### EM II Notes 2014_11_24: Leinard-Wiechert Potentials

There's sooo much going on today.  I'm back in the lab again, but I'm also studying for the last little bit of my EM II class.   Here are the EM notes for today.  Hopefully, I'll get a lab book up again in the morning.

Looking at the Leinard-Wiechert Potentials.

We'll have a particel mofin along hte path $\vec{r} = \vec{r_o}\left(t\right)$.  There is a quite lengthy explanation of IRFs, but I'll skip that for now and keep careful track of whether or not this comes back to bite me in the butt.  We define $\vec{R}\left(t^\prime\right) = \vec{r} - \vec{r_0}\left(t\right)$ which is the vector from the point charge at time $t^\prime$ to the observatin poitn $\left(\vec{r}, t\right)$.  This gives us a retarded time, $t^\prime$ determined by $t - t^\prime = R\left(t^\prime\right)$, where $R\left(t^\prime\right) = |\vec{R}\left(t^\prime\right)|$.  This makes far more sense if you translate one of the ever present ever invisible $1$s to a c to get $c\left(t - t^\prime\right) = R\left(t^\prime\right)$

The potentials in the IRf can be written as

$\phi = \dfrac{e}{R\left(t^\prime\right)}$, $\vec{A} = 0$.

A charge at rest will have 4-veclocity $U^\mu = \left(1, 0, 0, 0\right)$.

We can noew define the 4 potential to be $A^\mu = f U^\mu$.  We can also form a four vector version of $R^\mu$ as $R^\mu = \left(t - t^\prime, r - r_0\left(t^\prime\right)\right) = \left(t - t^\prime, \vec{R}\left(t^\prime\right)\right)$.  Looking at this, you should see a four space distance without the time axis turned negative.  In a sense, this fits because it isnt' squared yet.  In a sense it doesnt' because if it isn't squared, then the time componet shoudl have an $i$ out in front.  This is somewhat Wick rotated, to coin a somewhat fancy phrase.

In the special case where the charge truly isn't moving, then $f$ above shoudl be $e/R\left(t^\prime\right)$.  For the more general case where the charge is moving with four velocity $U^\mu$, we get

$f = \dfrac{e}{\left(-U^\nu R_\nu\right)}$, so $A^\mu = -\dfrac{eU^\mu}{U^\nu R^\nu}$

Here, we have rather mysteriously gotten our negative sign back in front of the time coordinate.  Ask the professor about this tomorrow.  The pertinent point is near equation 7.29.

Now, on to problem number 2
For 2.a., and b, see the Wake Forest notes:
\url{http://users.wfu.edu/natalie/s13phy712/lecturenote/lecture27/lecture27latexslides.pdf}

expression 17 and up give the appropriate curl.  If time allows take a look at Dr. Nevels article on graphically protraying E and B fields.  There's no reason everything shouldn't apply here since the L\&W potentials were derived classically.

The strategy is just to bludgeon through the curl of $\vec{A}$ equation and get the final result.  Then, bludgeon through the cross product of $\vec{E}$ and show that the results are equivalient.

### Cool Math Tricks: Deriving the Divergence, (Del or Nabla) into New (Cylindrical) Coordinate Systems

The following is a pretty lengthy procedure, but converting the divergence, (nabla, del) operator between coordinate systems comes up pretty often. While there are tables for converting between common coordinate systems, there seem to be fewer explanations of the procedure for deriving the conversion, so here goes!

What do we actually want?

To convert the Cartesian nabla

to the nabla for another coordinate system, say… cylindrical coordinates.

What we’ll need:

1. The Cartesian Nabla:

2. A set of equations relating the Cartesian coordinates to cylindrical coordinates:

3. A set of equations relating the Cartesian basis vectors to the basis vectors of the new coordinate system:

How to do it:

Use the chain rule for differentiation to convert the derivatives with respect to the Cartesian variables to derivatives with respect to the cylindrical variables.

The chain rule can be used to convert a differential operator in terms of one variable into a series of differential operators in terms of othe…

### Lost Phone

We were incredibly lucky to have both been in university settings when our kids were born.  When No. 1 arrived, we were both still grad students.  Not long after No. 2 arrived, (about 10 days to be exact), mom-person defended her dissertation and gained the appellation prependage Dr.

While there are lots of perks attendant to grad school, not the least of them phenomenal health insurance, that’s not the one that’s come to mind for me just now.  The one I’m most grateful for at the moment with respect to our kids was the opportunities for sheer independence.  Most days, we’d meet for lunch on the quad of whatever university we were hanging out at at the time, (physics research requires a bit of travel), to eat lunch.  During those lunches, the kids could crawl, toddle, or jog off into the distance.  There were no roads, and therefore no cars.  And, I realize now with a certain wistful bliss I had no knowledge of at the time, there were also very few people at hand that new what a baby…

### Lab Book 2014_07_10 More NaI Characterization

Summary: Much more plunking around with the NaI detector and sources today.  A Pb shield was built to eliminate cosmic ray muons as well as potassium 40 radiation from the concreted building.  The spectra are much cleaner, but still don't have the count rates or distinctive peaks that are expected.
New to the experiment?  Scroll to the bottom to see background and get caught up.
Lab Book Threshold for the QVT is currently set at -1.49 volts.  Remember to divide this by 100 to get the actual threshold voltage. A new spectrum recording the lines of all three sources, Cs 137, Co 60, and Sr 90, was started at approximately 10:55. Took data for about an hour.
Started the Cs 137 only spectrum at about 11:55 AM

Here’s the no-source background from yesterday
In comparison, here’s the 3 source spectrum from this morning.

The three source spectrum shows peak structure not exhibited by the background alone. I forgot to take scope pictures of the Cs137 run. I do however, have the printout, and…