Skip to content

Add files via upload #2

New issue

Have a question about this project? Sign up for a free GitHub account to open an issue and contact its maintainers and the community.

Sign up for GitHub

By clicking “Sign up for GitHub”, you agree to our terms of service and privacy statement. We’ll occasionally send you account related emails.

Already on GitHub? Sign in to your account

Open
Abhishek8322 wants to merge 1 commit into
base: main
Choose a base branch
from
Open

Add files via upload #2

Changes from all commits
Commits
Show all changes
1 commit
Select commit
File filter

Filter by extension

Filter by extension
Conversations
Failed to load comments.
Loading
Jump to
Jump to file
Failed to load files.
Loading
Diff view
Diff view
25 changes: 25 additions & 0 deletions me20b008.tex
View file
Open in desktop
Original file line number Diff line number Diff line change
@@ -0,0 +1,25 @@

\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}