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Physics 1

The electronic Field

takriban dakika 7 kusoma

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Mada za sehemu hiiElectrostaticsMada 3

Electric field

Electric field E\mathbf{E} is analogous to gravitational field g\mathbf{g}. It is a region around a charge where another charge experiences a force. The electric field intensity at a point is defined as:

E=Fq\mathbf{E} = \frac{\mathbf{F}}{q}

Coulomb's law

The electrostatic force between two point charges is given by:

F=kQ1Q2r2(9.1)F = k \frac{Q_1 Q_2}{r^2} \quad \text{(9.1)}

where k=14πε0k = \frac{1}{4 \pi \varepsilon_0} and ε0=8.854×1012  C2N1m2\varepsilon_0 = 8.854 \times 10^{-12} \; \text{C}^2 \text{N}^{-1} \text{m}^{-2}

So:

F=14πε0Q1Q2r2(9.2)F = \frac{1}{4 \pi \varepsilon_0} \frac{Q_1 Q_2}{r^2} \quad \text{(9.2)}

Relative permittivity:

εr=εε0\varepsilon_r = \frac{\varepsilon}{\varepsilon_0}

Vector form:

F21=kQ1Q2r3r(9.3)\mathbf{F}_{21} = k \frac{Q_1 Q_2}{r^3} \mathbf{r} \quad \text{(9.3)}

Superposition principle

F=i=1nFi\mathbf{F} = \sum_{i=1}^{n} \mathbf{F}_i

F=(Fx)2+(Fy)2F = \sqrt{\left(\sum F_x\right)^2 + \left(\sum F_y\right)^2}

Example 1

Q=1×107 C,  e=1.6×1019 CQ = 1 \times 10^{-7} \text{ C}, \; e = 1.6 \times 10^{-19} \text{ C}

n=Qe=1×1071.6×1019=6.25×1011 electronsn = \frac{Q}{e} = \frac{1 \times 10^{-7}}{1.6 \times 10^{-19}} = 6.25 \times 10^{11} \text{ electrons}

Example 2

r=5.3×1011 m,  Q1=Q2=1.6×1019 Cr = 5.3 \times 10^{-11} \text{ m}, \; Q_1 = Q_2 = 1.6 \times 10^{-19} \text{ C}

F=9.0×109(1.6×1019)2(5.3×1011)28.2×108 NF = \frac{9.0 \times 10^9 (1.6 \times 10^{-19})^2}{(5.3 \times 10^{-11})^2} \approx 8.2 \times 10^{-8} \text{ N}

Example 3

Three charges: Q1=1.0 nC,Q2=3.0 nC,Q3=5.0 nCQ_1 = 1.0 \text{ nC}, Q_2 = 3.0 \text{ nC}, Q_3 = 5.0 \text{ nC}

Distances: r31=0.02 m,r32=0.04 mr_{31} = 0.02 \text{ m}, r_{32} = 0.04 \text{ m}

F31=9×10915×1018(0.02)2=1.13×104 NF_{31} = \frac{9 \times 10^9 \cdot 1 \cdot 5 \times 10^{-18}}{(0.02)^2} = 1.13 \times 10^{-4} \text{ N}

F32=9×10935×1018(0.04)2=8.44×105 NF_{32} = \frac{9 \times 10^9 \cdot 3 \cdot 5 \times 10^{-18}}{(0.04)^2} = 8.44 \times 10^{-5} \text{ N}

F=F31+F32=1.97×104 N (left)\sum F = F_{31} + F_{32} = 1.97 \times 10^{-4} \text{ N (left)}

Example 4

Triangle side = 0.2 m. Charges: 2μC, 3μC, 4μC

F=9×10943×1012(0.2)2=2.7 NF = \frac{9 \times 10^9 \cdot 4 \cdot 3 \times 10^{-12}}{(0.2)^2} = 2.7 \text{ N}

Net vertical force: Fsin60=1.56 N-F \sin 60^\circ = -1.56 \text{ N}

Net horizontal force: Fcos60+F2μC=3.6 NF \cos 60^\circ + F_{2\mu C} = 3.6 \text{ N}

