College Physics Quiz: Magnetism And Moving Charges
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Magnetism And Moving ChargesQuestion 1 of 16

An electron moves in a circular path of radius 2.02.0 cm in a uniform magnetic field. If the magnetic field strength is doubled while keeping the electron's speed constant, what happens to the radius of the circular path?

The radius becomes 1.01.0 cm because rr is inversely proportional to BB
The radius becomes 4.04.0 cm because rr is proportional to B2B^2
The radius remains 2.02.0 cm because speed is unchanged
The radius becomes 1.41.4 cm because rr is proportional to B\sqrt{B}
The radius becomes 2.82.8 cm because rr is proportional to 2B\sqrt{2B}
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College Physics Quiz

College Physics Quiz: Magnetism And Moving Charges

Practice Magnetism And Moving Charges in College Physics with focused quiz questions that help you check what you know, review explanations, and build confidence with test-style prompts.

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This quiz focuses on Magnetism And Moving Charges, giving you a quick way to practice the rules, question types, and explanations that matter most for College Physics.

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Question 1

An electron moves in a circular path of radius 2.02.0 cm in a uniform magnetic field. If the magnetic field strength is doubled while keeping the electron's speed constant, what happens to the radius of the circular path?

  1. The radius becomes 1.01.0 cm because rr is inversely proportional to BB (correct answer)
  2. The radius becomes 4.04.0 cm because rr is proportional to B2B^2
  3. The radius remains 2.02.0 cm because speed is unchanged
  4. The radius becomes 1.41.4 cm because rr is proportional to B\sqrt{B}
  5. The radius becomes 2.82.8 cm because rr is proportional to 2B\sqrt{2B}
Explanation: When a charged particle moves in a magnetic field, it experiences a magnetic force that acts as the centripetal force, causing circular motion. The key relationship here comes from setting the magnetic force equal to the centripetal force. The magnetic force on a moving charged particle is FB=qvBF_B = qvB, where qq is the charge, vv is the speed, and BB is the magnetic field strength. For circular motion, this equals the centripetal force: Fc=mv2rF_c = \frac{mv^2}{r}, where mm is the mass and rr is the radius. Setting these equal: qvB=mv2rqvB = \frac{mv^2}{r} Solving for radius: r=mvqBr = \frac{mv}{qB} This equation shows that radius is inversely proportional to magnetic field strength. When BB doubles while speed remains constant, the radius becomes half its original value: rnew=2.0 cm2=1.0 cmr_{new} = \frac{2.0 \text{ cm}}{2} = 1.0 \text{ cm}. Answer A correctly identifies this inverse relationship. Answer B incorrectly suggests rB2r \propto B^2, which would make the radius increase dramatically with field strength. Answer C falls into the trap of thinking unchanged speed means unchanged radius, ignoring the magnetic field's role entirely. Answer D incorrectly proposes rBr \propto \sqrt{B}, which has no basis in the physics. Study tip: Always derive the radius formula r=mvqBr = \frac{mv}{qB} from first principles by equating magnetic and centripetal forces. This approach prevents memorization errors and clearly shows the inverse relationship between radius and magnetic field strength.

Question 2

A rectangular current loop with dimensions 0.200.20 m × 0.300.30 m carries a current of 2.52.5 A. The loop is placed in a uniform magnetic field of 0.400.40 T. What is the maximum possible magnetic torque on the loop?

