Abstract
The Bose-Einstein condensation of free relativistic particles [ε=(M2c4+c2p2)1/2−Mc2] is studied rigorously. For massless bosons (ε=cp), the condensation transition of third (second) order occurs in2 (3) dimensions (D). The molar heat capacity follows the T2 (T3) law below the condensation temperature Tc [kBTc=(2πħ2c2n/1.645)1/2 [(π2ħ3c3n/1.202)1/3], reaches4.38 (10.8) R at T=Tc, and approaches the high-temperature-limit value2 (3) R with no jump (a jump equal to6.75R) in2 (3)D. For finite-mass (M) bosons, the phase transition occurs only in3D with the condensation temperature Tc always smaller than that of the corresponding nonrelativistic bosons [ε=(2M)−1p2]. If the mass M is reduced to zero, the condensation temperature Tc grows monotonically and reaches eventually that of massless relativistic bosons. This mass-dependence of Tc is therefore distinct from the case of nonrelativistic bosons, where Tc grows to infinity as M →0. A brief discussion is given for a possible connection with the normal-to-super transition of the independently moving Cooper pairs (bosons).
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Fujita, S., Kimura, T. & Zheng, Y. On the Bose-Einstein condensation of free relativistic bosons with or without mass. Found Phys 21, 1117–1130 (1991). https://doi.org/10.1007/BF00733389
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DOI: https://doi.org/10.1007/BF00733389