurs when a solar neutrino interacts with a 37Cl nucleus (try rearranging beta-decay equations).

What is the probability that the neutrino will interact when traveling through 10m of detector? (think of the definition of cross-section).
Relevant Equations:: beta plus : p -> n + e- + v
beta minus: n -> p + e+ + anti-v

For the first part I thought you'd have either, p + anti-v -> n + e+ and n + v -> p + e-, but I thought it'd probably be the latter as it's a 'normal' neutrino not an anti neutrino? But do I need to include the actual elements in the equation?

For the second part I have multiplied the density by the cross section to get 1.9*10^-39 kgm-1 but I don't know if this is right or where to go next.
For part 1, the question refers to neutrinos, not antineutrinos. And Cl-37 is specifically named. So it looks like they are asking for a balanced equation starting:
## \nu + {^{37}Cl} →##
(I would describe this as a ‘reaction’ rather than a ‘decay’.)

For part 2, I agree with @haruspex.

Edt - typo'.
 
Last edited:
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  • #4
Steve4Physics said:
For part 1, the question refers to neutrinos, not antineutrinos. And Cl-37 is specifically named. So it looks like they are asking for a balanced equation starting:
## \nu + {^{37}Cl} →##
(I would describe this as a ‘reaction’ rather than a ‘decay’.)

For part 2, I agree with @haruspex.

Edt - typo'.

Would the element it decays to just be an isotope of Cl or am I supposed to be able to tell which new element it would be?
 
  • #5
Benlaww said:
Would the element it decays to just be an isotope of Cl or am I supposed to be able to tell which new element it would be?
Once you've figured out the reaction, you're supposed to be able to deduce whether the nucleus is still Cl or whether it is converted to something else.
 
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  • #6
haruspex said:
Can't help with the first part, but for the second...
Consider a pipe through the tank with a 1m2 cross section.
How many Cl atoms are in the pipe?
If you look along the pipe from one end, and assume you can see all the Cl atoms without overlap, what fraction of the cross section do they cover?

I'm still a bit confused with working this out, I have got the volume of the 'pipe' as 10 m^2 and so the density times volume gives 16220 kg and then I've divide this mass by the mass of 1 Cl atom to give 2.64*10^-26 atoms?..
 
  • #7
Hi @Benlaww. I can see you are struggling. Here is a guide for some of the basic steps you need to go through.

For part 1 you need to decide what has happened to the number of protons and neutrons inside the Cl-37 nucleus. Then (with reference to the periodic table if needed) you need to work out what the changed nucleus is. Here are some basic questions/steps:
Q1 how many protons in Cl-37?
Q2 how many neutrons in Cl-37?
Q3 how many protons in the changed nucleus?
Q4 how many neutrons in the changed nucleus?
Q5 what is the new nucleus?

For part 2 you imagine a 10m long cylinder full of C₂Cl₄. You can take the cross-sectional area as 1m² for convenience, or call it A (then A will cancel out later).
Q6 what is the volume of the cylinder?
Q7 what is the mass of C₂Cl₄ in the cylinder?
Q8 what is the molecular weight of C₂Cl₄?
Q9 how many moles of C₂Cl₄ are present in the cylinder?
Q10 how many molecules of C₂Cl₄ are present in the cylinder?
Q11 how many atoms of Cl are present in the cylinder?

Then you're nearly home.

Edited - typo's corrrected.
 
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  • #8
Steve4Physics said:
Hi @Benlaww. I can see you are struggling. Here is a guide for some of the basic steps you need to go through.

For part 1 you need to decide what has happened to the number of protons and neutrons inside the Cl-37 nucleus. Then (with reference to the periodic table if needed) you need to work out what the changed nucleus is. Here are some basic questions/steps:
Q1 how many protons in Cl-37?
Q2 how many neutrons in Cl-37?
Q3 how many protons in the changed nucleus?
Q4 how many neutrons in the changed nucleus?
Q5 what is the new nucleus?

For part 2 you imagine a 10m long cylinder full of C₂Cl₄. You can take the cross-sectional area as 1m² for convenience, or call it A (then A will cancel out later).
Q6 what is the volume of the cylinder?
Q7 what is the mass of C₂Cl₄ in the cylinder?
Q8 what is the molecular weight of C₂Cl₄?
Q9 how many moles of C₂Cl₄ are present in the cylinder?
Q10 how many molecules of C₂Cl₄ are present in the cylinder?
Q11 how many atoms of Cl are present in the cylinder?

Then you're nearly home.

Edited - typo's corrrected.

Thank you, I've got that I have 5.89 * 10^28 molecules of C2Cl4 but I'm still a bit confused on how it all relates.
 
  • #9
Benlaww said:
... I have 5.89 * 10^28 molecules of C2Cl4 ...
I disagree with your value for the number of molecules slightly. If you go by what the question says, all the chlorine is Cl-37. No other isotopes of chlorine are present. You should take the atomic weight of Cl-37 to be 37grams. The molecular mass of C₂Cl₄ is then 2*12 + 4*37 = 172grams = 0.172kg. That's the best value to use when calculating the number of molecules.

