An exponential Om(z) parameterization fitted to CC+BAO+Pantheon+ data gives late-time acceleration parameters but becomes unphysical at high redshift, and the f(T,T_G) gravity parameters are not actually fitted.
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Cosmological insights from an exponential $Om(z)$ function in $f(T,T_{G})$ gravity framework
An exponential Om(z) parameterization fitted to CC+BAO+Pantheon+ data gives late-time acceleration parameters but becomes unphysical at high redshift, and the f(T,T_G) gravity parameters are not actually fitted.