Calculating neutrino flux density

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SUMMARY

The discussion centers on calculating the neutrino flux density at the Earth's surface, given that the Sun is 150 Gm away and produces 2 x 1038 neutrinos per second. The initial calculation presented by a user, 1.3 x 1027, is incorrect due to improper unit application and misunderstanding of the concept of flux density. Participants emphasize the need to consider the solid angle subtended by the Earth from the Sun and the uniform distribution of neutrinos for accurate calculations.

PREREQUISITES
  • Understanding of neutrino physics and flux density concepts
  • Knowledge of solid angles in spherical geometry
  • Familiarity with units of measurement in physics, particularly for flux
  • Basic principles of particle distribution in astrophysics
NEXT STEPS
  • Study the concept of solid angles and their application in astrophysics
  • Learn about neutrino interactions and detection methods
  • Review the principles of flux density calculations in physics
  • Explore the distribution of particles in a spherical context
USEFUL FOR

Students preparing for A2 Physics exams, educators teaching particle physics, and anyone interested in astrophysical phenomena related to neutrinos.

carvell
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Third and final A2 Physics paper tomorrow.

Currently struggling with one of the articles we have been given to study before the exam. It's all about neutrinos. I've been given some questions to try, educated guesses by teachers on what could come up on the exam paper.

"If the Sun is 150 Gm away and produces 2 * 10^38 (2E38) neutrinos per second, what is the neutrino flux density at the Earth's surface?"

My best guess based on what I know about magnetic flux density so far is:

2E38 / 150G = 1.3E27

I realize that 150Gm isn't an area, but that's the best I could do!

Is there anyone that can confirm my answer/tell me it's all completely wrong?

Thanks.
 
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carvell said:
Third and final A2 Physics paper tomorrow.

Currently struggling with one of the articles we have been given to study before the exam. It's all about neutrinos. I've been given some questions to try, educated guesses by teachers on what could come up on the exam paper.

"If the Sun is 150 Gm away and produces 2 * 10^38 (2E38) neutrinos per second, what is the neutrino flux density at the Earth's surface?"

My best guess based on what I know about magnetic flux density so far is:

2E38 / 150G = 1.3E27

I realize that 150Gm isn't an area, but that's the best I could do!

Is there anyone that can confirm my answer/tell me it's all completely wrong?

Thanks.

Couple of things I can see wrong:
1) Units... your units are 1/(m*s)... this is wrong for flux
2) What does magnetic flux density have to do with this?

Try thinking about it this way: what size does the Earth look like from the sun? Can you find the solid angle subtended by the Earth at a radius of 150 Gm? Are you to assume that the particles are uniformally distributed
 

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