Feynman lectures on physics: random walk

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SUMMARY

The discussion focuses on the interpretation of formulas (6.11) and (6.12) from Volume 1 of the Feynman Lectures on Physics, which describe changes in internal energy of a system. Formula (6.11) relates the change in internal energy to changes in volume and pressure, while formula (6.12) incorporates the heat exchanged by the system. Participants emphasize the importance of providing specific references to the formulas for clarity and suggest that understanding the randomness of the distance from the starting point in a random walk is crucial for grasping these concepts.

PREREQUISITES
  • Understanding of basic thermodynamics concepts, including internal energy
  • Familiarity with random walk theory and its mathematical implications
  • Knowledge of algebraic manipulation of equations
  • Access to the Feynman Lectures on Physics, specifically Chapter 6
NEXT STEPS
  • Review the Feynman Lectures on Physics, Chapter 6, focusing on formulas (6.11) and (6.12)
  • Study the principles of thermodynamics, particularly the relationship between volume, pressure, and internal energy
  • Explore random walk theory and its applications in statistical mechanics
  • Learn about the concept of root mean square (rms) values in physics
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Students of physics, educators teaching thermodynamics, and anyone interested in the mathematical foundations of random processes and energy changes in systems.

YanaFFF
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Explain please
I do not understand the formulas (6.11) and (6.12) in volume 1 of the Feynman lectures on physics, the entire paragraph between equations (6.10) and (6.12) is generally not very clear. Please explain (preferably in simple language, I'm 13). Thanks!
 
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It would help if you provided links to those formulas for those of us a don’t have Feynman lectures on our shelves. It would also help if you were more specific about what exactly you don’t understand.
 
As kuruman says, it's helpful to provide links to things you want to ask questions about. We're helping out just for fun, and you're more likely to get help if we only have to click on one link rather than hunt through search engines for references. It isn't always possible to provide links, of course, but the Feynman Lectures are all online on CalTech's website - this is chapter 6.

He's proposing a game: toss a coin and if you get heads take a step to the left, if you get tails take a step to the right. If you keep repeating this game, how far will you be from your starting point? The answer is the difference between the number of heads you've got so far and the number of tails you've got so far. This is ##D##. He does algebra to get different expressions for ##D## in terms of the total number of tosses and the number of heads. This is useful because ##N## is not a random number and nor is 2, so the randomness of ##D## is dictated by the randomness of ##N_H##, and he already did the maths for that.

6.11 is just a rearrangement of ##D=2N_H-N##, stated in the paragraph above. 6.12 expects you to use 6.11 to see that the left hand side is the same as half the rms value of ##D## and then 6.10 to get the right hand side.

If that doesn't make sense, say which bits you don't follow and we'll see what we can do.
 
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Ibix said:
As kuruman says, it's helpful to provide links to things you want to ask questions about. We're helping out just for fun, and you're more likely to get help if we only have to click on one link rather than hunt through search engines for references. It isn't always possible to provide links, of course, but the Feynman Lectures are all online on CalTech's website - this is chapter 6.

He's proposing a game: toss a coin and if you get heads take a step to the left, if you get tails take a step to the right. If you keep repeating this game, how far will you be from your starting point? The answer is the difference between the number of heads you've got so far and the number of tails you've got so far. This is ##D##. He does algebra to get different expressions for ##D## in terms of the total number of tosses and the number of heads. This is useful because ##N## is not a random number and nor is 2, so the randomness of ##D## is dictated by the randomness of ##N_H##, and he already did the maths for that.

6.11 is just a rearrangement of ##D=2N_H-N##, stated in the paragraph above. 6.12 expects you to use 6.11 to see that the left hand side is the same as half the rms value of ##D## and then 6.10 to get the right hand side.

If that doesn't make sense, say which bits you don't follow and we'll see what we can do.
Thank you very much! That's exactly what I wanted to hear.
 
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Ibix said:
We're helping out just for fun, and you're more likely to get help if we only have to click on one link rather than hunt through search engines for references.
Especially when one is using a smartphone to search.
 
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Formulas (6.11) and (6.12) in Feynman's lectures on physics explain how the energy of a system changes if it is divided into two parts. This is called a change in the internal energy of the system. Formula (6.11) says that the change in internal energy depends on the change in the volume of the system and pressure. And formula (6.12) shows that the change in internal energy also depends on the heat received or lost by the system. Thus, these formulas help to understand how the energy of a system changes under different conditions.
 
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AlexisBlackwell said:
Formulas (6.11) and (6.12) in Feynman's lectures on physics explain how the energy of a system changes if it is divided into two parts. This is called a change in the internal energy of the system. Formula (6.11) says that the change in internal energy depends on the change in the volume of the system and pressure. And formula (6.12) shows that the change in internal energy also depends on the heat received or lost by the system. Thus, these formulas help to understand how the energy of a system changes under different conditions.
Say what?
 
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