We have used ac calorimetry to measure the specific heat of CuGeO3 bel
ow its spin-Peierls transition temperature in magnetic fields up to 7T
, and have compared it to values calculated from a model triplet magno
n dispersion curve. We find that the observed field dependence is much
smaller than that calculated with Zeeman splitting of the magnon gap,
but is consistent with that calculated assuming m=0 excitation (and m
ean-field, quadratic magnetic field dependence) only. This result impl
ies weak coupling between thermal phonons and m=+/-1 magnons, so that
population of the latter are frozen for times < 40 ms. A similar assum
ption accounts for the zero-field specific heat at temperatures above
4.5 K. Copyright (C) 1996 Elsevier Science Ltd