Did someone say something about a holiday?

Really? Already? Well gosh — I couldn’t hear you over the sound of me still reading research materials at home, working at a job, and now (having had a few days away from that) frantically preparing for Christmas.

Which is to say that I love you all dearly, and your regularly scheduled maths/politics/skepticism/whatever will be back with you shortly. Just…be gentle with me, okay?

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The Curious Case of Wikileaks

Yesterday, a large group of people gathered at the State Library in Melbourne to support Julian Assange and the Wikileaks organization. The rally was one of many international events organized under the banner of Rally4Wikileaks.

I’ve no strong opinion on Julian Assange personally. I have no desire to pre-judge his guilt or innocence with regards to the allegations made against him in Sweden: The best I hope for is a fair trial for Assange and a refusal by the Australian government to let him be extradited to the USA from either Sweden or the UK. Still, Assange has become a symbol of sorts — whether we like it or not. Wikileaks itself is under attack and it is up to us to let the governments of the world know that freedom of speech and (more appropriately) freedom of the press are not negotiable rights.

We live in an age where digital social networks have exponentially expanded the proportion of the world available to us. At the same time, information has undergone a paradoxical devaluing; the flood of data that rushes down the ‘tubes’ onto our desktop is now not enough for us.

Just as printing endless money won’t fix a broken economy, a rush of information is useless without a filter. That goes double for Julian Assange. While we can be thankful for the covert currency he provides, Wikileaks still only acts as a conduit to the mainstream media. In some ways the principle is the same: A good journalist never reveals his source; Wikileaks makes sure, then, that all journalists are good journalists.

It has been said that the Internet sees censorship as damage, and routes around it. This hasn’t stopped people from trying, of course — just review the ongoing net neutrality debate in the USA, and the Internet filter here in Australia. Viewed through that lens, Wikileaks is simply the latest episode in a series of attacks that should concern any informed citizen. There are people out there — in the media and in the government — who would try to control our networks and censor our information. Who would deny us transparency to avoid personal and political embarrassment.

Now is the time we act; we collect together and speak up. We lobby, we petition, we protest, and we make ourselves heard. There is a principle at stake here that we cannot and should not compromise on — and if each one of us does not stand up for ourselves, we mustn’t be surprised if no one stands up at all.

Apathy was never a strong defense of liberty, after all.

Open is not the opposite of closed.

So far, we’ve dealt with the motivation and definition of a metric space, and have also seen some standard examples. Pretty soon we’ll be moving onto different ways we can categorise metric spaces, but before we do that we’ll need to deal with a topic that is crucial to any kind of development: Open and closed sets.

The first misconception to do away with is the idea that open and closed sets set up a dichotomy in terms of classification. Once we’ve defined what they are, it might be a little clearer why that’s not the case — for now, just keep in mind that any one particular set can be:

  • Open
  • Closed
  • Open and closed
  • Neither open or closed

Also, I’m cheating here a little bit for the sake of simplicity; it’s possible for the open/closed distinction to be perfectly meaningless too. If I want ‘open’ and ‘closed’ to have any kind of meaning, we need to define which sets are open (under the restriction of some basic rules). If you’ve ever heard of topology, it’s exactly that: A topology for a particular space defines what the open sets are in that space.

Going through all the background for that is a bit fiddly, however, with not much payoff for what we’re interested in. So for the moment, we’ll work with the understanding that when I talk about open sets, I’m specifically talking about open sets in a metric space.

With that out of the way, the first thing we’ll need to see are open balls. The open ball of radius r centered at the point x \in X (where X is our set) is

B(x,r) = \{ y \in X : d(x,y)<r \}

which can be read as “the set of points in X of distance less than r away from x ” . So, for example, the open ball B(0,1) in \mathbb{R} is just the interval (-1,1) .

We call an element of a set A an interior point if we can find an open ball centred on that point which is entirely contained in A . I.e., a \in A is an interior point if and only if for some \epsilon > 0 ,

B(a,\epsilon) \subset A .

An open set is a set in which every point is an interior point. So for example, in \mathbb{R} the set (0,1) = \{x : 0<x<1\} is open, since for any given point I can always choose an interval that stays contained in (0,1) — e.g. \frac{1}{2} is interior, which I can show by choosing the open ball B\left(\frac{1}{2} , \frac{1}{4} \right) = \left( \frac{1}{4} , \frac{3}{4} \right) \subset (0,1) .

Now, imagine that you have some sequence of points \{x_n\} in a set B \subset X and suppose that they converge to some point that we shall call x . Then x is called an adherent point of B .

A set B is called closed if it contains all of its adherent points — in other words, any convergent sequence of points that lives entirely in B must have its limit also in B .

