Electric Charges And Fields Notes - Class 12 - Science Physics | Kedovo | Kedovo
Chapter Notes
Electric Charges And Fields
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Introduction to Electrostatics
Have you ever felt a small spark when taking off a sweater in dry weather, or seen lightning flash across the sky during a storm? These are common examples of static electricity. The study of these phenomena, which involve stationary electric charges, is called electrostatics. It explores the forces, fields, and potentials that arise from charges that are not in motion. The reason we experience these sparks or shocks is due to the discharge of electric charges that have built up on surfaces, often through rubbing.
Electric Charge
The concept of electric charge dates back to ancient Greece, around 600 BC, when Thales of Miletus observed that amber rubbed with wool could attract light objects. The word "electricity" itself comes from elektron, the Greek word for amber.
Through many experiments, scientists discovered that there are two types of electric charge. The fundamental rule governing their interaction is:
Like charges repel each other.
Unlike charges attract each other.
For example, two glass rods rubbed with silk will repel each other, but a glass rod will attract the silk cloth it was rubbed with. This property that distinguishes the two types of charges is called the polarity of charge.
Benjamin Franklin named these two types of charges positive and negative.
By convention, the charge on a glass rod rubbed with silk is positive.
The charge on a plastic rod rubbed with fur is negative.
An object with an electric charge is said to be electrified or charged. An object with no net charge is electrically neutral.
How do objects get charged?
All matter is made of atoms, which contain positive charges (protons) and negative charges (electrons). Usually, these charges are balanced, so the object is neutral. Charging an object involves transferring electrons from one body to another.
A body becomes positively charged when it loses electrons.
A body becomes negotively charged when it gains electrons.
When a glass rod is rubbed with silk, electrons move from the rod to the silk. The rod becomes positively charged, and the silk becomes negatively charged. No new charge is created; it is simply redistributed.
A gold-leaf electroscope is a simple device used to detect the presence of charge on an object. When a charged object touches the metal knob, the charge spreads to the thin gold leaves at the bottom, causing them to repel each other and diverge.
Conductors and Insulators
Materials can be classified based on how easily they allow electric charge to move through them.
Conductors are materials that allow electricity to pass through them easily. They have mobile electric charges (usually electrons) that are free to move. Examples include metals, the human body, and the Earth. When charge is given to a conductor, it quickly spreads over its entire surface.
Insulators are materials that offer high resistance to the passage of electricity. Their charges are not free to move. Examples include glass, plastic, wood, and nylon. If charge is put on an insulator, it stays in the same place.
Example
A plastic comb gets charged when you run it through dry hair because both are insulators, allowing charge to build up. A metal spoon does not, because it's a conductor. Any charge it acquires quickly flows through your body (also a conductor) to the ground.
Basic Properties of Electric Charge
Electric charge has three fundamental properties: additivity, conservation, and quantisation. For calculations involving forces between charges, we often treat charged bodies as point charges if their sizes are much smaller than the distance between them.
Additivity of Charges
Electric charge is a scalar quantity, meaning it has magnitude but no direction. The total charge of a system is simply the algebraic sum of all the individual charges in it. You must use the proper signs (positive or negative) when adding them.
If a system contains charges q1,q2,q3,…,qn, the total charge Q is:
Q=q1+q2+q3+…+qn
Example
If a system has five charges: +1,+2,−3,+4, and −5 (in some unit), the total charge is (+1)+(+2)+(−3)+(+4)+(−5)=−1 in the same unit.
Charge is Conserved
The law of conservation of charge states that the total charge of an isolated system always remains constant. When you rub two objects together, charge is transferred from one to the other, but the net charge of the system (the two objects) does not change. Charge cannot be created or destroyed, only moved around.
Even in nuclear processes where particles are created, charge is conserved. For instance, when a neutron (no charge) decays, it turns into a proton (positive charge) and an electron (negative charge). The net charge is zero both before and after the process.
Quantisation of Charge
Experimentally, it's found that all free charges are integral multiples of a basic unit of charge, denoted by e. This property is called the quantisation of charge.
The charge q on any body is given by the formula:
q=ne
Where n is an integer (0,±1,±2,…) and e is the elementary charge, which is the magnitude of the charge on a single electron or proton.
Charge on an electron = −e
Charge on a proton = +e
The value of the elementary charge in SI units is:
e=1.602192×10−19 C
The SI unit of charge is the coulomb (C).
