Bianchi type I in
f
(
T
) gravitational theories
Wanas M I
1, 4
, Nashed G G L
2, 3, 4, †,
, Ibrahim O A
1, 2
Evolution of Hubble parameters
H
1
=
Ȧ
(
t
)/
A
(
t
) and
H
2
=
Ḃ
(
t
)/
B
(
t
), where
m
= 2,
, and
.