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We compute the exact thermal partition functions of a massive scalar field on flat spacetime backgrounds of the form R^d-q T^q+1 and show that they possess an SL (q+1, Z) symmetry. Non-trivial relations between equivalent expressions for the result are obtained by doing the computation using functional, canonical and worldline methods. For q=1, the results exhibit modular symmetry and may be expressed in terms of massive Maass-Jacobi forms. In the complex case with chemical potential for U (1) charge turned on, the usual discussion of relativistic Bose-Einstein condensation is modified by the presence of the small dimensions.
Aggarwal et al. (Tue,) studied this question.