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University Physics Volume 2

7.2 Electric Potential and Potential Difference

University Physics Volume 27.2 Electric Potential and Potential Difference
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  1. Preface
  2. Unit 1. Thermodynamics
    1. 1 Temperature and Heat
      1. Introduction
      2. 1.1 Temperature and Thermal Equilibrium
      3. 1.2 Thermometers and Temperature Scales
      4. 1.3 Thermal Expansion
      5. 1.4 Heat Transfer, Specific Heat, and Calorimetry
      6. 1.5 Phase Changes
      7. 1.6 Mechanisms of Heat Transfer
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    2. 2 The Kinetic Theory of Gases
      1. Introduction
      2. 2.1 Molecular Model of an Ideal Gas
      3. 2.2 Pressure, Temperature, and RMS Speed
      4. 2.3 Heat Capacity and Equipartition of Energy
      5. 2.4 Distribution of Molecular Speeds
      6. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    3. 3 The First Law of Thermodynamics
      1. Introduction
      2. 3.1 Thermodynamic Systems
      3. 3.2 Work, Heat, and Internal Energy
      4. 3.3 First Law of Thermodynamics
      5. 3.4 Thermodynamic Processes
      6. 3.5 Heat Capacities of an Ideal Gas
      7. 3.6 Adiabatic Processes for an Ideal Gas
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    4. 4 The Second Law of Thermodynamics
      1. Introduction
      2. 4.1 Reversible and Irreversible Processes
      3. 4.2 Heat Engines
      4. 4.3 Refrigerators and Heat Pumps
      5. 4.4 Statements of the Second Law of Thermodynamics
      6. 4.5 The Carnot Cycle
      7. 4.6 Entropy
      8. 4.7 Entropy on a Microscopic Scale
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
  3. Unit 2. Electricity and Magnetism
    1. 5 Electric Charges and Fields
      1. Introduction
      2. 5.1 Electric Charge
      3. 5.2 Conductors, Insulators, and Charging by Induction
      4. 5.3 Coulomb's Law
      5. 5.4 Electric Field
      6. 5.5 Calculating Electric Fields of Charge Distributions
      7. 5.6 Electric Field Lines
      8. 5.7 Electric Dipoles
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
    2. 6 Gauss's Law
      1. Introduction
      2. 6.1 Electric Flux
      3. 6.2 Explaining Gauss’s Law
      4. 6.3 Applying Gauss’s Law
      5. 6.4 Conductors in Electrostatic Equilibrium
      6. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    3. 7 Electric Potential
      1. Introduction
      2. 7.1 Electric Potential Energy
      3. 7.2 Electric Potential and Potential Difference
      4. 7.3 Calculations of Electric Potential
      5. 7.4 Determining Field from Potential
      6. 7.5 Equipotential Surfaces and Conductors
      7. 7.6 Applications of Electrostatics
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    4. 8 Capacitance
      1. Introduction
      2. 8.1 Capacitors and Capacitance
      3. 8.2 Capacitors in Series and in Parallel
      4. 8.3 Energy Stored in a Capacitor
      5. 8.4 Capacitor with a Dielectric
      6. 8.5 Molecular Model of a Dielectric
      7. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    5. 9 Current and Resistance
      1. Introduction
      2. 9.1 Electrical Current
      3. 9.2 Model of Conduction in Metals
      4. 9.3 Resistivity and Resistance
      5. 9.4 Ohm's Law
