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LECTURES IN PHYSICS OF ELECTROMAGNETIC THEORY (ELECTRODYNAMICS) COMPILED BY DR. RAMADAN MOHAMMAD SALEM DEPARTMENT OF PHYSICS, FACULTY OF SCIENCE, ASWAN UNIVERSITY COURSES ELECTRODYNAMICS (PHYS303): 3RD YEAR PHYSICS, 1ST TERM ELECTROMAGNETIC THEORY (PHYS304): 3RD YEAR PHYSICS, 2ND TERM Ramose@Aswan©2021

Ramose@Aswan©2021

Contents Cover page Course syllabus References list Web sites Preface Introduction Electric fields Gauss’s law Electric flux and Gauss’s law (video) Electrostatic potential Energy stored in electric field Continuity equation Magnetostatics Electrodynamics Electromagnetics Energy stored in magnetic field Maxwell’s equations

Vector analysis Electrostatics Electric field in matter …………………………………………….. ……………………………………….

Preface Although my mother language is Arabic, I compile this book in English from two main references because the Arabic is not a scientific language, as people think. Early I’m tried to write the book in Arabic language with English thinking by Arabization method not translation, but the experiment was failed rapidly, and it cannot prevent the resistance to publish because I’m writing, not compiling, by hand writing. Finally after five years the same topic (electromagnetic theory) I’m deciding to compile from English sources with language thinking to understand this complex theory. Electromagnetic theory is a complex theory to understand for students because, I think, it includes a lot of mathematical treatments, these treatments are not alone, they based on the physical understanding of electricity and magnetism. Therefore, I select the word “physics” in the beginning of the book title. The complex part of this theory includes the vector analysis and mainly the meaning of differential vector operator, the only and main operator I think found in this topic. When I decided to select a title of the book, I’m searching on the internet about the available titles and I’m finding a titles like “mathematical foundations of electromagnetic theory”, “introduction to electromagnetic theory”, etc. but I did not found any title related to physics. Then I’m compiling the information in this book from introductory physics book (Serway, 8th ed., 2010) and from advanced one (Griffith, 3rd ed., 1999) to begin the topic with physical meaning in electricity and magnetism. The main topic I concentrated in this book is the Maxwell’s equations, which are incredible equations like Newton’s laws of motion. To obtain and explain these equations physically with mathematical meaning, the book begin in introductory level “electricity and magnetism” and gradually study the same topic with advanced view by study carefully the vector analysis to convert the study from physics to mathematics in electromagnetic theory.

Electrostatics, magnetostatics, electromagnetics and electrodynamics are the main topics studied carefully with physical meaning to achieve the remaining of the book. Maxwell’s equations were obtained in different forms, which are symmetrical form (I named physical form because their derivations are based on the physical understanding the laws of electricity and magnetism), integral form by studying the charge density, flux density and current density, differential form by introducing the differential vector operator “del or nabla”. Based on the differential form of Maxwell’s equations, the study progressed to advance topics like electromagnetic waves “solution of Maxwell’s equations in different form mainly differential”, continuity equation of charge “conservation law of charge”, Poynting vector “conservation law of energy” etc. Finally at advanced level the following topics are studied; potential and field, retarded potential and interaction of electromagnetic waves with matter. The target audiences are the students of Physics Department at Faculty of Science for three level for studying three courses: electricity and magnetism, electrodynamics and electromagnetic theory. The main philosophy of this book is based on the sayed “Every pot exudes what it contains” Ramadan Mohamad Salem 03072021 Aswan, Egypt

Physics of electromagnetic theory Contents Preface Introduction Chapter (1): Electrostatics Electric charges Electric force: Coulomb’s law) Electric field Electric field lines Electric flux Gauss’s law in electricity Gauss’s theorem Energy stored in electric field Electric potential (line integral) Chapter (2): Magnetostatics Magnetic charges Magnetic force Magnetic field

Magnetic flux Gauss’s law in magnetism Gauss’s theorem Magnetic potential (line integral) Chapter (3): Electromagnetics Faraday’s law Chapter (4): Electrodynamics Electric current and current density Microscopic model of the current Ohm’s law Charge continuity equation Electric power density Biot-Savart law Magnetic field due to thin, straight conductor Ampere’s law Ampere-Maxwell law

Introduction The history of electromagnetic theory begins with ancient measures to understand atmospheric electricity, in particular lightning.[1] People then had little understanding of electricity, and were unable to explain the phenomena. Scientific understanding into the nature of electricity grew throughout the eighteenth and nineteenth centuries through the work of researchers such as Coulomb, Ampère, Faraday and Maxwell. In the 19th century it had become clear that electricity and magnetism were related, and their theories were unified: wherever charges are in motion electric current results, and magnetism is due to electric current. The source for electric field is electric charge, whereas that for magnetic field is electric current (charges in motion). In the first half of the 19th century many very important additions were made to the world's knowledge concerning electricity and magnetism. For example, in 1820 Hans Christian Ørsted of Copenhagen discovered the deflecting effect of an electric current traversing a wire upon- a suspended magnetic needle. In 1864 James Clerk Maxwell of Edinburgh announced his electromagnetic theory of light, which was perhaps the greatest single step in the world's knowledge of electricity. Maxwell had studied and commented on the field of electricity and magnetism. Around 1862, while lecturing at King's College, Maxwell calculated that the speed of propagation of an electromagnetic field is approximately that of the speed of light. He considered this to be more than just a coincidence, and commented \"We can scarcely avoid the conclusion that light consists in the transverse undulations of the same medium which is the cause of electric and magnetic phenomena. Working on the problem further, Maxwell showed that the equations predict the existence of waves of oscillating electric and magnetic fields that travel through empty space at a speed that could be predicted from simple electrical experiments; using the data available at the time, Maxwell obtained a velocity of 310,740,000 m/s. In his 1864 paper A Dynamical Theory of the Electromagnetic Field, Maxwell wrote, The agreement of the results seems to show that light and magnetism are affections of the same substance, and that light is an

