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Problem C The partition function for an ideal gas is given by integrating over all possible position and momen- tum configurations, weighted by a Boltzmann factor, for each particle (6 integrals per particle over z, v, z, pz, py, pz _ each running from-oo to +oo) and multiplying all N of these together (the factor of h is included to cancel the dimensions of dpdr; the factor of N! is included to divide out the multiplicity of particle-particle exchange) a) Consider a gas in which all particles are ultra-relativistic (i.e. E pe); Calculate the partition function for this gas. (Hint: calculate the integral for one particle and then raise the entire solution to the N) b) Use this partition function to derive expressions for each of the following quantities: F, S, U, E, ?? (standard deviation), p, P, and Cv. (hint: you should recover the ideal gas law for P(V, T, N) and you should find that U 3NkT) c) Compare the thermodynamic quantities (U, P, S and Cv) to what we used throughout the first half of class for a non-relativistic gas.

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ca) (χ İN., p.lv 듀IT CAA dal 3p4 アBNk. 孟2p 2kT유형근 2. 2. 날하 3N-I つ丁 トニ갉 옮@vkr) =akT ONoT = 3NkT 2- TI V ㄇˇ N-I TV

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