GCE AS/A level 1322/01 PHYSICS ASSESSMENT UNIT PH2: WAVES AND PARTICLES

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Surname Centre Number Candidate Number Other Names 2 GCE AS/A level 1322/01 PHYSICS ASSESSMENT UNIT PH2: WAVES AND PARTICLES P.M. FRIDAY, 25 May 2012 1½ hours ADDITIONAL MATERIALS In addition to this paper, you will require a calculator and a Data Booklet. INSTRUCTIONS TO CANDIDATES For s use Question Maximum Mark 1. 8 2. 6 3. 8 4. 8 5. 8 6. 11 7. 13 8. 10 9. 8 Total 80 Mark Awarded 1322 010001 Use black ink or black ball-point pen. Write your name, centre number and candidate number in the spaces at the top of this page. Answer all questions. Write your answers in the spaces provided in this booklet. INFORMATION FOR CANDIDATES The total number of marks available for this paper is 80. The number of marks is given in brackets at the end of each question or part-question. You are reminded of the necessity for good English and orderly presentation in your answers. You are reminded to show all working. Credit is given for correct working even when the final answer is incorrect. VP*(S12-1322-01)

2 1. (a) A water wave is travelling from left to right along a canal. The diagram shows the wave at one instant. A 2.0 m B direction of travel of wave (i) (I) Show that the wavelength of the wave is 0.80 m. [1] (II) How do the amplitudes compare for water particles A and B? [1] A graph of displacement, y (vertical component) against time is given alongside for water particle A. y / m 0.1 PARTICLE A (I) Calculate the frequency. [1] 0.1 0 0 0.2 0.4 time / s y / m 0.1 PARTICLE B (II) Sketch the corresponding graph for particle B on the axes given. [2] 0 0 0.2 0.4 0.1 time / s (iii) Calculate the speed of the wave. [1]

3 (b) When the wave in the first diagram has travelled further, it reaches a length of the canal where the water is shallower. The wavelength in the shallow water is 0.60 m. Calculate the speed of the wave in the shallow water, giving your reasoning. [2] 1322 010003 Turn over.

4 2. The apparatus shown is set up to produce a clear display on the screen of Young s fringes. 1.8 m laser slits with separation 0.45 mm (measured between centres) screen (a) The bright fringes result from constructive interference. Explain, in terms of phase and path difference, why there are bright fringes. You may add to the diagram above, or draw your own diagram(s) to assist your explanation. [2]

5 (b) (i) The centres of the bright fringes are measured to be 2.4 mm apart. Calculate the wavelength of the light from the laser. [2] To obtain an accurate value of wavelength, it is better to use a diffraction grating than a double slit. Give two reasons for this. [2] 1322 010005 Turn over.

6 3. The cavity of a laser has reflecting ends a distance L apart. Assuming there is a node at each end, the possible wavelengths of stationary waves are given by the equation 2L λ = n in which n is a whole number. (a) Label relevant lengths on the diagram, and hence show how this equation arises. [The stationary wave is shown as if it were a stationary wave on a stretched string.] [2] (b) For a particular semiconductor laser, L = 0.2050 mm. (i) Using the equation above, show that a stationary wave of wavelength 820.0 nm can exist in the cavity, but that a stationary wave of wavelength 821.0 nm cannot. [2] Find the next wavelength above 820.0 nm of stationary wave that could exist in the cavity. [2] (c) A stationary wave is equivalent to a superposition of progressive waves of equal amplitude travelling in opposite directions. Why is this condition not exactly met in a laser emitting a beam of light? [2]

4. (a) A rod made of clear plastic of refractive index 1.55 is shaped as shown. The surrounding air has refractive index 1.00. 7 (i) Calculate the critical angle for light approaching a boundary between the plastic and the air. [2] Hence complete the path of the beam in the diagram, showing its emergence into the air. [2] 45 45 (b) The bottom of the rod now dips into water, of refractive index 1.33. (i) Calculate the angle of refraction of the beam into the water at P. [2] 1322 010007 Sketch the refracted beam on the diagram. [1] (iii) Suggest how this plastic rod might be used as part of a device to give a warning when the water level in a tank falls below a certain height. [1] P water Turn over.