electromagnetic disturbance propagated through the field according to electromagnetic laws……………………………………………….. https://en.wikipedia.org/wiki/History_of_electromagnetic_theory The laws of electricity and magnetism 1-Gauss’s law of electricity ∮ (1) 2-Gauss’s law of magnetism (2) ∮ (3) 3-Faraday’s law of induction ∮ 4-Ampere’s law (4) ∮ Modification of Ampere’s law by Maxwell (Ampere- Maxwell law) – displacement current ∮ (5)

Maxwell’s equation (integral form) Charge density (line, surface, and volume charge density) – open path begin at point a and end at point b l(a,b) closed path L (enclose open surface S) L(S) closed surface A (enclose volume V) A(V) Volume V is enclosed within a closed surface A (A(V)) Open surface S is enclosed within a closed path L (L(S)) Electric volume charge density (6) ∫ (7) Substitution from Eq(8) in Eq(1), then (8) ∮ (∫ ) (9) ∮ (10) ∫ The left side of Eq(7) can be written as

∮ (8) ∫ (9) Then Eq (10) can be written as Eq (9) is the differential form of first Maxwell’s equation On the other hand Eq(8) can be written as ∮ ∫( ) (10)) Eq (8) is the divergence theorem (Gauss’s theorem)

1 Electrostatic fields In this chapter, we begin the study of electromagnetism. The link to our previous study is through the concept of force. The electromagnetic force between charged particles is one of the fundamental forces of nature. We begin by describing some basic properties of one manifestation of the electromagnetic force, the electric force. We then discuss Coulomb’s law, which is the fundamental law governing the electric force between any two charged particles. Next, we introduce the concept of an electric field associated with a charge distribution and describe its effect on other charged particles. We then show how to use Coulomb’s law to calculate the electric field for a given charge distribution. Properties of electric charges A number of simple experiments demonstrate the existence of electric forces. For example, after rubbing a balloon on your hair on a dry day, you will find that the balloon attracts bits of paper. The attractive force is often strong enough to suspend the paper from the balloon. When materials behave in this way, they are said to be electrified or to have become electrically charged. You can easily electrify your body by vigorously rubbing your shoes on a wool rug. Evidence of the electric charge on your body can be detected by lightly touching (and startling) a friend. Under the right conditions, you will see a spark when you touch and both of you will feel a slight tingle. (Experiments such as these work best on a dry day because an excessive amount of moisture in the air can cause any charge you build up to ―leak‖ from your body to the Earth.) In a series of simple experiments, it was found that there are two kinds of electric charges, which were given the names positive and negative by Benjamin Franklin (1706–1790). On the basis of experimental observations, we conclude that charges of the same sign repel one another and charges with opposite signs attract one another.

2 Charge is conserved Another important aspect of electricity that arises from experimental observations is that electric charge is always conserved in an isolated system. That is, when one object is rubbed against another, charge is not created in the process. The electrified state is due to a transfer of charge from one object to the other. One object gains some amount of negative charge while the other gains an equal amount of positive charge. Charge is quantized In 1909, Robert Millikan (1868–1953) discovered that electric charge always occurs as integral multiples of a fundamental amount of charge e.In modern terms, the electric charge q is said to be quantized, where q is the standard symbol used for charge as a variable. That is, electric charge exists as discrete ―packets,‖ and we can write Where N is some integer. Other experiments in the same period showed that the electron has a charge -e and the proton has a charge of equal magnitude but opposite sign +e. Some particles, such as the neutron, have no charge.

3 Charge configurations: Continues charge distributions Very often, the distances between charges in a group of charges are much smaller than the distance from the group to a point where the electric field is to be calculated. In such situations, the system of charges can be modeled as continuous. That is, the system of closely spaced charges is equivalent to a total charge that is continuously distributed along some line, over some surface, or throughout some volume. it is convenient to use the concept of a charge density along with the following notations: 1- If a charge Q is uniformly distributed throughout a volume V, the volume charge density V is defined by where V has units of coulombs per cubic meter (C/m3). 2- If a charge Q is uniformly distributed on a surface of area S, the surface charge density S is defined by where S has units of coulombs per square meter (C/m2). 3- If a charge Q is uniformly distributed along a line of length l the linear charge density l is defined by where l has units of coulombs per meter (C/m)

