38
Chapter 23 Electric Potential Physics for Scientists & Engineers, 3 rd Edition Douglas C. Giancoli © Prentice Hall

Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

  • Upload
    others

  • View
    7

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Chapter 23

Electric Potential

Physics for Scientists & Engineers, 3rd EditionDouglas C. Giancoli

© Prentice Hall

Page 2: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

10P04 -

Potential Energyand Potential

Start with Gravity

Page 3: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

11P04 -

Gravity: Force and Work

Gravitational Force on m due to M:

2ˆg

MmGr

= −F r

Work done by gravity moving m from A to B:

g

B

g AW d= ⋅∫ F s PATH

INTEGRAL

Page 4: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

12P04 -

Work Done by Earth’s GravityWork done by gravity moving m from A to B:

ggW d= ⋅∫F s

( )2ˆ ˆˆ

B

A

GMm

rdr rdθ−⎛ ⎞= ⋅ +⎜ ⎟

⎝ ⎠∫ r r θ

1 1

B A

GMmr r

⎛ ⎞= −⎜ ⎟

⎝ ⎠

2

B

A

r

r

GMm drr

= −∫B

A

r

r

GMm

r= ⎡ ⎤⎢ ⎥⎣ ⎦

What is the sign moving from rA to rB?

Page 5: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

13P04 -

Work Near Earth’s Surface

2 ˆ ˆE

GM gr

≈ − = −g y yG roughly constant:

Work done by gravity moving m from A to B:

( )ˆB

Amg d= − ⋅∫ y sg gW d= ⋅∫F s

By

yAmgdy= −∫ ( )B Amg y y= − −

Wg depends only on endpoints– not on path taken –Conservative Force

Page 6: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

14P04 -

Potential Energy (Joules)B

g B A g g extAU U U d W W∆ = − = − ⋅ = − = +∫ F s

02ˆ(1) g g

GMm GMmU Ur r

= − → = − +F r

• U0: constant depending on reference point• Only potential difference ∆U has

physical significance

0ˆ(2) g gmg U mgy U= − → = +F y

Page 7: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

15P04 -

Gravitational Potential(Joules/kilogram)

Define gravitational potential difference:

g( / )B Bg

g A A

UV m d d

m∆

∆ = = − ⋅ = − ⋅∫ ∫F s g s

gFieldForce Energy Potential

Just as , g gU V→ ∆ → ∆F g

That is, two particle interaction single particle effect

Page 8: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

17P04 -

Move to Electrostatics

Page 9: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

19P04 -

Potential & Energy

B

A

V d∆ ≡ − ⋅∫E sUnits:

Joules/Coulomb = Volts

Work done to move q from A to B:

ext B AW U U U= ∆ = −

q V= ∆ Joules

Page 10: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

18P04 -

Gravity - Electrostatics

2ˆMG

r= −g r

Mass M Charge q (±)

2ˆe

qkr

=E r

g m=F g E q=F EBoth forces are conservative, so…

B

g gAU d∆ = − ⋅∫ F s

B

EAU d∆ = − ⋅∫ F s

B

AV d∆ = − ⋅∫ E s

B

g AV d∆ = − ⋅∫ g s

Page 11: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

20P04 -

Potential: Summary Thus Far

Charges CREATE Potential Landscapes

0 0"0"

( )V V V V d= + ∆ ≡ − ⋅∫r

r E s

Page 12: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

21P04 -

Potential Landscape

Positive Charge

Negative Charge

Page 13: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

22P04 -

Potential: Summary Thus Far

Charges CREATE Potential Landscapes

0 0"0"

( )V V V V d= + ∆ ≡ − ⋅∫r

r E s

Charges FEEL Potential Landscapes

( ) ( )U qV=r r

We work with ∆U (∆V) because only changes matter

Page 14: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-4

Page 15: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-5

Page 16: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

26P04 -

Potential Created by Pt Charge

θrsd ˆˆ θdrdr +=

B

B A AV V V d∆ = − = − ⋅∫ E s

2

ˆr

kQ rE =

2 2

ˆB B

A A

drkQ d kQr r

= − ⋅ = −∫ ∫r s

1 1

B A

kQr r

⎛ ⎞= −⎜ ⎟

⎝ ⎠

Take V = 0 at r = ∞:

