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author | Prashant S | 2020-04-14 10:25:32 +0530 |
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committer | GitHub | 2020-04-14 10:25:32 +0530 |
commit | 06b09e7d29d252fb2f5a056eeb8bd1264ff6a333 (patch) | |
tree | 2b1df110e24ff0174830d7f825f43ff1c134d1af /Quantum_Physics_Of_Atoms_by_Molecules/1-Thermal_Radiation_and_Plancks_Postulate.ipynb | |
parent | abb52650288b08a680335531742a7126ad0fb846 (diff) | |
parent | 476705d693c7122d34f9b049fa79b935405c9b49 (diff) | |
download | all-scilab-tbc-books-ipynb-master.tar.gz all-scilab-tbc-books-ipynb-master.tar.bz2 all-scilab-tbc-books-ipynb-master.zip |
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diff --git a/Quantum_Physics_Of_Atoms_by_Molecules/1-Thermal_Radiation_and_Plancks_Postulate.ipynb b/Quantum_Physics_Of_Atoms_by_Molecules/1-Thermal_Radiation_and_Plancks_Postulate.ipynb new file mode 100644 index 0000000..a1e69df --- /dev/null +++ b/Quantum_Physics_Of_Atoms_by_Molecules/1-Thermal_Radiation_and_Plancks_Postulate.ipynb @@ -0,0 +1,91 @@ +{ +"cells": [ + { + "cell_type": "markdown", + "metadata": {}, + "source": [ + "# Chapter 1: Thermal Radiation and Plancks Postulate" + ] + }, +{ + "cell_type": "markdown", + "metadata": {}, + "source": [ + "## Example 1.1: Surface_temperature_calculatio.sce" + ] + }, + { +"cell_type": "code", + "execution_count": null, + "metadata": { + "collapsed": true + }, + "outputs": [], +"source": [ +"//Example 1.1, page 24\n", +"clear\n", +"//For sun\n", +"sigma=5.67*10^-8//w/m^2-k^4\n", +"T=5700//in K\n", +"ST_sun=sigma*T^4\n", +"printf('\n Surface temperature of sun is %e W/m^2.',ST_sun)\n", +"//For north star\n", +"T=8300//in K\n", +"ST_Northstar=sigma*T^4\n", +"printf('\n Surface temperature of sun is %e W/m^2.',ST_Northstar)" + ] + } +, +{ + "cell_type": "markdown", + "metadata": {}, + "source": [ + "## Example 1.6: Continious_or_dis_continious_energy.sce" + ] + }, + { +"cell_type": "code", + "execution_count": null, + "metadata": { + "collapsed": true + }, + "outputs": [], +"source": [ +"//Example 1.6, apge 39\n", +"clc\n", +"g=9.8//in m/s^2, constant\n", +"l=.1//in m\n", +"m=0.01//in kg\n", +"h=6.63*10^-34//Joule-sec\n", +"theta=0.1//in radians\n", +"v=(1/(2*%pi)*sqrt(g/l))\n", +"printf('\n Oscillation frequency of pendulam %f per sec.',v)\n", +"E=m*g*l*(1-cos(theta))\n", +"printf('\n Energy of pendulum at its maximum potential %e Joule.',E)\n", +"Delta_e=h*v\n", +"printf('\n Delta E %e Joule',Delta_e)" + ] + } +], +"metadata": { + "kernelspec": { + "display_name": "Scilab", + "language": "scilab", + "name": "scilab" + }, + "language_info": { + "file_extension": ".sce", + "help_links": [ + { + "text": "MetaKernel Magics", + "url": "https://github.com/calysto/metakernel/blob/master/metakernel/magics/README.md" + } + ], + "mimetype": "text/x-octave", + "name": "scilab", + "version": "0.7.1" + } + }, + "nbformat": 4, + "nbformat_minor": 0 +} |