[BUG] PDT as a special case of the (n dim) Divergence Theorem
Matthias Kawski
kawski at asu.edu
Fri Apr 30 20:29:46 PDT 2004
On Fri, 30 Apr 2004, Smith, Alexander J. wrote:
> .... This statement does not need any of the fancy set up for
> the abstract Stokes' theorem, i.e., forms on a manifold. All you
> need is an inner product in R^n...which you can define again in
> the obvious way.
I believe it is a very long way from the usual first encounter
with line integrals in calculus to any reasonably deep under-
standing. But just because we may not want to tell our calculus
studenst the whole truth, does not mean that we should not do
the very best to understand it. It was many years after Ph.D.
that I got to a level where I am reasonably happy with it.
I believe the following are a few key observations:
* In line and surface integrals do not integrate (tangent)
vector fields, but differential forms (that is, cotangent
vector fields).
* Line and surface integrals do NOT involve any inner products.
(Even Stewart gets this right -- but it is very painful there.
I prefer to use dot-products when convenient, but keep in mind
that the integral theorems are solidly on the diff form side.)
* However, if a metric is present (e.g. same units along the
axes), then the metric can be used to convert tangent into
cotangent vector fields (column into row vectors) and vice
versa. (In linear algebra v --> v^T or v --> v^T*G=<v^TG,.>)
* Some of the most powerful applications of the integral thms
of vector calculus are not in physical 3-space, but e.g. in
thermodymanics. The best known is the conversion of heat into
mechanical energy via e.g. the Carnot-cyle. Green's theorem
integrates the field pdV around the contour etc. Putting
arrows and angles into this picture is a disasetr from all
that I know.
We probably don't want to mention these applic's in the first
time around, but we should be reasonably correct and forward-
looking that the theorems we do in the first round actually
can be generalized, and are not plain DEAD ENDS.
* I personally found it very useful in my classes even in the
1st round to quite casually distinguish contra and covariant
vector fields -- it is so easy, just bring in units:
The differential of a function, say, temperature is measured
in degrees per inch. The velocity of the bug in inches per
second. Now change from inches to centimeters, and one field
is multiplied by 2.54, the other divided by 2.54. Clearly
something is going on. Students accept this very readily,
and it helps much as an organizing principle: fields that
arise as derivatives (gradient fields) should be irrotaional
(no spinning), whereas in velocity fields (e.g fluid flow)
the first look is whether they are divergence free (neither
expanding nor contracting).
At least according to AbrahamMarsden the gradient is the
"transpose" of the differential ... this can cause trouble
w/ units... don't go too far in the first round. What matters
is that the default plan for gradient fields is to evaluate
circulation/work/line integrals. The default plan for fluid
velocity fields is to look for flux across a curve / surface.
This situation gets quite a bit harder when looking at fields
that mix both properties -- most typically the Liouville
"vector field" representation of complex analytic functions
(analyticity <--> Cauchy-Schwarz-equations < --> curl and
divergence free). 3D is even more fun -- and this is where
E and M fields are. The problem with them is that they have
TOO MUCH symmetry, i.e. they lack some of the distinctive
features that are give-awayas for what is to be done with
other fields.
This is why I hold off with fully 3-D E-M fields until late.
This is closely related to the most fundamental fact that
d^2=0 (curl-test, divergence-test). It is very natural to
take a curl of a gradient, and to take a div of a curl,
but unless in dim 2 where all is same, it is strange to
look at the div of a agrad or at the curl fo a curl.
They do occur (e.g. the Laplacian is very important),
but they always involve a Hodge-star operator, which
converts a k-form into an n-k form. I prefer to develop
most intuition in settings where this operator does not
come in. (Easiest write-up[ is in old version of Marsden/
Tromba in the appendix< or advanced in Flanders).
Just on the side recall that Hodge star makes sense only
in Riemannina settings, i.e. when a metric is given, or when
the coordnate axes are labels w/ the same (or comparable
units).
* Re the divergence form of Green's theorem in the plane -- it
is a straight-forward analogy to the 3 D divergence theorem
(much closer than the circulation formulaiton of Green's thm
is to the special case of Stokes for surfaces in 3D).
I understand that Tevian disagrees -- but when I see my fluid
mechanics coallgues play w/ Navier Stokes etc. i see all the
time models for 3D flows that have a translational symmetry,
and very often are analyzed via cross-sections. Thus the flow
across a surface in 3D becomes the flow of a 2D field across
a curve (w/ trivial product in perpendicular direction).
In class we talk about flood irrigation -- 1/2 a foot deep
flow across a few acres. The vertical components and variation
of the fluid flow are negligible. In EM, consider the fields
along a wire carrying a current -- they are 3D, but all
analysis takes place in a plane perpendicular to the wire
(times a trivial height).
The absolutely crucial difference is that when considering
2D- fields and BOTH line integrals in depths, then one can
use visual images to devlop intuition. In 3D hardly any
nontrivial fiedl can bve pictured by a nonexpert (w/o prior
info on what one expects to see). I do 6 weeks of 2D and
then a few days of 3D.
* Re distinguishing all the different kinds of fields, the best
that I know is Gabriel Weinreich's little book on "Geometric
Vectors" (or similau). U of Chicago Press. about $20. small
paperback. As I recall he is a physicist who tried to teach
us math folks who simple it is to organize all these fields.
Matthias
**********************************************************
Matthias Kawski http://math.asu.edu/~kawski
Dept. of Mathematics and Statistics kawski at asu.edu
Arizona State University office: (480) 965 3376
Tempe, Arizona 85287-1804 home: (480) 893 0107
**********************************************************
More information about the BUG
mailing list