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William edited After_removing_the_background_maxima__.tex
over 8 years ago
Commit id: 75d672bd04d45caa24267ca8ff9a69c92b618136
deletions | additions
diff --git a/After_removing_the_background_maxima__.tex b/After_removing_the_background_maxima__.tex
index a1e8d52..b64e5fa 100644
--- a/After_removing_the_background_maxima__.tex
+++ b/After_removing_the_background_maxima__.tex
...
E_a [eV] (Dips) &= 4.72\pm.25\\
\end{split}
\end{equation}
The value of the excitation energy found from the linear fit was then compared to the known value of the lowest excitation energy for Mercury I ($4.67ev$ and $4.89ev$)
(citation needed) (NIST database values) . For the dips, when $n=0.5$, $E_{a}=4.72\pm.25eV$. For the peaks, when $n=0.5$, $E_{a}=4.63\pm.23eV$. The values found from the linear fits of the data agree with the accepted values of $E_{a}$ within uncertainty. Thus, excitation value found for the lowest state of Mercury quantitatively agrees with the expected value.\\