PHYS 202 Notes, Week 5people.physics.tamu.edu/christian/files/phys202/week5.pdf · PHYS 202 Notes,...

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I mportant points Magnetic fields (symbol B ) are vec- tor fields arising from permanent magnets or from moving charges. Magnetic forces act on moving charges (currents). Right hand rule describes the direc- tion of the magnetic force on a positive charge (negative charge is the oppo- site). I mportant equations Magnitude of the magnetic force on a moving charge: F = |q|v B F = |q|vB F = |q|vBsinφ Figure 1: Magnetic field lines for a bar magnet. 1 The SI units of magnetic field are the Tesla, or T. 1T= 1N/(A · m) 2 The unit Gauss, or G, is also sometimes used. 1G = 10 -4 T PHYS 202 Notes, Week 5 Greg Christian February 16 & 18, 2016 Last updated: 02/18/2016 at 12:15:30 This week we introduce magnetic forces and related concepts. Magnetic Fields and Forces So far we’ve focused on the electric field and electric force, which orig- inates from stationary charges. However, it has a counterpart, the mag- netic field, which originates from moving charges. Background You are probably familiar with the magnetic field already from day- to-day life, with things like refrigerator magnets. These are examples of permanent magnets, which have been known for thousands of years. The magnetic force related to permanent magnets was originally de- scribed in terms of North and South poles. Like charges, opposites poles attract and like poles repel. Magnetic Field Lines Like the electric field, the magnetic field is a vector field. This means that at every point in space it has a magnitude and a direction. Also like the electric field, you can draw field lines which describe the strength and direction of the magnetic field at different points in space. Figure 1 shows an example of magnetic field lines for a bar magnet. The arrows denote the direction of the magnetic field, and the density of the lines represents the field strength, or magnitude. Magnetic fields are denoted by the symbol B . Note that we use the vector notation since the magnetic field has both magnitude and direction. 1, 2 Magnetic Force Later on, we’ll learn about how magnetic fields are created. Right now, let’s focus on the forces they provide to moving charges. Let’s assume we have a charged particle q moving in some direction with velocity v , inside a magnetic field given by the vector B (c.f. Figure 2). The magnitude of the magnetic force F is given by: F = |q|vB sin φ. (1)

Transcript of PHYS 202 Notes, Week 5people.physics.tamu.edu/christian/files/phys202/week5.pdf · PHYS 202 Notes,...

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Important points

• Magnetic fields (symbol#»B ) are vec-

tor fields arising from permanentmagnets or from moving charges.

• Magnetic forces act on movingcharges (currents).

• Right hand rule describes the direc-tion of the magnetic force on a positivecharge (negative charge is the oppo-site).

Important equations

• Magnitude of the magnetic force on amoving charge:

F = |q|v⊥B

F = |q|vB⊥F = |q|vBsinφ

Figure 1: Magnetic field lines for a barmagnet.1 The SI units of magnetic field are theTesla, or T. 1T = 1N/(A ·m)2 The unit Gauss, or G, is also sometimesused. 1G = 10−4T

PHYS 202 Notes, Week 5Greg Christian

February 16 & 18, 2016Last updated: 02/18/2016 at 12:15:30

This week we introduce magnetic forces and related concepts.

Magnetic Fields and Forces

So far we’ve focused on the electric field and electric force, which orig-inates from stationary charges. However, it has a counterpart, the mag-netic field, which originates from moving charges.

Background

You are probably familiar with the magnetic field already from day-to-day life, with things like refrigerator magnets. These are examplesof permanent magnets, which have been known for thousands of years.The magnetic force related to permanent magnets was originally de-scribed in terms of North and South poles. Like charges, oppositespoles attract and like poles repel.

Magnetic Field Lines

Like the electric field, the magnetic field is a vector field. This meansthat at every point in space it has a magnitude and a direction. Also likethe electric field, you can draw field lines which describe the strengthand direction of the magnetic field at different points in space. Figure 1

shows an example of magnetic field lines for a bar magnet. The arrowsdenote the direction of the magnetic field, and the density of the linesrepresents the field strength, or magnitude.