      6. 9.5 Electrical Energy and Power
      7. 9.6 Superconductors
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    6. 10 Direct-Current Circuits
      1. Introduction
      2. 10.1 Electromotive Force
      3. 10.2 Resistors in Series and Parallel
      4. 10.3 Kirchhoff's Rules
      5. 10.4 Electrical Measuring Instruments
      6. 10.5 RC Circuits
      7. 10.6 Household Wiring and Electrical Safety
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    7. 11 Magnetic Forces and Fields
      1. Introduction
      2. 11.1 Magnetism and Its Historical Discoveries
      3. 11.2 Magnetic Fields and Lines
      4. 11.3 Motion of a Charged Particle in a Magnetic Field
      5. 11.4 Magnetic Force on a Current-Carrying Conductor
      6. 11.5 Force and Torque on a Current Loop
      7. 11.6 The Hall Effect
      8. 11.7 Applications of Magnetic Forces and Fields
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    8. 12 Sources of Magnetic Fields
      1. Introduction
      2. 12.1 The Biot-Savart Law
      3. 12.2 Magnetic Field Due to a Thin Straight Wire
      4. 12.3 Magnetic Force between Two Parallel Currents
      5. 12.4 Magnetic Field of a Current Loop
      6. 12.5 Ampère’s Law
      7. 12.6 Solenoids and Toroids
      8. 12.7 Magnetism in Matter
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    9. 13 Electromagnetic Induction
      1. Introduction
      2. 13.1 Faraday’s Law
      3. 13.2 Lenz's Law
      4. 13.3 Motional Emf
      5. 13.4 Induced Electric Fields
      6. 13.5 Eddy Currents
      7. 13.6 Electric Generators and Back Emf
      8. 13.7 Applications of Electromagnetic Induction
      9. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    10. 14 Inductance
      1. Introduction
      2. 14.1 Mutual Inductance
      3. 14.2 Self-Inductance and Inductors
      4. 14.3 Energy in a Magnetic Field
      5. 14.4 RL Circuits
      6. 14.5 Oscillations in an LC Circuit
      7. 14.6 RLC Series Circuits
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    11. 15 Alternating-Current Circuits
      1. Introduction
      2. 15.1 AC Sources
      3. 15.2 Simple AC Circuits
      4. 15.3 RLC Series Circuits with AC
      5. 15.4 Power in an AC Circuit
      6. 15.5 Resonance in an AC Circuit
      7. 15.6 Transformers
      8. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
    12. 16 Electromagnetic Waves
      1. Introduction
      2. 16.1 Maxwell’s Equations and Electromagnetic Waves
      3. 16.2 Plane Electromagnetic Waves
      4. 16.3 Energy Carried by Electromagnetic Waves
      5. 16.4 Momentum and Radiation Pressure
      6. 16.5 The Electromagnetic Spectrum
      7. Chapter Review
        1. Key Terms
        2. Key Equations
        3. Summary
        4. Conceptual Questions
        5. Problems
        6. Additional Problems
        7. Challenge Problems
  4. A | Units
  5. B | Conversion Factors
  6. C | Fundamental Constants
  7. D | Astronomical Data
  8. E | Mathematical Formulas
  9. F | Chemistry
  10. G | The Greek Alphabet
  11. Answer Key
    1. Chapter 1
    2. Chapter 2
    3. Chapter 3
    4. Chapter 4
    5. Chapter 5
    6. Chapter 6
    7. Chapter 7
    8. Chapter 8
    9. Chapter 9
    10. Chapter 10
    11. Chapter 11
    12. Chapter 12
    13. Chapter 13
    14. Chapter 14
    15. Chapter 15
    16. Chapter 16
  12. Index

