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Physics Exam Answers: Spring Semester 2005 - 6 Level One F31SE1: From Marconi to Mars 3. Max. data rate = 42M bits s-1. 4. Data rate = 704 k bits s-1; Bandwidth (a) 704 kHz; (b) 704 kHz; (c) 176 kHz. 5. D = 4625 → 4800; fref = 0.2 MHz. 6. Min. sensitivity = 0.1 V. 7. VSWR = 1.5 ; Power radiated by antenna = 19.2 W ; Same value of VSWR given by a load of 33Ω. Minimum transmitter power required = 3.3W. 8. Plasma density = 5 1014 m-3 ; Height of layer = 120 km. F31SM3: Vibrations and Waves 1. (a) A = F0 M 10 i 4 2 (d) Resonance when = (b) Amplitude = F0 M 10 2 16 2 2 s-1. 02 2k , where 0 = m k m 2. (c) Freq. of normal modes are 0 and 3. (a) Wavelength = 1m. (b) Wavelength = 1m. (c) = = 4π rad. (d) v = 2ms-1. 4. (d) k = 15 kg s-2. (f) = 1.5 s-1. 5. (c) c = 6 ms-1 ; (d) Mass per unit length = 0.28 Kgm-1; (e) Amplitude = 0.1 m. (f) Wavelength = 0.4 m. 6. (e) vg ka ka cos ; (f) v p 0 sin . 2 k 2 2 0 a F31SQ1: Space-Time and Matter 1. 10 years. 2. m(v)/m0 = 3.20 ; min. freq. = 1.24 1020 Hz. 44 3. Max. kinetic energy = 1.45 eV ; Velocity = 7.14 105 ms-1. 4. Lowest energy of neutron = 92.5 keV. 5. Single step: E3→1 = 1.937 10-18 J ; 3→1 = 1.02 10-7 m. Two step: 3→2 = 6.55 10-7 m.; 2→1 = 1.21 10-7 m. 6. 1 Each daughter particle has momentum Mc 2 7. Kinetic energy (electrons) = 1100.0 eV; Kinetic energy (neutrons) = 0.60 eV. 8. A= 2m 2 1 M 2 ; Prob. = 0.609 L F31ST1: Thermal and Kinetic 2. v nb 1 1 an2 ; same as ideal gas for a = b = 0. W nRT ln 2 v1 nb V1 V2 3. From given data, kB = 1.36 10-23 JK-1. 4. STotal = 728 JK-1. 5. Total rate of heat flow = 6.25 W ; Temperature at junction = 20.6C. 6. Fraction of C due to vib. modes: CO2 – 27% ; SO2 – 21%. 7. Total work done during cycle = - 6.563 kJ. 8. (b) EA = EB = 5ε ; B is most probable; (c) T = 295 K F31SV1:Environmental Physics 4. Flow rate = 2.08 m3s-1. 6. Solar constant (Venus) = 2639 Wm-2. Net flux = 478 Wm-2 ; Equil. T = 303 K; Fractional increase in T for new Albedo is ).66%. 7. Fraction of land area required is about 40%. 8. Energy released = 196 MeV. 45 Level Two F32SA5: The Structure of Galaxies 2. (b) E = ½Mfuel c2 ; (c) Rate of mass accretion = 1.3 10-3 M๏ year-1. 6. R 9 109 M๏. (b) Rmin = R0 sin l ; M (<R) = K pc 7. (b) No escape ; (c) M (r) = 4πmkr ; (d) Vc2 (r) = 4πGmk. 8. (d) Distance = 19 Mpc. F32SB3: Molecular Biophysics 1. Data suggests that AT and GC occur as base pairs. 4. Radius of molecules = 3.98 10-9 m. 5. [D] = 1.35mM at 37C and 0.83mM at 2C. 6. a = 1.33 nm. ; A is simple cubic and B is face-centred cubic. 8. Max. tensile force = 9.2 10-9 N. F32SO1: Optics 2. 32.4 nm. 3. Lines per metre = 1.82 105 m-1 ; optimum blaze angle 7. 4. fsr = 0.018 nm. ; min = 6 10-4 nm. 5. System resolution = 2 105 lines per metre ; PSF width 5 10-6 m.; contrast ratio is 60%. 6. Effective focal length = 0.75 m. 7. Assuming = 650 nm., thickness of CeF3 and ZrO2 coatings are 98.5nm and 77.4 nm resp. Reflectance = 0.0012 46 F32YQ1: Quantum Physics 1. x 57.9 nm. ; E = 569.4 eV. 5. m me2 α= ; E10 2 2 2 40 6. Energy splitting = ½ λ. 7. (b) Transmitted flux = 9. 