4 Electric force: Coulomb’s law Charles Coulomb measured the magnitudes of the electric forces between charged objects. From Coulomb’s experiments, we can generalize the properties of the electric force (sometimes called the electrostatic force) between two stationary charged particles. We use the term point charge to refer to a charged particle of zero size. The electrical behavior of electrons and protons is very well described by modeling them as point charges. From experimental observations, we find that the magnitude of the electric force (sometimes called the Coulomb force) between two point charges is given by Coulomb’s law. where ke is a constant called the Coulomb constant. In his experiments. Experiments also show that the electric force, like the gravitational force, is conservative. The value of the Coulomb constant depends on the choice of units. The SI unit of charge is the coulomb (C). The Coulomb constant ke in SI units has the value This constant is also written in the form where the constant o (Greek letter epsilon) is known as the permittivity of free space and has the value The smallest unit of free charge e known in nature, the charge on an electron (-e) or a proton (+e), has a magnitude

5 Therefore, 1 C of charge is approximately equal to the charge of 6.24x1018 electrons or protons. This number is very small when compared with the number of free electrons in 1 cm3 of copper, which is on the order of 1023. Vector form of Coulomb’s law When dealing with Coulomb’s law, remember that force is a vector quantity and must be treated accordingly. Coulomb’s law expressed in vector form for the electric force exerted by a charge q1 on a second charge q2, written F12, is where r12 is a unit vector directed from q1 toward q2 as shown in Active Figure 23.6a. Because the electric force obeys Newton’s third law, the electric force exerted by q2 on q1 is equal in magnitude to the force exerted by q1 on q2 and in the opposite direction; that is, Finally, Coulomb’s law shows that if q1 and q2 have the same sign, the product q1q2 is positive and the electric force on one particle is directed away from the other particle. If q1 and q2 are of opposite sign, the product q1q2 is negative and the electric force on one particle is directed toward the other particle. These signs describe the relative direction of the force but not the absolute direction. A negative product indicates an attractive force, and a positive product indicates a repulsive force. The absolute direction of the force on a charge depends on the

6 location of the other charge. For example, if an x axis lies along the two charges, the product q1q2 is positive, but F12 points in the positive x direction and F21 points in the negative x direction. When more than two charges are present, the force between any pair of them is given by Equation 23.6. Therefore, the resultant force on any one of them equals the vector sum of the forces exerted by the other individual charges. For example, if four charges are present, the resultant force exerted by particles 2, 3, and 4 on particle 1 is The electric field The forces are classified as two types based on their effect, contact force and field force. The gravitational force and electric force are field forces. Field forces can act through space, producing an effect even when no physical contact occurs between interacting objects. The gravitational field g at a point in space due to a source particle was defined as the force acting on a test particle of mass m, i.e. the gravitational field equal to the gravitational for per unit mass In general the field is influence zone of force, in which the force affect. The gravitational field is the influence zone of gravitational force, the force affect inside this zone. The field of electric charge is the influence zone of electric force. The concept of a field was developed by Michael Faraday (1791–1867) in the context of electric forces. In this approach, an electric field is said to exist in the region of space around a charged object, the source charge. When another charged object—the test charge—enters this region, electric field, an electric force acts on it. As an example, consider the following Figure

7 A small positive test charge q0 placed at point P near an object carrying a much larger positive charge Q experiences an electric field E at point P established by the source charge Q. We will always assume that the test charge is so small that the field of the source charge is unaffected by its presence We define the electric field due to the source charge at the location of the test charge to be the electric force on the test charge per unit charge, or, to be more specific, the electric field vector E at a point in space is defined as the electric force Fe acting on a positive test charge q0 placed at that point divided by the test charge The vector E has the SI units of Newtons per Coulomb (N/C). The direction of E as shown in the Figure is the direction of the force a positive test charge experiences when placed in the field. Note that E is the field produced by some charge or charge distribution separate from the test charge; it is not the field produced by the test charge itself. Also note that the existence of an electric field is a property of its source; the presence of the test charge is not necessary for the field to exist. The test charge serves as a detector of the electric field: an electric field exists at a point if a test charge at that point experiences an electric force. From equation ( ), the electric force is given by

8 This equation gives us the force on a charged particle q placed in an electric field. If q is positive, the force is in the same direction as the field. If q is negative, the force and the field are in opposite directions. To determine the direction of an electric field, consider a point charge q as a source charge. This charge creates an electric field at all points in space surrounding it. A test charge q0 is placed at point P, a distance r from the source charge, as in the following Figure. We imagine using the test charge to determine the direction of the electric force and therefore that of the electric field. According to Coulomb’s law, the force exerted by q on the test charge is where r is a unit vector directed from q toward qo. This force is directed away from the source charge q. Because the electric field at P, the position of the test charge, is defined by the electric field at P created by q If the source charge q is positive, Active Figure 23.11b shows the situation with the test charge removed: the source charge sets up an electric field at P, directed away from q. If q is negative as in Active Figure 23.11c, the force on the test charge is toward the source charge, so the electric field at P is directed toward the source charge as in Active Figure 23.11d.