Learning Objectives

By the end of this section, you will be able to:
  • Define electric potential, voltage, and potential difference
  • Define the electron-volt
  • Calculate electric potential and potential difference from potential energy and electric field
  • Describe systems in which the electron-volt is a useful unit
  • Apply conservation of energy to electric systems

Recall that earlier we defined electric field to be a quantity independent of the test charge in a given system, which would nonetheless allow us to calculate the force that would result on an arbitrary test charge. (The default assumption in the absence of other information is that the test charge is positive.) We briefly defined a field for gravity, but gravity is always attractive, whereas the electric force can be either attractive or repulsive. Therefore, although potential energy is perfectly adequate in a gravitational system, it is convenient to define a quantity that allows us to calculate the work on a charge independent of the magnitude of the charge. Calculating the work directly may be difficult, since W=F·dW=F·d and the direction and magnitude of FF can be complex for multiple charges, for odd-shaped objects, and along arbitrary paths. But we do know that because F=qEF=qE, the work, and hence ΔU,ΔU, is proportional to the test charge q. To have a physical quantity that is independent of test charge, we define electric potential V (or simply potential, since electric is understood) to be the potential energy per unit charge:

Electric Potential

The electric potential energy per unit charge is

V=Uq.V=Uq.
(7.4)

Since U is proportional to q, the dependence on q cancels. Thus, V does not depend on q. The change in potential energy ΔUΔU is crucial, so we are concerned with the difference in potential or potential difference ΔVΔV between two points, where

ΔV=VBVA=ΔUq.ΔV=VBVA=ΔUq.

Electric Potential Difference

The electric potential difference between points A and B, VBVA,VBVA, is defined to be the change in potential energy of a charge q moved from A to B, divided by the charge. Units of potential difference are joules per coulomb, given the name volt (V) after Alessandro Volta.

1V=1J/C1V=1J/C

The familiar term voltage is the common name for electric potential difference. Keep in mind that whenever a voltage is quoted, it is understood to be the potential difference between two points. For example, every battery has two terminals, and its voltage is the potential difference between them. More fundamentally, the point you choose to be zero volts is arbitrary. This is analogous to the fact that gravitational potential energy has an arbitrary zero, such as sea level or perhaps a lecture hall floor. It is worthwhile to emphasize the distinction between potential difference and electrical potential energy.

Potential Difference and Electrical Potential Energy

The relationship between potential difference (or voltage) and electrical potential energy is given by

ΔV=ΔUqorΔU=qΔV.ΔV=ΔUqorΔU=qΔV.
(7.5)

Voltage is not the same as energy. Voltage is the energy per unit charge. Thus, a motorcycle battery and a car battery can both have the same voltage (more precisely, the same potential difference between battery terminals), yet one stores much more energy than the other because ΔU=qΔV.ΔU=qΔV. The car battery can move more charge than the motorcycle battery, although both are 12-V batteries.

Example 7.4

Calculating Energy You have a 12.0-V motorcycle battery that can move 5000 C of charge, and a 12.0-V car battery that can move 60,000 C of charge. How much energy does each deliver? (Assume that the numerical value of each charge is accurate to three significant figures.)

Strategy To say we have a 12.0-V battery means that its terminals have a 12.0-V potential difference. When such a battery moves charge, it puts the charge through a potential difference of 12.0 V, and the charge is given a change in potential energy equal to ΔU=qΔV.ΔU=qΔV. To find the energy output, we multiply the charge moved by the potential difference.

Solution For the motorcycle battery, q=5000Cq=5000C and ΔV=12.0VΔV=12.0V. The total energy delivered by the motorcycle battery is

ΔUcycle=(5000C)(12.0V)=(5000C)(12.0J/C)=6.00×104J.ΔUcycle=(5000C)(12.0V)=(5000C)(12.0J/C)=6.00×104J.

Similarly, for the car battery, q=60,000Cq=60,000C and

ΔUcar=(60,000C)(12.0V)=7.20×105J.ΔUcar=(60,000C)(12.0V)=7.20×105J.

Significance Voltage and energy are related, but they are not the same thing. The voltages of the batteries are identical, but the energy supplied by each is quite different. A car battery has a much larger engine to start than a motorcycle. Note also that as a battery is discharged, some of its energy is used internally and its terminal voltage drops, such as when headlights dim because of a depleted car battery. The energy supplied by the battery is still calculated as in this example, but not all of the energy is available for external use.

Check Your Understanding 7.4

How much energy does a 1.5-V AAA battery have that can move 100 C?