4r 2 a 0 Prob. of finding electron between r and r +dr is 3 e dr ; a0 e2 4 0 k 2 C ; me 2 T 4k k 2 2 r 3 e2 (a) <r> = a0 ; (b) <V(r)> = . 2 40 a0 Results of measurement of z compt. of angular momentum are 2ħ with a probability of ½ in each case. 10. Given configuration gives rise to the following multiplets: 3 F4, 3F3, 3F2, 1F3, 3D3, 3D2, 3D1, 1D2, 3P2, 3P1, 3P0, 1P1. 11. Value of Z for most stable isotope for A =120 is Z = 51. F32ST2 Thermal and Statistical Physics 1. TV1/3 = constant; Radius of bubble for explosion = 1.33mm. 2. Photon energy = 3.97 10-19 J. ; S = 9.9 10-22 JK-1 ; W/Wi = exp (72). 3. k BT 0.038 ; Z = 26.3 4. Prob. of Cu on lattice site is 0.6 ; Entropy of system: SN = 0.673 NkB. 5. rev = 0.44 ; (inventor’s engine) = 0.46 6. 4 2 / 3 (b) T S S0 . 9 7. (b) Work done by system = mC 2T1iT2i 47 1/ 2 T1i T2i 8. U U U U S k B N 1 ln ln N 1 N 1ln N 1 ; T kB U 1 / k B T ; 1 N 1 N e ln1 U / 48 Level Three F33SA7: Extreme Astrophysics 3. (b) M 108 M๏; (c) ‘a’ would be 10 times higher and there would be no change in ‘b’ 5. (a) (i) Blackbody ; (ii) Line emission ; (iii) Blackbody ; (iv) Synchrotron. 6. (d) INS < IWD (M=0.5M๏) < IWD (M=1.0M๏). 8. (d) M 1.7 107 M๏ ; (e) effects of relativistic beaming expected. F33SB5: Diagnostic Medical Physics (Non-Ionising Radiation) 1. Flip angle = 27 . 4. R1 = 6.2 s-1mM-1 ; T1 (tissue) = 1 s. 5. Signal increase is 15%. 7. Resonances separated by 120 Hz ; = 5.09 ppm ; this would change to 4.55ppm for pH of 6.8. 8. (b)(iii) (a) Br -87fT ; dBr/dr -1.3 104 fTm-1 ; (b) Br -0.34fT ; dBr/dr -13fTm-1. F33SN5: Theoretical Elementary Particle Physics 1. Mass of + = 780MeV. 6. (c) M 2 GeV. 7. (a) E = 5.1 eV ; (b) 1st state: J = 0, P = -1, C = +1 ; 2nd state: J = 1, P = -1, C = -1. (d) (2)/ (3) 137 8. (b) Oscillator length 1600 km. F33SO2: Laser Physics and Matter-Light Interactions 1. (a) vp = 108ms-1 ; (b) = 1.42 107 m-1 ; (c) R = 0.257 . 2. Population difference = 8.4 1019 . 4. Sodium becomes transparent to light below 205 nm. 49 6. vsound = 5852 ms-1 in direction parallel to incoming photon; for new geometry, frequency shift is 61 GHz at 22.5 to ingoing photon. 7. d = 1.26 m. ; transmitted light is circularly polarised (clockwise looking in direction of propagation) . 8. Approx. number of modes in output is 3 or 4 ; Lmax = 3.34mm. F33SQ6: Magnetic Resonance 5. (i) = 357 kHz ; (ii) = 178.5 kHz ; (iii) = 223.1 kHz. F33SS2: Solid State Physics 2 3. ELO = 33meV. 4. me*/me = 0.093 ; r = 6.9 . 6. k = 2.7π/a is equivalent to 0.7π/a in the first B.Z. ; (a) vs (b) TA C b ; M1 M 2 2 2C 2C 2C M1 M 2 ; TO ; (c) TO 0 M2 M1 M 1M 2 E EG 3 m kT ln h ; when mh* = me* , G ; for Si, n = 1.67 1016 m-2 . 2 2 4 me 7. = 8. 20 nm. F33SV3: Atmospheric Physics and Meteorology 1. Lower level: N = 1.12 1011 m-3 ; height = 120 km. Upper level: N = 4.5 1011 m-3 ; height = 225 km. ; Ratio = 171. 2. 112 D.U. 3. Lower boundary at 198 km. 5. (b) Thickness = 654 m. 50 6. cu 7. T10 = 267K ; T50 = 256.1K 8. (d) max = 6 10-5 rad s-1. 9. I 1500 A ; q = 14.1 C ; E0 = 4.98 103 Vm-1 ; E10 = -6.9 Vm-1 ; x = 8.4 km. k 2 l 2 ; c = 0.2 ms-1 east to west. 51