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184_notes:conservation_theorems [2017/11/30 01:29] – dmcpadden | 184_notes:conservation_theorems [2021/07/06 17:36] (current) – bartonmo | ||
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Chapters 18 and 19 (and Chapters 2, 3, 6, 11, and 13) in Matter and Interactions (4th edition) | Chapters 18 and 19 (and Chapters 2, 3, 6, 11, and 13) in Matter and Interactions (4th edition) | ||
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===== Conservation Theorems ===== | ===== Conservation Theorems ===== | ||
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ΔQsys=0whenIext=0 | ΔQsys=0whenIext=0 | ||
- | ==== Linear and Angular Momentum Conservation in E&M ==== | + | {{youtube> |
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+ | ===== Linear and Angular Momentum Conservation in E& | ||
We have not talked much about linear and angular momentum conservation in an electromagnetic system because they extend beyond the scope of this course. This is because to truly understand the relationship between these and the electromagnetic field, we must develop an understanding that the electromagnetic field can have linear and angular momentum. That's right, the field itself has momentum that can push physical objects or twist them. This might seem very strange, but it is definitely the case that the electromagnetic field itself can have both. | We have not talked much about linear and angular momentum conservation in an electromagnetic system because they extend beyond the scope of this course. This is because to truly understand the relationship between these and the electromagnetic field, we must develop an understanding that the electromagnetic field can have linear and angular momentum. That's right, the field itself has momentum that can push physical objects or twist them. This might seem very strange, but it is definitely the case that the electromagnetic field itself can have both. | ||
- | A common example of this comes from astrophysics. When a star is going through fusion, it has a lot of gas pushing outward from the core. In addition, light is carried outward. This is complicated process, but the gas and light run into material in front of them as they move towards the stellar surface. These pushes by the gas and light cause a pressure on the material in front of them; pushing them outward. However, the gas in front of the outward moving gas and light is gravitationally attracted to any matter behind it. This careful balance of the gravitational pressure, gas pressure, and radiation pressure (the momentum imparted by collisions of electromagnetic radiation with material) determines the size, temperature, | + | A common example of this comes from astrophysics. When a star is going through fusion, it has a lot of gas pushing outward from the core. In addition, light is carried outward. This is a complicated process, but the gas and light run into the material in front of them as they move towards the stellar surface. These pushes by the gas and light causes |
- | ==== Energy and Charge Conservation in E&M ==== | + | ===== Energy and Charge Conservation in E& |
Energy and charge conservation in electromagnetism is much easier to illustrate as both govern the movement of current in electronic circuits. In a typical circuit there are energy providers, [[184_notes: | Energy and charge conservation in electromagnetism is much easier to illustrate as both govern the movement of current in electronic circuits. In a typical circuit there are energy providers, [[184_notes: | ||
- | === Energy Conservation in a Circuit === | + | ===== Energy Conservation in a Circuit |
A simple circuit consists of a single battery and a single resistor. There' | A simple circuit consists of a single battery and a single resistor. There' | ||
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ΔVbattery=−ΔVresistor | ΔVbattery=−ΔVresistor | ||
- | where the minus sign indicates that the electric potential across the battery is negative as it is a user of energy. This calculation where we go around the loop adding up the energy per unit charge provided and used was called the loop rule and it gave us a way to determine the current through a resistor (or other elements in a circuit). | + | where the minus sign indicates that the electric potential across the battery is negative as it is a user of energy. This calculation where we go around the loop adding up the energy per unit charge provided and used was [[184_notes: |
- | === Charge Conservation in a Circuit === | + | ===== Charge Conservation in a Circuit |
- | Charge conservation in a circuit is a bit more subtle but explains how the current | + | Charge conservation in a circuit is a bit more subtle but explains how the current |
We can apply charge conservation by choosing the resistor as our system. In this case, the amount of charge that builds up is zero as the system is in steady state, | We can apply charge conservation by choosing the resistor as our system. In this case, the amount of charge that builds up is zero as the system is in steady state, | ||
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|Iin|=|Iout| | |Iin|=|Iout| | ||
- | Thus, the current going into the resistor, but be equal to the current coming out of it. We could choose any other part of the circuit like this and make the same argument, which means that charge conservation leads to an important result -- namely that the current into any branch is the same as that coming out. This was called the node or junction rule. | + | Thus, the current going into the resistor, but be equal to the current coming out of it. We could choose any other part of the circuit like this and make the same argument, which means that charge conservation leads to an important result -- namely that the current into any branch is the same as that coming out. [[184_notes: |
- | ==== Effects and Applications ==== | + | |
+ | ===== Effects and Applications | ||
Armed with these conservation theorems, namely energy and charge conservation, | Armed with these conservation theorems, namely energy and charge conservation, | ||
- | === Resistors in a circuit === | + | ===== Resistors in a circuit ===== |
+ | [{{ 184_notes: | ||
- | Two resistors in series (end-to-end) must have the same current running through them, but they can use different amounts of energy per unit charge | + | [[184_notes: |
Req=R1+R2 | Req=R1+R2 | ||
- | Two resistors in parallel (connected off the same branch) must use the same energy per unit charge, but they can drive different currents as long as the sum of those currents is equal to the total before the branch splits. This leads to their combine effective result as reducing the overall resistance of the circuit, | + | [{{184_notes: |
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1Req=1R1+1R2 | 1Req=1R1+1R2 | ||
- | === Capacitors in a circuit === | + | ===== Capacitors in a circuit ===== |
+ | [{{ 184_notes: | ||
- | Two fully charged | + | [[184_notes: |
1Ceq=1C1+1C2 | 1Ceq=1C1+1C2 | ||
- | Two fully charged | + | [{{184_notes: |
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+ | [[184_notes: | ||
Ceq=C1+C2 | Ceq=C1+C2 |