Note that the energies calculated in the previous example are absolute values. The change in potential energy for the battery is negative, since it loses energy. These batteries, like many electrical systems, actually move negative charge—electrons in particular. The batteries repel electrons from their negative terminals (A) through whatever circuitry is involved and attract them to their positive terminals (B), as shown in Figure 7.12. The change in potential is ΔV=VBVA=+12VΔV=VBVA=+12V and the charge q is negative, so that ΔU=qΔVΔU=qΔV is negative, meaning the potential energy of the battery has decreased when q has moved from A to B.

The figure shows a headlight connected to terminals of a 12V battery. The charge q flows out from terminal A of the battery and back into terminal B of the battery.
Figure 7.12 A battery moves negative charge from its negative terminal through a headlight to its positive terminal. Appropriate combinations of chemicals in the battery separate charges so that the negative terminal has an excess of negative charge, which is repelled by it and attracted to the excess positive charge on the other terminal. In terms of potential, the positive terminal is at a higher voltage than the negative terminal. Inside the battery, both positive and negative charges move.

Example 7.5

How Many Electrons Move through a Headlight Each Second? When a 12.0-V car battery powers a single 30.0-W headlight, how many electrons pass through it each second?

Strategy To find the number of electrons, we must first find the charge that moves in 1.00 s. The charge moved is related to voltage and energy through the equations ΔU=qΔV.ΔU=qΔV. A 30.0-W lamp uses 30.0 joules per second. Since the battery loses energy, we have ΔU=−30JΔU=−30J and, since the electrons are going from the negative terminal to the positive, we see that ΔV=+12.0V.ΔV=+12.0V.

Solution To find the charge q moved, we solve the equation ΔU=qΔV:ΔU=qΔV:

q=ΔUΔV.q=ΔUΔV.

Entering the values for ΔUΔU and ΔVΔV, we get

q=−30.0J+12.0V=−30.0J+12.0J/C=−2.50C.q=−30.0J+12.0V=−30.0J+12.0J/C=−2.50C.

The number of electrons nene is the total charge divided by the charge per electron. That is,

ne=−2.50C−1.60×10−19C/e=1.56×1019electrons.ne=−2.50C−1.60×10−19C/e=1.56×1019electrons.

Significance This is a very large number. It is no wonder that we do not ordinarily observe individual electrons with so many being present in ordinary systems. In fact, electricity had been in use for many decades before it was determined that the moving charges in many circumstances were negative. Positive charge moving in the opposite direction of negative charge often produces identical effects; this makes it difficult to determine which is moving or whether both are moving.

Check Your Understanding 7.5

How many electrons would go through a 24.0-W lamp?

The Electron-Volt

The energy per electron is very small in macroscopic situations like that in the previous example—a tiny fraction of a joule. But on a submicroscopic scale, such energy per particle (electron, proton, or ion) can be of great importance. For example, even a tiny fraction of a joule can be great enough for these particles to destroy organic molecules and harm living tissue. The particle may do its damage by direct collision, or it may create harmful X-rays, which can also inflict damage. It is useful to have an energy unit related to submicroscopic effects.

Figure 7.13 shows a situation related to the definition of such an energy unit. An electron is accelerated between two charged metal plates, as it might be in an old-model television tube or oscilloscope. The electron gains kinetic energy that is later converted into another form—light in the television tube, for example. (Note that in terms of energy, “downhill” for the electron is “uphill” for a positive charge.) Since energy is related to voltage by ΔU=qΔVΔU=qΔV, we can think of the joule as a coulomb-volt.

Part a shows an electron gun with two metal plates and an electron between the plates. The metal plates are connected to terminals of a battery and have opposite charges with a potential difference V subscript AB. Part b shows the photo of an electron gun.
Figure 7.13 A typical electron gun accelerates electrons using a potential difference between two separated metal plates. By conservation of energy, the kinetic energy has to equal the change in potential energy, so KE=qVKE=qV. The energy of the electron in electron-volts is numerically the same as the voltage between the plates. For example, a 5000-V potential difference produces 5000-eV electrons. The conceptual construct, namely two parallel plates with a hole in one, is shown in (a), while a real electron gun is shown in (b).