8 5. (a) Pulses of monochromatic light are sent from A to B through a multimode optical fibre. The graphs show the pulse at A and when it arrives at B. PULSE AT A PULSE AT B light power light power 0 0.1 0.2 0.3 8.0 8.1 8.2 8.3 time / µs time / µs leading edge leading edge (i) By considering the leading edge (the start) of the pulse, calculate the distance from A to B along the axis of the fibre. The refractive index of the fibre s core is 1.50. [3] Explain why the pulse is spread out over time when it arrives at B. A sketched diagram may help your explanation. [2]

(b) Suppose a second pulse is sent from A to B. 9 (i) State the minimum time interval t min, between the leading edges of the first and second pulses at A, for them to arrive at B without overlapping. [1] Show the second pulse on both graphs opposite, if the time interval between pulses at A is t min. [2] 1322 010009 Turn over.

10 6. (a) State, in terms of energy, the meaning of each term in Einstein s photoelectric equation E kmax = hf φ. (i) E kmax... [1] hf... [1] φ (iii)...... [1] (b) Monochromatic light of frequency 7.40 10 14 Hz is shone on to a caesium surface, and E kmax is measured. The procedure is repeated for three other frequencies, enabling four points to be plotted on the grid below. 2.0 E kmax / 10 19 J 1.0 0 2 3 4 5 6 7 8 9 10 frequency / 10 14 Hz (i) Showing your working, determine from the grid above (I) a value for the Planck constant, [2] (II) the work function of caesium. [2]

11 When a lithium surface is used instead of a caesium surface, E kmax is found to be 0.40 10 19 J for light of frequency 7.40 10 14 Hz. (I) Draw the expected line of E kmax against frequency on the same grid. [2] (II) This line cannot be checked satisfactorily by experiment using visible light. Name the region of the electromagnetic spectrum which is required. [1] (III) What is different about lithium, as compared to caesium, which makes it necessary to use this region of the electromagnetic spectrum? [1] Turn over.

12 7. A simplified energy level diagram for the amplifying medium of a 3-level laser is given. level P level U 2.10 10 19 J (a) Suppose that the laser is at room temperature and that it is not being pumped. level O (ground state) 0 (i) Compare the (electron) populations of the three levels. [1] A photon of energy 2.10 10 19 J in the laser cavity could interact with the amplifying medium. Name the process involved, and explain briefly what happens. [2] (b) The laser is now pumped, to create a population inversion between levels U and O. (i) Explain what is meant by a population inversion. [1] Draw two arrows on the diagram to show how the population inversion is achieved. [1] (iii) Explain in detail how light amplification takes place. [4] (iv) Calculate the wavelength of the radiation emitted. [2]

13 (c) In a 4-level laser the light output results from a transition to a lower level which is above the ground state. Explain the advantage over a 3-level system. [2] Turn over.

14 8. Cepheid variables are stars whose brightness varies in a characteristic, regular way. The variation is shown below for one such star. brightness / arbitrary units 0 5 10 15 time / days The mean power, P, emitted as electromagnetic radiation from a Cepheid variable is related to the period of its brightness variation, as shown alongside. (a) (i) Use the graphs to determine P for the star, showing briefly how you obtained your answer. P / 10 30 W 1.2 1.0 0.8 0.6 0.4 [2] 0.2 0 2 4 6 8 period / days The mean intensity of the radiation from the star, as measured at the Earth is 8.0 10 13 W m 2. Using your answer to (a)(i), calculate the distance, r, between the star and the Earth. [2]

15 (b) The maximum power emitted by the star during its cycle of variation is estimated to be 9.5 10 29 W, and the spectrum of its radiation corresponding to this point in its cycle is given below. 6 5 spectral intensity / arbitrary units 4 3 2 1 0 0 200 400 600 800 1000 1200 wavelength / nm (i) Use Wien s law to calculate the temperature of the star. [2] Calculate the diameter of the star. [4] Turn over.

16 9. (a) An electron and a positron can annihilate (destroy) each other, in this interaction: e + e + γ + γ (i) Explain how lepton number is conserved in this interaction. [2] State which force (strong, weak or electromagnetic) is involved in this interaction, giving a reason for your answer. [1] (b) A proton and an antiproton can annihilate each other, in this strong interaction: p + p + + x By applying conservation rules, suggest the identity of particle x. [2] (c) The + is unstable. It can decay, thus: + y + v e (i) Identify y. [1] Which force is involved? [1] (d) Show below, as an equation, how the might decay. [1]...... +... THERE ARE NO MORE QUESTIONS IN THE EXAMINATION.

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