Rotational Transitions

From AstroBaki
Revision as of 15:02, 1 October 2020 by Aparsons (talk | contribs) (Created page with 'Course Home ===Short Topical Videos=== * [ Rotational Transitions in Molecules (Aaron Parsons)] ===Reference…')
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigationJump to search

Course Home

Short Topical Videos

Reference Materials

Need to Review?

<latex> \documentclass[11pt]{article} \usepackage{fullpage} \usepackage{amsmath} \usepackage{eufrak} \begin{document} \section*{ Rotational Transitions }

\subsection{Order of Magnitude Energies}

Molecules can rotate, and have rotational energies that depend on their angular momentum. If $J$ is the quantum angular momentum number, $$ E_{rot} \sim \frac{\hbar^2 J (J+1)}{2I} $$ $$ I \sim M L^2 $$ For small $J$, $$ E_{rot} \sim \frac{m}{M} E_{elec} $$

So the electronic, vibrational, and rotational energy states have contributions that scale with the electron-to-nucleus mass ratio: $$ E_{elec} : E_{vib} : E_{rot} \sim 1: \left(\frac{m}{M}\right)^{1/2} : \left(\frac{m}{M}\right) $$

Rotational energies can be described using the angular momentum number $J$: $$E_{rot} = \frac{\hbar^2}{2I} J (J+1) $$

where $J = 0,\ 1,\ 2,\ ...$, $I$ is the moment of inertia, and for diatomic molecules, we can use the reduced mass $\mu$: $$ I = \mu L^2 $$ $$ \mu = \frac{m_1 m_2}{m_1 + m_2} $$

\end{document} <\latex>