Electron-Volt

On the submicroscopic scale, it is more convenient to define an energy unit called the electron-volt (eV), which is the energy given to a fundamental charge accelerated through a potential difference of 1 V. In equation form,

1eV=(1.60×10−19C)(1V)=(1.60×10−19C)(1J/C)=1.60×10−19J.1eV=(1.60×10−19C)(1V)=(1.60×10−19C)(1J/C)=1.60×10−19J.

An electron accelerated through a potential difference of 1 V is given an energy of 1 eV. It follows that an electron accelerated through 50 V gains 50 eV. A potential difference of 100,000 V (100 kV) gives an electron an energy of 100,000 eV (100 keV), and so on. Similarly, an ion with a double positive charge accelerated through 100 V gains 200 eV of energy. These simple relationships between accelerating voltage and particle charges make the electron-volt a simple and convenient energy unit in such circumstances.

The electron-volt is commonly employed in submicroscopic processes—chemical valence energies and molecular and nuclear binding energies are among the quantities often expressed in electron-volts. For example, about 5 eV of energy is required to break up certain organic molecules. If a proton is accelerated from rest through a potential difference of 30 kV, it acquires an energy of 30 keV (30,000 eV) and can break up as many as 6000 of these molecules (30,000eV÷5eVper molecule=6000molecules).(30,000eV÷5eVper molecule=6000molecules). Nuclear decay energies are on the order of 1 MeV (1,000,000 eV) per event and can thus produce significant biological damage.

Conservation of Energy

The total energy of a system is conserved if there is no net addition (or subtraction) due to work or heat transfer. For conservative forces, such as the electrostatic force, conservation of energy states that mechanical energy is a constant.

Mechanical energy is the sum of the kinetic energy and potential energy of a system; that is, K+U=constant.K+U=constant. A loss of U for a charged particle becomes an increase in its K. Conservation of energy is stated in equation form as

K+U=constantK+U=constant

or

Ki+Ui=Kf+UfKi+Ui=Kf+Uf

where i and f stand for initial and final conditions. As we have found many times before, considering energy can give us insights and facilitate problem solving.

Example 7.6

Electrical Potential Energy Converted into Kinetic Energy Calculate the final speed of a free electron accelerated from rest through a potential difference of 100 V. (Assume that this numerical value is accurate to three significant figures.)

Strategy We have a system with only conservative forces. Assuming the electron is accelerated in a vacuum, and neglecting the gravitational force (we will check on this assumption later), all of the electrical potential energy is converted into kinetic energy. We can identify the initial and final forms of energy to be Ki=0,Kf=12mv2,Ui=qV,Uf=0.Ki=0,Kf=12mv2,Ui=qV,Uf=0.

Solution Conservation of energy states that

Ki+Ui=Kf+Uf.Ki+Ui=Kf+Uf.

Entering the forms identified above, we obtain

qV=mv22.qV=mv22.

We solve this for v:

v=2qVm.v=2qVm.

Entering values for q, V, and m gives

v=2(−1.60×10−19C)(100J/C)9.11×10−31kg=5.93×106m/s.v=2(−1.60×10−19C)(100J/C)9.11×10−31kg=5.93×106m/s.

Significance Note that both the charge and the initial voltage are negative, as in Figure 7.13. From the discussion of electric charge and electric field, we know that electrostatic forces on small particles are generally very large compared with the gravitational force. The large final speed confirms that the gravitational force is indeed negligible here. The large speed also indicates how easy it is to accelerate electrons with small voltages because of their very small mass. Voltages much higher than the 100 V in this problem are typically used in electron guns. These higher voltages produce electron speeds so great that effects from special relativity must be taken into account and hence are reserved for a later chapter (Relativity). That is why we consider a low voltage (accurately) in this example.

Check Your Understanding 7.6

How would this example change with a positron? A positron is identical to an electron except the charge is positive.

