Recent content by Mike Karr
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Undergrad Understand Poynting Density of Flow of Energy w/Weak Physics Background
PeterDonis, thank you! It's nice when the problem is easier than it seems. And especially for the general tip about "weird quirks." I'll be on the lookout.- Mike Karr
- Post #10
- Forum: Special and General Relativity
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Undergrad Understand Poynting Density of Flow of Energy w/Weak Physics Background
that that => what that- Mike Karr
- Post #5
- Forum: Special and General Relativity
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Undergrad Understand Poynting Density of Flow of Energy w/Weak Physics Background
Well, I have been inducted into the joys of electromagnetic units, and I have certainly been confused for a while. However, if I ignore all that and use only formulas in MTW, I can derive: ## \nabla \cdot \frac{E \times B}{4 \pi} = - \frac{\partial}{\partial t}(\frac{E^2 + B^2}{8 \pi}) - E...- Mike Karr
- Post #4
- Forum: Special and General Relativity
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Undergrad Understand Poynting Density of Flow of Energy w/Weak Physics Background
My physics background is weak. My search found lots of ## E \times B ## and ## E^2 + B^2##, often associated with ## \mu_0 ## and ## \epsilon_0 ##, but never divided by ## 4 \pi ## and ## 8 \pi ##, respectively. Could someone provide a reference? Or a derivation? Thanks.- Mike Karr
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- Density Energy Exercise Flow
- Replies: 9
- Forum: Special and General Relativity
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Graduate MTW Gravitation: Exercise 5.1 | Beginner GR Stress-Energy Tensor Symmetry
ergospherical, thanks for your answer. What I was doing wrong was using the wrong components in ##F^{\alpha\beta} ##---I swapped the 0th row and 0th column. But your answer is much more clever, using formulas for ##E_i## and especially for ##B_i## that I would never have thought of. Also, I...- Mike Karr
- Post #15
- Forum: Special and General Relativity
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Graduate MTW Gravitation: Exercise 5.1 | Beginner GR Stress-Energy Tensor Symmetry
Sorry, I got unconfused too quickly. I don't get the correct answer for ## T^{00} ##. Let's look at the two terms of equation 5.22. The last one is simple, I think: ## - \frac{1}{4} \eta^{\mu\nu} F_{\alpha\beta} F^{\alpha\beta} = - \frac{1}{4} \eta^{\mu\nu} 2(E_x^2 + E_y^2 + E_z^2 + B_x^2...- Mike Karr
- Post #13
- Forum: Special and General Relativity
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Graduate MTW Gravitation: Exercise 5.1 | Beginner GR Stress-Energy Tensor Symmetry
Of course. Sorry to bother you with something so trivial.- Mike Karr
- Post #4
- Forum: Special and General Relativity
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Graduate MTW Gravitation: Exercise 5.1 | Beginner GR Stress-Energy Tensor Symmetry
I am a beginner in GR, working my through Gravitation by the above authors. If there is a better place to ask this question, please let me know. I understand (from section 5.7) that the stress-energy tensor is symmetric, and from equation 5.23 (p. 141), it is explicitly symmetric. But...- Mike Karr
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- Exercise Symmetry Tensor Wheeler
- Replies: 15
- Forum: Special and General Relativity