7.25 With the previous problem in mind prove that dn (v) dv n₂ = n(v) + v
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- 1.16. Establish thermodynamically the formulae v (7)= = S and v (R), V = N. Express the pressure P of an ideal classical gas in terms of the variables and 7, and verify the μl above formulae.Example of numerical instability: Take y′ = −5y, y(0) = 1. We know that the solution should decay to zero as x grows. Using Euler’s method, start with h= 1 and compute y1, y2, y3, y4 to try to approximate y(4). What happened? Now halve the interval. Keep halving the interval and approximating y(4) until the numbers you are getting start to stabilize (that is, until they start going towards zero).11.1.3 Show that the electrostatic potential produced by a charge q at z = a for r < a is y(r) = 9 Απέρα n=0 (7) Pn(cos 0).