Nicotra Fan Selection Software [BEST] Download
Nicotra Fan Selection Software [BEST] Download
Nicotra Fan Selection Software Download
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Thanks for browsing our website. The magnetic field energy density $w_B$ can also be expressed in terms of the Hubble parameter $H$ [@Hodzas:2015zaa]: $$\begin{aligned}
w_B \approx (\textrm{e}^{ -2N}-1)H^2\,.\end{aligned}$$ Inserting the numerical values we find $$\begin{aligned}
\label{eq:DW2}
w_B \approx \left(-7.99 \cdot 10^{ -4} -9.19\cdot 10^{ -5} + \frac{0.5384}{N}
\right)H^2\,.\end{aligned}$$ Clearly, the dark energy equation of state parameter given by equation may be driven to a negative value for certain values of $N$. However, when the gauge parameter is close to $\eta = 10$, the coupling becomes small and the effect of the extra dimensions is suppressed. For example, if we take the gauge parameter to be $\eta = 9$ and the extra dimensions $N$ to be $N = 1$, $N = 2$ and $N = 3$, we find the following numerical values for the dark energy equation of state parameter $$\begin{aligned}
w_{B,1} = \frac{0.000023 – 0.000037}{H^2}\,,\,
w_{B,2} = \frac{0.000043 – 0.000063}{H^2}\,,\,
w_{B,3} = \frac{0.000074 – 0.000144}{H^2}\,.\end{aligned}$$ In view of this, we note that the present model may provide us with a cosmologically viable setup if the extra dimensions are large. This is clear from the plots presented in figure \[
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