  1. 0.0600.060 N⋅m when the loop's area vector is parallel to the field
  2. 0.0600.060 N⋅m when the loop's area vector is perpendicular to the field (correct answer)
  3. 0.1200.120 N⋅m when the loop's area vector is parallel to the field
  4. 0.0300.030 N⋅m when the loop's area vector is perpendicular to the field
  5. 0.2000.200 N⋅m when the loop's area vector makes a 45° angle with the field
Explanation: When you encounter a current loop in a magnetic field, you're dealing with magnetic torque, which depends on how the loop's orientation relates to the field direction. The key insight is understanding when torque is maximized versus minimized. The magnetic torque on a current loop is given by τ=μBsinθ\tau = \mu B \sin\theta, where μ\mu is the magnetic dipole moment, BB is the magnetic field strength, and θ\theta is the angle between the loop's area vector (perpendicular to the loop's plane) and the magnetic field. The magnetic dipole moment equals IAIA, where II is current and AA is area. First, calculate the magnetic dipole moment: μ=IA=(2.5 A)(0.20 m×0.30 m)=2.5×0.06=0.15 A⋅m2\mu = IA = (2.5\text{ A})(0.20\text{ m} \times 0.30\text{ m}) = 2.5 \times 0.06 = 0.15\text{ A⋅m}^2 Maximum torque occurs when sinθ=1\sin\theta = 1, which happens when θ=90°\theta = 90° (the area vector is perpendicular to the field): τmax=(0.15)(0.40)(1)=0.060 N⋅m\tau_{max} = (0.15)(0.40)(1) = 0.060\text{ N⋅m} Answer A gives the right magnitude but incorrectly states this occurs when the area vector is parallel to the field. When parallel, θ=0°\theta = 0° and sinθ=0\sin\theta = 0, producing zero torque. Answer C uses the wrong area calculation (likely 0.20+0.30=0.500.20 + 0.30 = 0.50 instead of 0.20×0.30=0.060.20 \times 0.30 = 0.06). Answer D has the wrong magnitude and wrong orientation condition. Answer B correctly identifies both the magnitude (0.060 N⋅m) and the condition for maximum torque (area vector perpendicular to field). Remember: maximum magnetic torque occurs when the loop's area vector is perpendicular to the magnetic field, while zero torque occurs when they're parallel.

Question 3

A conducting rod of length 0.500.50 m moves with velocity v=8.0\vec{v} = 8.0 m/s i^\hat{i} through a uniform magnetic field B=0.25\vec{B} = 0.25 T k^\hat{k}. What is the motional EMF induced across the rod?

  1. E=1.0\mathcal{E} = 1.0 V with the rod's left end at higher potential than the right end (correct answer)
  2. E=1.0\mathcal{E} = 1.0 V with the rod's right end at higher potential than the left end
  3. E=2.0\mathcal{E} = 2.0 V with potential difference depending on the rod's orientation
  4. E=0.5\mathcal{E} = 0.5 V with uniform potential distribution along the rod's length
  5. E=4.0\mathcal{E} = 4.0 V with the direction determined by Lenz's law
Explanation: When you see a conducting rod moving through a magnetic field, you're dealing with motional EMF - the voltage induced when a conductor cuts through magnetic field lines. The key is using the right-hand rule to determine both magnitude and polarity. The magnitude of motional EMF is given by E=BvL\mathcal{E} = BvL when the velocity is perpendicular to the magnetic field. Here, v=8.0 m/s i^\vec{v} = 8.0 \text{ m/s } \hat{i} (positive x-direction) and B=0.25 T k^\vec{B} = 0.25 \text{ T } \hat{k} (positive z-direction) are indeed perpendicular. So: E=(0.25 T)(8.0 m/s)(0.50 m)=1.0 V\mathcal{E} = (0.25 \text{ T})(8.0 \text{ m/s})(0.50 \text{ m}) = 1.0 \text{ V} To find polarity, use the right-hand rule for v×B\vec{v} \times \vec{B}. Point your fingers in the direction of velocity (+x+x), curl them toward the magnetic field direction (+z+z), and your thumb points in the direction of the magnetic force on positive charges. This gives v×B\vec{v} \times \vec{B} in the y-y direction, meaning positive charges accumulate at the left end, making it higher potential. Choice B gets the magnitude right but reverses the polarity - this happens if you incorrectly apply the right-hand rule or confuse the direction of charge separation. Choice C suggests the wrong magnitude and implies orientation matters beyond the velocity-field relationship, which isn't true for perpendicular motion. Choice D has the wrong magnitude (half the correct value) and incorrectly suggests uniform potential distribution, when charge separation creates the EMF. Remember: motional EMF problems always require both magnitude calculation (BvLBvL for perpendicular motion) and polarity determination using v×B\vec{v} \times \vec{B}.

Question 4

In a cyclotron, deuterons (charge +e+e, mass 3.34×10273.34 \times 10^{-27} kg) are accelerated in a magnetic field of 1.51.5 T. What is the cyclotron frequency for these particles?