9 To calculate the electric field at a point P due to a group of point charges, we first calculate the electric field vectors at P individually using Equation 23.9 and then add them vectorially. In other words, at any point P, the total electric field due to a group of source charges equals the vector sum of the electric fields of all the charges. This superposition principle applied to fields follows directly from the vector addition of electric forces. Therefore, the electric field at point P due to a group of source charges can be expressed as the vector sum ∑ where ri is the distance from the ith source charge qi to the point P and r^ i is a unit vector directed from qi toward P. Electric field of continuous charge distributions Very often, the distances between charges in a group of charges are much smaller than the distance from the group to a point where the electric field is to be calculated. In such situations, the system of charges can be modeled as continuous. That is, the system of closely spaced charges is equivalent to a total charge that is continuously distributed along some line, over some surface, or throughout some volume. To set up the process for evaluating the electric field created by a continuous charge distribution, let’s use the following procedure. First, divide the charge distribution into small elements, each of which contains a small charge q as shown in Figure 23.14.

10 Next, use Equation 23.9 to calculate the electric field due to one of these elements at a point P. Finally, evaluate the total electric field at P due to the charge distribution by summing the contributions of all the charge elements (that is, by applying the superposition principle). The electric field at P due to one charge element carrying charge q is where r is the distance from the charge element to point P and r is a unit vector directed from the element toward P. The total electric field at P due to all elements in the charge distribution is approximately ∑ where the index i refers to the ith element in the distribution. Because the charge distribution is modeled as continuous, the total field at P in the limit q --> 0 is ∑∫ where the integration is over the entire charge distribution. The integration in Equation 23.11 is a vector operation and must be treated appropriately. For line charge density ∫ For surface charge density ∫ For volume charge density ∫

11 Calculation method of electric field The following procedure is recommended for solving problems that involve the determination of an electric field due to individual charges or a charge distribution. 1. Conceptualize. Establish a mental representation of the problem: think carefully about the individual charges or the charge distribution and imagine what type of electric field it would create. Appeal to any symmetry in the arrangement of charges to help you visualize the electric field. 2. Categorize. Are you analyzing a group of individual charges or a continuous charge distribution? The answer to this question tells you how to proceed in the Analyze step. 3. Analyze. (a) If you are analyzing a group of individual charges, use the superposition principle: when several point charges are present, the resultant field at a point in space is the vector sum of the individual fields due to the individual charges (Eq. 23.10). Be very careful in the manipulation of vector quantities. It may be useful to review the material on vector addition in Chapter 3. If you are analyzing a continuous charge distribution, replace the vector sums for evaluating the total electric field from individual charges by vector integrals. The charge distribution is divided into infinitesimal pieces, and the vector sum is carried out by integrating over the entire charge distribution (Eq. 23.11). Consider symmetry when dealing with either a distribution of point charges or a continuous charge distribution. Take advantage of any symmetry in the system you observed in the Conceptualize step to simplify your calculations. The cancellation of field components perpendicular to the axis in Example 23.7 is an example of the application of symmetry. 4. Finalize. Check to see if your electric field expression is consistent with the mental representation and if it reflects any symmetry that you noted previously. Imagine varying parameters such as the distance of the observation point from the charges or the radius of any circular objects to see if the mathematical result changes in a reasonable way.

12 Electric field lines In this section we explore a means of visualizing the electric field in a pictorial representation. A convenient way of visualizing electric field patterns is to draw lines, called electric field lines and first introduced by Faraday, that are related to the electric field in a region of space in the following manner: 1- The electric field vector E is tangent to the electric field line at each point. The line has a direction, indicated by an arrow head, that is the same as that of the electric field vector. The direction of the line is that of the force on a positive test charge placed in the field. 2- The number of lines per unit area through a surface perpendicular to the lines is proportional to the magnitude of the electric field in that region. Therefore, the field lines are close together where the electric field is strong and far apart where the field is weak. These properties are illustrated in Figure ( ). The density of field lines through surface A is greater than the density of lines through surface B. Therefore, the magnitude of the electric field is larger on surface A than on surface B. Furthermore, because the lines at different locations point in different directions, the field is nonuniform. Is this relationship between strength of the electric field and the density of field lines consistent with equation ⃗̂

13 The expression we obtained for E using Coulomb’s law? To answer this question, consider an imaginary spherical surface of radius r concentric with a point charge. From symmetry, we see that the magnitude of the electric field is the same everywhere on the surface of the sphere. The number of lines N that emerge from the charge is equal to the number that penetrate the spherical surface. Hence, the number of lines per unit area on the sphere is Where A the surface area of the sphere. Because E is proportional to the number of lines per unit area (N/A), we see that E varies as 1/r2; this finding is consistent with Equation. Representative electric field lines for the field due to a single positive point charge are shown in the Figure This two-dimensional drawing shows only the field lines that lie in the plane containing the point charge. The lines are actually directed radially outward from the charge in all directions; therefore, instead of the flat ―wheel‖ of lines shown, you should picture an entire spherical distribution of lines. Because a positive test charge placed in this field would be repelled by the positive source charge, the lines are directed radially away from the source charge.