rkQrV =)(ChargePoint

Page 17: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

28P04 -

Potential Landscape

Positive Charge

Negative Charge

Page 18: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-8

Page 19: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-7

Page 20: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-9

Page 21: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

42P05 -

Potential from E

Page 22: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

45P05 -

Potential for Uniformly Charged Non-Conducting Solid Sphere

Page 23: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

43P05 -

Potential for Uniformly Charged Non-Conducting Solid SphereFrom Gauss’s Law

20

30

ˆ,4

ˆ,4

Q r Rr

Qr r RR

πε

πε

⎧ >⎪⎪= ⎨⎪ <⎪⎩

rE

r

B

B AA

V V d− = − ⋅∫E sUse

( )0

BV V=

− ∞Region 1: r > a

204

r Q drrπε∞

= −∫0

14

Qrπε

=

Point Charge!

Page 24: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

44P05 -

Potential for Uniformly Charged Non-Conducting Solid Sphere

( ) ( )R r

RdrE r R drE r R

∞= − > − <∫ ∫

Region 2: r < a( )

0

DV V=

− ∞

2

20

1 38

Q rR Rπε⎛ ⎞

= −⎜ ⎟⎝ ⎠

2 30 04 4

R r

R

Q Qrdr drr Rπε πε∞

= − −∫ ∫

( )2 23

0 0

1 1 14 4 2

Q Q r RR Rπε πε

= − −

Page 25: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-6 (a)

Page 26: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-6 (b)

Page 27: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

46P05 -

Group Problem: Charge SlabInfinite slab with uniform charge density ρThickness is 2d (from x=-d to x=d). If V=0 at x=0 (definition) then what is V(x) for x>0?

Page 28: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

47P05 -

Group Problem: Spherical ShellsThese two spherical shells have equal but opposite charge.

Find E everywhere

Find V everywhere (assume V(∞) = 0)

Page 29: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-11

Page 30: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-12

Page 31: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-36

Page 32: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-27

Page 33: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

Figure 23-23

dmaria
Cross-Out
dmaria
Replacement Text
shell
Page 34: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

30P04 -

Deriving E from V

ˆx∆ = ∆s i

A = (x,y,z), B=(x+∆x,y,z)

B

A

V d∆ = − ⋅∫E s

( , , )

( , , )

x x y z

x y z

V d+∆

∆ = − ⋅∫ E s ≅ − ⋅∆E s ˆ( ) xx E x= − ⋅ ∆ = − ∆E i

xV VEx x

∆ ∂≅ − → −

∆ ∂Ex = Rate of change in V

with y and z held constant

Page 35: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

31P04 -

Deriving E from VIf we do all coordinates:

V= −∇E

ˆ ˆ ˆV V Vx y z

⎛ ⎞∂ ∂ ∂= − +⎜ ⎟∂ ∂ ∂⎝ ⎠

E i + j k

ˆ ˆ ˆ Vx y z

⎛ ⎞∂ ∂ ∂= − +⎜ ⎟∂ ∂ ∂⎝ ⎠

i + j k

Gradient (del) operator:

ˆ ˆ ˆx y z∂ ∂ ∂

∇ ≡ +∂ ∂ ∂i j+ k

Page 36: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

34P04 -

Configuration EnergyHow much energy to put two charges as pictured?

1) First charge is free2) Second charge sees first:

1 2

1212 2 2 1

14 o

q qU W q V

rπε= = =

Page 37: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

35P04 -

Configuration EnergyHow much energy to put three charges as pictured?

1) Know how to do first two2) Bring in third:

( )3 3 1 2W q V V= + 3 1 2

0 13 234q q q

r rπε⎛ ⎞

= +⎜ ⎟⎝ ⎠

Total configuration energy:

1 3 2 31 22 3 12 13 23

0 12 13 23

14

q q q qq qU W W U U Ur r rπε

⎛ ⎞= + = + + = + +⎜ ⎟

⎝ ⎠

Page 38: Douglas C. Giancoli Chapter 23 - Physics & Astronomyphysics.gmu.edu/~Dmaria/Phys260spring2011/Other sources/Ch23.pdfP04-11 Gravity: Force and Work Gravitational Force on m due to M:

36P04 -

In Class Problem

How much energy in joules is required to put the three charges in the configuration pictured if they start out at infinity?

What is the electric potential in volts at point P?

Suppose you move a fourth change +3Q from infinity in to point P. How much energy does that require (joules)?