Electric field of a point charge

E=Fq(9.4)E = \frac{F}{q} \quad \text{(9.4)}

Using Coulomb's law:

F=14πε0qoqr2F = \frac{1}{4 \pi \varepsilon_0} \frac{|q_o q|}{r^2}

Then,

E=14πε0qor2(9.5)E = \frac{1}{4 \pi \varepsilon_0} \frac{q_o}{r^2} \quad \text{(9.5)}

Electric field lines

Originate from positive and terminate on negative charges. They never cross each other and are perpendicular to conductors' surfaces.

Example

Two charges 2μC2 \mu \text{C} at 20 cm apart:

At midpoint, E1=E2E_1 = E_2, but in opposite directions ⇒ E=0\sum E = 0

Example

Q=3.3 nC,εr=5,r=0.1 mQ = 3.3 \text{ nC}, \varepsilon_r = 5, r = 0.1 \text{ m}

ε=ε0εr=58.854×1012\varepsilon = \varepsilon_0 \varepsilon_r = 5 \cdot 8.854 \times 10^{-12}

E=14πεQr2=9×10953.3×1090.01594  N/CE = \frac{1}{4 \pi \varepsilon} \frac{Q}{r^2} = \frac{9 \times 10^9}{5} \cdot \frac{3.3 \times 10^{-9}}{0.01} \approx 594 \; \text{N/C}

Electric field due to continuous charge distribution

In practice, we deal with charge distribution along a line, over a surface, or within a volume. The linear, surface, and volume charge densities are:

λ=dQdl,σ=dQdA,ρ=dQdV\lambda = \frac{dQ}{dl}, \quad \sigma = \frac{dQ}{dA}, \quad \rho = \frac{dQ}{dV}

These represent the charge per unit length, area, and volume, respectively. The electric field due to a continuous distribution is the sum (integral) of infinitesimal fields dEdE from elements dQdQ.

Vector form: The infinitesimal electric field due to an element dQdQ at position r\vec{r}' is:

dE=14πε0dQ(rr)rr3d\vec{E} = \frac{1}{4\pi\varepsilon_0} \frac{dQ (\vec{r} - \vec{r}')}{|\vec{r} - \vec{r}'|^3}

and the total electric field is:

E=14πε0(rr)rr3dq\vec{E} = \frac{1}{4\pi\varepsilon_0} \int \frac{(\vec{r} - \vec{r}')}{|\vec{r} - \vec{r}'|^3} \, dq

a. Electric field due to a line of charge

dE=kdQr2,dEx=dEcosθ=kdQr2xrdE = k \frac{dQ}{r^2}, \quad dE_x = dE \cos \theta = k \frac{dQ}{r^2} \frac{x}{r}

dQ=λdydQ = \lambda dy

Total field:

Ep=abdEx=kλabxdy(x2+y2)3/2E_p = \int_{-a}^{b} dE_x = k\lambda \int_{-a}^{b} \frac{x \, dy}{(x^2 + y^2)^{3/2}}

=kλxx2+y2ab=kλxx2+b2+kλxx2+a2= \frac{k\lambda x}{\sqrt{x^2 + y^2}} \Big|_{-a}^{b} = \frac{k\lambda x}{\sqrt{x^2 + b^2}} + \frac{k\lambda x}{\sqrt{x^2 + a^2}}

As a,ba, b \to \infty:

Ep=2kλx=λ2πε0xE_p = \frac{2k\lambda}{x} = \frac{\lambda}{2\pi \varepsilon_0 x}

Note: This result demonstrates the inverse dependence on distance from an infinite line of charge, unlike the inverse-square law for point charges.

