9702/43

Physics 9702/43May/June 2016

Cambridge A-Level · A Level Structured Questions · worked solutions for every part, with the mark scheme

13
questions
100
marks
120
minutes

Topics Magnetic Fields · Quantum Physics · Gravitational Fields · Ideal Gases · Oscillations · Medical Physics · +6 more

Q1Gravitational FieldsFree sample
(a)

By reference to the definition of gravitational potential, explain why gravitational potential is a negative quantity.

2M
DifficultyMedium-Easy
Worked solution

Answer

Gravitational potential at a point is the work done per unit mass by an external agent in bringing a test mass from infinity to the point (taking ϕ=0\phi = 0 at infinity).

Because the gravitational force is attractive, the field does positive work on the mass as it moves from infinity to the point, so the external work done per unit mass is negative. Hence ϕ\phi is negative.

Final answer

Gravitational potential is negative because, taking (\phi=0) at infinity, the attractive gravitational field does positive work bringing a mass in from infinity, so the external work done per unit mass is negative.

Detailed explanation

Background Concept

Gravitational potential ϕ\phi at a point is defined as the work done per unit mass by an external agent in bringing a small test mass from infinity to that point, with no change in kinetic energy.

Mathematically,

ϕ=Wextm\phi = \frac{W_{\text{ext}}}{m}

A standard reference choice is ϕ=0\phi = 0 at r=r = \infty. Gravitational potential energy is then

U=mϕ.U = m\phi.

Understanding the Question

You are asked to explain (not calculate) why ϕ\phi comes out negative when we use the usual definition and reference point at infinity.

So you must connect:

  • the attractive nature of gravity,
  • the sign of work done by the field / external agent,
  • the fact that ϕ()=0\phi(\infty)=0 is the chosen zero.

Approach

Start from the definition ϕ=Wext/m\phi = W_{\text{ext}}/m for a move from infinity to a point. Decide whether the external agent must do positive or negative work in this move.

Step-by-Step Reasoning

  1. A gravitational field attracts a mass toward the star/planet. That means the gravitational force is directed inward.
  2. Consider a test mass moving from infinity toward the mass creating the field. Its displacement is also inward.
  3. Since force and displacement are in the same direction, the gravitational field does positive work on the mass.
  4. If we bring the mass in slowly so that its kinetic energy does not increase, an external agent must remove energy (do negative work) to prevent the mass from speeding up.
  5. Therefore WextW_{\text{ext}} for moving from infinity to the point is negative, so ϕ=Wext/m\phi = W_{\text{ext}}/m is negative.
  6. With ϕ()=0\phi(\infty)=0, any point in an attractive gravitational field has ϕ<0\phi<0.

Key Takeaways

  • ϕ\phi is defined via work done per unit mass from infinity.
  • Gravity is attractive, so the field does positive work bringing masses in.
  • With ϕ()=0\phi(\infty)=0, this makes ϕ\phi negative everywhere finite.

Common Mistakes

  • Saying “potential is negative because gravity is attractive” without linking to the work-done definition.
  • Mixing up work done by the field (positive inward) with work done by the external agent (negative if speed is kept constant).
  • Forgetting that the negativity depends on choosing ϕ=0\phi=0 at infinity.

Things to Be Careful About

  • The sign depends on the reference: Cambridge assumes ϕ()=0\phi(\infty)=0.
  • Make clear it is work done per unit mass by an external agent (or equivalently the negative of work done by the field) that sets the sign.
Techniques used
use the definition of gravitational potential as work done per unit massapply the reference condition that potential is zero at infinityreason about the sign of work done against a gravitational field
(b)

Two stars A and B have their surfaces separated by a distance of 1.4×1012 m1.4 \times 10^{12}\ \text{m}, as illustrated in Fig. 1.1.

Point P lies on the line joining the centres of the two stars. The distance xx of point P from the surface of star A may be varied.

The variation with distance xx of the gravitational potential ϕ\phi at point P is shown in Fig. 1.2.

A rock of mass 180 kg180\ \text{kg} moves along the line joining the centres of the two stars, from star A towards star B.

(i)

Use data from Fig. 1.2 to calculate the change in kinetic energy of the rock when it moves from the point where x=0.1×1012 mx = 0.1 \times 10^{12}\ \text{m} to the point where x=1.2×1012 mx = 1.2 \times 10^{12}\ \text{m}.
State whether this change is an increase or a decrease.

change = ______ J\text{J}

3M
DifficultyMedium-Easy
Worked solution

Working

From Fig. 1.2:

ϕ1=10×108 J kg1(x=0.1×1012 m)\phi_1 = -10 \times 10^8\ \text{J kg}^{-1}\quad (x = 0.1 \times 10^{12}\ \text{m}) ϕ2=14×108 J kg1(x=1.2×1012 m)\phi_2 = -14 \times 10^8\ \text{J kg}^{-1}\quad (x = 1.2 \times 10^{12}\ \text{m}) Δϕ=ϕ2ϕ1=(14(10))×108=4.0×108 J kg1\Delta \phi = \phi_2 - \phi_1 = (-14 - (-10))\times 10^8 = -4.0\times 10^8\ \text{J kg}^{-1} ΔU=mΔϕ=180(4.0×108)=7.2×1010 J\Delta U = m\Delta \phi = 180(-4.0\times 10^8) = -7.2\times 10^{10}\ \text{J} ΔK=ΔU=+7.2×1010 J\Delta K = -\Delta U = +7.2\times 10^{10}\ \text{J}

Answer

Change in kinetic energy =7.2×1010 J= 7.2\times 10^{10}\ \text{J} (increase).

Final answer

7.2 × 10^10 J, increase

Detailed explanation

Background Concept

Gravitational potential ϕ\phi is potential energy per unit mass:

ϕ=Um\phi = \frac{U}{m}

So a change in potential corresponds to a change in gravitational potential energy:

ΔU=mΔϕ.\Delta U = m\Delta \phi.

If only gravitational forces do work (no engines, no friction), mechanical energy is conserved:

ΔK+ΔU=0ΔK=ΔU.\Delta K + \Delta U = 0 \quad \Rightarrow \quad \Delta K = -\Delta U.

Understanding the Question

A 180 kg180\ \text{kg} rock moves from x=0.1×1012 mx=0.1\times 10^{12}\ \text{m} to x=1.2×1012 mx=1.2\times 10^{12}\ \text{m}. The graph gives ϕ\phi at those points (in units of 108 J kg110^8\ \text{J kg}^{-1}). You must find how much the rock’s kinetic energy changes and state whether it increases or decreases.

Approach

  1. Read ϕ\phi at the two xx values.
  2. Calculate Δϕ=ϕ2ϕ1\Delta \phi = \phi_2 - \phi_1.
  3. Convert to ΔU=mΔϕ\Delta U = m\Delta \phi.
  4. Use ΔK=ΔU\Delta K = -\Delta U.

Step-by-Step Reasoning

  1. From the graph, at x=0.1×1012 mx=0.1\times 10^{12}\ \text{m}, ϕ110×108 J kg1\phi_1 \approx -10\times 10^8\ \text{J kg}^{-1}.
  2. At x=1.2×1012 mx=1.2\times 10^{12}\ \text{m}, ϕ214×108 J kg1\phi_2 \approx -14\times 10^8\ \text{J kg}^{-1}.
  3. The potential becomes more negative, so
Δϕ=14×108(10×108)=4×108 J kg1.\Delta \phi = -14\times 10^8 - (-10\times 10^8) = -4\times 10^8\ \text{J kg}^{-1}.
  1. Multiply by mass to get the change in potential energy:
ΔU=180×(4×108)=7.2×1010 J.\Delta U = 180\times (-4\times 10^8) = -7.2\times 10^{10}\ \text{J}.

The negative sign means gravitational potential energy decreases (the rock has moved to a “lower” potential).

  1. With conservation of mechanical energy (gravity only), the kinetic energy must increase by the same amount:
ΔK=ΔU=+7.2×1010 J.\Delta K = -\Delta U = +7.2\times 10^{10}\ \text{J}.

Key Takeaways

  • ϕ\phi is energy per unit mass, so multiply by mm to get UU.
  • A decrease in UU corresponds to an increase in KK when only conservative forces act.
  • Always track signs carefully with negative potentials.

Common Mistakes

  • Using ΔK=mΔϕ\Delta K = m\Delta \phi instead of ΔK=mΔϕ\Delta K = -m\Delta \phi.
  • Forgetting the graph’s scale factor (108 J kg110^8\ \text{J kg}^{-1}).
  • Stating “decrease” because ϕ\phi decreases (more negative), without converting properly to energy changes.

Things to Be Careful About

  • The graph values are approximate; sensible rounding (2–3 s.f.) is expected.
  • Keep units consistent: ϕ\phi in J kg1\text{J kg}^{-1} leads to UU in J\text{J} after multiplying by kg.
Techniques used
read numerical values from a potential-distance graphcalculate a change in potential from two graph readingsuse energy conservation to relate change in potential energy to change in kinetic energy
(ii)

At a point where x=0.1×1012 mx = 0.1 \times 10^{12}\ \text{m}, the speed of the rock is vv.

