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184_notes:maxwells_eq [2017/11/30 05:57] – [Putting Together Maxwell's Equations] pwirving | 184_notes:maxwells_eq [2021/07/06 17:53] (current) – bartonmo | ||
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Section 22.4 and 23.1 in Matter and Interactions (4th edition) | Section 22.4 and 23.1 in Matter and Interactions (4th edition) | ||
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===== Putting Together Maxwell' | ===== Putting Together Maxwell' | ||
Now that we have added the final addition to Ampere' | Now that we have added the final addition to Ampere' | ||
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{{youtube> | {{youtube> | ||
- | ==== The Four Maxwell' | + | ===== The Four Maxwell' |
- | First we have Gauss' | + | First we have [[184_notes: |
∫→E∙d→A=Qencϵ0 | ∫→E∙d→A=Qencϵ0 | ||
These electric fields point away from positive charges and towards negative charges. | These electric fields point away from positive charges and towards negative charges. | ||
- | Next we have Faraday' | + | Next we have [[184_notes: |
−∫→E∙d→l=dΦBdt | −∫→E∙d→l=dΦBdt | ||
These electric fields point in a direction that oppose the change in flux that created them. | These electric fields point in a direction that oppose the change in flux that created them. | ||
- | After that we have Gauss' | + | After that we have [[184_notes: |
∫→B∙d→A=0 | ∫→B∙d→A=0 | ||
This equation says that there is no magnetic field that points away or towards a source. This tells us that **there are no magnetic monopoles** (i.e., a north pole cannot exist without a south pole). | This equation says that there is no magnetic field that points away or towards a source. This tells us that **there are no magnetic monopoles** (i.e., a north pole cannot exist without a south pole). | ||
- | Finally, we have Ampere' | + | Finally, we have [[184_notes: |
∫→B∙d→l=μ0Ienc+μ0ϵ0dΦEdt | ∫→B∙d→l=μ0Ienc+μ0ϵ0dΦEdt | ||
- | These equations are important because, as we learned, once you have the electric or magnetic field, you can relate those fields to the electric or magnetic force; to energy, electric potential, or work; and apply those principles to circuit applications like capacitors, resistors, and current. Ultimately, with the conservation of charge, these Maxwell' | + | These equations are important because, as we learned, once you have the [[184_notes: |
- | ==== Limitations on Classical E&M ==== | + | ===== Limitations on Classical E& |
- | This theory of electromagnetism is classical in that it applies to systems of many atoms and electrons. We have constructed arguments for single charges or even small atomic systems, but these charges and systems are governed by quantum mechanics. So, while we might have a classical picture of the atom and electron cloud, a better model is more complicated and requires a quantum theory of electromagnetism in which both atomic systems and the field are treated quantum mechanically. This reformulation of electromagnetism helps us do cutting research and development as electronic systems become increasingly smaller and push on the limits of quantum mechanics. | + | This theory of electromagnetism is classical in that it applies to systems of many atoms and electrons. We have constructed arguments for single charges or even small atomic systems, but in reality, |
- | However, this classical theory is one of the most complete theories in science for the range of physical systems it can describe. It works at the astronomical scale and is consistent with relativity and it works down to the microscopic level (up to the quantum limit). | + | Even so, this classical theory is one of the most complete theories in science for the range of physical systems it can describe. It works at the astronomical scale and is consistent with relativity, and it works down to the microscopic level (up to the quantum limit). |