  1. f=1.15×107f = 1.15 \times 10^7 Hz, independent of the deuteron's speed (correct answer)
  2. f=2.30×107f = 2.30 \times 10^7 Hz, proportional to the magnetic field strength
  3. f=7.67×106f = 7.67 \times 10^6 Hz, inversely proportional to the particle mass
  4. f=5.75×106f = 5.75 \times 10^6 Hz, dependent on the radius of the circular orbit
  5. f=3.45×107f = 3.45 \times 10^7 Hz, increasing with particle kinetic energy
Explanation: When you encounter cyclotron problems, focus on the fundamental relationship between charged particles moving in magnetic fields. A cyclotron uses a uniform magnetic field to bend charged particles into circular paths, and the key insight is that the frequency of this circular motion depends only on the particle's charge-to-mass ratio and the magnetic field strength. The cyclotron frequency is given by f=qB2πmf = \frac{qB}{2\pi m}, where qq is the charge, BB is the magnetic field, and mm is the mass. For deuterons: f=(1.6×1019)(1.5)2π(3.34×1027)=1.15×107f = \frac{(1.6 \times 10^{-19})(1.5)}{2\pi(3.34 \times 10^{-27})} = 1.15 \times 10^7 Hz. Crucially, notice that velocity doesn't appear in this formula—the frequency is independent of the particle's speed. Choice A is correct because it gives the right numerical value and correctly identifies that frequency is independent of speed. This speed-independence is what makes cyclotrons work: particles stay synchronized with the alternating electric field regardless of how fast they're moving. Choice B has the wrong numerical value—it's exactly double the correct answer, suggesting an error like forgetting the 2π2\pi factor. While it correctly notes the proportional relationship to magnetic field, the calculation is wrong. Choice C gives an incorrect value and incorrectly describes the mass relationship as "inversely proportional" when the full relationship is more complex (involves the charge-to-mass ratio). Choice D provides a wrong value and incorrectly suggests frequency depends on orbital radius, when actually both frequency and radius are consequences of the same underlying physics. Remember: cyclotron frequency depends only on qq, BB, and mm—never on speed or radius.

Question 5

A charged particle moving in crossed electric and magnetic fields follows a cycloid path. If E=2000\vec{E} = 2000 V/m j^\hat{j} and B=0.10\vec{B} = 0.10 T k^\hat{k}, what is the drift velocity of the guiding center?

  1. vd=2.0×104\vec{v}_d = 2.0 \times 10^4 m/s i^\hat{i} independent of particle charge and mass (correct answer)
  2. vd=2.0×104\vec{v}_d = 2.0 \times 10^4 m/s j^\hat{j} in the direction of the electric field
  3. vd=200\vec{v}_d = 200 m/s i^\hat{i} proportional to the particle's charge-to-mass ratio
  4. vd=2.0×103\vec{v}_d = 2.0 \times 10^3 m/s k^\hat{k} parallel to the magnetic field direction
  5. vd=1.0×104\vec{v}_d = 1.0 \times 10^4 m/s i^\hat{i} for particles with specific kinetic energy
Explanation: When you encounter crossed electric and magnetic fields, you're dealing with the E×B drift phenomenon. This occurs when a charged particle experiences both electric and magnetic forces simultaneously, causing it to drift perpendicular to both field directions. The drift velocity formula is vd=E×BB2\vec{v}_d = \frac{\vec{E} \times \vec{B}}{B^2}. Notice this depends only on the field magnitudes and directions, not on the particle's charge or mass. Let's calculate: vd=(2000j^)×(0.10k^)(0.10)2=200(j^×k^)0.01=200i^0.01=2.0×104 m/s i^\vec{v}_d = \frac{(2000 \hat{j}) \times (0.10 \hat{k})}{(0.10)^2} = \frac{200(\hat{j} \times \hat{k})}{0.01} = \frac{200\hat{i}}{0.01} = 2.0 \times 10^4 \text{ m/s } \hat{i} Using the right-hand rule: j^×k^=i^\hat{j} \times \hat{k} = \hat{i}, so the drift is in the i^\hat{i} direction. A is correct: the magnitude and direction match our calculation, and it correctly states the drift is independent of particle properties. B incorrectly suggests drift occurs in the electric field direction (j^\hat{j}). The drift is always perpendicular to both fields. C has the wrong magnitude (off by a factor of 100) and incorrectly claims the drift depends on charge-to-mass ratio. While individual particle motion does depend on q/m, the guiding center drift does not. D suggests drift parallel to the magnetic field, which is impossible since the cross product E×B\vec{E} \times \vec{B} is perpendicular to both fields. Study tip: Remember that E×B drift is universal—all charged particles drift at the same velocity regardless of their charge or mass, and always perpendicular to both fields.