Note
At a macroscopic (large-scale) level, we deal with charges that are enormous compared to e. For instance, a charge of 1μC (10−6 C) contains about 1013 electrons. At this scale, the "grainy" or discrete nature of charge isn't noticeable, and we can treat charge as if it were continuous. However, at the microscopic level, quantisation is a crucial concept.
Example
Example If 109 electrons move out of a body to another body every second, how much time is required to get a total charge of 1 C on the other body?
Given
Number of electrons transferred per second, nsec=109
Total charge to be accumulated, Q=1 C
Elementary charge, e=1.6×10−19 C
To Find
The time required, t, to accumulate a charge of 1 C.
Formula
Charge transferred per second, qsec=nsec×e
Total time, t=qsecQ
Solution
First, calculate the charge transferred in one second:
qsec=109×(1.6×10−19 C)=1.6×10−10 C/s
Now, calculate the total time required to accumulate 1 C:
t=1.6×10−10 C/s1 C=6.25×109 s
To convert this to years:
t=365×24×3600 s/year6.25×109 s≈198 years
Final Answer It would take approximately 198 years to accumulate a charge of 1 C. This shows that one coulomb is a very large unit of charge for practical purposes.
Example
Example How much positive and negative charge is there in a cup of water?
Given
Mass of water in a cup (assumed), m=250 g
Molecular mass of water (H2O), M=18 g/mol
Avogadro's number, NA=6.02×1023 molecules/mol
A water molecule (H2O) has 2 Hydrogen atoms (1 proton, 1 electron each) and 1 Oxygen atom (8 protons, 8 electrons). Total = 10 protons and 10 electrons.
To Find
The total positive and negative charge in the cup of water.
Formula
Number of molecules, N=(Mm)×NA
Total charge, Q=N×(number of protons or electrons per molecule)×e
Solution
First, find the number of molecules in 250 g of water:
N=(18 g/mol250 g)×(6.02×1023 molecules/mol)
The total positive charge (from 10 protons per molecule) and total negative charge (from 10 electrons per molecule) have the same magnitude. Let's calculate this magnitude:
Q=(18250×6.02×1023)×10×(1.6×10−19 C)Q≈1.34×107 C
Final Answer A cup of water contains approximately 1.34×107 C of positive charge and 1.34×107 C of negative charge.
Coulomb's Law
Coulomb's Law is a fundamental law that quantifies the electrostatic force between two stationary point charges. It states that the force is:
Directly proportional to the product of the magnitudes of the two charges.
Inversely proportional to the square of the distance between them.
Acts along the line connecting the two charges.
The magnitude of the force F between two point charges q1 and q2 separated by a distance r in a vacuum is given by:
F=kr2∣q1q2∣
Here, k is the electrostatic force constant. For convenience, k is usually written as k=4πε01, where ε0 is the permittivity of free space.
So, Coulomb's Law is written as:
F=4πε01r2∣q1q2∣
In SI units:
ε0≈8.854×10−12 C2N−1m−2
k≈9×109 N m2C−2
Coulomb's Law in Vector Form
Force is a vector, so it's more complete to write Coulomb's law in vector form. Let r1 and r2 be the position vectors of charges q1 and q2. The force on charge q2 due to q1, denoted by F21, is:
F21=4πε01r212q1q2r^21
where r21=r2−r1 is the vector from q1 to q2, and r^21 is the unit vector in that direction.
If q1 and q2 have the same sign, the product q1q2 is positive, and F21 is in the direction of r^21 (repulsion).
If q1 and q2 have opposite signs, the product q1q2 is negative, and F21 is in the direction opposite to r^21 (attraction).
The force on q1 due to q2 is F12=−F21, which is consistent with Newton's third law.
Example
Example Compare the strength of electrostatic and gravitational forces and estimate the accelerations of an electron and a proton.
Given
Distance between electron and proton, r=1A˚=10−10 m
Mass of proton, mp=1.67×10−27 kg
Mass of electron, me=9.11×10−31 kg
Charge, e=1.6×10−19 C
k=4πε01=9×109 N m2C−2
Gravitational constant, G=6.67×10−11 N m2kg−2
To Find
(a) Ratio of magnitudes of electric force (Fe) to gravitational force (FG) for (i) an electron and a proton, and (ii) two protons.
(b) Acceleration of the electron (ae) and proton (ap) when they are 1A˚ apart.