Magnetic fields are denoted by the symbol#»B. Note that we use

the vector notation since the magnetic field has both magnitude anddirection.1,2

Magnetic Force

Later on, we’ll learn about how magnetic fields are created. Right now,let’s focus on the forces they provide to moving charges. Let’s assumewe have a charged particle q moving in some direction with velocity#»v , inside a magnetic field given by the vector

#»B (c.f. Figure 2). The

magnitude of the magnetic force F is given by:

F = |q|vB sin φ. (1)

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Figure 2: The magnitude of the mag-netic force is given by: F = |q|vB sin φ =|q|v⊥B = |q|vB⊥.

Alternatively, we can define the “perpendicular component of thevelocity” as v⊥ = v sin φ and write

F = |q|v⊥B. (2)

And similarly we can define the “perpendicular component of thefield” as B⊥ = B sin φ, with

F = |q|vB⊥. (3)

The direction of the magnetic force is given by something called theright hand rule. This is a procedure you can use to figure out the direc-tion of the magnetic force on a moving charge q, given its velocity #»vand a magnetic field

#»B. The procedure is:

1. Draw #»v and#»B with their tails together.

2. Identify the plane containing both #»v and#»B.

3. Using your right hand, curl your fingers from #»v to#»B along the

smaller angle in the plane from step 2.4. The direction of your thumb is the direction of the magnetic force

on a positive charge.

Note that the direction of your thumb defines the force direction on apositive charge. The force direction on a negative would be in the exactopposite direction. When dealing with negative charges, use the righthand rule as described, then just reverse the direction as a last step.

The right hand rule for determining the direction of the magneticforce is illustrated in Figure 3. You can also find a nice YouTube videodemonstrating this at the following link (replace her #»a with #»v and

bwith

#»B): https://www.youtube.com/watch?v=zGyfiOqiR4s

F out of board

Place fingers indirection of v. Rotate towards

direction of B.

F into board

Place fingers indirection of v.

Rotate towardsdirection of B.

Figure 3: Illustration of the right handrule for magnetic forces on a movingpositive charge.

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Important points

• Moving charges in a uniform mag-netic field undergo circular motion.

• Current-carrying wires in a magneticfield experience a force.

Important equations

• Circular motion

F = |q|vB = mv2/R

R = mv/(|q|B)

• Cyclotron frequency

ω = |q|B/m

• Force on a current-carrying wire:

F = IlB sin φ

= IlB⊥

Figure 4: Circular trajectory of a chargedparticle moving in a magnetic field.

Figure 5: Illustration of helical motion.

Motion of Charged Particles in a Magnetic Field

Imagine that a positively charged particle with velocity #»v enters auniform magnetic field. Initially, #»v and

#»B are perpendicular, as in

the bottom of Figure 4. The direction of#»B is into the page, and the

direction of the velocity is to the right. The following sequence ofevents then happens:

1. The charge experiences a force upwards (c.f. Eq. (1) and the righthand rule).

2. The force deflects the charge away from its initial trajectory. It’s nowmoving slightly upwards and to the right. However the magnituideof v stays the same.

3. The direction of the force also changes, such that it’s still perpendic-ular to #»v .

4. Repeat ad infinitum: the particle is undergoing circular motion.

When a particle undergoes circular motion in a magnetic field, theequation of motion is given by:

F = |q|vB = mv2

R, (4)

where R is the radius of the circle. Thus you can solve for the radiusof the circle R:

R =mv|q|B . (5)

Note that this is independent of the charge magnitude. In other words,positive and negative charges move in the same circular orbit. How-ever, the direction of their motions is reversed.