Electric flux and Gauss's law

Φ=EA=EAcosθ\Phi = \vec{E} \cdot \vec{A} = EA \cos \theta

For curved surfaces or non-uniform fields:

Φ=EcosθdA=EdA\Phi = \int E \cos \theta \, dA = \int \vec{E} \cdot d\vec{A}

Example 8

Φ=EAcos30=(2.0×103)(π0.12)cos3054Nm2/C\Phi = E A \cos 30^\circ = (2.0 \times 10^3)(\pi \cdot 0.1^2) \cos 30^\circ \approx 54 \, \text{Nm}^2\text{/C}

Gauss's law

EdA=Qε0\oint \vec{E} \cdot d\vec{A} = \frac{Q}{\varepsilon_0}

Steps:

  1. Choose symmetric Gaussian surface
  2. Ensure EdA\vec{E} \parallel d\vec{A}
  3. Integrate over the entire surface

Advanced symmetries: Gauss's law is powerful when applied to systems with high symmetry:

  • Plane symmetry → Infinite plane sheet
  • Cylindrical symmetry → Line charge, coaxial cables
  • Spherical symmetry → Spherical shells, point charges

Limitation: Gauss's law is always true, but only useful for calculating E\vec{E} when symmetry simplifies the surface integral.

b. Electric field due to a spherical charge

For a solid sphere (radius R, charge density ρ\rho):

Q=43πR3ρQ = \frac{4}{3}\pi R^3 \rho

Outside (r>Rr > R):

E=Q4πε0r2E = \frac{Q}{4\pi\varepsilon_0 r^2}

Inside (r<Rr < R):

Q=Q(r3R3),E=Qr4πε0R3Q' = Q \left( \frac{r^3}{R^3} \right), \quad E = \frac{Qr}{4\pi\varepsilon_0 R^3}

Graphical insight: Electric field increases linearly inside a uniformly charged sphere, reaches maximum at the surface, then decreases as 1/r21/r^2 outside.

c. Solid conducting sphere

Outside (r>Rr > R):

E=Q4πε0r2E = \frac{Q}{4\pi\varepsilon_0 r^2}

Inside (r<Rr < R):

E=0E = 0

Reason: In electrostatics, charges on conductors reside on the surface. The field inside a conductor in equilibrium is zero.

d. Hollow conducting sphere

Outside (r>R2r > R_2):

E=Q4πε0r2E = \frac{Q}{4\pi\varepsilon_0 r^2}

Inside hollow (r<R1r < R_1):

E=0E = 0

Between shells (R1<r<R2R_1 < r < R_2):

E=Q(r3R13)4πε0r2(R23R13)E = \frac{Q(r^3 - R_1^3)}{4\pi\varepsilon_0 r^2 (R_2^3 - R_1^3)}

Note: Inside a cavity of a conductor, the electric field is zero if no charge is present inside.

f. Electric field due to plane charge

For an infinite plane:

E=σ2ε0E = \frac{\sigma}{2\varepsilon_0}

Two sheets with σ1,σ2\sigma_1, \sigma_2:

Region I: E=12ε0(σ1+σ2)E = -\frac{1}{2\varepsilon_0}(\sigma_1 + \sigma_2)

Region II: E=12ε0(σ1σ2)E = -\frac{1}{2\varepsilon_0}(\sigma_1 - \sigma_2)

Region III: E=12ε0(σ1+σ2)E = \frac{1}{2\varepsilon_0}(\sigma_1 + \sigma_2)

Parallel plate capacitors mimic plane charge distribution behavior. Between the plates, the field is:

E=σε0(if equal and opposite)E = \frac{\sigma}{\varepsilon_0} \quad \text{(if equal and opposite)}

This uniform field is essential in applications like CRTs, capacitors, and sensors.

Additional concept: Superposition of electric fields

The principle of superposition allows for calculating the net electric field due to multiple sources:

Enet=E1+E2+E3+\vec{E}_{\text{net}} = \vec{E}_1 + \vec{E}_2 + \vec{E}_3 + \cdots

This is crucial when dealing with complex configurations of charges.

Application: Charged cylindrical shell (Advanced Gauss's law)

Consider a long cylindrical shell of radius RR carrying surface charge density σ\sigma. Using a cylindrical Gaussian surface:

  • r>Rr > R: E=σRε0rE = \frac{\sigma R}{\varepsilon_0 r}
  • r<Rr < R: E=0E = 0

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