In this episode several different mathematical topics are mentioned, but we're going to focus on LIGO and Benford's law.
LIGO is the place where the fictional character Larry works, but it is also a scientific project in real life. It is a joint project by Caltech and MIT which is designed to detect gravitational waves. These can be understood by analogy to waves in a pond. (Look here for more information about waves.) Imagine a very still pond on a windless day. The top of pond will be completely flat. We can describe this mathematically by assigning each point of the pond a number H(x,y,t) corresponding to its height, and in this case, each point in the pond has the same height. This is described by the equation H(x,y,t) = c, where c is a constant. Now if a rock is dropped into the middle of the pond, the function H(x,y,t) will no longer be a constant, but will vary as a function of time t and position x,y. The function in general is difficult to describe because it depends on the boundary of the pond as well as how you choose to model dropping the rock, but if you fix the position and just look at the height of one point as a function of time, (i.e. f(t) = H(x,y,t)), then you get something like f(t) = cos(t).
Now to understand gravitational waves, we have to describe gravity in a way similar to our description of the height of the pond. To do this, we have a function G(x,y,z,t) which to each point in space x,y,z and time t assigns some kind of mathematical object to describe the gravity. Let's think for a bit about what we need to describe gravity. We can feel a force from gravity, and the strength (or magnitude) of that force depends on where we are. However, the direction of that force also varies depending on where we are. A mathematical object which describes a direction and magnitude is called a vector, so our function G must assign a vector to each point in space and time.
Now the goal of LIGO is to detect such waves. The basic idea of how this is done is as follows. The scientists built two mile-long tubes that are perpendicular to each other. Then a laser beam is split so that it travels down each othe tubes at exactly the same time. At the end of each tube are mirrors that reflect the beam back to its starting point. The tubes are built with very precise lengths so that if there are no gravitational waves, then the two beams are exactly out of phase so they cancel out (this means that if you write the equation for the intensity of the two beams at the point where they meet, they look something like cos(t) and cos(t + &pi ), so when they add together you get 0, which means there's no laser light). However, if there is a gravitational wave that is oriented in the right direction, it will change the length of one of the tubes but not the length of the other, and this will make it so that the two beams aren't out of phase anymore. This means there will be a brief flash of light where the two beams meet.
1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | |
Area of Rivers | 31.0 | 16.4 | 10.7 | 11.3 | 7.2 | 8.6 | 5.5 | 4.2 | 5.1 |
There is a simple intuitive explanation for this phenomenan. Many quantities in nature satisfy the property that is the quantity changes randomly, the amount of the change is likely to be proportional to quantity. Another way to say this is that if q is the quantity that changes randomly, it is likely to fall into the range .9*q to 1.1*q. Then if q starts with a large digit, like an 8, it is much more likely to change to a number that starts with a different digit than it would be if q started with a 1.
Let's give a more precise mathematical explanation. The above paragraph
states that many quantities that arise in nature can be modelled as
a product of a large number of random numbers between .9 and 1.1.
Then we have the equations
Let's diverge just a little bit to talk about the Central Limit Theorem. The statement of the theorem is that the sum of many independent and identically-distributed random variables is well approximated by a normal distribution. To understand this, first we'll do an example, and then we'll apply the statement to the example.
Now we can apply this to our situation to conclude that the distribution
for log(q) will look like a Bell curve. Now how is the
first digit of q is related to log(q)? If we are taking
all the logarithms using base 10, then since ,
we can let a be the integer part of log(q) and b
be the decimal part. Then the first digit of q only depends on
b. Now to figure out the distribution of the first digit of
q, all we need to do is figure out the distribution of b.
To do this, we break up the graph of the distribution of log(q),
(which is similar to a Bell curve) up into slices that have width 1 and then
take the average of all these. If the Bell curve is very wide (which
corresponds to q having a large range of possible values), then
since the Bell curve is symmetric, the distribution of b should be
close to flat, so b has an almost equal chance of being any number
between 0 and 1. Now if , then the first digit of
will be a 1, which leads to the formula
Let's test our predictions. We can do this by generating a random number q and then multiplying it by R random numbers each of which ranges from .9 to 1.1. We'll do this N times and then record the results in the table below.
Starting digit: | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 |
Count: | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 |
Percentage: |