@leslietownes While in graduate school in the 70s, my father was TAing a class, and made reference to the Beatles. The class had no idea who the Beatles were, until one of the students said "Oh, yeah! That was, like, Paul McCartney's band before Wings!"
Man, last semester, I had a student who was angry that I taught things which are not in the book. We spent two days on complex numbers so that I could show them some Newton fractals (and I didn't even test them on that shit!). We did a little bit of analytic geometry so that we could look at functions from a different perspective. And, god forbid, we spend two days sequential convergence because epsilon-delta is (a) rather technical and (b) not super intuitive at first glance.
@robjohn You'll be amused to know that after your comment, DrPotato admitted I'd been correct all along (re integration by parts with a non-well-defined function).
@Xander I think lower-level students (no offense intended) tend to be more wedded to "following the book" than more advanced students. I admit that in precalc and calc I tried to conform to the book's conventions, etc., to minimize Angst.
Yes, I think sequences are pedagogically quite good, but since we don't usually teach them until the end of Calc II, there is a logistical issue there.
when i taught out of a book i absolutely hated, i made sure to have all homework and exam problems clearly linked to assigned reading in the book. and sometimes even exercises in the book.
My frustration is that I stick to the book very closely (as much as I dislike it), but take one class out of every two weeks for "enrichment" (and sell it to the students as such). But even this one hour every two weeks is, it seems, too much.
Given a linear ODE with constant coefficients of this form: $y^{(n)}+a_1 y^{(n-1)}+...+a_1 y^{(1)}=\sin (ax+b)$, I want to know how to find its particular solution using inverse operator. How can the particular solution can be found using inverse oprator method?
It develops like this: If we have $dy/dx=f(x)$, say, then we re-write it as $Dy=f(x)$. Clearly, $y=\int f(x)\, dx$. Based on this we can define: $\frac 1D. f(x):=\int f(x)\, dx$ so that $y=\frac 1D. f(x)$.
I've been reading endless stories about all the disasters with Amtrak, especially with the recent snow. Definitely the case that the generic customer is very dissatisfied.
I'll explain with an example. Suppose we have $y''-3y'+2y=xe^x$ so we have $(D-2)(D-1)y=xe^x$. From here, $y=\frac 1{(D-2)}\frac 1{(D-1)}(xe^x)=\frac 1{D-2}. e^x\int xe^xe^{-x}\,dx=-1/2(1+x)^2e^x$
while RHS can be simplified. I have one problem: We may not that we'll have (n-1) more such factors. So isn't that going to complicate the calculations?
partial fraction suggestion seems nice. However, that will also give complicated final solution, I think. I mean -using partial fractions-are we able to reach this type of nice closed form: if p(D)y=sin (ax+b) then $y=\frac 1{p(D=\text{something})} \sin (ax+b)$?
$p(D)y=\sin (ax+b)$. Suppose that $p(D)=(D-r_1)(D-r_2)...(D-r_n)$, where $r_i$'s may be complex or real. $y=\sum_{i=1}^n \frac {a_i}{D-r_i} (\sin (ax+b))$, where $a_i$'s are constant obtained by converting $1/(D-r_1)(D-r_2)...(D-r_n)$ into partial fractions.
It follows that $y=\sum a_i e^{r_ix}\int e^{-r_ix}\sin(ax+b)\,dx$
gonna follow my nose with Laplace transform. If $y'(x)-ay(x)=f(x)$, then $(s-a)Y(s) = F(s) + y(0^-)$. for a particular solution, we can choose $y(0^-)=0$. Then $Y(s)=(s-a)^{-1}F(s)$
Semiclassic: So if $\phi$ is the fundamental solution, i.e., solves $\phi'-a\phi = \delta_0$, then the solution is given by convolution with $\phi$. I think this gets us to the same place. So what is $e^{ax}\int e^{-ax}\delta_0(x)\,dx$?
But the book did something along these lines: note that $D^2\sin (ax+b)=-a^2\sin(ax+b), D^4\sin (ax+b)=a^4\sin(ax+b),..., (D^2)^r\sin(ax+b)=(-a^2)^r$ so $p(D^2)\sin(ax+b)=p(-a^2)\sin (ax+b)$ so $\frac 1{p(D^2)}\sin (ax+b)=\frac 1{p(-a^2)} \sin (ax+b)$.