Cyclotron Frequency

The quantity m/(|q|B) describes the frequency of the orbit. This is oftencalled the cyclotron frequency, ω:

ω =|q|Bm

. (6)

Helical Motion

If the direction of the velocity is initially not perpendicular to the mag-netic field, then it will always maintain some component parallel tothe field. This results in a spiral motion, called helical motion, depictedin Figure 5.

Force on a wire

As mentioned in the last chapter, currents are nothing more than mov-ing charges inside a conductor, like a copper wire. As moving charges,

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F = IlB sinϕ

ϕ

ϕ

l

Figure 6: Magnetic force on a current-carrying wire.

Important points

• Closed current loops in a magneticfield experience a net torque, but nonet force.

• The torque tends to rotate the loop inthe direction of decreasing angle be-tween it and the magnetic field.

Important equations

• Torque on a current loop

τ = IAB sin φ

• Magnetic moment

– Single loop: µ = IA– Multi-loop solenoid: µ = NIA

• Solenoid torque

τ = NIAB sin φ

B

I

Fup

Fdown

FleftFrightϕ

τ

Figure 7: Illustration of force and torqueon a closed current loop in a magneticfield.

they experience a force due to a magnetic field. The force on each in-dividual charge carrier will be given by Eq. (1). Summing up all of theforces on individual charge carriers gives an expression for the magni-tude of the net force on a section of wire with length l and current I:

F = IlB sin φ, (7)

where φ is the angle between the wire and the field direction. Figure 6

shows an example.The direction of the force on a wire is given by the right hand rule,

in the exact same way as we already learned for individual charges.The only difference is that now you initially place your fingers in thedirection of the current and rotate towards the magnetic field. This isbecause current corresponds to the movement of positive charges.

Magnetic Torque and Force on Current Loops

As you saw in Example Problem 20.30 (page 17), the net force on aclosed current loop in a magnetic field is zero. This is because theforces on opposite sides of the loop cancel each other (since they arecarrying the same magnitude of current in opposite directions).

The torque on closed current loops in a magnetic field is not zero,however. This is because the opposing forces act on different locationson the loop. So while they cancel in terms of producing a net force,they can still cause the object to rotate as a result of having a net torque.

The torque on a current loop is illustrated in Figure 7. The forceon the top of the loop (

#»F up) and the force of the bottom of the loop

(#»F down) both tend to rotate the loop into the angle φ made between

the normal to the plane of the loop and the magnetic field#»B. The

magnitude of the torque is given by

τ = IAB sin φ, (8)

where

• I is the current flowing through the loop• A is the area of the loop• B is the magnetic field• φ is the angle between the magnetic field and the vector perpendic-

ular to the plane of the loop

The units of torque are N ·m.The direction of the torque always tends to rotate the loop into the

angle φ, that is, it tries to align the plane of the loop perpendicular tothe magnetic field (or to make φ = 0).

When the loop is perpendicular to the magnetic field (so when φ =

0), the torque is zero. This follows from Eq. (8) since sin (0) = 0.

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Figure 8: Example of a solenoid made ofmany loops of wire placed together.

Conceptually, it means that#»F up and

#»F down no longer push and pull

on the loop in a way that makes it rotate. Imagine Figure 7 with theloop drawn perpendicular to the field to visualize this.

Solenoids

So far, we’ve been dealing with single current loops in a magnetic field.However, we can also place many loops very close together. Thisconfiguration is called a solenoid. An example is shown in Figure 8.Solenoids experience a torque just like a single current loop, exceptthe magnitude is multiplied by N, the number of loops making up thesolenoid:

τ = NIAB sin φ. (9)

Magnetic Moment

In Eq. (8), the quantity IA is sometimes called the magnetic moment, orµ:

µ = IA. (10)

This is the expression for the magnetic moment of a single loop. Forsolenoids, we have to multiply by N to get the magnetic moment:

µ = NIA. (11)

Then in both cases, we can write the torque equation as

τ = µB sin φ. (12)

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phys 202 notes, week 5 6

Important points

• Magnetic fields are produced bymoving charges. In practice, thismeans currents flowing throughwires.