Question 6

Two ions with the same charge +e+e but different masses (m1=20m_1 = 20 u and m2=22m_2 = 22 u, where u =1.66×1027= 1.66 \times 10^{-27} kg) are accelerated through the same potential difference and then enter a uniform magnetic field. What is the ratio of their circular path radii r1/r2r_1/r_2?

  1. r1/r2=0.91r_1/r_2 = 0.91 because lighter ions have smaller radii at the same energy
  2. r1/r2=0.95r_1/r_2 = 0.95 reflecting the square root of the mass ratio (correct answer)
  3. r1/r2=1.10r_1/r_2 = 1.10 because radius is proportional to mass for equal charges
  4. r1/r2=1.05r_1/r_2 = 1.05 accounting for the velocity difference after acceleration
  5. r1/r2=1.00r_1/r_2 = 1.00 because both ions have the same charge and energy
Explanation: When charged particles are accelerated through a potential difference and then enter a magnetic field, you need to connect two key physics principles: energy conservation during acceleration and circular motion in magnetic fields. First, when both ions accelerate through the same potential difference VV, they gain equal kinetic energy: qV=12mv2qV = \frac{1}{2}mv^2. Since both have charge +e+e, their velocities after acceleration are v=2eVmv = \sqrt{\frac{2eV}{m}}. The lighter ion (m1m_1) will have a higher velocity than the heavier ion (m2m_2). In the magnetic field, the radius of circular motion is given by r=mveBr = \frac{mv}{eB}. Substituting the velocity expression: r=m2eVmeB=2meVeBr = \frac{m\sqrt{\frac{2eV}{m}}}{eB} = \frac{\sqrt{2meV}}{eB}. This shows that radius is proportional to m\sqrt{m} when charge and energy are constant. Therefore: r1r2=m1m2=2022=0.909=0.95\frac{r_1}{r_2} = \sqrt{\frac{m_1}{m_2}} = \sqrt{\frac{20}{22}} = \sqrt{0.909} = 0.95 Choice B is correct because it properly reflects this square root relationship between mass and radius. Choice A gives approximately the right numerical value but incorrectly states that lighter ions have smaller radii "at the same energy" - while true numerically, the reasoning misses the square root dependence. Choice C incorrectly suggests direct proportionality to mass. Choice D's value is wrong and the reasoning about "velocity difference" doesn't lead to the correct mathematical relationship. Remember: for equal charges and equal accelerating potentials, radius ratios in magnetic fields always follow the square root of mass ratios.

Question 7

A solenoid with n=2000n = 2000 turns/meter carries a current I=3.0I = 3.0 A. A proton moves parallel to the solenoid axis with speed v=5.0×105v = 5.0 \times 10^5 m/s inside the solenoid. What is the magnetic force on the proton?

  1. F=0F = 0 N because v\vec{v} is parallel to B\vec{B} inside the solenoid (correct answer)
  2. F=4.8×1016F = 4.8 \times 10^{-16} N perpendicular to both velocity and field
  3. F=9.6×1016F = 9.6 \times 10^{-16} N directed radially outward from the solenoid axis
  4. F=2.4×1016F = 2.4 \times 10^{-16} N directed along the solenoid axis opposing motion
  5. F=1.2×1015F = 1.2 \times 10^{-15} N with direction determined by the current direction
Explanation: When you encounter magnetic force problems, immediately think about the Lorentz force equation: F=q(v×B)\vec{F} = q(\vec{v} \times \vec{B}). The key insight is that the cross product means force only exists when velocity and magnetic field are not parallel. Inside a solenoid, the magnetic field lines run parallel to the axis, creating a uniform field along the solenoid's length. Since the proton moves parallel to this same axis, its velocity vector v\vec{v} is parallel to the magnetic field vector B\vec{B}. When two vectors are parallel, their cross product equals zero, making F=q(v×B)=0\vec{F} = q(\vec{v} \times \vec{B}) = 0. Answer A correctly identifies this: the force is zero because velocity and field are parallel. Answer B incorrectly assumes the vectors are perpendicular and attempts a calculation using F=qvBF = qvB, but this only applies when vB\vec{v} \perp \vec{B}. Answer C makes the same perpendicular assumption as B but suggests a radially outward force, which would require the velocity to be perpendicular to the field. Answer D incorrectly suggests a force opposing motion along the axis. This misconception might arise from confusing magnetic force with other resistive forces, but magnetic forces are always perpendicular to velocity (when they exist at all). Study tip: Remember that magnetic force depends entirely on the angle between v\vec{v} and B\vec{B}. When parallel (0°) or antiparallel (180°), sinθ=0\sin \theta = 0 and force vanishes. Maximum force occurs at 90°.

