physics 212 lecture 3, slide 1 physics 212 lecture 3 today's concepts: electric flux and field...
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Physics 212 Lecture 3, Slide 3 Our Comments SmartPhysics scores will not be visible in the main gradebook for a few weeks You will need to understand integrals in this course!!! Forces and Fields are Vectors Always Draw a Picture First… What do the Forces/Fields Look Like?Prelecture Infinite line of charge E Lecture Finite line of charge (constant ) E Worked Example Finite line of charge (non-constant ) E Homework Arc of charge (constant ) E WORKS FOR ALL !! The “1/4 shell problem” is not special !! It’s the same as all the others!TRANSCRIPT
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 11
Physics 212Physics 212Lecture 3Lecture 3
Today's Concepts:Today's Concepts:
Electric Flux and Field LinesElectric Flux and Field Lines
Gauss’s LawGauss’s Law
MusicWho is the Artist?Who is the Artist?
A)A) Professor LonghairProfessor LonghairB)B) Henry ButlerHenry ButlerC)C) David EganDavid EganD)D) Dr. JohnDr. JohnE)E) Allen ToussaintAllen Toussaint
WHY?WHY?
Mardi Gras is 4 weeks from todayMardi Gras is 4 weeks from today
Physics 212 Lecture 13Physics 212 Lecture 13
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 33
Our Comments• SmartPhysics scores will not be visible in the main gradebook for a
few weeks• You will need to understand integrals in this course!!!• Forces and Fields are Vectors• Always Draw a Picture First… What do the Forces/Fields Look Like?
PrelecturePrelecture
Infinite line of chargeInfinite line of charge
EELectureLecture
Finite line of chargeFinite line of charge(constant (constant ))
EEWorked ExampleWorked Example
Finite line of chargeFinite line of charge(non-constant (non-constant ))
EE
HomeworkHomework
Arc of chargeArc of charge(constant (constant ))
EE2 20
1ˆ ˆ4
dq dqE k r rr r
WORKS FOR ALL !!WORKS FOR ALL !!
The “1/4 shell problem” is not The “1/4 shell problem” is not special !!special !!
It’s the same as all the others!It’s the same as all the others!
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 44
Electric Field LinesElectric Field Lines
Direction & Density of Lines Direction & Density of Lines representrepresent
Direction & Magnitude ofDirection & Magnitude of EE
Point Charge:Point Charge:Direction is radialDirection is radialDensity Density 1/R 1/R22
0707
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 55
Electric Field LinesElectric Field Lines
Dipole Charge Distribution:Dipole Charge Distribution:Direction & Direction & DensityDensity
much more interesting…much more interesting…
simulationsimulation0808
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 66
Preflight 3
Checkpoint 3.1
simulationsimulation0909
The following three questions pertain to the electric field lines due to the two charges shown. Compare the magnitude of the two chargesA. |Q1| > |Q2| B. |Q1| = |Q2| C. |Q1| < |Q2|D. There isn’t enough information to determine the relative magnitude of the charges
“more field lines emanating from the charge 1, so must be more field lines emanating from the charge 1, so must be greater in magnitude.greater in magnitude.”
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 77
Checkpoint 3.3
1010 simulationsimulation
What do we know about the signs of the charges from looking at the picture?A. Q1 and Q2 have the same signB. Q1 and Q2 have the opposite sign C. There isn’t enough information to determine the relative signs of the charges
““The field lines leave one and go to the other..The field lines leave one and go to the other..””
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 88
Preflight 3
Checkpoint 3.5
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Compare the magnitude of the electric field at point A and B.A. |EA| > |EB| B. |EA| = |EB| C. |EA| < |EB|D. There isn’t enough information to determine the relative magnitude of the electric field at points A and B
““Since the electric field lines are denser near Since the electric field lines are denser near point B the magnitude of the electric field is point B the magnitude of the electric field is greater at point B than at point A.greater at point B than at point A.””
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 99
Point Charges
+2q
-q
What charges are inside the red circle?What charges are inside the red circle?
+Q +Q
-Q
+2Q
-Q -2Q
+Q
-Q
A B C D E
“Telling the difference between positive and negative charges while looking at field lines. Does field line density from a certain charge give information about the sign of the charge?”
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1010
Which of the following field line pictures best represents the electric field from two charges that have the same sign but different magnitudes?
A B
C D
simulationsimulation1515
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1111
Electric Flux “Counts Field Lines”Electric Flux “Counts Field Lines”
SS
E dA
Flux through surface S
Integral of on surface S
E dA
““I still feel a little unclear about flux integrals. Can you go over some more example problems?” I still feel a little unclear about flux integrals. Can you go over some more example problems?”
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1212
“The flux is directly proportional to the charge enclosed by the Gaussian surface, therefore Case 1 will have 2 times the flux of of Case 2 because it has two charges enclosed, versus 1 in Case 2. “
“The flux is the measure of field lines passing through the surface. Once calculated, it can be shown that the surface area of both cylinders are the same.”
Checkpoint 1
(A)(A)11=2=222 11==22
(B)(B)11=1/2=1/222
(C)(C)nonenone(D)(D)
TAKE s TO BE RADIUS !TAKE s TO BE RADIUS !
L/2
An infinitely long charged rod has uniform charge density and passes through a cylinder (gray). The cylinder in Case 2 has twice the radius and half the length compared with the cylinder in Case 1.
