Gabriel Maia
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Hi. I'm reading a solution to a problem concerning a gas of photons. In the solution, the energy of the gas is given as
E=2\sum_{\vec{k}} \frac{\displaystyle \epsilon_{\vec{k}}}{\displaystyle \exp[\beta\epsilon_{\vec{k}}]+1}
where \epsilon_{\vec{k}} is one photon's energy. It is said then that in the thermodynamic limit we have
\sum_{\vec{k}} \rightarrow \frac{\displaystyle V}{\displaystyle (2\pi)}\int_{0}^{\infty}\,4\pi\,k^{2}dkCould you explain how is this change from the summation to the integral is done?
Thank you very much.
E=2\sum_{\vec{k}} \frac{\displaystyle \epsilon_{\vec{k}}}{\displaystyle \exp[\beta\epsilon_{\vec{k}}]+1}
where \epsilon_{\vec{k}} is one photon's energy. It is said then that in the thermodynamic limit we have
\sum_{\vec{k}} \rightarrow \frac{\displaystyle V}{\displaystyle (2\pi)}\int_{0}^{\infty}\,4\pi\,k^{2}dkCould you explain how is this change from the summation to the integral is done?
Thank you very much.