Node Rule: Difference between revisions

Revision as of 17:10, 23 November 2016

Claimed by Ingrid Cai

Improved by Sehyeong An

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The node (or junction) rule states that the current flowing in is equal to the current that flows out. I₁ + I₄ = I₂ + I₃ + I₅

Kirchoff's node rule, also known as Kirchoff's junction rule, further exercises the law of Conservation of Energy and states that if current is constant, all the current that flows through one junction must be equal to all the current that flows out of the junction. This rule can be applied both to conventional and electron currents.

Definition

The node rule is one of Kirchhoff's laws regarding circuits and current. This law states that at any junction in an electrical circuit, the amount of current flowing into the junction is equal to the amount of current flowing out of the junction. This law is also referred to as Kirchhoff's junction rule, Kirchhoff's nodal rule, Kirchhoff's current law, and Kirchhoff's first law. This rule is an application of the conservation of electric charge, basically that charge within a circuit cannot be created or destroyed.

A Mathematical Model

Another way to write the Node Rule is:

[math]\displaystyle{ \Sigma \Delta {I} = 0 }[/math]

where I stands for the current of the individual parts or wires in a circuit and the sign of the current that flows into the junction is opposite of the current that flows out of the junction. This simply supports the idea that energy cannot be created or destroyed because the total current must remain equal regardless of the path it takes.

Kirchhoff's Laws

Kirchhoff developed two very important rules that allow us to "solve" simple circuits, or find out different values for the different components involved in the circuit. The node rule is Kirchhoff's first rule, but there is one more, called the loop rule or Kirchhoff's Voltage Law. The loop rule states that, going around in a loop within a circuit, one will find that the voltages around the loop will sum to 0. Because voltage is just energy per unit charge, and both energy and charge are conserved, this is basically stating that no charge or energy is lost or created within the circuit.

Examples

Ex. 1

Figure 1 displays a node in a circuit. I₁ is equal to 10 amps. I₂ is equal to 4 amps. What is I₃?

You can solve for I₃ using the node rule. The current flowing into the node is I₁, or 10 amps, and the current flowing out of the node is I₂ + I₃. We know that the current flowing in must equal the current flowing out, so 10 amps = 4 amps + I₃. Therefore I₃ must equal 6 amps.

Ex. 2

In Figure 2, I₁ equal 23 amps, I₂ equals 5 amps and I₃ equals 42 amps. What is I₄?

The current flowing into the node is I₁ + I₂, or 23 amps plus 5 amps, or 28 amps. The current flowing out of the node is I₃ + I₄, or 42 amps plus I₄. Applying the node rule, 28 amps = 42 amps + I₄. So I₄ equals -14 amps. But how could we get a negative current? Getting a negative current is physically (no pun intended) impossible, but when our current comes out negative, it simply lets us know that we guessed the direction of I₄ incorrectly. We assumed that the unknown current flows out instead of into the node when, in fact, the current flows into the node. Therefore the amount of current that flows out of I₄ equals 14 amps.

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Figure 3

Ex. 3

The junction rule can be extended to more complicated problems such as when wires have a different cross-sectional areas or electron mobilities.

In Figure 3, we have three wires that are connected to a battery with emf = 1.5 V at steady state, but the thin wire and thick wire are made of different materials. The thin wire has an electron mobility of 4 x 10^-5 (m/s)(V/m) while the thick wire has an electron mobility of 8 x 10^-5. They both have an electron density of 6 x 10²⁸. The thin wire has a cross sectional area of 9 x 10^-8 m² and the thick wire has a cross sectional area of 6 x 10^-7 m². The length of each thin wire is 0.10 m and the length of the thick wire is 0.05 m.

Calculate the magnitude of the electric field at the center of the thick wire and the thin wires.

Using the node rule, we know that the conventional current flowing through the thick wire is equal to the conventional current flowing through the thin wire.

I_thick = I_thin

Plugging in our equation for conventional current:

|q|n_thickA_thicku_thickE_thick = |q|n_thinA_thinu_thinE_thin

Cancelling out the charge and electron density and rearranging the equation we find that:

E_thick =(A_thinu_thin/A_thicku_thick) * E_thin

= ([9 x 10^-8 m² * 4 x 10^-5 (m/s)(V/m)]/[6 x 10^-7 m² * 8 x 10^-5 (m/s)(V/m)]) * E_thin

E_thick = 0.075 * E_thin

Now that we know the corresponding ratios of the electric fields, we can apply the Loop Rule and solve.