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1313
Checkpoint 1
(A)(A)11=2=222 11==22
(B)(B)11=1/2=1/222
(C)(C)nonenone(D)(D)
TAKE s TO BE RADIUS !TAKE s TO BE RADIUS !
L/2
An infinitely long charged rod has uniform charge density l and passes through a cylinder (gray). The cylinder in Case 2 has twice the radius and half the length compared with the cylinder in Case 1.
Definition of Flux:Definition of Flux:
surface
AdE
E constant on barrel of cylinderE constant on barrel of cylinderE perpendicular to barrel surfaceE perpendicular to barrel surface(E parallel to dA)(E parallel to dA)
Case 1
sE
01 2
LsA )2(1 01
L
Case 2
)2(2 02 sE
sLLsA 22/))2(2(2 02
)2/(
L
RESULT: GAUSS’ LAW proportional to charge enclosed !
“The flux is the measure of field lines passing through the surface. Once calculated, it can be shown that the surface area of both cylinders are the same.”
WHAT IS WRONG WITH THIS REASONINGWHAT IS WRONG WITH THIS REASONING????
THE E FIELD AT THE BARREL SURFACE THE E FIELD AT THE BARREL SURFACE IS NOT THE SAME IN THE TWO CASES !!IS NOT THE SAME IN THE TWO CASES !!
barrelbarrel
EAAdE
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1414
Direction Matters:Direction Matters:
0SS
E dA
ddAA
ddAA
ddAA ddAA
ddAAEE
EE
EE
EE
EE
EE
EEEE
EE
For a closed surface, For a closed surface, AA points outward points outward
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1515
Direction Matters:Direction Matters:
0SS
E dA
ddAA
ddAA
ddAA ddAA
ddAAEE
EE
EE
EE
EE
EE
EEEE
EE
For a closed surface, For a closed surface, AA points outward points outward
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1616
Trapezoid in Constant Field0 ˆE E x
Label faces:1: x = 0
2: z = +a3: x = +a4: slanted
0E
y
z
Define n = Flux through Face n
AA
BB
CC
1 < 0
1 = 0
1 > 0
AA
BB
CC
2 < 0
2 = 0
2 > 0
AA
BB
CC
3 < 0
3 = 0
3 > 0
AA
BB
CC
< 0
= 0
> 0
x1 2
34
dAdA
EE
0 AdE
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1717
Trapezoid in Constant Field + Q0 ˆE E x
Label faces:1: x = 0
2: z = +a3: x = +a
Define n = Flux through Face n = Flux through Trapezoid
AA
BB
CC
1 increases
1 decreases
1 remains same
Add a charge +Q at (-a,a/2,a/2)
+Q
How does Flux change?
AA
BB
CC
increases
decreases
remains same
AA
BB
CC
3 increases
3 decreases
3 remains same
x
y
z
0E
x1 2
3
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1818
Q
Gauss LawGauss Law
ddAA
ddAA
ddAA ddAA
ddAAEE
EE
EE
EE
EE
EE
EEEE
EE
o
enclosed
surfaceclosed
SQAdE
4141
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 1919
Checkpoint 2.3
(A) increases
(B) decreases
(C) stays same
4343
““The flux throughout the entire The flux throughout the entire surface does not change as the surface does not change as the charge moves, for it is still in the charge moves, for it is still in the sphere. However, if it was moved sphere. However, if it was moved outside of the sphere, the fluxes outside of the sphere, the fluxes would be different because one would be different because one would be zero!would be zero!““
Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 2020
““charge is closer, field is larger, more charge is closer, field is larger, more lines through a so increase in flux.lines through a so increase in flux.““
““as long as the charge is within the as long as the charge is within the shell, the flux will remain the sameshell, the flux will remain the same” ”
Checkpoint 2.1
(A)dA increasesdB decreases
(B)dA decreasesdB increases
(C)dA stays samedB stays same
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 2121
The total flux is the same in both cases (just the total number of lines)
The flux through the right (left) hemisphere is smaller (bigger) for case 2.
11 22
Think of it this way:Think of it this way:
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 2222
Things to notice about Gauss’s LawThings to notice about Gauss’s Law
If If QQenclosedenclosed is the same, is the same, the flux has to the flux has to be the samebe the same, which means that the , which means that the integral must yield the same result integral must yield the same result for any surfacefor any surface..
o
enclosed
surfaceclosed
SQAdE
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 2323
Things to notice about Gauss’s LawThings to notice about Gauss’s Law
In cases of high symmetry it may be possible to bring In cases of high symmetry it may be possible to bring EE outside outside the integral. In these cases we can solve Gauss Law for the integral. In these cases we can solve Gauss Law for EE
So - if we can figure out So - if we can figure out QQenclosedenclosed and the area of the and the area of the surface surface AA, then we know , then we know EE ! !
This is the topic of the next lecture…This is the topic of the next lecture…
“Gausses law and what concepts are most important that we know .”
o
enclosed
surfaceclosed
QAdE
o
enclosed
surfaceclosed
QEAAdE
0
enclosedQE
A
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Physics 212 Lecture 3, Slide Physics 212 Lecture 3, Slide 2424
Final Thoughts….• Keep plugging away
– Prelecture 4 and Checkpoint 4 due Thursday– Homework 2 due next Tuesday … 7 questions mostly Gauss’ law –
try them today!
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