Question 8

A mass spectrometer uses crossed electric and magnetic fields as a velocity selector. If E=5.0×104\vec{E} = 5.0 \times 10^4 V/m j^\hat{j} and B=0.25\vec{B} = 0.25 T k^\hat{k}, what velocity must a positively charged particle have to travel undeflected through the selector?

  1. v=2.0×105\vec{v} = 2.0 \times 10^5 m/s i^\hat{i} regardless of the particle's charge (correct answer)
  2. v=1.25×106\vec{v} = 1.25 \times 10^6 m/s i^\hat{i} for particles with charge +e+e
  3. v=2.0×105\vec{v} = 2.0 \times 10^5 m/s k^\hat{k} regardless of the particle's mass
  4. v=2.0×105\vec{v} = 2.0 \times 10^5 m/s i^-\hat{i} for negatively charged particles
  5. v=5.0×104\vec{v} = 5.0 \times 10^4 m/s i^\hat{i} regardless of field strength
Explanation: When you encounter a velocity selector problem, you're dealing with the principle that charged particles travel undeflected when electric and magnetic forces balance perfectly. This happens when qE+qv×B=0q\vec{E} + q\vec{v} \times \vec{B} = 0, which simplifies to E=v×B\vec{E} = -\vec{v} \times \vec{B}. To find the required velocity, you need to determine what v\vec{v} satisfies this condition. Given E=5.0×104j^\vec{E} = 5.0 \times 10^4 \hat{j} V/m and B=0.25k^\vec{B} = 0.25 \hat{k} T, let's test v=vi^\vec{v} = v\hat{i}. Using the cross product: v×B=vi^×0.25k^=0.25vj^\vec{v} \times \vec{B} = v\hat{i} \times 0.25\hat{k} = -0.25v\hat{j}. For balance: 5.0×104j^=(0.25vj^)=0.25vj^5.0 \times 10^4\hat{j} = -(-0.25v\hat{j}) = 0.25v\hat{j}. Solving: v=5.0×1040.25=2.0×105v = \frac{5.0 \times 10^4}{0.25} = 2.0 \times 10^5 m/s. Notice that charge qq cancels out completely, making this velocity universal for any charged particle. Choice A is correct because it gives the right magnitude, direction, and correctly states the charge independence. Choice B has the wrong magnitude (off by a factor of about 6) and incorrectly suggests charge dependence. Choice C has the wrong direction—velocity in the k^\hat{k} direction wouldn't create the needed force balance. Choice D gives the wrong direction (i^-\hat{i} instead of +i^+\hat{i}) and incorrectly focuses on negative charges when the velocity requirement is universal. Remember: In velocity selectors, the required velocity depends only on the field strengths (v=E/Bv = E/B), never on the particle's charge or mass—these quantities cancel out in the force balance equation.

Question 9

Two parallel wires carry currents I1=5.0I_1 = 5.0 A and I2=3.0I_2 = 3.0 A in opposite directions. The wires are separated by a distance of 0.100.10 m. What is the magnitude of the magnetic force per unit length on wire 2 due to wire 1?

  1. 3.0×1053.0 \times 10^{-5} N/m, and the force is repulsive between the wires (correct answer)
  2. 1.5×1051.5 \times 10^{-5} N/m, and the force is attractive between the wires
  3. 3.0×1053.0 \times 10^{-5} N/m, and the force is attractive between the wires
  4. 6.0×1056.0 \times 10^{-5} N/m, and the force is repulsive between the wires
  5. 1.0×1041.0 \times 10^{-4} N/m, and the force is repulsive between the wires
Explanation: When you encounter problems about magnetic forces between current-carrying wires, you need to apply two key concepts: the magnetic field created by a current-carrying wire, and the force experienced by a current in a magnetic field. First, calculate the magnetic field created by wire 1 at the location of wire 2. The magnetic field around a long straight wire is B=μ0I2πrB = \frac{\mu_0 I}{2\pi r}, where μ0=4π×107\mu_0 = 4\pi \times 10^{-7} T·m/A. So B1=(4π×107)(5.0)2π(0.10)=1.0×105B_1 = \frac{(4\pi \times 10^{-7})(5.0)}{2\pi(0.10)} = 1.0 \times 10^{-5} T. Next, find the force per unit length on wire 2 using F/L=I2B1=(3.0)(1.0×105)=3.0×105F/L = I_2 B_1 = (3.0)(1.0 \times 10^{-5}) = 3.0 \times 10^{-5} N/m. To determine the direction, remember that parallel currents in the same direction attract, while currents in opposite directions repel. Since the currents flow in opposite directions, the force is repulsive. Answer A is correct with the right magnitude and direction. Answer B has the wrong magnitude (half the correct value) – this might result from incorrectly using the average current instead of the proper formula. Answer C has the correct magnitude but wrong direction, confusing the rule about parallel vs. antiparallel currents. Answer D has twice the correct magnitude, possibly from incorrectly doubling the force or using I1+I2I_1 + I_2 instead of just I2I_2. Remember: opposite currents repel, same-direction currents attract. Always calculate the field from one wire first, then find the force on the other wire in that field.

