summaryrefslogtreecommitdiff
path: root/blackbody_new.tex
diff options
context:
space:
mode:
authorEugeniy E. Mikhailov <evgmik@gmail.com>2020-09-17 09:55:22 -0400
committerEugeniy E. Mikhailov <evgmik@gmail.com>2020-09-17 09:55:22 -0400
commit4dfcc8bd35c5881988f4b09fa2131448214e5513 (patch)
tree254dc59de40c4b594750a5f415ac8dd78fbae5ac /blackbody_new.tex
parent3598bbeb1f11117acb7de81dbab1052ab546d72a (diff)
downloadmanual_for_Experimental_Atomic_Physics-4dfcc8bd35c5881988f4b09fa2131448214e5513.tar.gz
manual_for_Experimental_Atomic_Physics-4dfcc8bd35c5881988f4b09fa2131448214e5513.zip
modified the assignment for black body
Diffstat (limited to 'blackbody_new.tex')
-rw-r--r--blackbody_new.tex12
1 files changed, 11 insertions, 1 deletions
diff --git a/blackbody_new.tex b/blackbody_new.tex
index c3bf73d..102a027 100644
--- a/blackbody_new.tex
+++ b/blackbody_new.tex
@@ -155,7 +155,17 @@ In the lab report plot the reading from the radiation sensor (convert to $W/m^2$
\begin{equation}\label{SBlmod}
S =\epsilon\sigma T^4
\end{equation}
-where the coefficient $\epsilon$ is called \emph{emissivity} and is defined as the ratio of the energy radiated from a material's surface to that radiated by a perfect blackbody at the same temperature. The values of $\epsilon$ vary from 0 to 1, with one corresponding to an ideal blackbody. All real materials have $\epsilon<1$, although some come quite close to the ideal (for example, carbon black has $\epsilon=0.95$). However, emissivity of a tungsten wire varies from $\epsilon=0.032$ (at $30^{\circ} C$) to $\epsilon=0.35$ (at $3300^{\circ}C$). Using the result of your fit, and assuming we know the Stephan-Boltzman constant $\sigma$ by some other means, what is $\epsilon$ and what is the uncertainty on it? Is it consistent with tungsten? What else could be affecting this measurement?
+where the coefficient $\epsilon$ is called \emph{emissivity} and is defined as the ratio of the energy radiated from a material's surface to that radiated by a perfect blackbody at the same temperature. The values of $\epsilon$ vary from 0 to 1, with one corresponding to an ideal blackbody. All real materials have $\epsilon<1$, although some come quite close to the ideal (for example, carbon black has $\epsilon=0.95$). However, emissivity of a tungsten wire varies from $\epsilon=0.032$ (at $30^{\circ} C$) to $\epsilon=0.35$ (at $3300^{\circ}C$).
+
+Unfortunately, it is impossible to measure the exact value of emissivity
+from the experimental data, as one needs to know the surface area of the
+filament and the precise distance from it to the detector. However, we
+should be able to qualitatively verify the validity of Eq.~(\ref{SBlmod}). From
+fitting experimental data, find the proportionality coefficient between the
+emitted radiation and the filament temperature $T^4$ and its uncertainty.
+Estimate the quality of the linear fit (a linear fit would assume that the
+emissivity does not depend on temperature).
+
Let us examine the quality of the fit more carefully. For that it is convenient to make a separate plot of the \emph{residual} - the difference between the experimental points and the fit values. For a proper fit function, we expect the residuals to be randomly distributed around zero. Analyze your results. Do the points seem to systematically differ from the fit line in a particular region? Can you think of a reason why that would be?