Figure 1.

Spatial volume, the Hubble parameter and scalar expansion versus cosmic time for the appropriate choice of constants: a1 = 4, b1 = 1 and γ = 2.2."

Figure 2.

Tsallis holographic dark energy density versus cosmic time for the appropriate choice of constants: a1 = 4, b1 = 1, δ = 0.5, 1.0, 1.5 and γ = 2.2."

Figure 3.

The behavior of dark energy density versus cosmic time t for the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, n = 1 and γ = 2.2."

Figure 4.

The behavior of dark energy pressure versus cosmic time t for the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, n = 1 and γ = 2.2."

Figure 5.

The dark energy equation of state parameter versus cosmic time for the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, n = 1 and γ = 2.2."

Figure 6.

The stability factor (velocity of sound) of the dark energy model versus cosmic time for the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, n = 1 and γ = 2.2."

Figure 7.

The behavior of the NEC, ${\rho }_{d}+{p}_{d}\geqslant 0$ in the dark energy model versus cosmic time for the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, 3, 5, 7, n = 1 and γ = 2.2."

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."

Figure 9.

The behavior of the DEC, ${\rho }_{d}-\left|{p}_{d}\right|\geqslant 0$ 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."

Figure 10.

The conditions for validity of the thermodynamical parameter in the dark energy model versus cosmic time for the appropriate choice of constants: a1 = 4, b1 = 1, α = 0.1, β = 36, m = 1, n = 1 and γ = 2.2."