in series $\mathrm{R}_{\mathrm{eq}}=2 \mathrm{R},$ in parallel $\mathrm{R}_{\mathrm{eq}}=\mathrm{R} / 2$
$\Delta Q=\frac{\Delta T}{2 R} \times 12=\frac{\Delta T}{R / 2} t$
$\Rightarrow \frac{\Delta \mathrm{T}}{2 \mathrm{R}} \times 12=\frac{\Delta \mathrm{T}}{\mathrm{R} / 2} \mathrm{t}$
$\Rightarrow \mathrm{t}=3$ minutes
| Column $-\,I$ | Column $-\,II$ |
| $(a)$ Wein's constant | $(i)$ $Wm^{-2}\,K^{-4}$ |
| $(b)$ Stefan-Boltzmaan's constant. | $(ii)$ $Wm^{-1}\,K^{4}$ |
| $(iii)$ $mK$ |
$Reason :$ Peak emission wavelengths of a black body is proportional to the fourth-power of temperature.


