Take the 2-minute tour ×
Physics Stack Exchange is a question and answer site for active researchers, academics and students of physics. It's 100% free, no registration required.

I was talking to Roger Penrose about calculus in the appendix in his book Cycles Of Time and he said I'd need a good understanding of calculus if I wanted to read his book in great depth. He said I even need calculus to understand the movement of a particle in depth.

What is the calculus that describes the movement of a particle and how is it conducted?

share|improve this question
1  
I seriously doubt you were talking with Penrose :) –  Colin K May 22 '12 at 15:16
    
That comment was just unnecessary. Cor, some people (you). And I can assure you, I was. –  Olly Price May 22 '12 at 15:36
    
Why would I lie about that? –  Olly Price May 22 '12 at 15:37
4  
I think we have a case of jealousy here! –  Olly Price May 22 '12 at 15:53
8  
@OllyPrice: I met Penrose after a popular talk, and he was very nice, and when I mentioned a property of deSitter black hole solutions (that they turn inside out), he listened, his eyes lit up, and he immediately began sketching out what he called "Carter diagrams" (what everyone else calls Penrose diagrams) to figure out what was happening, and I think I looked like a crazy hobo then. He is a wonderfully kind and approachable person, and will not dismiss anyone, and I am sure that you are honestly reporting things. But you really should learn calculus before talking to him more. –  Ron Maimon May 23 '12 at 3:21
show 4 more comments

4 Answers

Here is a brief historical ideosyncratic intro to calculus.

Calculus of finite differences

Consider this problem from a typical IQ test:

2 5 10 17 26 ?

What's the next number you expect in the sequence (this is not hard, you should do it). The n-th term in the sequence is given by:

$$ n^2 + 1 $$

as you can see by substituting n=1,2,3,4,5, so the next term is 37. But if you did the problem, you probably noticed first that the differences are:

5-2 = 3 10-5 = 5 17-10 = 7 26-17 = 9

and then filled in 37 by adding 11 to 26. This thing you did above, of finding the difference between successive terms, is called "taking the first difference", and given any sequence of numbers $A_n$, the derived sequence

$$ \Delta A_n = A_{n+1} - A_{n} $$

From the definition, you can check $$ \Delta 1 = 0 $$ $$ \Delta n = 1 $$ $$ \Delta n^2 = 2n+1 $$ $$ \Delta n^3 = 3n^2+3n+1 $$ $$ \Delta n^4 = 4n^3 + 6n^2 + 4n + 1 $$ $$ \Delta 2^n = 2^n $$ $$ \Delta {1\over n} = - {1\over n(n+1)}$$

and you can prove the general properties

$$ A_n + \Delta A_n = A_{n+1} $$ $$ \Delta (A + B) = \Delta A + \Delta B $$ $$ \Delta cA = c \Delta A $$

This says that $\Delta$ is a linear operator. Further, you have a product rule

$$ \Delta (AB) = A \Delta B + B \Delta A + \Delta A\Delta B $$ $$ \Delta (AB)_n = A_{n+1} \Delta B_n + B_n \Delta A_n $$

So now you can see that

$$ \Delta (n^2 - n) = (2n+1 - 1) = 2n $$ $$ \Delta (n^2 2^n) = (2n+1) 2^{n+1} + n^2 2^n = (n^2 + 4n + 2) 2^n $$

And so on. It is good practice toward calculus to find the derived sequence of all common functions. This was done by early modern mathematicians, and this calculus of finite differences directly inspired calculus.

The main identity is the fundamental theorem of derived sequences--- the sum of the derived sequence is found from the original sequence. For example, 3+5+7+9+11 = 37 - 2 (because adding the differences steps up the sequence). Convince yourself that it is true (or prove it by induction). So that

$$\sum_{k=a}^{b} \Delta A_k = A_{b+1} - A_a $$

This is a remarkable formula, because now you learn a summation formula from each difference formula above:

$$\sum_{n=a}^b (2n+1) = (b+1)^2 - a^2 $$ $$\sum_{n=a}^b (2n) = 2 \sum_{k=a}^b n = b(b+1) - a(a-1) $$ $$\sum_{n=a}^b 2^n = 2^{b+1} - 2^a $$

The second difference is defined as the difference of the difference:

$$ \Delta^2 A_n = \Delta \Delta A_n = (A_{n+2} -2 A_{n+1} +A_n) $$

So that

$$ \Delta A_n + \Delta^2 A_n = \Delta A_{n+1}$$

and this says

$$ A_{n+2} = A_n + \Delta A_n + \Delta A_{n+1} = A_n + 2\Delta A_n + \Delta^2 A_n $$

and so on for third differences etc. You can prove that if two sequences have all of

$$ A_0, \Delta A_0, \Delta^2A_0, \Delta^3 A_0 , ... $$

equal, then the two sequences are equal, since the only way for the n-th differences to agree is if the first n terms are equal.

There is a nice quantity you can define:

$$ n^{(k)} = n(n-1)(n-2)...(n-k+1) $$

and for completeness, $n^(0)=1$. The factorial $n!=n^{(n)}$ by definition. This alternate definition of raising to a power has the property that

$$ \Delta n^{(k)} = k n^{(k-1)} $$

And in terms of this quantity, there is a formal expression for the n-th term of any sequence

$$ A_n = A_0 + \Delta A_0 n + \Delta^2 A_0 {n^{(2)}\over 2!} + \Delta^3 A_0 {n^{(4)}\over 4!} + ...$$

and this gives an explicit polynomial expression whose first n differences at 0 coincide with those of the sequence A. This allow you to fit a polynomial to any evenly spaced points easily.

