We point out that any torsion degrees of freedom will produce an effec
tive potential to the K and (K) over bar with opposite sign. This will
allow us to constrain the background torsion field from the K-physics
. The most stringent bound on the cosmological background torsion [T<S
UP>0</SUP>] < 10<SUP>-26</SUP><INF></INF> GeV comes from the direct me
asurement of the CPT violation. (C) 1998 Published by Elsevier Science
B.V. All rights reserved.