Determine the minimum speed vv such that the rock reaches the point where x=1.2×1012 mx = 1.2 \times 10^{12}\ \text{m}.

minimum speed = ______ m s1\text{m s}^{-1}

3M
DifficultyMedium
Worked solution

Working

From Fig. 1.2, maximum potential along the path is

ϕmax4.4×108 J kg1\phi_{\max} \approx -4.4\times 10^8\ \text{J kg}^{-1}

At x=0.1×1012 mx=0.1\times 10^{12}\ \text{m},

ϕ1=10×108 J kg1\phi_1 = -10\times 10^8\ \text{J kg}^{-1}

Minimum speed occurs when the rock just reaches ϕmax\phi_{\max} with zero kinetic energy:

12v2=ϕmaxϕ1\frac{1}{2}v^2 = \phi_{\max} - \phi_1 12v2=(4.4(10))×108=5.6×108\frac{1}{2}v^2 = (-4.4 - (-10))\times 10^8 = 5.6\times 10^8 v=2(5.6×108)=1.12×1093.3×104 m s1v = \sqrt{2(5.6\times 10^8)} = \sqrt{1.12\times 10^9} \approx 3.3\times 10^4\ \text{m s}^{-1}

Answer

Minimum speed 3.3×104 m s1\approx 3.3\times 10^4\ \text{m s}^{-1}.

Final answer

3.3 × 10^4 m s^-1

Detailed explanation

Background Concept

In a conservative field (like gravity), total mechanical energy per unit mass is conserved:

Km+ϕ=constant,where Km=12v2.\frac{K}{m} + \phi = \text{constant}, \quad \text{where } \frac{K}{m} = \frac{1}{2}v^2.

So between two points 1 and 2,

12v12+ϕ1=12v22+ϕ2.\frac{1}{2}v_1^2 + \phi_1 = \frac{1}{2}v_2^2 + \phi_2.

A key idea here is a “potential barrier”: if the potential increases to a maximum somewhere along the path, the object must have enough initial kinetic energy to reach that maximum.

Understanding the Question

The rock starts at x=0.1×1012 mx=0.1\times 10^{12}\ \text{m} with speed vv. It must travel toward star B and reach x=1.2×1012 mx=1.2\times 10^{12}\ \text{m}. The graph shows that ϕ\phi first rises (becomes less negative) to a maximum around x0.6×1012 mx\approx 0.6\times 10^{12}\ \text{m}, then falls.

The minimum starting speed is the one that just allows the rock to get over the highest point of ϕ(x)\phi(x); once it has passed that point, it will then move to lower potential and speed up again.

Approach

  1. Read ϕ1\phi_1 at the start.
  2. Find the maximum value ϕmax\phi_{\max} on the graph between start and destination.
  3. Set the kinetic energy at the top of the barrier to zero (minimum condition).
  4. Use conservation of energy per unit mass to solve for vv.

Step-by-Step Reasoning

  1. Starting potential (from graph):
ϕ1=10×108 J kg1.\phi_1 = -10\times 10^8\ \text{J kg}^{-1}.
  1. The curve reaches a maximum (least negative) value of about
ϕmax4.4×108 J kg1.\phi_{\max} \approx -4.4\times 10^8\ \text{J kg}^{-1}.
  1. To just reach this point, the rock arrives with v=0v=0 there. Apply energy per unit mass conservation between start and the maximum point:
12v2+ϕ1=0+ϕmax.\frac{1}{2}v^2 + \phi_1 = 0 + \phi_{\max}.

Rearrange:

12v2=ϕmaxϕ1.\frac{1}{2}v^2 = \phi_{\max} - \phi_1.
  1. Substitute:
ϕmaxϕ1=(4.4(10))×108=5.6×108 J kg1.\phi_{\max} - \phi_1 = (-4.4 - (-10))\times 10^8 = 5.6\times 10^8\ \text{J kg}^{-1}.
  1. Solve for vv:
v=2(5.6×108)=1.12×1093.3×104 m s1.v = \sqrt{2(5.6\times 10^8)} = \sqrt{1.12\times 10^9} \approx 3.3\times 10^4\ \text{m s}^{-1}.

(The mass cancels automatically because we used energy per unit mass.)

Key Takeaways

  • Minimum launch speed is determined by the highest potential along the route, not the potential at the final point.
  • Use energy per unit mass: 12v2\frac{1}{2}v^2 pairs naturally with ϕ\phi.
  • Reading the correct feature (the maximum) from the graph is the main physics skill here.

Common Mistakes

  • Using ϕ\phi at x=1.2×1012 mx=1.2\times 10^{12}\ \text{m} instead of ϕmax\phi_{\max}.
  • Forgetting that ϕ\phi values are negative and mishandling ϕmaxϕ1\phi_{\max} - \phi_1.
  • Not including the factor of 2 when solving from 12v2\frac{1}{2}v^2.

Things to Be Careful About

  • Ensure you pick the maximum of the curve (least negative value), not the minimum.
  • Keep the 10810^8 scale factor from the axis.
  • Quote vv to a sensible number of significant figures given the graph reading (typically 2 s.f. or 3 s.f.).
Techniques used
identify the maximum potential barrier from a potential-distance graphapply conservation of mechanical energy between two pointsequate kinetic energy per unit mass to a change in potential

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