M. J. S. Houndjo, Oliver F. Piattella
We consider cosmological scenarios based on $f(R,T)$ theories of gravity ($R$
is the Ricci scalar and $T$ is the trace of the energy-momentum tensor) and
numerically reconstruct the function $f(R,T)$ which is able to reproduce the
same expansion history generated, in the standard General Relativity theory, by
dark matter and holographic dark energy. We consider two special $f(R,T)$
models: in the first instance, we investigate the modification $R + 2f(T)$,
i.e. the usual Einstein-Hilbert term plus a $f(T)$ correction. In the second
instance, we consider a $f(R)+\lambda T$ theory, i.e. a $T$ correction to the
renown $f(R)$ theory of gravity.
View original:
http://arxiv.org/abs/1111.4275
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