Question 10

A magnetic dipole with magnetic moment μ=2.5×103\vec{\mu} = 2.5 \times 10^{-3} A⋅m² k^\hat{k} is placed in a uniform magnetic field B=0.20\vec{B} = 0.20 T i^\hat{i}. What is the potential energy of this configuration?

  1. U=5.0×104U = -5.0 \times 10^{-4} J because the dipole opposes the field direction
  2. U=0U = 0 J because the dipole and field are perpendicular to each other (correct answer)
  3. U=+5.0×104U = +5.0 \times 10^{-4} J because the dipole is misaligned with the field
  4. U=1.0×103U = -1.0 \times 10^{-3} J accounting for the full magnetic moment magnitude
  5. U=+2.5×104U = +2.5 \times 10^{-4} J with energy stored in the magnetic field configuration
Explanation: When you encounter magnetic dipole problems, focus on the fundamental relationship between magnetic moment and field. The potential energy of a magnetic dipole in a magnetic field is given by U=μBU = -\vec{\mu} \cdot \vec{B}, where the dot product determines both magnitude and sign. Let's calculate this step by step. You have μ=2.5×103k^\vec{\mu} = 2.5 \times 10^{-3} \hat{k} A⋅m² and B=0.20i^\vec{B} = 0.20 \hat{i} T. The dot product μB=(2.5×103k^)(0.20i^)\vec{\mu} \cdot \vec{B} = (2.5 \times 10^{-3} \hat{k}) \cdot (0.20 \hat{i}). Since k^\hat{k} and i^\hat{i} are perpendicular unit vectors, k^i^=0\hat{k} \cdot \hat{i} = 0. Therefore, U=μB=0U = -\vec{\mu} \cdot \vec{B} = 0 J. Answer B is correct. Choice A incorrectly assumes the dipole opposes the field, which would only be true if they were anti-parallel (giving negative potential energy). Choice C suggests the dipole is "misaligned" with positive energy, but this would require the dipole to be anti-parallel to the field. Choice D appears to use an incorrect formula or calculation, possibly treating the vectors as if they were parallel. Remember that potential energy depends on the angle between vectors: minimum (most negative) when parallel, maximum (most positive) when anti-parallel, and zero when perpendicular. Always use the dot product formula U=μBU = -\vec{\mu} \cdot \vec{B} rather than just multiplying magnitudes—the vector relationship is crucial for determining both the magnitude and sign of the potential energy.

Question 11

A charged particle undergoes cyclotron motion in a magnetic field. If the magnetic field strength is increased by a factor of 3 while the particle's kinetic energy is doubled, what happens to the radius of the cyclotron orbit?