14 The electric field lines representing the field due to a single negative point charge are directed toward the charge. In either case, the lines are along the radial direction and extend all the way to infinity. Notice that the lines become closer together as they approach the charge, indicating that the strength of the field increases as we move toward the source charge. The rules for drawing electric field lines are as follows: 1- The lines must begin on a positive charge and terminate on a negative charge. In the case of an excess of one type of charge, some lines will begin or end infinitely far away. 2- The number of lines drawn leaving a positive charge or approaching a negative charge is proportional to the magnitude of the charge. 3- No two field lines can cross. The electric field lines for two point charges of equal magnitude but opposite signs (an electric dipole) are shown in the Figure.

15 Because the charges are of equal magnitude, the number of lines that begin at the positive charge must equal the number that terminate at the negative charge. At points very near the charges, the lines are nearly radial, as for a single isolated charge. The high density of lines between the charges indicates a region of strong electric field. Figure ( ) shows the electric field lines in the vicinity of two equal positive point charges. Again, the lines are nearly radial at points close to either charge, and the same number of lines emerges from each charge because the charges are equal in magnitude. Because there are no negative charges available, the electric field lines end infinitely far away. At great distances from the charges, the field is approximately equal to that of a single point charge of magnitude 2q. Finally, in Figure ( ), we sketch the electric field lines associated with a positive charge +2q and a negative charge -q. In this case, the number of lines leaving +2q is twice the number terminating at -q. Hence, only half the lines that leave the positive charge reach the negative charge. The remaining half terminate on a negative charge we assume to be at infinity. At distances much greater than the charge separation, the electric field lines are equivalent to those of a single charge +q.

16 Solved problems Example 23.2

1 Gauss’s law in electrostatics (surface integral) In previous Chapter 23, we showed how to calculate the electric field due to a given charge distribution by integrating over the distribution. In this chapter, we describe Gauss’s law and an alternative procedure for calculating electric fields. Gauss’s law is based on the inverse-square behavior of the electric force between point charges. Although Gauss’s law is a direct consequence of Coulomb’s law, it is more convenient for calculating the electric fields of highly symmetric charge distributions and makes it possible to deal with complicated problems using qualitative reasoning. As we show in this chapter, Gauss’s law is important in understanding and verifying the properties of conductors in electrostatic equilibrium. Electric flux The concept of electric field lines was described qualitatively in previous chapter. We now treat electric field lines in a more quantitative way. Consider an electric field that is uniform in both magnitude and direction as shown in Figure The field lines penetrate a rectangular open surface of area S (open surface S is enclosed by closed path L), whose plane is oriented perpendicular to the field. The

2 number of lines per unit area (in other words, the line density) is proportional to the magnitude of the electric field E. Therefore, the magnitude of electric field is equal to the change electric flux with area the total number of lines penetrating the open surface is given by ∫ If the open surface with uniform area S, then ∫ This product of the magnitude of the electric field E and surface area S of open surface perpendicular to the field is called the electric flux E. The Electric flux is proportional to the number of electric field lines penetrating some surface. If the surface under consideration is not perpendicular to the field, the flux through it must be less than that given by ES. Consider Figure (- ),

3 where the normal to the surface of area S is at an angle  to the uniform electric field. Notice that the number of lines that cross this area S is equal to the number of lines that cross the area S, which is a projection of area S onto a plane oriented perpendicular to the field. The Figure shows that the two areas. Because the flux through S equals the flux through S, the flux through S is given by Then the product between two vectors, electric field vector E and area vector dS, is scalar product. (A.B=A B cos ) From this result, we see that the flux through a surface of fixed area S has a maximum value ES when the surface is perpendicular to the field (when the normal to the surface is parallel to the field. The normal to the surface is called area vector dS, which it is determine the orientation of surface. Although area is normally treated as a scalar quantity but sometimes, its very useful to treat is as a vector. An area vector of a dimensional object is defined as a vector whose length is proportional to the area of that object and whose direction is perpendicular to the plane of that area.

4 When the electric field vector E is perpendicular to the surface S, then the electric field vector E is parallel to the area vector dS. That is =0 (cos =1), then the flux equal to its maximum value EdS. The flux equal zero when the angle between electric field vector E is parallel to the surface, ie. The angle between E and dS equal to 90 (cos 90=0). We assumed a uniform electric field in the preceding discussion. In more general situations, the electric field may vary over a large surface. Therefore, the definition of flux given by Equation (-) has meaning only for a small element of area over which the field is approximately constant (area vector dS, for open surface). Consider a general surface divided into a large number of small elements, each area element has a direction determined by area vecttor dA, for closed surface. It is convenient to define a vector dS, for open surface or dA for a closed surface, whose magnitude represents the area of the ith element of the large surface and whose direction is defined to be perpendicular to the surface element as shown in Figure (-)

5 The electric field vector E at the location of this element, which makes an angle  with the area vector dA, for closed surface, and dS for open surface, is given by For an open surface S encloses by a closed path L, L(S); For a closed surface A encloses a volume V, A(V); Summing the contributions of all elements gives an approximation to the total flux through the surface The electric flux through open surface and closed surface are given by ∫ For open surface L(S), and ∮ For a closed surface A(V). If the area of each element approaches zero, the number of elements approaches infinity. Equation (-) is a surface integral, which means it must be evaluated over the surface in question. In general, the value of E depends both on the field pattern and on the surface.

