Physics 212 Lecture 3 Todays Concepts Electric Flux

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Physics 212 Lecture 3 Today's Concepts: Electric Flux and Field Lines Gauss’s Law Physics

Physics 212 Lecture 3 Today's Concepts: Electric Flux and Field Lines Gauss’s Law Physics 212 Lecture 3, Slide 1

Music Who is the Artist? A) B) C) D) E) Professor Longhair Henry Butler

Music Who is the Artist? A) B) C) D) E) Professor Longhair Henry Butler David Egan Dr. John Allen Toussaint WHY? Mardi Gras is 4 weeks from today Physics 212 Lecture 13

Our Comments • Smart. Physics scores will not be visible in the main gradebook

Our Comments • Smart. Physics 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 E Lecture Worked Example E E Infinite line of charge WORKS FOR ALL !! Finite line of charge (constant l) Homework E Arc of charge (constant l) Finite line of charge (non-constant l) The “ 1/4 shell problem” is not special !! It’s the same as all the others! Physics 212 Lecture 3, Slide 3

Electric Field Lines Direction & Density of Lines represent Direction & Magnitude of E

Electric Field Lines Direction & Density of Lines represent Direction & Magnitude of E Point Charge: Direction is radial Density 1/R 2 07 Physics 212 Lecture 3, Slide 4

Electric Field Lines Dipole Charge Distribution: Direction & Density much more interesting… 08 simulation

Electric Field Lines Dipole Charge Distribution: Direction & Density much more interesting… 08 simulation Physics 212 Lecture 3, Slide 5

Checkpoint 3. 1 Preflight 3 The following three questions pertain to the electric field

Checkpoint 3. 1 Preflight 3 The following three questions pertain to the electric field lines due to the two charges shown. Compare the magnitude of the two charges A. |Q 1| > |Q 2| B. |Q 1| = |Q 2| C. |Q 1| < |Q 2| 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 greater in magnitude. ” magnitude. 09 simulation Physics 212 Lecture 3, Slide 6

Checkpoint 3. 3 What do we know about the signs of the charges from

Checkpoint 3. 3 What do we know about the signs of the charges from looking at the picture? A. Q 1 and Q 2 have the same sign B. Q 1 and Q 2 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. . ” 10 simulation Physics 212 Lecture 3, Slide 7

Checkpoint 3. 5 Preflight 3 Compare the magnitude of the electric field at point

Checkpoint 3. 5 Preflight 3 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 point B the magnitude of the electric field is greater at point B than at point A. ” 12 Physics 212 Lecture 3, Slide 8

Point Charges “Telling the difference between positive and negative charges while looking at field

Point Charges “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? ” -q +2 q What charges are inside the red circle? 13 -Q -Q -2 Q +Q +Q +2 Q +Q A B C D -Q E Physics 212 Lecture 3, Slide 9

Which of the following field line pictures best represents the electric field from two

Which of the following field line pictures best represents the electric field from two charges that have the same sign but different magnitudes? 15 A B C D simulation Physics 212 Lecture 3, Slide 10

Electric Flux “Counts Field Lines” “I still feel a little unclear about flux integrals.

Electric Flux “Counts Field Lines” “I still feel a little unclear about flux integrals. Can you go over some more example problems? ” Flux through surface S 18 Integral of on surface S Physics 212 Lecture 3, Slide 11

Checkpoint 1 “The flux is directly proportional to the charge enclosed by the Gaussian

Checkpoint 1 “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. “ 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 TAKE s TO BE RADIUS ! with the cylinder in Case 1. L/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. ” F 1=2 F 2 (A) 23 F 1=F 2 (B) F 1=1/2 F 2 (C) none (D) Physics 212 Lecture 3, Slide 12

Checkpoint 1 An infinitely long charged rod has uniform charge density l and passes