An example of a closed set in \mathbb{R} is the interval [0,1] = \{x : 0 \leq x \leq 1\} . Showing this is true is slightly more work than showing that (0,1) is open (though quite easy if you have a few other simple tricks in your mathematical arsenal); however I invite people to play around constructing sequences in that interval, and noting that they all must converge in the interval.

Now, just to finish up: We’ve seen an example of an open set, and one of a closed set; so what of the others categories? For a set that is neither open nor closed, we turn to the interval [0,1) = \{x: 0 \leq x <1 \} . It is clearly not open — 0 \in [0,1) , but any open ball around 0 will necessarily contain negative numbers which are not in our original set. It is also not closed, which we can see by examining the sequence

x_n = 1 - \frac{1}{n} .

Every element of that sequence is found in our interval (i.e. x_n \in [0,1) \,\, \forall n \in \mathbb{N} ), yet the limit as n \rightarrow \infty is clearly 1 \notin [0,1) .

Finally, for a set that is both open and closed, we turn to the set \mathbb{R} itself. By construction, every convergent sequence in \mathbb{R} converges to a point in \mathbb{R} (the details of that are unimportant for this discussion — though it should, at least, seem quite true); and if I choose any point in \mathbb{R} and place around it an open ball of any radius, it will still be contained in \mathbb{R} .

Somewhat paradoxically, another example of a set that is both open and closed is the empty set which contains no elements, \emptyset . It fulfills all of the criteria by dint of it being completely trivial — for instance it is technically true that every convergent sequence in the empty set has a limit in the empty set, even if this is only achieved by having no sequences to begin with. The sneaky little bugger.

Want to know how the world will end?

Hat tip to @lukeweston on Twitter who put me on to this — there’s a free public lecture on tonight at the Melbourne Convention and Exhibition Centre that sounds like it’ll be a lot of fun.

Professor Jocelyn Bell Burnell, the astrophysicist best know as one of the discoverers of pulsars, will be giving a talk titled Will the World End in 2012? The Astronomical Evidence. From the description:

What’s all this about the end of the world in 2012? Just what is meant to happen, and how likely is it to happen? This talk examines the threats from space and explains how much truth there is in the suggestions that killer asteroids, lethal solar flares or the black hole at the centre of the Milky Way (for example) could cause the end of the Earth.

Details are:

Date: Wednesday 8 December 2010 (i.e. TODAY)

Time: 7pm – 8.30pm

Location: Plenary Hall 1, Ground Floor (enter via doors 5 & 6); Melbourne Convention & Exhibition Centre

As I mention before, the talk is free — bookings, however, are essential. It’s easy enough to book though: Just go here, and you’ll be done in mere seconds! Sadly I won’t be able to attend due to a prior engagement, but you should all definitely head along. I’ll be very jealous of you.

The Nightmares Will Never End

Also, is it just me, or is it possible that Grimace is actually the good guy in this situation? Saving children from obesity and diabetes, while Ronald dons a particularly unconvincing disguise, before taking the kids out for milkshakes like some nineteen-fifties paedophile?

Metriculicious Examples

I mentioned that before we moved on to anything else, I’d chuck some examples of metric spaces out there. So…what are we waiting for? Let’s do this crazy thing.

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“Can we see where the malaria happens?”

Bellekitten is off and away…

…well, to Sydney today. Then Chile and the Gemini South Observatory tomorrow.

Keep an eye on her blog — my understanding is that she’ll be posting some stuff up from La Serena over the next ten weeks.

The Abstruse Abstractification of Distance

In everyday life, we take certain geometrical facts for granted. For example, that two parallel lines will never meet, or that given two points in space we can (theoretically) draw a straight line between them. These and other such common sense ideas form the basis of what is traditionally called Euclidean geometry; otherwise known as “all that crap about right angle triangles they taught you in school”.

If you look back on high school maths with the same fond resentment as I do, it’s likely that you remember a smattering of random facts that may or may not have proved useful to you at some point. For example, there’s Pythagoras’ Theorem, that states for a right angle triangle with hypotenuse {H} and two other sides {A} and {B} it is true that

\displaystyle H^2 = A^2 + B^2 .

There was also some discussion, of course, about similar and congruent triangles — talk which seemed pointless and boring to me at the time. Looking back on it now, I’m still not sure what they thought was added to the curriculum by drilling such terms into us. If nothing else it made the memorisation of terms seem more important than the understanding of concepts, a theme that I’m sure has turned many more than me off maths in high school.

But now I want to do something that might seem a little bit odd for people who have had little exposure to tertiary maths — for those who have taken university level courses, the process will seem wholly unremarkable. I want to focus on one particular aspect of geometry, and toss away everything else until I wind up with something that looks completely different (on the surface) to what I started with. Read more »

Obligatory TAMOz Roundup…

So…TAMOz? It was good. Mostly, it was really good. Of course, as one might expect there were highlights and low/average-lights; but on the whole the quality of the conference was excellent. To summarise the most important bits…

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