Formula
Fe=kr2e2FG=Gr2m1m2F=ma⟹a=F/m
Solution
(a) (i) Ratio for an electron and a proton
The ratio of the magnitudes of the forces is independent of the distance r:
FGFe=Gmpme/r2ke2/r2=Gmpmeke2FGFe=(6.67×10−11)(1.67×10−27)(9.11×10−31)(9×109)(1.6×10−19)2≈2.4×1039
(a) (ii) Ratio for two protonsFGFe=Gmpmpke2FGFe=(6.67×10−11)(1.67×10−27)2(9×109)(1.6×10−19)2≈1.3×1036
This shows that electrical forces are enormously stronger than gravitational forces.
(b) Accelerations of electron and proton
First, calculate the magnitude of the electric force between them at r=10−10 m:
∣F∣=kr2e2=(9×109 Nm2/C2)×(10−10 m)2(1.6×10−19 C)2∣F∣=2.3×10−8 N
Now, find the accelerations using a=F/m:
Acceleration of the electron:
ae=9.11×10−31 kg2.3×10−8 N=2.5×1022 m/s2
Acceleration of the proton:
ap=1.67×10−27 kg2.3×10−8 N=1.4×1019 m/s2
Final Answer The ratios show the immense strength of the electric force. The accelerations are huge, indicating that for atomic particles, gravity's effect is negligible compared to the electrostatic force.
Forces between Multiple Charges
What if there are more than two charges? To find the force on one charge due to several others, we use the principle of superposition.
This principle states that the total force on any given charge is the vector sum of the individual forces exerted on it by all other charges. The force between any two charges is calculated using Coulomb's law and is unaffected by the presence of other charges.
For a system of charges q1,q2,…,qn, the total force F1 on charge q1 is:
F1=F12+F13+…+F1nF1=4πε01∑i=2nr1i2q1qir^1i
Example
Example Consider three charges q1,q2,q3 each equal to q at the vertices of an equilateral triangle of side l. What is the force on a charge Q (with the same sign as q) placed at the centroid of the triangle?
Given
Three charges, q1=q2=q3=q, at the vertices of an equilateral triangle.
Side length of the triangle = l.
A charge Q is placed at the centroid O.
To Find
The net force on charge Q.
Solution
The centroid of an equilateral triangle is equidistant from all three vertices. Let this distance be r. The distance from a vertex to the centroid (AO, BO, CO) is r=l/3.
The force on Q due to the charge q at vertex A is F1. Its magnitude is:
F1=4πε01r2Qq=4πε01(l/3)2Qq=4πε03l2Qq
This force is directed along AO (repulsive).
Similarly, the forces on Q due to charges at B and C, F2 and F3, have the same magnitude and are directed along BO and CO, respectively.
The three force vectors F1,F2,F3 are equal in magnitude and are 120∘ apart. By symmetry, the vector sum of these three forces must be zero. If you place three equal vectors at 120∘ to each other, their resultant is zero.
Fnet=F1+F2+F3=0
Final Answer The force on the charge Q placed at the centroid is zero.
Electric Field
Instead of thinking about forces acting at a distance, it's useful to introduce the concept of a field. A source charge Q creates an electric field in the space around it. When another charge q (a test charge) is placed in this field, it experiences a force.
The electric field E at a point is defined as the electrostatic force F experienced by a small positive test charge q placed at that point, divided by the magnitude of the test charge.
E=limq→0qF
The test charge q must be negligibly small so it doesn't disturb the source charge(s).
The SI unit for electric field is newtons per coulomb (N/C).
For a single source charge Q, the electric field at a distance r is:
E=4πε01r2Qr^
If Q is positive, E points radially outward.
If Q is negative, E points radially inward.
The force on any charge q placed in an electric field E is given by:
F=qE
Electric Field due to a System of Charges
Just like with forces, the electric field from multiple source charges follows the superposition principle. The total electric field at a point is the vector sum of the electric fields from each individual charge.
E(r)=E1(r)+E2(r)+…+En(r)E(r)=4πε01∑i=1nriP2qir^iP
Note
Physical Significance of the Electric Field
The concept of a field is powerful because it explains how forces are transmitted. Instead of "action at a distance," we can say that a charge creates a field, and this field acts on other charges. This becomes essential when dealing with moving charges, as changes in the field propagate at the speed of light, not instantaneously. Fields are considered physical entities that can store and transport energy.
Example
Example Two point charges q1=+10−8 C and q2=−10−8 C are placed 0.1 m apart. Calculate the electric fields at points A, B, and C as shown in the figure.