(In real life the chlorine atoms will be a mixture of mainly Cl-35 and Cl-37. But, from the wording in the question, you are meant to take all the chlorine to be Cl-37 in this problem. That changes the molcular weight you need to use for the C₂Cl₄.)

After this correction, you have successfully answered Q10 (see post #7). What is the answer to Q11?

Then, thinking about what @haruspex said in post #2, what is the total area of the Cl-37 nuclei as ‘seen’ by the incident neutrinos? (Remember each nucleus presents an area of 12fb).

Did you sort out part 1 of the question?
 
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  • #10
Steve4Physics said:
I disagree with your value for the number of molecules slightly. If you go by what the question says, all the chlorine is Cl-37. No other isotopes of chlorine are present. You should take the atomic weight of Cl-37 to be 37grams. The molecular mass of C₂Cl₄ is then 2*12 + 4*37 = 172grams = 0.172kg. That's the best value to use when calculating the number of molecules.

(In real life the chlorine atoms will be a mixture of mainly Cl-35 and Cl-37. But, from the wording in the question, you are meant to take all the chlorine to be Cl-37 in this problem. That changes the molcular weight you need to use for the C₂Cl₄.)

After this correction, you have successfully answered Q10 (see post #7). What is the answer to Q11?

Then, thinking about what @haruspex said in post #2, what is the total area of the Cl-37 nuclei as ‘seen’ by the incident neutrinos? (Remember each nucleus presents an area of 12fb).

Did you sort out part 1 of the question?

I think I got part 1, I've got that Cl-37 + v --> Ar-37 + e-

Changing the molecular mass to 0.172kg, I then get 5.68 * 10^28 molecules so then the number of Cl atoms would be four times this? giving 2.27 * 10^29. So the total area is 2.73 * 10^30 fb.
 
  • #11
Benlaww said:
I think I got part 1, I've got that Cl-37 + v --> Ar-37 + e-

Changing the molecular mass to 0.172kg, I then get 5.68 * 10^28 molecules so then the number of Cl atoms would be four times this? giving 2.27 * 10^29. So the total area is 2.73 * 10^30 fb.
Agreed on all points!

(Note, each molecule contains four Cl-37 atoms. So there is no 'trick' - you are just multiplying the number of molecules by four to get the number of Cl-37 atoms.)

Consider this simple problem. A sheet of paper has area 100cm². Three coins, each with area 2cm², are placed (non-overlapping) on the paper. A drop of rain fall towards the paper. What is the probability that the rainsdrop hits a coin?

If you can do that, the neutrino calculation is essentially the same. (Of course you will need to work in square metres.)
 
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  • #12
Steve4Physics said:
Agreed on all points!

(Note, each molecule contains four Cl-37 atoms. So there is no 'trick' - you are just multiplying the number of molecules by four to get the number of Cl-37 atoms.)

Consider this simple problem. A sheet of paper has area 100cm². Three coins, each with area 2cm², are placed (non-overlapping) on the paper. A drop of rain fall towards the paper. What is the probability that the rainsdrop hits a coin?

If you can do that, the neutrino calculation is essentially the same. (Of course you will need to work in square metres.)
Thank you!
 
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1. What are solar neutrinos and how do they interact with nuclear physics?

Solar neutrinos are subatomic particles that are produced by nuclear reactions in the core of the sun. They interact with nuclear physics through a process called neutrino scattering, where they collide with atomic nuclei and transfer energy and momentum.

2. Why is the study of solar neutrinos important in nuclear physics?

The study of solar neutrinos is important because it can provide valuable information about the processes occurring in the core of the sun, which is predominantly driven by nuclear reactions. This can help us better understand the fundamental principles of nuclear physics and the behavior of matter under extreme conditions.

3. How are solar neutrinos detected and measured?

Solar neutrinos are detected and measured using large underground detectors, such as the Super-Kamiokande in Japan or the Sudbury Neutrino Observatory in Canada. These detectors use a process called neutrino capture, where the neutrinos interact with a target material and produce a detectable signal.

4. What challenges are faced in studying solar neutrinos interacting with nuclear physics?

One of the main challenges in studying solar neutrinos interacting with nuclear physics is the extremely low interaction rate. Only a small fraction of neutrinos that pass through the Earth actually interact with the detectors, making it difficult to obtain accurate measurements. Additionally, the energy and direction of the neutrinos are difficult to determine, making it challenging to identify the specific nuclear reactions that produced them.

5. How do solar neutrinos contribute to our understanding of the universe?

Solar neutrinos contribute to our understanding of the universe by providing insights into the nuclear reactions that power the sun and other stars. They also play a role in the search for dark matter, as they can interact with and potentially reveal information about this elusive substance. Additionally, studying solar neutrinos can help us better understand the behavior of neutrinos, which are one of the most abundant particles in the universe.

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