  1. The radius decreases by a factor of 3/22.13/\sqrt{2} \approx 2.1 due to both field and energy changes (correct answer)
  2. The radius increases by a factor of 2/30.47\sqrt{2}/3 \approx 0.47 accounting for higher energy
  3. The radius decreases by a factor of 324.23\sqrt{2} \approx 4.2 from the combined effects
  4. The radius remains unchanged because energy and field changes cancel
  5. The radius decreases by a factor of 66 due to independent field and energy contributions
Explanation: When you encounter cyclotron motion problems, focus on the fundamental relationship between magnetic force and centripetal force. A charged particle moving perpendicular to a magnetic field follows a circular path where the magnetic force qvBqvB provides the centripetal force mv2r\frac{mv^2}{r}. Setting these equal gives us qvB=mv2rqvB = \frac{mv^2}{r}, which simplifies to r=mvqBr = \frac{mv}{qB}. This shows that radius depends on momentum (mvmv) and is inversely proportional to magnetic field strength (BB). To find how radius changes, you need to determine how velocity changes when kinetic energy doubles. Since KE=12mv2KE = \frac{1}{2}mv^2, doubling kinetic energy means vnew=2voriginalv_{new} = \sqrt{2} \cdot v_{original}. Therefore, the new radius becomes rnew=m2vq3B=23mvqB=23roriginalr_{new} = \frac{m \cdot \sqrt{2}v}{q \cdot 3B} = \frac{\sqrt{2}}{3} \cdot \frac{mv}{qB} = \frac{\sqrt{2}}{3} \cdot r_{original}. The radius decreases by a factor of 322.1\frac{3}{\sqrt{2}} \approx 2.1, making choice A correct. Choice B incorrectly states the radius increases and gives the reciprocal of the correct factor. Choice C multiplies the factors instead of dividing, yielding 323\sqrt{2} rather than 32\frac{3}{\sqrt{2}}. Choice D wrongly assumes the effects cancel—they don't because one factor affects the numerator (velocity) while the other affects the denominator (magnetic field). Study tip: Always write out the cyclotron radius formula r=mvqBr = \frac{mv}{qB} and systematically analyze how each variable changes. Remember that kinetic energy changes affect velocity by a square root factor.

Question 12

Two identical charged particles are simultaneously released from rest at the same point in a uniform magnetic field B=0.30\vec{B} = 0.30 T. One particle has charge +q+q and the other has charge q-q. After t=1.0×106t = 1.0 \times 10^{-6} s, what is the relationship between their positions?

  1. They are at the same location having followed identical paths
  2. They are at different locations, separated by a distance proportional to t2t^2
  3. They remain at the original release point indefinitely (correct answer)
  4. They move in opposite directions along straight lines through the release point
Explanation: This is a subtle question about the magnetic force law. The magnetic force on a moving charge is F=qv×B\vec{F} = q\vec{v} \times \vec{B}. Since both particles are released from rest, their initial velocity v=0\vec{v} = 0. With zero velocity, the magnetic force is zero regardless of the charge sign or magnitude. Newton's first law states that objects at rest remain at rest unless acted upon by a net force. Since there is no magnetic force on stationary charges, both particles remain at the release point indefinitely. This demonstrates that magnetic fields can only influence moving charges, not stationary ones.

Question 13

A solenoid with 10001000 turns per meter carries a current of 2.02.0 A. A proton enters the solenoid parallel to its axis with speed v=5.0×106v = 5.0 \times 10^6 m/s. What is the proton's trajectory inside the solenoid?

  1. Parabolic path curving toward the solenoid wall
  2. Circular path perpendicular to the axis with radius 0.0520.052 m
  3. Helical path with decreasing radius due to field gradients
  4. Straight line parallel to the axis at constant speed (correct answer)
Explanation: When you encounter problems involving charged particles moving through magnetic fields, the key is understanding how the magnetic force depends on both the particle's velocity and the magnetic field direction. Inside a solenoid, the magnetic field lines run parallel to the axis. The magnetic force on a charged particle is given by F=qv×B\vec{F} = q\vec{v} \times \vec{B}, where the cross product means the force is perpendicular to both velocity and magnetic field. Since the proton enters parallel to the axis (same direction as the field), the angle between v\vec{v} and B\vec{B} is zero. The cross product of parallel vectors equals zero, so there's no magnetic force acting on the proton. With no force, the proton continues in a straight line at constant speed according to Newton's first law. Choice A suggests a parabolic path, which would require a constant force perpendicular to the initial velocity—but we've established there's no force here. Choice B describes circular motion, which occurs when a charged particle enters a magnetic field perpendicular to the field lines, not parallel to them. The radius calculation would be relevant for perpendicular entry, but that's not our scenario. Choice C mentions helical motion, which happens when a particle has both parallel and perpendicular velocity components relative to the field—again, not applicable since our proton enters purely parallel to the axis. Remember: magnetic force only acts when there's a velocity component perpendicular to the magnetic field. Parallel motion through uniform magnetic fields produces no force and no deflection.

Question 14

An electron enters a region with crossed electric and magnetic fields. The electric field E=2000\vec{E} = 2000 N/C points in the +y+y direction, and the magnetic field B=0.40\vec{B} = 0.40 T points in the +z+z direction. If the electron travels in a straight line without deflection, what must be its velocity?