Given
q1=+10−8 C
q2=−10−8 C
Distance between charges = 0.1 m
Point A is the midpoint between the charges.
Point B is 0.05 m from q1 and 0.15 m from q2.
Point C is 0.1 m from both q1 and q2, forming an equilateral triangle.
To Find
The electric field at points A, B, and C.
Formula
E=4πε01r2qr^
Solution
At Point A (Midpoint):
The distance from A to both q1 and q2 is r=0.05 m.
Field due to q1 (E1A): Points to the right (away from positive charge).
E1A=(9×109)(0.05)210−8=3.6×104 N/C
Field due to q2 (E2A): Also points to the right (towards negative charge).
E2A=(9×109)(0.05)2∣−10−8∣=3.6×104 N/C
The total field at A is the sum of these two vectors, which are in the same direction.
EA=E1A+E2A=7.2×104 N/C
The direction is to the right.
At Point B:
Field due to q1 (E1B): Points to the left (away from q1). Distance is 0.05 m.
E1B=(9×109)(0.05)210−8=3.6×104 N/C
Field due to q2 (E2B): Points to the right (towards q2). Distance is 0.15 m.
E2B=(9×109)(0.15)2∣−10−8∣=4×103 N/C
The total field at B is the vector difference.
EB=E1B−E2B=3.6×104−0.4×104=3.2×104 N/C
The direction is to the left (the direction of the larger vector).
At Point C:
The distance from C to both charges is r=0.10 m. The magnitudes of the fields are equal.
E1C=E2C=(9×109)(0.10)210−8=9×103 N/C
E1C points away from q1.
E2C points towards q2.
The angle between these vectors is 120∘. When we add them, the vertical components cancel out. The horizontal components (pointing to the right) add up. The angle inside the parallelogram is 60∘ (π/3 radians).
EC=E1Ccos(60∘)+E2Ccos(60∘)EC=(9×103)(21)+(9×103)(21)=9×103 N/C
The direction is to the right.
Electric Field Lines
Electric field lines are a way to visualize electric fields. They are imaginary curves drawn in a region of space so that the tangent to the curve at any point gives the direction of the electric field at that point. They are also known as lines of force.
Properties of Electric Field Lines:
Direction: The tangent to a field line at any point gives the direction of the electric field E at that point. Arrows on the lines indicate this direction.
Strength: The density of the field lines (how close they are to each other) represents the magnitude of the electric field. Field lines are close together where the field is strong and far apart where it is weak.
Origin and Termination: Field lines originate from positive charges and terminate on negative charges. For a single charge, they may start or end at infinity.
Continuity: Field lines are continuous curves and do not have sudden breaks in a charge-free region.
No Crossing: Two field lines can never cross each other. If they did, it would mean the electric field has two different directions at the same point, which is impossible.
No Closed Loops: Electrostatic field lines do not form closed loops. This is because the electrostatic force is a conservative force.
Electric Flux
Electric flux is a measure of the "flow" of the electric field through a given area. Imagine holding a ring in a flowing stream; the amount of water passing through the ring depends on its area and how it's oriented relative to the flow. Electric flux is an analogous concept.
For a small planar area element ΔS in a uniform electric field E, the electric flux Δϕ is defined as the dot product of the electric field and the area vector:
Δϕ=E⋅ΔS=EΔScosθ
where θ is the angle between the electric field vector E and the normal to the surface (the direction of ΔS).
The area element ΔS is a vector whose magnitude is the area ΔS and whose direction is perpendicular (normal) to the surface.
For a closed surface, the direction of the area vector is always taken to be the outward normal.
The SI unit of electric flux is N m2C−1.
The total flux ϕ through an entire surface S is the sum (or integral) of the flux through all the small area elements that make up the surface:
ϕ≈∑E⋅ΔS
Electric Dipole
An electric dipole is a pair of equal and opposite point charges, +q and -q, separated by a small distance, 2a.
The electric dipole moment (p) is a vector quantity that characterizes the dipole.
Magnitude:p=q×(2a)
Direction: From the negative charge (-q) to the positive charge (+q).
The SI unit for dipole moment is coulomb-meter (C m).
The Field of an Electric Dipole
The electric field of a dipole decreases more rapidly with distance than that of a single point charge. At large distances (r≫a), the field strength is proportional to 1/r3.
(i) For points on the axis (Axial Line)
The electric field at a point P on the axis of the dipole, at a distance r from its center, is:
E=4πε01(r2−a2)22pr
For large distances (r≫a):
E≈4πε01r32p
The field is in the same direction as the dipole moment p.