6 Electric flux through closed surface We are often interested in evaluating the flux through a closed surface A(V), defined as a surface that divides space into an inside and an outside region so that one cannot move from one region to the other without crossing the surface. The surface of a sphere, for example, is a closed surface. Consider the closed surface in Figure.

7 The area vectors dA of each small area elements point in different directions for the various surface elements, but at each point they are normal to the surface and, by convention, always point outward. At the area element labeled dA1, the field lines are crossing the surface from the inside to the outside and <90; hence, the flux is positive (cos >0). For area element dA2, the field lines graze the surface (perpendicular to dA2); therefore, =90 (cos 90=0) and the flux is zero. For area elements such as dA3, where the field lines are crossing the surface from outside to inside, >90, (cos <0) and the flux is negative because cos  is negative. The net flux through closed surface The net flux through the surface is proportional to the net number of lines leaving the surface, where the net number means the number of lines leaving the surface minus the number of lines entering the surface. If more lines are leaving than entering, the net flux is positive. If more lines are entering than leaving, the net flux is negative. Using an integral over a closed surface, we can write the net flux through a closed surface A(V) as ∮

8 Gauss's law of electrostatics In this section, we describe a general relationship between the net electric flux through a closed surface (often called a gaussian surface) and the charge enclosed by the surface. This relationship, known as Gauss’s law, is of fundamental importance in the study of electric fields. Consider a positive point charge q located at the center of a sphere of radius r as shown in Figure (-) The magnitude of the electric field everywhere on the surface of the sphere is The field lines are directed radially outward and hence are perpendicular to the surface at every point on the surface. That is, at each surface point, E is parallel to the area vector dA. Therefore, the net electric flux through the closed surface (Gaussian surface) is given by ∮

9 The electric field E is electrostatics field, by symmetry E is constant over the surface, and the closed integral is around the sphere of radius r (area of sphere 4r2, then ∮ ∮ ( ) ( )( ) Then the net ((or total) electric flux through a spherical closed surface is given by ∮ Equation (-) shows that the net flux through the spherical surface is proportional to the charge inside the surface. The flux is independent of the radius r because the area of the spherical surface is proportional to r2, whereas the electric field is proportional to 1/r2. Therefore, in the product of area and electric field, the dependence on r cancels. Now consider several closed surfaces surrounding a charge q as shown in Figure (--).

10 Surface A1 is spherical, but surfaces A2 and A3 are not. From Equation (-), the flux that passes through A1 has the value q/€0. As discussed in the preceding section, flux is proportional to the number of electric field lines passing through a surface. The construction shown in Figure (-) shows that the number of lines through A1 is equal to the number of lines through the nonspherical surfaces A2 and S3. Therefore, the net flux through any closed surface surrounding a point charge q is given by q/€0 and is independent of the shape of that surface. Now consider a point charge located outside a closed surface of arbitrary shape as shown in the above Figure. As can be seen from this construction, any electric field line entering the surface leaves the surface at another point. The number of electric field lines entering the surface equals the number leaving the surface. Therefore, the net electric flux through a closed surface that surrounds no charge is zero. Gauss’s law for charges system Let’s extend these arguments to two generalized cases: (1) that of many point charges and (2) that of a continuous distribution of charge. We once again use the superposition principle, which states that the electric field due to many charges is the vector sum of the electric fields produced by the individual charges. Therefore, the flux through any closed surface can be expressed as ∮ ⃗ ⃗⃗⃗⃗⃗ ∮(⃗⃗⃗⃗⃗ ⃗⃗⃗⃗⃗ ) ⃗⃗⃗⃗⃗ Where E is the total electric field at any point on the surface produced by the vector addition of the electric fields at that point due to the individual charges. ⃗ ⃗⃗⃗⃗⃗ ⃗⃗⃗⃗⃗ Consider the system of charges shown in Active Figure

11 The surface S surrounds only one charge, q1; hence, the net flux through S is q1/o. The flux through S due to charges q2, q3, and q4 outside it is zero because each electric field line from these charges that enters S at one point leaves it at another. The surface S’ surrounds charges q2 and q3; hence, the net flux through it is (q2+q3)/o. Finally, the net flux through surface S” is zero because there is no charge inside this surface. That is, all the electric field lines that enter S” at one point leave at another. Charge q4 does not contribute to the net flux through any of the surfaces. The mathematical form of Gauss’s law is a generalization of what we have just described and states that the net flux through any closed surface is ∮ where E represents the electric field at any point on the surface and Q represents the net charge inside the surface. When using Equation (---) you should note that although the charge Q is the net charge inside the gaussian surface, E represents the total electric field, which includes contributions from charges both inside and outside the surface. In principle, Gauss’s law can be solved for E to determine the electric field due to a system of charges or a continuous distribution of charge. In practice, however, this type of solution is applicable only in a limited number of highly symmetric situations.