Voltage and Electric Field

So far, we have explored the relationship between voltage and energy. Now we want to explore the relationship between voltage and electric field. We will start with the general case for a non-uniform EE field. Recall that our general formula for the potential energy of a test charge q at point P relative to reference point R is

UP=RPF·dl.UP=RPF·dl.

When we substitute in the definition of electric field (E=F/q),(E=F/q), this becomes

UP=qRPE·dl.UP=qRPE·dl.

Applying our definition of potential (V=U/q)(V=U/q) to this potential energy, we find that, in general,

VP=RPE·dl.VP=RPE·dl.
(7.6)

From our previous discussion of the potential energy of a charge in an electric field, the result is independent of the path chosen, and hence we can pick the integral path that is most convenient.

Consider the special case of a positive point charge q at the origin. To calculate the potential caused by q at a distance r from the origin relative to a reference of 0 at infinity (recall that we did the same for potential energy), let P=rP=r and R=,R=, with dl=dr=r^drdl=dr=r^dr and use E=kqr2r^.E=kqr2r^. When we evaluate the integral

VP=RPE·dlVP=RPE·dl

for this system, we have

Vr=rkqr2r^·r^dr,Vr=rkqr2r^·r^dr,

which simplifies to

Vr=rkqr2dr=kqrkq=kqr.Vr=rkqr2dr=kqrkq=kqr.

This result,

Vr=kqrVr=kqr

is the standard form of the potential of a point charge. This will be explored further in the next section.

To examine another interesting special case, suppose a uniform electric field EE is produced by placing a potential difference (or voltage) ΔVΔV across two parallel metal plates, labeled A and B (Figure 7.14). Examining this situation will tell us what voltage is needed to produce a certain electric field strength. It will also reveal a more fundamental relationship between electric potential and electric field.

The figure shows electric field between two plates (A and B) with opposite charges. The plates are separated by distance d and have a potential difference V subscript AB. A positive charge q is located between the plates and moves from A to B.
Figure 7.14 The relationship between V and E for parallel conducting plates is E=V/dE=V/d. (Note that ΔV=VABΔV=VAB in magnitude. For a charge that is moved from plate A at higher potential to plate B at lower potential, a minus sign needs to be included as follows: ΔV=VAVB=VAB.ΔV=VAVB=VAB.)

From a physicist’s point of view, either ΔVΔV or EE can be used to describe any interaction between charges. However, ΔVΔV is a scalar quantity and has no direction, whereas EE is a vector quantity, having both magnitude and direction. (Note that the magnitude of the electric field, a scalar quantity, is represented by E.) The relationship between ΔVΔV and EE is revealed by calculating the work done by the electric force in moving a charge from point A to point B. But, as noted earlier, arbitrary charge distributions require calculus. We therefore look at a uniform electric field as an interesting special case.

The work done by the electric field in Figure 7.14 to move a positive charge q from A, the positive plate, higher potential, to B, the negative plate, lower potential, is

W=ΔU=qΔV.W=ΔU=qΔV.

The potential difference between points A and B is

ΔV=(VBVA)=VAVB=VAB.ΔV=(VBVA)=VAVB=VAB.

Entering this into the expression for work yields

W=qVAB.W=qVAB.

Work is W=F·d=FdcosθW=F·d=Fdcosθ; here cosθ=1cosθ=1, since the path is parallel to the field. Thus, W=FdW=Fd. Since F=qEF=qE, we see that W=qEdW=qEd.

Substituting this expression for work into the previous equation gives

qEd=qVAB.qEd=qVAB.

The charge cancels, so we obtain for the voltage between points A and B

VAB=EdE=VABd}(uniformE-field only)VAB=EdE=VABd}(uniformE-field only)

where d is the distance from A to B, or the distance between the plates in Figure 7.14. Note that this equation implies that the units for electric field are volts per meter. We already know the units for electric field are newtons per coulomb; thus, the following relation among units is valid:

1N/C=1V/m.1N/C=1V/m.

