Gauss' Law and Electric Fields: Calculation and Symmetries, Study notes of Physics

A chapter from a physics textbook focusing on gauss' law and its application to calculate electric fields in various symmetrical charge distributions, including spherical, cylindrical, and rectangular symmetries. It covers topics such as conductors, spherical symmetry, axial symmetry, and rectangular symmetry, providing equations and solutions for different scenarios.

Typology: Study notes

Pre 2010

Uploaded on 09/17/2009

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PHY2049: Chapter 23

First Beams at LHC!

PHY2049: Chapter 23

Gauss’ Law Says

Î

Total flux depends only on the amount ofenclosed charge, not on shape and size of theGaussian surface.

Î

Charges outside have

no effect on the total

flux. ÎThis does not mean they do not contribute to E

Remember:

‹Outward E field, flux > 0 ‹Inward E field,

flux < 0

enc ε^0 q

d S^

∫^

A
E

PHY2049: Chapter 23

Use Gauss’ Law to Calculate E Fields Î

Spherical symmetry^ ‹

E field vs r inside uniformly charged sphere ‹

Charges on concentric spherical conducting shells Î

Cylindrical symmetry^ ‹

E field vs r for line charge ‹

E field vs r inside uniformly charged cylinder Î

Rectangular symmetry^ ‹

E field for charged plane ‹

E field between conductors, e.g. capacitors

PHY2049: Chapter 23

Spherical Symmetry (1)

ÎInsulator or conductor?

‹^ Conducting sphere cannot be uniformly charged ÎInside

‹^ By symmetry, E must be radially symmetric ‹^ E field has constant mag.,

⊥^

to Gaussian surface

ÎOutside

Gaussian surface

(sphere)

Gauss’ Law

Solve for E

Uniformly Charged Sphere

enc^0

2 ) (^4) (

q ε

rπ E

d S^

∫^

A
E

+^ +

+^

+^ +

+^

+^ +

+^ +

+^

+^ +

+^

+^ +

+^ +

+^

+^ +

+^

+^ +

+^ +

+^

+^ +

+^

+^ +

+^ +

+^

+^ +

+^

+^ +

+^ +

+^

+^ +

+^ +

+^

3 4 3 Q Rπ Q ρ = 3 3

3 ) (^4) ( 3

r R Q rπ ρ^

= Q 3 0 2 0

3 3

(^14)

4

/

Qr^ R πε

r πε

R Qr E^

=

=

2 0 (^14)

Q r πε

E^

=

Volume chargedensity

PHY2049: Chapter 23

Axial Symmetry (1):

Line Charge

ÎInfinitely long line, uniformly charged

‹^ By symmetry, E must be axially symmetric ‹^ On curved surface, E field has constantmag.,

to Gaussian surface

‹^ Through top and bottom surfaces, no

Φ

E

since E is ||

Solve for E

enc^0

0 0 ) 2 (^

q ε

rπ h E

d S^

∫^

A
E

Gauss’ Law

λ r πε E

0 (^12) =^

λ: linear charge density

PHY2049: Chapter 23

Axial Symmetry (2):

Uniformly Charged Cylinder

ÎInfinitely tall cylinder, uniformly charged

‹^ By symmetry, E must be axially symmetric ‹^ On curved surface, E field has constant mag.,^ ⊥

to Gaussian surface ‹^ Through top and bottom surfaces, no

Φ

sinceE

E is ||

)

(^

(^2) r πh ρ

Solve for E

enc^0

0 0 ) 2 (^

q ε

rπ h E

d S^

∫^

A
E

Gaussian surface

(cylindrical) ρ

R r

h

Gauss’ law

rρ ε

E

0 (^12) =

ρ: volumecharge density

PHY2049: Chapter 23

λ πε

E

0 2

1

Some Comparisons

total^2 r 0

q

E^

r

0 σ 2 ε

E^

No distance dependence!

Î

Spherically symmetric charge distribution Î

Uniformly charged, infinitely long (i.e., verylong) line Î

Uniformly charged plane