Checkpoint 1 An infinitely long charged rod has uniform charge density l and passes through a cylinder WHAT IS WRONG WITH THIS REASONING? ? (gray). The cylinder in Case 2 has twice the radius and half the length compared with the “The flux is the measure of field TAKE s TO BE RADIUS ! cylinder in Case 1. lines passing through the surface. Once calculated, it can be shown that the surface area of both cylinders are the same. ” THE E FIELD AT THE BARREL SURFACE IS NOT THE SAME IN THE TWO CASES !! L/2 Definition of Flux: E constant on barrel of cylinder E perpendicular to barrel surface (E parallel to d. A) Case 1 26 F 1=2 F 2 (A) F 1 RESULT: = F 2 F GAUSS’ 1=1/2 F 2 LAW none (D) ! (B) F proportional to charge (C) enclosed Case 2 Physics 212 Lecture 3, Slide 13

Direction Matters: E E E d. A For a closed surface, A points outward

Direction Matters: E E E d. A For a closed surface, A points outward d. A E E d. A E 29 E E Physics 212 Lecture 3, Slide 14

Direction Matters: E E E d. A For a closed surface, A points outward

Direction Matters: E E E d. A For a closed surface, A points outward d. A E E d. A E 30 E E Physics 212 Lecture 3, Slide 15

Trapezoid in Constant Field y Label faces: 1: x = 0 2: z =

Trapezoid in Constant Field y Label faces: 1: x = 0 2: z = +a 3: x = +a 4: slanted 4 3 1 2 x Define Fn = Flux through Face n d. A z 31 E A F 1 < 0 A F 2 < 0 A F 3 < 0 A F 4 < 0 B F 1 = 0 B F 2 = 0 B F 3 = 0 B F 4 = 0 C F 1 > 0 C F 2 > 0 C F 3 > 0 C F 4 > 0 Physics 212 Lecture 3, Slide 16

Trapezoid in Constant Field + Q y Label faces: 1: x = 0 2:

Trapezoid in Constant Field + Q y Label faces: 1: x = 0 2: z = +a 3: x = +a 3 +Q 36 2 x Define Fn = Flux through Face n F = Flux through Trapezoid z 1 Add a charge +Q at (-a, a/2) How does Flux change? A F 1 increases A F 3 increases A F increases B F 1 decreases B F 3 decreases B F decreases C F 1 remains same C F 3 remains same C F remains same Physics 212 Lecture 3, Slide 17

Gauss Law E E Q E d. A E 41 E d. A E

Gauss Law E E Q E d. A E 41 E d. A E Physics 212 Lecture 3, Slide 18

Checkpoint 2. 3 (A) F increases 43 (B) F decreases (C) F stays same

Checkpoint 2. 3 (A) F increases 43 (B) F decreases (C) F stays same “The flux throughout the entire surface does not change as the charge moves, for it is still in the sphere. However, if it was moved outside of the sphere, the fluxes would be different because one would be zero!“ Physics 212 Lecture 3, Slide 19

Checkpoint 2. 1 “charge is closer, field is larger, more lines through a so

Checkpoint 2. 1 “charge is closer, field is larger, more lines through a so increase in flux. “ “as long as the charge is within the shell, the flux will remain the same” (A) d. FA increases d. FB decreases 44 (B) d. FA decreases d. FB increases (C) d. FA stays same d. FB stays same Physics 212 Lecture 3, Slide 20

Think of it this way: 1 2 The total flux is the same in

Think of it this way: 1 2 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. 45 Physics 212 Lecture 3, Slide 21

Things to notice about Gauss’s Law If Qenclosed is the same, the flux has

Things to notice about Gauss’s Law If Qenclosed is the same, the flux has to be the same, which means that the integral must yield the same result for any surface. 47 Physics 212 Lecture 3, Slide 22

Things to notice about Gauss’s Law “Gausses law and what concepts are most important

Things to notice about Gauss’s Law “Gausses law and what concepts are most important that we know. ” In cases of high symmetry it may be possible to bring E outside the integral. In these cases we can solve Gauss Law for E So - if we can figure out Qenclosed and the area of the surface A, then we know E ! This is the topic of the next lecture… 48 Physics 212 Lecture 3, Slide 23

Final Thoughts…. • Keep plugging away – Prelecture 4 and Checkpoint 4 due Thursday

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! 50 Physics 212 Lecture 3, Slide 24