Can anyone help on this ?
I did this
c = 2.998 10^8;
h = 6.62607015 10^-34;
Kb = 1.380649 10^-23;
i[\[Lambda]_,
T_] := ((2 Pi h c^2)/(\[Lambda]^5 (Exp[(h c)/(\[Lambda] Kb T)] -
1)));
M = Plot[i[\[Lambda], 3000], {\[Lambda], 0, 2.5 10^-6},
PlotRange -> Automatic,
PlotStyle -> {Thickness [0.005], Green},
Filling -> Axis, FillingStyle -> Green ];
N = [i[\[Lambda], 4000], {\[Lambda], 0, 2.5 10^-6},
PlotRange -> Automatic ,
PlotStyle -> {Thickness [0.005], Blue, Dashed},
Filling -> Axis];
O = [i[\[Lambda], 5000], {\[Lambda], 0, 2.5 10^-6},
PlotRange -> Automatic ,
PlotStyle -> {Thickness [0.005], Orange}];
Show[M , N , O, GridLines -> Automatic , PlotRange -> Automatic ,
Frame -> True , AxesLabel -> {\[Lambda][m], (watts/m^3)},
Epilog -> {Insert [
Framed[Style["T=3000K", 10], Background -> White], {8.23 10^-7,
5.42 10^13}],
Insert [
Framed[Style["T=4000K", 10], Background -> White], {8.23 10^-7,
1.64 10^13}],
Insert [
Framed[Style["T=5000K", 10], Background -> White], {8.75 10^-7,
3.90 10^13}]}] // Quiet
and I get this "is too small to represent as a normalized machine number; precision
may be lost". Can anyone help please
PlanckRadiationLaw[]
? $\endgroup$N
, for example, is a built-in which I would definitely not want to overwrite. $\endgroup$