emf - E_thinL_thin - E_thickL_thick - E_thinL_thin = 0

Combine and substitute E_thin:

emf - 2 * E_thinL_thin - 0.075 * E_thinL_thick = 0

emf - E_thin(2 * L_thin + 0.075 * L_thick) = 0

E_thin = emf/(2 * L_thin + 0.075 * L_thick) = 1.5/(2 * 0.1 + 0.075 * 0.05) = 7.36 V/m

E_thick = 0.075 * E_thin = 0.075 * 7.36 = 0.552 V/m

Limitations

Time-Varying Currents

Kirchhoff's law is based off the conservation of charge along with the nature of conductors. This law assumes that current will immediately flow from one end of the conductor to the other, which may not be true for time-varying currents, especially with higher frequencies.

Regions vs Circuits

Throughout a region, the charge can vary and be non-uniform, unlike in a wire. According to the law of conservation of charge, the only way to have a non-uniform charge density is if there is a net flow of current in or out of the region, which clearly violates the Node Rule. Therefore the node rule cannot be applied to regions with non-uniform charge densities. When looking at a junction in an electric circuit, we are looking at a point and therefore the point (which is infinitesimally small) must have a uniform charge distribution. In general, wires should have a uniform charge distribution across their length, because they are conductors and allow for the movement of charge.

Other Topics

Solving Circuits

In order to solve circuits, we must first define a couple characteristics of circuits.

The voltage of a (perfect, or non-resistive) wire is equal to its length (in meters) times its electric field.

The voltage of an ohmic resistor (including a resistive wire) is equal to current times resistance.

The voltage of a capacitor is equal to the charge on the capacitor divided by its capacitance.

There are other characteristics and equations that may be useful, but these two are the most important and used. If you are confused by any of the components of circuits mentioned above, visit the "Components" page. Below is a circuit. Using the node and loop rules we will find the current at points a, b, c, d, and e, and the charge on the capacitor after the switch has been closed for a very long time.

First you must realize that when the capacitor is fully charged, no current will flow through the capacitor, which is an important characteristic of a capacitor. From this we can say that the current through point c is 0.

Using the node rule, we can see that the current through resistor 1 and resistor 2 must be the same because, since no current flows through the wire connected the capacitor, all of the current must flow through one loop containing both resistors. So the current at a, b, d and e must all be the same. Due to the loop rule, the emf of the battery must be equal to I*R₁ + I*R₂. Therefore, I = emf/(R₁ + R₂); this is the current through points a, b, d and e. Using the loop rule, we can look at the loop containing the capacitor and resistor 2. We know the voltage in resistor 2 is equal to I*R₂. We know the voltage of the capacitor is equal to its charge divided by C (its capacitance). Because of the loop rule, we know that these two voltages must be equal, so I*R₂ = Q/C. Therefore, Q = I*R₂*C. Replacing I with the current we found above, Q = (emf/(R₁ + R₂))*R₂*C. As you can see, in order to solve this circuit, we had to use the node rule. In fact, we used the node rule at the very beginning of solving this circuit and there was no way possible we could have solved this problem without the node rule.

History

Gustav Kirchhoff was a German physicist who lived during the 19th century. There are many equations and laws named after him that he helped to discover, one of them being the node rule. His circuit laws (the node rule and loop rule) were the first laws that he conceived, and he actually did this during his years in school and later wrote his doctoral dissertation on them. He created these laws in a time where electricity was a fairly new concept and was not widely used. His other achievements included coining the term "black body" radiation in 1862, which would later lead to important findings in the field of thermal radiation. In addition to his circuit laws, he is also known for his law of thermochemistry and three laws of spectroscopy, the latter of which helped lead to quantum mechanics.

Connectedness

The Node Rule is connected to a lot of other topics in physics. The loop rule is the most important one, as the node rule and loop rule in conjunction allow us to solve circuits. The node rule is also connected to other concepts such as voltage, current and electricity. The Node Rule is also supports the law of conservation of energy because in essence, current is simply the flow of electric charge, and since you cannot (at least as of now) create energy or electrons out of nothing, everything that is put into the system must come out somehow. Therefore, all the current that is applied, must come out the other end.

See the "Further Reading" section to read more on these topics.

References

Matter & Interactions 4th Edition by Ruth W. Chabay & Bruce A. Sherwood

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 '''Claimed by Ingrid Cai '''
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 [[File:Junction.gif|thumb|The node (or junction) rule states that the current flowing in is equal to the current that flows out. I<sub>1</sub> + I<sub>4</sub> = I<sub>2</sub> + I<sub>3</sub> + I<sub>5</sub>]]