(ii) For points on the equatorial plane
The electric field at a point P on the plane perpendicular to the dipole axis and passing through its center, at a distance r from the center, is:
E=−4πε01(r2+a2)3/2p
For large distances (r≫a):
E≈−4πε01r3p
The field is in the direction opposite to the dipole moment p.
Note
A point dipole is an ideal dipole where the separation 2a→0 and the charge q→∞ in such a way that the product p=q×2a remains finite. For a point dipole, the approximate formulas for large distances are exact for any r.
Example
Example Two charges ±10μC are placed 5.0 mm apart. Determine the electric field at (a) a point P on the axis of the dipole 15 cm away from its centre O on the side of the positive charge, and (b) a point Q, 15 cm away from O on a line passing through O and normal to the axis of the dipole.
Given
Charge, q=10μC=10−5 C
Separation, 2a=5.0 mm=5×10−3 m (so a=2.5×10−3 m)
Distance to points P and Q, r=15 cm=0.15 m
To Find
(a) Electric field at axial point P, EP
(b) Electric field at equatorial point Q, EQ
Formula
Since r=15 cm is much larger than a=0.25 cm (r/a=60), we can use the simplified formulas for large distances.
Dipole moment magnitude: p=q×(2a)
Axial field: Eaxial=4πε01r32p
Equatorial field: Eequatorial=4πε01r3p
Solution
First, calculate the magnitude of the dipole moment:
p=(10−5 C)×(5×10−3 m)=5×10−8 C m
The direction of p is from the negative to the positive charge.
(a) Field at axial point P
The point P is on the side of the positive charge, so the field will be in the same direction as the dipole moment.
EP=(9×109 N m2C−2)×(0.15 m)32×(5×10−8 C m)EP=(9×109)×0.00337510×10−8=2.66×105 N/C
Answer for part (a) = 2.7×105 N/C (using the more precise calculation from the text), directed along the dipole axis from negative to positive charge.
(b) Field at equatorial point Q
The field at an equatorial point is directed opposite to the dipole moment.
EQ=(9×109 N m2C−2)×(0.15 m)35×10−8 C mEQ=(9×109)×0.0033755×10−8=1.33×105 N/C
Answer for part (b) = 1.33×105 N/C, directed opposite to the dipole moment (parallel to the axis).
Dipole in a Uniform External Field
Consider a dipole with moment p placed in a uniform external electric field E.
The positive charge +q experiences a force qE.
The negative charge -q experiences a force −qE.
Since the field is uniform, the net force on the dipole is zero (qE−qE=0). The dipole will not accelerate linearly.
However, because the forces act at different points, they create a torque that causes the dipole to rotate. The magnitude of this torque (τ) is:
τ=pEsinθ
where θ is the angle between the dipole moment p and the electric field E.
In vector form, the torque is given by the cross product:
τ=p×E
This torque tends to align the dipole with the electric field. The torque is maximum when θ=90∘ and zero when the dipole is aligned with the field (θ=0∘).
If the electric field is non-uniform, the net force on the dipole is generally non-zero, and it will experience both a torque and a net force.
Example
A charged comb attracts neutral pieces of paper. The comb's non-uniform electric field first induces a dipole moment in the paper (polarizes it). Then, because the field is stronger closer to the comb, the attractive force on the side of the paper closer to the comb is greater than the repulsive force on the farther side, resulting in a net attractive force.
Continuous Charge Distribution
For many practical situations, like the charge on a metal sheet, it's more convenient to work with a continuous charge distribution rather than individual point charges. We define charge densities for this purpose.
Linear Charge Density (λ): Charge per unit length. Used for objects like a thin wire.
λ=ΔlΔQ
Unit: C/m
Surface Charge Density (σ): Charge per unit area. Used for objects like a thin sheet.
σ=ΔSΔQ
Unit: C/m2
Volume Charge Density (ρ): Charge per unit volume. Used for three-dimensional objects.
ρ=ΔVΔQ
Unit: C/m3
To find the electric field from a continuous charge distribution, we can imagine it is made of infinitely many small charge elements (ρΔV). We calculate the field from each element using Coulomb's law and then sum (integrate) all their contributions using the superposition principle.
Gauss's Law
Gauss's Law provides a powerful relationship between the electric flux through a closed surface and the net charge enclosed within that surface.
