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The thermal energy of a classical ideal gas is ##U=f k_{\text{B}} N T/2##, where ##f## is the number of "relevant degrees of freedom" (i.e., ##f=3## for a monatomic, ##f=5## for a twoatomic, and ##f=6## for multiatomic gases); ##k## is Boltzmann's constant and ##N## is the number of particles/molecules, and ##T## the (absolute) temperature.
Then you have the ideal-gas law ##p V=N k_{\text{B}} T##, which is obviously different from ##U## by a factor.
Then you have the ideal-gas law ##p V=N k_{\text{B}} T##, which is obviously different from ##U## by a factor.