Furthermore, we may extend this to the integral form. Substituting Equation 7.5 into our definition for the potential difference between points A and B, we obtain

VBA=VBVA=RBE·dl+RAE·dlVBA=VBVA=RBE·dl+RAE·dl

which simplifies to

VBVA=ABE·dl.VBVA=ABE·dl.

As a demonstration, from this we may calculate the potential difference between two points (A and B) equidistant from a point charge q at the origin, as shown in Figure 7.15.

The figure shows a charge q equidistant from two points, A and B.
Figure 7.15 The arc for calculating the potential difference between two points that are equidistant from a point charge at the origin.

To do this, we integrate around an arc of the circle of constant radius r between A and B, which means we let dl=rφ^dφ,dl=rφ^dφ, while using E=kqr2r^E=kqr2r^. Thus,

ΔVBA=VBVA=ABE·dlΔVBA=VBVA=ABE·dl
(7.7)

for this system becomes

VBVA=ABkqr2r^·rφ^dφ.VBVA=ABkqr2r^·rφ^dφ.

However, r^·φ^=0r^·φ^=0 and therefore

VBVA=0.VBVA=0.

This result, that there is no difference in potential along a constant radius from a point charge, will come in handy when we map potentials.

Example 7.7

What Is the Highest Voltage Possible between Two Plates? Dry air can support a maximum electric field strength of about 3.0×106V/m.3.0×106V/m. Above that value, the field creates enough ionization in the air to make the air a conductor. This allows a discharge or spark that reduces the field. What, then, is the maximum voltage between two parallel conducting plates separated by 2.5 cm of dry air?

Strategy We are given the maximum electric field E between the plates and the distance d between them. We can use the equation VAB=EdVAB=Ed to calculate the maximum voltage.

Solution The potential difference or voltage between the plates is

VAB=Ed.VAB=Ed.

Entering the given values for E and d gives

VAB=(3.0×106V/m)(0.025m)=7.5×104VVAB=(3.0×106V/m)(0.025m)=7.5×104V

or

VAB=75kV.VAB=75kV.

(The answer is quoted to only two digits, since the maximum field strength is approximate.)

Significance One of the implications of this result is that it takes about 75 kV to make a spark jump across a 2.5-cm (1-in.) gap, or 150 kV for a 5-cm spark. This limits the voltages that can exist between conductors, perhaps on a power transmission line. A smaller voltage can cause a spark if there are spines on the surface, since sharp points have larger field strengths than smooth surfaces. Humid air breaks down at a lower field strength, meaning that a smaller voltage will make a spark jump through humid air. The largest voltages can be built up with static electricity on dry days (Figure 7.16).

The first photo shows a spark chamber and the second photo shows its operation.
Figure 7.16 A spark chamber is used to trace the paths of high-energy particles. Ionization created by the particles as they pass through the gas between the plates allows a spark to jump. The sparks are perpendicular to the plates, following electric field lines between them. The potential difference between adjacent plates is not high enough to cause sparks without the ionization produced by particles from accelerator experiments (or cosmic rays). This form of detector is now archaic and no longer in use except for demonstration purposes. (credit b: modification of work by Jack Collins)

Example 7.8

Field and Force inside an Electron Gun An electron gun (Figure 7.13) has parallel plates separated by 4.00 cm and gives electrons 25.0 keV of energy. (a) What is the electric field strength between the plates? (b) What force would this field exert on a piece of plastic with a 0.500-μC0.500-μC charge that gets between the plates?

Strategy Since the voltage and plate separation are given, the electric field strength can be calculated directly from the expression E=VABdE=VABd. Once we know the electric field strength, we can find the force on a charge by using F=qE.F=qE. Since the electric field is in only one direction, we can write this equation in terms of the magnitudes, F=qEF=qE.

