Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Configurational entropy in $f(T)$ gravity   The evolution of the configurational entropy of the universe relies on the
growth rate of density fluctuations and on the Hubble parameter. In this work,
I present the evolution of configurational entropy for the power-law $f(T)$
gravity model of the form $f(T) = \zeta (-T)^ b$, where, $\zeta = (6
H_{0}^{2})^{(1-s)}\frac{\Omega_{P_{0}}}{2 s -1}$ and $b$ a free parameter. From
the analysis, I report that the configurational entropy in $f(T)$ gravity is
negative and decreases with increasing scale factor and therefore consistent
with an accelerating universe. The decrease in configurational entropy is the
highest when $b$ vanishes since the effect of dark energy is maximum when
$b=0$. Additionally, I find that as the parameter $b$ increases, the growth
rate, growing mode, and the matter density parameter evolve slowly whereas the
Hubble parameter evolves rapidly. The rapid evolution of the Hubble parameter
in conjunction with the growth rate for the $b=0$ may provide an explanation
for the large dissipation of configurational entropy.

23
The categories of this paper are: solv-int
26
The categories of this paper are: bayes-an
0
The categories of this paper are: hep-ph
8
The categories of this paper are: hep-ex
34
The categories of this paper are: chem-ph
10
The categories of this paper are: q-bio
17
The categories of this paper are: q-fin
29
The categories of this paper are: funct-an
35
The categories of this paper are: mtrl-th
30
The categories of this paper are: q-alg
24
The categories of this paper are: dg-ga
2
The categories of this paper are: math
25
The categories of this paper are: patt-sol
20
The categories of this paper are: acc-phys
32
The categories of this paper are: atom-ph
3
The categories of this paper are: physics