From fd18bff4e44a5db95eb5a329b1a0550de4fa967e Mon Sep 17 00:00:00 2001
From: Abhishek Yadav <85741764+Abhishek8322@users.noreply.github.com>
Date: Wed, 30 Jun 2021 12:13:56 +0530
Subject: [PATCH] Add files via upload

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+
+\begin{document}
+\section{Abhishek Yadav}
+\subsection{Planck's Radiation Law}
+\begin{equation}
+	\rho(\nu,T)={\frac{8 \pi h \nu^3}{c^3}}  {\frac{1}{\exp_k^{\frac{h \nu}{k_BT}} - 1}}
+	\label{eqn:1}
+\end{equation}
+The Planck's Law describes the energy density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given Temperature T, and there is no net flow of matter or energy between the body and its environment.
+The equation~\ref{eqn:1} depicts mathematical form of the Plank's Law. \\
+Here \\
+$\rho$ - Energy Density \\
+$\nu$  - Frequency of radiation emitted \\
+$k_B$  -  Boltzmann Constant \\
+k      -  Kaniadakis Parameter \\
+T      - Temperature \\
+The equation shows the fequency dependency of the the energy density ~\cite{meb008}.The ~\ref{fig:me20b008} shows the graph of variation of energydensity vs frequency.
+\begin{figure}[h]
+        \begin{center}
+		\includegraphics[width=200pt,height=200pt]{me20b008.eps}
+		\end{center}
+        \caption{Variation of energy density with the frequency, for the different values of Kaniadakis Parameter}
+        \label{fig:me20b008}
+\end{figure}
+