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| author | prashantsinalkar | 2017-10-10 12:27:19 +0530 |
|---|---|---|
| committer | prashantsinalkar | 2017-10-10 12:27:19 +0530 |
| commit | 7f60ea012dd2524dae921a2a35adbf7ef21f2bb6 (patch) | |
| tree | dbb9e3ddb5fc829e7c5c7e6be99b2c4ba356132c /3710/CH5/EX5.2 | |
| parent | b1f5c3f8d6671b4331cef1dcebdf63b7a43a3a2b (diff) | |
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initial commit / add all books
Diffstat (limited to '3710/CH5/EX5.2')
| -rw-r--r-- | 3710/CH5/EX5.2/Ex5_2.sce | 19 |
1 files changed, 19 insertions, 0 deletions
diff --git a/3710/CH5/EX5.2/Ex5_2.sce b/3710/CH5/EX5.2/Ex5_2.sce new file mode 100644 index 000000000..6b5cf48af --- /dev/null +++ b/3710/CH5/EX5.2/Ex5_2.sce @@ -0,0 +1,19 @@ +//Example 5.2, Page Number 176
+//Relative Populations of energy levels
+clc;
+T=300 //Given Room Temperature in Kelvin
+l=550*(10**-9) //Average Wavelength of Visible Radiation in meter
+h=6.6*(10**-34) //Planck's Constant in meter square kilogram per second
+c=3*(10**8) //Speed Of Light in meters per second
+k=1.38*(10**-23) //Boltzman Constant in meter square kilogram per second square Kelvin
+e=1.6*(10**-19) //Charge of an Electron in Coulombs
+
+E=(h*c)/l //E is the given Energy Difference
+E1=E/e
+
+N=exp((-1*E)/(k*T)) //N is the ratio of N2 and N1
+
+mprintf("\tThe Given Energy Difference of the Two Levels is %.2f eV\n",E1);
+
+mprintf("\tThe Relative Population of the Energy Levels is %.2e\n",N);
+//The minor difference arising is due to a round off error
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