Solution

  1. The expression for the magnitude of the electric field between two uniform metal plates is
    E=VABd.E=VABd.

    Since the electron is a single charge and is given 25.0 keV of energy, the potential difference must be 25.0 kV. Entering this value for VABVAB and the plate separation of 0.0400 m, we obtain
    E=25.0kV0.0400m=6.25×105V/m.E=25.0kV0.0400m=6.25×105V/m.
  2. The magnitude of the force on a charge in an electric field is obtained from the equation
    F=qE.F=qE.

    Substituting known values gives
    F=(0.500×10−6C)(6.25×105V/m)=0.313N.F=(0.500×10−6C)(6.25×105V/m)=0.313N.

Significance Note that the units are newtons, since 1V/m=1N/C1V/m=1N/C. Because the electric field is uniform between the plates, the force on the charge is the same no matter where the charge is located between the plates.

Example 7.9

Calculating Potential of a Point Charge Given a point charge q=+2.0nCq=+2.0nC at the origin, calculate the potential difference between point P1P1 a distance a=4.0cma=4.0cm from q, and P2P2 a distance b=12.0cmb=12.0cm from q, where the two points have an angle of φ=24°φ=24° between them (Figure 7.17).

The figure shows two points P subscript 1 and P subscript 2 at distances a and b from the origin and having an angle phi between them.
Figure 7.17 Find the difference in potential between P1P1 and P2P2.

Strategy Do this in two steps. The first step is to use VBVA=ABE·dlVBVA=ABE·dl and let A=a=4.0cmA=a=4.0cm and B=b=12.0cm,B=b=12.0cm, with dl=dr=r^drdl=dr=r^dr and E=kqr2r^.E=kqr2r^. Then perform the integral. The second step is to integrate VBVA=ABE·dlVBVA=ABE·dl around an arc of constant radius r, which means we let dl=rφ^dφdl=rφ^dφ with limits 0φ24°,0φ24°, still using E=kqr2r^E=kqr2r^. Then add the two results together.

Solution For the first part, VBVA=ABE·dlVBVA=ABE·dl for this system becomes VbVa=abkqr2r^·r^drVbVa=abkqr2r^·r^dr which computes to

ΔV=abkqr2dr=kq[1a1b]=(8.99×109Nm2/C2)(2.0×10−9C)[10.040m10.12m]=300V.ΔV=abkqr2dr=kq[1a1b]=(8.99×109Nm2/C2)(2.0×10−9C)[10.040m10.12m]=300V.

For the second step, VBVA=ABE·dlVBVA=ABE·dl becomes ΔV=024°kqr2r^·rφ^dφΔV=024°kqr2r^·rφ^dφ, but r^·φ^=0r^·φ^=0 and therefore ΔV=0.ΔV=0. Adding the two parts together, we get 300 V.

Significance We have demonstrated the use of the integral form of the potential difference to obtain a numerical result. Notice that, in this particular system, we could have also used the formula for the potential due to a point charge at the two points and simply taken the difference.

Check Your Understanding 7.7

From the examples, how does the energy of a lightning strike vary with the height of the clouds from the ground? Consider the cloud-ground system to be two parallel plates.

Before presenting problems involving electrostatics, we suggest a problem-solving strategy to follow for this topic.

Problem-Solving Strategy: Electrostatics

  1. Examine the situation to determine if static electricity is involved; this may concern separated stationary charges, the forces among them, and the electric fields they create.
  2. Identify the system of interest. This includes noting the number, locations, and types of charges involved.
  3. Identify exactly what needs to be determined in the problem (identify the unknowns). A written list is useful. Determine whether the Coulomb force is to be considered directly—if so, it may be useful to draw a free-body diagram, using electric field lines.
  4. Make a list of what is given or can be inferred from the problem as stated (identify the knowns). It is important to distinguish the Coulomb force F from the electric field E, for example.
  5. Solve the appropriate equation for the quantity to be determined (the unknown) or draw the field lines as requested.
  6. Examine the answer to see if it is reasonable: Does it make sense? Are units correct and the numbers involved reasonable?
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