• The magnitude and direction of themagnetic field depends on the ge-ometry of the current-carrying wiresproducing it.

Important equations

• Field of a long, straight conductor

B = µ0 I/(2πr)

• Field at the center of N current loops(solenoid):

B = µ0 NI/(2R)

B = µ0nI (for L� R)

• Field inside a toroidal solenoid

B = µ0 NI/(2πr)

B = µ0nI (for b� [b− a])

• Ampere’s law

∑ B‖∆s = µ0 Iencl

3 Having no relationship to µ the mag-netic moment other than an unfortunatechoice of Greek symbols.

I

B

B = μ0I/(2πr)

Figure 9: Magnetic field produced by along, straight wire.

B

IR

B = μ0I/(2R)

Figure 10: Magnetic field produced by acurrent loop.

Producing Magnetic Fields

So far, we’ve only been concerned with the force that the magnetic fieldhas on moving charges (or currents). Now we turn to looking at howwe can produce magnetic fields, i.e. where the magnetic fields actuallycome from.

In general, magnetic fields are produced by moving charges. In prac-tice, this usually means currents flowing through a conductor. Theexact form of the magnetic field varies for different conductor geome-tries, which we’ll now explain in more detail.

Long Straight Wire

One of the simplest ways to produce a magnetic field is with a long,straight wire, as in Figure 9. In this configuration, the magnetic fieldis radial, that is, it curls around the wire having the same magnitude atany given distance from the wire. This is given by

B =µ0 I2πr

, (13)

with

• I the current flowing through the wire• r the radial distance from the wire• µ0 = 4π × 10−7 T·m/A a new fundamental constant.3

The direction of the field is given by a new version of the right handrule, also illustrated in Figure 9. To find the field direction,

1. Place your right thumb in the direction of the current flow.2. Curl your fingers around. The direction in which they curl is the

direction of#»B.

Current Loops

Another common geometry, especially in applications, are current loops,like the one shown in Figure 10. Here, the field at the center of the loopis given by

B =µ0 I2R

, (14)

where R is the radius of the loop. The direction is again given by avariation of the right hand rule:

1. Curl your right hand’s fingers in the direction of the current flow.2. Your thumb will point in the direction of

#»B.

For configurations with multiple loops, N in total, the field is justgiven by multiplying Eq. (14) by N:

B = Nµ0 I2R

. (15)

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1mn = 10

L

R

In general: B = μ0NI/(2R)If L >> R: B = μ0nI

Figure 11: Magnetic field of a longsolenoid.

II

I

BB

r

B=0

B=0

I

In general: B = μ0NI/(2πr)If b >> (b - a): B = μ0nI

Figure 12: Example of a toroidalsolenoid, or toroid.

Long Solenoids

In general, the field at the center of a solenoid is given by Eq. (15).However for a very long solenoid we can make an approximation tosimplify things. Consider a solenoid of length L and loop radius R,with L much larger than R (c.f. Figure 11). Let the solenoid have aloop density n, that is there are n loops per meter. In this case, thefield at the center of the solenoid is given by

B = µ0nI. (16)

Note that this is independent of both the length and the radius: the fielddepends only on the density of turns n and the current.

The direction of#»B inside the solenoid is determined by the same

right hand rule as in the previous section, for “short” solenoids.

Toroidal Solenoids

Another common geometry is a toroidal solenoid, or a toroid. This isbasically a bunch of wires looped around a doughnut-shaped circle,as in Figure 12. In this geometry, the magnetic field is only presentinside the loops. Its magnitude varies depending on the distance rfrom the center of the doughnut:

B =µ0NI2πr

. (17)

Take note that r is the distance from the center of the doughnut, as shownin the figure. It is not the distance from the inner surface of the dough-nut.