12 In the next section, we use Gauss’s law to evaluate the electric field for charge distributions that have spherical, cylindrical, or planar symmetry. If one chooses the gaussian surface surrounding the charge distribution carefully, the integral in Equation (--) can be simplified and the electric field determined. Application of Gauss’s law to various charge distributions As mentioned earlier, Gauss’s law is useful for determining electric fields when the charge distribution is highly symmetric. The following examples demonstrate ways of choosing the gaussian surface over which the surface integral given by Equation 24.6 can be simplified and the electric field determined. In choosing the surface, always take advantage of the symmetry of the charge distribution so that E can be removed from the integral. The goal in this type of calculation is to determine a surface for which each portion of the surface satisfies one or more of the following conditions: 1- The value of the electric field can be argued by symmetry to be constant over the portion of the surface. 2- The dot product in Equation (--) can be expressed as a simple algebraic product E.dA because E and dA are parallel. 3- The dot product in Equation 24.6 is zero because E and dA are perpendicular. 4- The electric field is zero over the portion of the surface. Different portions of the gaussian surface can satisfy different conditions as long as every portion satisfies at least one condition. All four conditions are used in examples throughout the remainder of this chapter and will be identified by number. If the charge distribution does not have sufficient symmetry such that a gaussian surface that satisfies these conditions can be found, Gauss’s law is not useful for determining the electric field for that charge distribution. Gaussian Surfaces Are Not Real A gaussian surface is an imaginary surface you construct to satisfy the conditions listed here. It does not have to coincide with a physical surface in the situation. Conductors in electrostatic equilibrium A good electrical conductor contains charges (electrons) that are not bound to any atom and therefore are free to move about within the material. When there is no net

13 motion of charge within a conductor, the conductor is in electrostatic equilibrium. A conductor in electrostatic equilibrium has the following properties: 1- The electric field is zero everywhere inside the conductor, whether the conductor is solid or hollow. 2- If the conductor is isolated and carries a charge, the charge resides on its surface. 3- The electric field at a point just outside a charged conductor is perpendicular to the surface of the conductor and has a magnitude /0, where  is the surface charge density at that point. 4- On an irregularly shaped conductor, the surface charge density is greatest at locations where the radius of curvature of the surface is smallest. We verify the first three properties in the discussion that follows. The fourth property is presented here (but not verified until Chapter 25) to provide a complete list of properties for conductors in electrostatic equilibrium. We can understand the first property by considering a conducting slab placed in an external field E, fig (--). A conducting slab in an external electric field E . The charges induced on the two surfaces of the slab produce an electric field that opposes the external field, giving a resultant field of zero inside the slab. . The electric field inside the conductor must be zero, assuming electrostatic equilibrium exists. If the field were not zero, free electrons in the conductor would experience an electric force (F=qE ) and would accelerate due to this force. This motion of electrons, however, would mean that the conductor is not in electrostatic equilibrium. Therefore, the existence of electrostatic equilibrium is consistent only with a zero field in the conductor.

14 Let’s investigate how this zero field is accomplished. Before the external field is applied, free electrons are uniformly distributed throughout the conductor. When the external field is applied, the free electrons accelerate to the left in Figure, causing a plane of negative charge to accumulate on the left surface. The movement of electrons to the left results in a plane of positive charge on the right surface. These planes of charge create an additional electric field inside the conductor that opposes the external field. As the electrons move, the surface charge densities on the left and right surfaces increase until the magnitude of the internal field equals that of the external field, resulting in a net field of zero inside the conductor. The time it takes a good conductor to reach equilibrium is on the order of 10-16 s, which for most purposes can be considered instantaneous. If the conductor is hollow, the electric field inside the conductor is also zero, whether we consider points in the conductor or in the cavity within the conductor. The zero value of the electric field in the cavity is easiest to argue with the concept of electric potential, so we will address this issue in Section 25.6. Gauss’s law can be used to verify the second property of a conductor in electrostatic equilibrium. Figure shows an arbitrarily shaped conductor. A Gaussian surface is drawn inside the conductor and can be very close to the conductor’s surface. As we have just shown, the electric field everywhere inside the conductor is zero when it is in

15 electrostatic equilibrium. Therefore, the electric field must be zero at every point on the gaussian surface, in accordance with condition (4) in Section 24.3, and the net flux through this gaussian surface is zero. From this result and Gauss’s law, we conclude that the net charge inside the gaussian surface is zero. Because there can be no net charge inside the gaussian surface (which is arbitrarily close to the conductor’s surface), any net charge on the conductor must reside on its surface. Gauss’s law does not indicate how this excess charge is distributed on the conductor’s surface, only that it resides exclusively on the surface. To verify the third property, let’s begin with the perpendicularity of the field to the surface. If the field vector E had a component parallel to the conductor’s surface, free electrons would experience an electric force and move along the surface; in such a case, the conductor would not be in equilibrium. Therefore, the field vector must be perpendicular to the surface. To determine the magnitude of the electric field, we use Gauss’s law and draw a gaussian surface in the shape of a small cylinder whose end faces are parallel to the conductor’s surface as in Fig (--) Part of the cylinder is just outside the conductor, and part is inside. The field is perpendicular to the conductor’s surface from the condition of electrostatic equilibrium. Therefore, condition (3) in Section 24.3 is satisfied for the curved part of the cylindrical gaussian surface: there is no flux through this part of the gaussian