I'll proceed a little differently but with the same goal. $$(D-a)\phi(x) = f(x)\implies (i k -a)\tilde{y}(k)=\tilde{f}(k)\implies \tilde{y}(k)=(ik-a)^{-1}\tilde{f}(k)$$
Yeah, I have notes in my lecture notes from 1987 on issues like this. Solving $u'' = a^2 u$ doesn't work with FT because we need boundary conditions at $\pm\infty$.
lol lecture notes from 1987. week 1, the geocentric model. week 2, how to identify a witch. week 3, linear differential equations [guest lecturer: leonhard euler]
which connects two valid facts---"earth's distance to sun changes over the year", and "North America is hot during June / July August"---via invalid reasoning
the fact that aphelion, farthest distance, occurs in July is testament to that :P
@Thor Re your intersection theory question. I don't normally think about open embeddings, but what if we embed a torus into an infinite-genus torus and push the intersection off to infinity?
the torus doesn't embed into the infinite-genus surface. but I don't think I understand the idea either. we're looking at intersections coming from the space we're embedding, so how do you mean "pushing off to infinity"?
Well, I need a twice-punctured torus, I guess, but that's still enough to have intersections. I was going to push the torus off to infinity in the infinite one. I dunno. I don't think about these things.
We just passed through perihelion. Here's a plot of the Sun-Earth distance, using my program here: astronomy.stackexchange.com/a/47345/16685 Data points are for 0:00 UTC
But it still does have a measurable effect on the climate. So southern hemisphere summers are a little hotter, and shorter. But other factors are more important. We have less land mass down here, and a big circumpolar current. So it gets pretty cold below 40°S, and not many people live further south than that. Whereas 40°N is still fairly temperate.
@Semiclassical Oh, sure. In terms of the seasons, that 23° angle between the ecliptic & equatorial planes is way more important than the eccentricity. But they're both important in determining the difference between apparent solar time & mean solar time, aka the Equation of Time. physics.stackexchange.com/a/469884/123208
@Semiclassical Kepler was a pretty amazing dude. And a great writer, although he does tend to ramble all over the place. And get a bit mystical. :) He took a couple of years off astronomy & geometry to defend his mother against charges of witchcraft. And they won the case, which was quite unusual.
Kepler's mathematics is even more impressive when you remembervhe did that stuff before calculus was invented, and analytical geometry was still in its infancy. Of course, there were techniques for finding areas under curves, and rates of change, but they weren't codified or well-organised.
@AkivaWeinberger Sure. So if you run the Euclidean algorithm on a pair of adjacent Fibonacci numbers, you descend through the Fibonacci sequence. Each quotient is 1, so the algorithm descends at its slowest possible speed. This is reflected in the continued fraction for the golden ratio. It's sometimes said that it's the most irrational number because its continued fraction has the slowest possible convergence.
@Semiclassical Well, quadratic irrationals are nice because their continued fractions are periodic. Continued fractions have a long history, and a lot of the "big names" in early modern number theory put a lot of time into studying them. At that time, they were one of our few tools for tackling irrationals. The continued fraction is a compact way of representing the recursive solutions to Pell's equation.
Continued fraction convergents give you the best rational approximations of a number, which gives them an advantage over representations using some arbitrary base like 10, 2 or 16. Sadly, they're a bit painful when you need to do arithmetic on the number. ;)
There are families of cute continued fractions for powers of e. Last week, I learned there are nice continued fractions for the incomplete gamma functions. math.stackexchange.com/a/4339669/207316
But getting back to orbit stuff... Yesterday, I was playing with the vis-viva equation, which gives the speed of a body in an elliptical orbit. It's usually written in terms of $r$, but it's easy enough to write it in terms of $\theta$, as I mention here: physics.stackexchange.com/a/675868/123208
Hi, I am trying to prove that the operator $X\mapsto \mathcal{L}_{X}g$ is a closed operator when working on a compact manifold. I know I need to limit my domain so that I will have a Norm space into a norm space, since the space of smooth sections over a manifold is not a norm space. Is there a way to do so?
We get $v^2 = GM\left(\frac{1+2e\cos\theta+e^2}{a(1-e^2)}\right)$, where $e$ is the eccentricity. That's a family of limaçons, with a circle for $e=0$, and approaching a cardioid as $e$ approaches 1 (where the orbit becomes unbound).
The following script plots the curves (in green), along with circles showing the minimum & maximum (in red & blue).
more generally, if $M$ is compact and $E\rightarrow M$ is a vector bundle with a bundle metric, then this constructions defines a norm on the space $\Gamma(E)$ of global sections
the Riemannian metric induces a bundle metric on $T^2T^{\ast}M$, so you also get a norm on $\Gamma(T^2T^{\ast}M)$ that way
They’ve messed up more on the mobile activity page: now the navigation pop-up menu takes up a whole row and I can hardly see any of the content past the headers. Ugh!
The other day i was solving this: Determine an odd function $f:\Bbb R \to \Bbb R$ that holds $f(1) = 1$ and the relation $\displaystyle \int_{-a}^{a} (a^x - x^2)f'''(x) dx = a^3$
Hey, how do the rules of modulus fair for inequalities?
I found an identity for expressions of the form $\lfloor\frac{ab}{c}\rfloor$ that I might be able to use because the conditions ever so conveniently work out for doubling the precision of a given quotient approximation.