  1. 5.0×1035.0 \times 10^3 m/s in the +x+x direction (correct answer)
  2. 5.0×1035.0 \times 10^3 m/s in the x-x direction
  3. 8.0×1028.0 \times 10^2 m/s in the +x+x direction
  4. 8.0×1028.0 \times 10^2 m/s in the x-x direction
Explanation: For straight-line motion in crossed fields, the electric and magnetic forces must balance: FE+FB=0\vec{F}_E + \vec{F}_B = 0, so qE+qv×B=0q\vec{E} + q\vec{v} \times \vec{B} = 0. The electric force on the electron is FE=(e)(+y)=eE\vec{F}_E = (-e)(+y) = -e\vec{E} in the y-y direction. For balance, the magnetic force must be +eE+e\vec{E} in the +y+y direction. Using FB=(e)v×B\vec{F}_B = (-e)\vec{v} \times \vec{B}, if v\vec{v} is in the +x+x direction, then v×B=(+x)×(+z)=y\vec{v} \times \vec{B} = (+x) \times (+z) = -y, so FB=(e)(y)=+ey\vec{F}_B = (-e)(-y) = +ey. Setting magnitudes equal: eE=evBeE = evB, so v=EB=20000.40=5.0×103v = \frac{E}{B} = \frac{2000}{0.40} = 5.0 \times 10^3 m/s.

Question 15

A charged particle moves in a circular path in a uniform magnetic field. If the magnetic field strength is doubled while the particle's kinetic energy remains constant, how does the radius of the circular path change?

  1. The radius increases by a factor of 22
  2. The radius decreases by a factor of 22 (correct answer)
  3. The radius increases by a factor of 2\sqrt{2}
  4. The radius decreases by a factor of 2\sqrt{2}
Explanation: For a charged particle in a magnetic field, the radius is given by r=mvqB=2mKqBr = \frac{mv}{qB} = \frac{\sqrt{2mK}}{qB}, where KK is the kinetic energy. Since K=12mv2K = \frac{1}{2}mv^2, we have v=2Kmv = \sqrt{\frac{2K}{m}}. If the kinetic energy KK remains constant and BB is doubled, then rnew=2mKq(2B)=122mKqB=rold2r_{new} = \frac{\sqrt{2mK}}{q(2B)} = \frac{1}{2} \cdot \frac{\sqrt{2mK}}{qB} = \frac{r_{old}}{2}. Therefore, the radius decreases by a factor of 2.

Question 16

A proton moving at 4.0×1064.0 \times 10^6 m/s enters a uniform magnetic field of 0.250.25 T at an angle of 30°30° to the field lines. What is the pitch (distance traveled parallel to the field in one complete revolution) of the resulting helical path?

  1. 0.520.52 m (correct answer)
  2. 0.300.30 m
  3. 0.420.42 m
  4. 0.600.60 m
Explanation: The velocity has components parallel and perpendicular to B\vec{B}: v=vcos(30°)=(4.0×106)(32)=3.46×106v_{\parallel} = v\cos(30°) = (4.0 \times 10^6)(\frac{\sqrt{3}}{2}) = 3.46 \times 10^6 m/s and v=vsin(30°)=(4.0×106)(0.5)=2.0×106v_{\perp} = v\sin(30°) = (4.0 \times 10^6)(0.5) = 2.0 \times 10^6 m/s. The period of circular motion is T=2πmqB=2π(1.67×1027)(1.6×1019)(0.25)=2.61×107T = \frac{2\pi m}{qB} = \frac{2\pi(1.67 \times 10^{-27})}{(1.6 \times 10^{-19})(0.25)} = 2.61 \times 10^{-7} s. The pitch is p=vT=(3.46×106)(2.61×107)=0.90p = v_{\parallel}T = (3.46 \times 10^6)(2.61 \times 10^{-7}) = 0.90 m. This doesn't match any option, let me recalculate more carefully. Actually, T=2πmqB=2π(1.67×1027)(1.6×1019)(0.25)=1.5×107T = \frac{2\pi m}{qB} = \frac{2\pi(1.67 \times 10^{-27})}{(1.6 \times 10^{-19})(0.25)} = 1.5 \times 10^{-7} s, so p=(3.46×106)(1.5×107)=0.52p = (3.46 \times 10^6)(1.5 \times 10^{-7}) = 0.52 m.