Energy conditions of the f(T, B) gravity dark energy model with the validity of thermodynamics

S H Shekh,V R Chirde,P K Sahoo

Figure 8. The behavior of the SEC, ${\rho }_{d}+3{p}_{d}\geqslant 0$ versus cosmic time with the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, n = 1 and γ = 2.2.