The direction of#»B is again given by a variation of the right hand

rule: curl your right hand’s fingers in the direction that the currentflows, and your thumb will point in the direction of

#»B.

Like normal solenoids, we can make some approximations in cer-tain cases. If the radial thickness of the core, i.e. (b− a) in the figure,is much smaller than the total radius (b in the figure), then the fieldinside the toroid is given by

B = µ0nI, (18)

where n is again the number of turns per meter.

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phys 202 notes, week 5 8

Summary

Figure 13 summarizes the magnetic fields produced by the most com-mon current geometries.

I

B

B = μ0I/(2πr)

B

IR

B = μ0I/(2R)

1mn = 10

L

R

In general: B = μ0NI/(2R)If L >> R: B = μ0nI

II

I

BB

r

B=0

B=0

I

In general: B = μ0NI/(2πr)If b >> (b - a): B = μ0nI

long, straight wire single current loop

solenoid toroid

Figure 13: Magnetic fields produced bycommon current geometries.

Ampere’s Law

For a general current geometry, we can use something called Ampere’sLaw to figure out the magnetic field. Ampere’s law is analogous toGauss’s Law in electrostatics. Ampere’s law can be thought of as aprocedure, or pseudo-algorithm, for finding out magnetic fields:

1. Construct an imaginary closed curve surrounding one or more con-ductors.

2. Divide this curve into segments, calling each one ∆s.

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3. At each segment, take the component of#»B parallel to ∆s and call it

B‖.4. Sum up all of the products B‖∆s going completely around the closed

curve.5. The sum in step 4 is equal to µ0 times the total enclosed current,

Iencl .

Mathematically, this is expressed as

∑ B‖∆s = µ0 Iencl . (19)

Figure 14 shows a general example of Ampere’s law being applied.

Figure 14: Illustration of Ampere’s law.

For a specific example of Ampere’s law, let’s revisit the “long straightwire” problem we already encountered (Figures 9 and 15). To applyAmpere’s law to find the field, we do the following:

1. Choose our closed curve to be a circle at some radius r.2. The enclosed current is just the current in the wire, I.

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Figure 15: Ampere’s law applied to along, straight wire.

Important points

• Parallel wires enact forces on eachother.

Important equations

F/l = µ0 I I′/(2πr)

3. For each small piece of the circle, with length ∆s, B‖ is perpendicu-lar to the direction of the arc, and we can take the product B‖∆s.

4. Summing up all the B‖∆s in step 3 just gives the total field B timesthe circumference of the circle:

∑ B⊥∆s = B (2πr) .

5. From Ampere’s law and step 4, we get

2πrB = µ0 I.

6. Finally, we can solve for B:

B = µ0 I/(2πr).

Force Between Parallel Conductors

When we have two long, parallel wires close together (Figure ??), wehave a situation where each is both creating a magnetic field and experi-encing a magnetic force. This is because the moving charges in wire Acreate a magnetic field (according to Eq. (13)) which exhibits a force onthe moving charges in wire B. Likewise, the moving charges in wire Bcreate a magnetic field exhibiting a force on wire A.

From the force equation, Eq. (7), and the equation for magnetic fieldof a long wire, Eq. (13), we can derive an expression for the force perunit length on either wire. Let’s assume we have two long, straightwires separated by a distance r. One (wire A) carries current I and theother (wire B) carries current I′. The force on some length l of wire Bis given by Eq. (7):

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phys 202 notes, week 5 11

F = I′Bl, (20)

where B is the field produced by wire A. This is given by Eq. (13):

B =µ0 I2πr

. (21)

Combining Equations (20) and (21) gives

F = I′(

µ0 I2πr

)l. (22)

Thus the force per unit length is

F/l =µ0 I I′

2πr. (23)

Alternatively, we could have switched the roles of wire A and wire Band come up with the exact same result, since the labelings I and I′

are arbitrary. Thus Eq. (23) equally applies to both wires A and B.

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Example Problems

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phys 202 notes, week 5 17

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