Answers to even numbered problems appear below:


Due 1/22/98   B1:2)  E;  B1:4)  1.7e14 J;  B2:2a) 2 DOF, b) 3 DOF, c) 2 DOF, d) 3DOF;  B2:4a) 4.86e22, b) 300J; S17:48a) 2000J, b) 4.46 C degrees.

Due 1/29/98  B2:6) 25%;  B2:9a) v(He) = 5.73 v(Xe),  b) one,  c) 1360 m/s; S16:22) 16 atm;  S16:28) 2.49 kg; S16:36a) 4.14e-16 J, b) 7.04e5 m/s.

Due 2/5/98  B3:6a) +4kJ, b) 14K;  B3:8) 8MJ;  S17:26)Wab>0, delUab>0, Qab>0, Wbc=0, delUbc<0, Qbc<0, Wca<0, delUca<0, Qca<0;  S17:28a) 7.5L, b) 300K.

Due 2/10/98  B4:8) eff. = 0.083@300K and falls of nonlinearly to 0.025@1000K; B4:10a) 40%, b) 60kJ, c) 90kJ.

Due 2/19/98  B5:8a) N1=73, N2=27,  b) 0.027eV;   B5:16a) exp(-392), b) exp(-20.4) = 1.4e-9;  Handout(a) 2.7e-34, 0.37;  b) 4e-32, 100;  c) -12eV;  d) N2 cannot be greater than E1 in thermal equilibrium;  e) infinity, 27,380K;  f) 4.8e-14Hz, 621nm;  g) 0.022eV, sunlight would be transmitted through atmosphere, but sky would look black;  h) ratio doesn't change (depends only upon energy difference, not # levels present);  i) both N1 and N2 decrease (normalization constant decreases with added energy levels).

Due 2/24/98  B7:2a) +/- 0.057eV, b) 4.4 kT;  B8:4) 3.21eV;  B8:6a) 18km, b) 5.5e7 eV.

Due 3/5/98  19:4a) 8.23e-8N, b) 2.2e6m/s;  19:18a) 0.858 kNm^2/C, b) zero, c) 0.657 kNm^2/C;  19:26a) zero, b)0.365e6 N/C, c) 1.46e6 N/C, d) 0.65e6 N/C;  19:34a) zero, b) 8.0e7 N/C, c) zero, d) 0.735e7 N/C.

Due 3/19/98  20:8) -0.39V (initial position higher potential than final); 20:12a) zero, b)zero, c) 45 kV;  20:16a)-380nJ(-=>attractive), b) 103V;  20:20a) -11V, -32V, b) 7 V/m.

Due 3/24/98  20:30a) 48e-6C, b) 6e-6C;  20:46) 2.5e-3m^3.

Due 3/31/98  21:16a) const, b) double, c) double, d) const;  21:18) 448 A;  21:28a) 17ohms, b) 2A, 1.2A, 0.8A; 21:46) 2.2hrs.

Due 4/10/98  22:2a) 8.7e-14N, b) 5.2e13 m/s^2;  22:10a->b) zero; b->c) 4e-2N, along -x; c->d) 4e-2, along -z; d->a) 5.7e-2, midway between x and z;  22:16) 12.5T;  22:18) 2.6e-7T.

Due 4/16/98  23:8a) 0.5A, b) 2 W, c) 2W;  2312a) L->R, b) L->R, c) L->R, d) into page; 23:14) 19.6sin(314t) volts;  23:20) 14.2 cos(120t) mV.

Due 4/23/98  24:Q8) E accelerates charges;  24:6) 300sin(20pi*x-6pi e9t) V/m; 24:18a) 1.33e-8J/m^3, b) 1.33e-8J/m^3, c) 7.96 W/m^2;  24:34a) 6.88 units, b) 5.63 units;  24:40) 1e6J.

Due 4/30/98  9:Q10) Einstein won't see any image - frequencies of light incident shifted up out of visible range;  9:6) 0.87c;   9:8) 0.95c;  9:20a) 17.3m, b) 3.3 degrees.


Exam 1

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Exam 2

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Exam 3

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