16 surface because E is parallel to the surface. There is no flux through the flat face of the cylinder inside the conductor because here E= 0, which satisfies condition (4). Hence, the net flux through the Gaussian surface is equal to that through only the flat face outside the conductor, where the field is perpendicular to the gaussian surface. Using conditions (1) and (2) for this face, the flux is EA, where E is the electric field just outside the conductor and A is the area of the cylinder’s face. Applying Gauss’s law to this surface gives ∮ Then Solving for E gives for the electric field immediately outside a charged conductor: Derivation of Coulomb’s law from Gauss’s law Gauss’s law for electrostatics is used for determination of electric fields in some problems in which the objects possess spherical symmetry, cylindrical symmetry, planar symmetry or combination of these. Let us discuss the applications of gauss law of electrostatics: To derive Coulomb’s Law from gauss law or to find the intensity of electric field due to a point charge +q at any point in space using Gauss’s law, draw a Gaussian sphere of radius r at the center of which charge +q is located.

17 All the points on this surface are equivalent and according to the symmetric consideration the electric field E has the same magnitude at every point on the surface of the sphere and it is radially outward in direction. Therefore, for an area element dA around any point P on the Gaussian surface both E and dA are directed radially outward, that is, the angle between E and dS is zero. Therefore, ∮ ∮ () () This equation is the expression for the magnitude of the intensity of electric field E at a point distant r from the point charge +q deduced from Coulomb’s law. The electric force arising from this field on a test point charge is This equation gives the Coulomb’s law for electric force.

18 Solved problems

Electrostatic potential Line integral and gradient In Chapter (--), we linked our new study of electromagnetism to our earlier studies of force. Now we make a new link to our earlier investigations into energy. The concept of potential energy was introduced in Chapter (--) in connection with such conservative forces as the gravitational force and the elastic force exerted by a spring. By using the law of conservation of energy, we could solve various problems in mechanics that were insoluble with an approach using forces. The concept of potential energy is also of great value in the study of electricity. Because the electrostatic force is conservative, electrostatic phenomena can be conveniently described in terms of an electric potential energy. This idea enables us to define a quantity known as electric potential. Because the electric potential at any point in an electric field is a scalar quantity, we can use it to describe electrostatic phenomena more simply than if we were to rely only on the electric field and electric forces. The concept of electric potential is of great practical value in the operation of electric circuits and devices that we will study in later chapters. Electric potential and potential difference When a test charge qo is placed in an electric field E created by some source charge distribution, the electric force acting on the test charge is qoE . The electric force is conservative because the force between charges described by Coulomb’s law is conservative. When the test charge is moved in the field by some external agent, the work done by the field on the charge is equal to the negative of the work done by the external agent causing the displacement. This situation is analogous to that of lifting an object with mass in a gravitational field: the work done by the external agent is +mgh, and the work done by the gravitational force is -mgh.

That is, in general, means that any field (gravitational, electric and also the human field) prevent any object to enter or leave it. If any object (mass in gravitational field and charge in electric field) try to move or displace for entering or leaving the field, this need a work W, the field will be done a work in opposite direction –W to fix the object in its original place. When analyzing electric and magnetic fields, it is common practice to use the notation dl to represent an infinitesimal displacement vector that is oriented tangent to an open path through space. This open path may be straight or curved, and an integral performed along this path is called either a path integral or a line integral. For an infinitesimal displacement dl of a point charge qo immersed in an electric field, the work done within the charge–field system by the electric field on the charge is As this amount of work is done by the field, the potential energy of the charge–field system is changed by an amount For a finite displacement of the charge from point A to point B, the change in potential energy of the system

Where ∫ The integration is performed along the path that qo follows as it moves from point A to point B. Because the electric force is conservative, this line integral does not depend on the path taken from A to B. For a given position of the test charge in the field, the charge–field system has a potential energy U relative to the configuration of the system that is defined as U = 0. Dividing the potential energy by the test charge gives a physical quantity that depends only on the source charge distribution and has a value at every point in an electric field. This quantity is called the electric potential , where ∫ Because potential energy is a scalar quantity, electric potential also is a scalar quantity, therefore the electric potential is called scalar electric potential. As described by Equation (--), if the test charge is moved between two positions A and B in an electric field, the charge–field system experiences a change in potential energy. The potential difference V between two points A and B in an electric field is defined as the change in potential energy of the system when a test charge qo is moved between the points divided by the test charge:

∫ In this definition, the infinitesimal displacement dl is interpreted as the displacement between two points in space rather than the displacement of a point charge. Just as with potential energy, only differences in electric potential are meaningful. We often take the value of the electric potential to be zero at some convenient point in an electric field. Potential difference should not be confused with difference in potential energy. The potential difference between A and B exists solely because of a source charge and depends on the source charge distribution (consider points A and B without the presence of the test charge). For a potential energy to exist, we must have.a system of two or more charges. The potential energy belongs to the system and changes only if a charge is moved relative to the rest of the system. If an external agent moves a test charge from A to B without changing the kinetic energy of the test charge, the agent performs work that changes the potential energy of the system: Imagine an arbitrary charge q located in an electric field. From Equation (--), the work done by an external agent in moving a charge q through an electric field at constant velocity is The SI unit of both electric potential and potential difference is joules per coulomb (J/C) which is defined as a volt (V). It is a scalar product