The law states: The total electric flux (ϕ) through any closed surface (called a Gaussian surface) is equal to the net charge enclosed (qenc) divided by the permittivity of free space (ε0).
ϕ=∮E⋅dS=ε0qenc
Key Points about Gauss's Law:
It is true for any closed surface, regardless of its shape or size.
The charge qenc is the algebraic sum of all charges inside the surface.
The electric field E on the left side of the equation is the total field due to all charges, both inside and outside the surface.
The law is most useful for calculating the electric field for charge distributions with a high degree of symmetry (spherical, cylindrical, planar).
Gauss's law is a direct consequence of the inverse-square nature of Coulomb's law.
Example
Example The electric field components in Fig. 1.24 are Ex=αx1/2,Ey=Ez=0, in which α=800 N/C m1/2. Calculate (a) the flux through the cube, and (b) the charge within the cube. Assume that a=0.1 m.
Given
Electric field, Ex=αx1/2 with α=800 N/C m1/2
Ey=0,Ez=0
Side of cube, a=0.1 m
The cube is placed with one corner at the origin, extending from x=a to x=2a.
To Find
(a) The net flux ϕ through the cube.
(b) The net charge q inside the cube.
Formula
Flux, ϕ=E⋅ΔS=EΔScosθ
Gauss's Law, q=ϕε0
Solution
(a) The electric field is only in the x-direction. Therefore, flux is non-zero only through the faces perpendicular to the x-axis (the left and right faces).
Left Face: Located at x=a. The area vector points in the −x direction, so θ=180∘.
EL=αa1/2ϕL=EL⋅A=ELa2cos(180∘)=−αa1/2a2=−αa5/2
Right Face: Located at x=2a. The area vector points in the +x direction, so θ=0∘.
ER=α(2a)1/2=α2a1/2ϕR=ER⋅A=ERa2cos(0∘)=(α2a1/2)a2=α2a5/2
The net flux is the sum of the fluxes through all faces.
ϕnet=ϕL+ϕR=−αa5/2+α2a5/2=αa5/2(2−1)
Substitute the values:
ϕnet=800×(0.1)5/2(2−1)=800×(0.00316)×(0.414)≈1.05 N m2C−1
(b) Using Gauss's Law to find the enclosed charge:
q=ϕnetε0=(1.05 N m2C−1)×(8.854×10−12 C2N−1m−2)q≈9.27×10−12 C
Final Answer
(a) The net flux is 1.05 N m2C−1.
(b) The charge within the cube is 9.27×10−12 C.
Applications of Gauss's Law
Gauss's law simplifies electric field calculations for symmetric charge distributions.
Field due to an Infinitely Long Straight Uniformly Charged Wire
For a long wire with uniform linear charge density λ, the electric field is radial and perpendicular to the wire. We use a cylindrical Gaussian surface of radius r and length l.
Flux passes only through the curved part of the cylinder.
Flux ϕ=E×(Area)=E×(2πrl).
Charge enclosed qenc=λl.
Applying Gauss's law: E(2πrl)=ε0λl.
The magnitude of the electric field is:
E=2πε0rλ
The field strength decreases as 1/r.
Field due to a Uniformly Charged Infinite Plane Sheet
For a large plane sheet with uniform surface charge density σ, the electric field is uniform and perpendicular to the sheet. We use a cylindrical or rectangular box as the Gaussian surface, piercing the sheet.
Flux passes only through the two end faces (area A).
Flux ϕ=EA+EA=2EA.
Charge enclosed qenc=σA.
Applying Gauss's law: 2EA=ε0σA.
The magnitude of the electric field is:
E=2ε0σ
Remarkably, the field is constant and does not depend on the distance from the sheet.
Field due to a Uniformly Charged Thin Spherical Shell
For a thin spherical shell of radius R and total charge q (surface charge density σ), the field has spherical symmetry. We use a spherical Gaussian surface of radius r.
(i) Field outside the shell (r>R)
The Gaussian surface encloses the entire charge q.
Flux ϕ=E×(4πr2).
Charge enclosed qenc=q.
Applying Gauss's law: E(4πr2)=ε0q.
The electric field is:
E=4πε01r2qr^
Outside the shell, the field is identical to that of a point charge q located at the center.
(ii) Field inside the shell (r<R)
The Gaussian surface is inside the shell and encloses no charge.
Charge enclosed qenc=0.
Applying Gauss's law: E(4πr2)=0.
The electric field is:
E=0
The electric field is zero everywhere inside a uniformly charged thin spherical shell.
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