Timeline for What is meant by “Energy is exactly conserved locally in GR. Inflation and Dark Energy isn't an exception to this.”?
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Dec 8, 2020 at 8:02 | history | bumped | CommunityBot | This question has answers that may be good or bad; the system has marked it active so that they can be reviewed. | |
Aug 9, 2020 at 9:06 | history | bumped | CommunityBot | This question has answers that may be good or bad; the system has marked it active so that they can be reviewed. | |
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Apr 2, 2019 at 12:01 | history | bumped | CommunityBot | This question has answers that may be good or bad; the system has marked it active so that they can be reviewed. | |
Jul 26, 2018 at 0:57 | history | undeleted | parker | ||
Jul 23, 2018 at 10:10 | history | deleted | parker | via Vote | |
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Jul 20, 2018 at 18:22 | history | edited | parker | CC BY-SA 4.0 |
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Jul 20, 2018 at 18:08 | history | edited | parker | CC BY-SA 4.0 |
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Jul 20, 2018 at 11:01 | comment | added | Bert Barrois | The author probably means that the covariant derivative of the stress-energy tensor vanishes. So does the covariant derivative of Einstein’s cosmological constant term (“dark energy”). | |
Jul 20, 2018 at 5:17 | answer | added | Virgo | timeline score: -1 | |
Jul 18, 2018 at 18:46 | history | edited | parker | CC BY-SA 4.0 |
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Jul 18, 2018 at 9:19 | comment | added | johndecker | You should probably ask the authors directly. Note that GR locally is SR, and in SR energy is conserved. Note that "locally" includes time, so delta-t should be small enough that space doesn't expand enough to have a measurable effect. | |
Jul 18, 2018 at 4:34 | history | edited | parker | CC BY-SA 4.0 |
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Jul 18, 2018 at 4:27 | history | asked | parker | CC BY-SA 4.0 |