The above looks like an infinite sum, but on an integer position, only finitely many terms are nonzero. If it is convergent as an infinite series, you might expect it to interpolate good non-integer values for a reasonably well behaved sequence.

This is called the Gregory series, and it was developed by Gregory in the early half of the 17th century. Gregory used this to give infinite polynomial series expansions for common trigonometric functions, including the arc-tangent. This stuff seems like a bag of formal tricks that is not particularly more insightful than what you can see just by piddling around with intuition. Still, it allows you to quickly prove all the annoying sum identities you learn in high-school.

Infinitesimal Calculus

Consider now a sequence defined not at the points 1,2,3,..., but on a very fine grid of points spaced $\epsilon$ apart, so that the n-th point is at position $n\epsilon$. All the ideas of the previous section transfer to this situation, since all you have to do is rescale everything to make the unit of length $\epsilon$, and the points lie on top of the integers.

In this case, the sequence $A(n)$ turns into a function $A(x)$ defined on all x's on the lattice. The derived sequence is

$$ \Delta_\epsilon A = A(x+\epsilon) - A(x) $$

And you can see that as $\epsilon$ goes to zero, it goes to zero. For a typical function, like multiplication or raising 2 to a power, we can ask, how does it go to zero?

$$ \Delta x^2 = (x+\epsilon)^2 - x^2 = 2x \epsilon + \epsilon^2 $$

This is just the rescaled version of the first difference of $n^2$ (you can work it out directly, and it is good if you do). The lesson is that the thing tends to vanish linearly, meaning that if $\epsilon$ is small, and it is made twice as small, your derived sequence is generally made about twice as small.

So you can take out this scaling and define the derivative of f

$$ {df\over dx} = {\Delta f \over \epsilon} = {\Delta f\over \Delta x} $$

Where the idea here is that you define the derivative for each $\epsilon$, and let $\epsilon$ become so miniscule that the derivative stops changing. This never happens for any finite nonzero positive value of $\epsilon$, so it is formally useful to introduce the concept of an infinitesimal $\epsilon$.

An infinitesimal $\epsilon$ is an $\epsilon$ that is so small, that it behaves as if it were zero for the purpose of order of magnitude comparison, but it is not yet zero. It can be formally defined as a procedure: given any quantity you can calculate with $\epsilon$, the quantity for infinitesimal $\epsilon$ is defined as the limiting value as $\epsilon$ gets smaller of the finite quantity.

I will call the limiting infinitesimal $dx$, as in "the difference between successive allowed values of x". It is important not to read this as "d times x", but as a rounder version of $\Delta A$, which is not $\Delta$ times $A$, but $\Delta$ of $A$. Then the derivative can be calculated from the finite differences:

$$ { d x^2 \over dx} = 2x + dx = 2x $$

Where I have thrown away the infinitesimal term. Likewise the analog of $x^{(k)}$ is $$ x^(k) = x(x-dx)(x-2dx)...(x-ndx) = x^k $$

So that

$$ {d\over dx} x^k = k x^{k-1} $$

Further,

$$ {d\over dx} {1\over x} = - {1\over x^2}$$

Since the small lattice analog of ${1\over x(x+1)}$ is $1\over x(x+dx)$.

The derivative of a function f is also called f'. There is a notion of a second derivative, derived from the second difference--- it is the derivative of the derivative. On a lattice:

$$f''(x) = { f(x+\epsilon) - 2f(x) + f(x-\epsilon)\over \epsilon^2}$$

In the limit as $\epsilon$ goes to zero. This is the formula for the second difference, but now divided by $\epsilon^2$ as required from the typical way the second difference vanishes. The difference vanishes as the first power of $\epsilon$, and if you were to divide out by $\epsilon$, you would get something constant, and the difference of this thing vanishes as $\epsilon$. So the second difference goes to zero as the second power of $\epsilon$.

You can define third derivatives, and so on. A physicist generally has to be familiar with these discrete forms of the second derivative, since there are many cases, like atomic lattices in a solid, where there is a real, actual $\epsilon$, and you are only dealing with an approximate continuum. It is likely that every notion of spatial continuum is related to a limiting quantity which in our universe is large, but finite.

The properties of calculus of finite differences translate to derivatives very simply:

  • {d\over dx}(f+g) = f' + g'
  • {d\over dx} (fg) = f'g + fg'

Anyway, going to infinitesimal calculus gives you a few new things: 1. The formulas simplify somewhat, since you are only interested in asymptotics. 2. The derivative gives a meaning to the notion of "how far do you go in an infinitesimal amount of time", and this defines the notion of velocity at a given time. 3. The derivative obeys the chain rule.

The chain rule is a rule for composite functions, f(g(x)). In the discrete case, you couldn't do anything regarding this, because there is no relation between f(g(n+1)) and f(g(n)) that is simple regarding f and g, since the steps g takes might be large. You can write this as

$$ f(g(n+1)) = f(g(n) + \Delta g) $$

but now you are stuck, since $\Delta g$ is not necessarily an integer.

But for infinitesimal lattices, $\Delta g$ is still infinitesimal, and this problem vanishes. We know that $\Delta g$ is small, so

$$f(g(x+\epsilon)) = f(g(x) + g'(x)\epsilon) = f(g(x)) + f'(g(x))g'(x)\epsilon$$,

so you learn the derivative of composite functions. From this, you learn

$$ {1\over x^n} = - {1\over (x^n)^2} n x^{n-1} = -{n\over x^{n+1}}$$

This derivative fits the same pattern as positive powers, except plugging in a negative number in the exponent. From the chain rule, you have the following theorem. If f(x) and g(x) are inverse functions, then:

$$ f(g(x)) = x$$

Differentiating both sides:

$$ f'(g(x))g'(x) =1 $$

so the derivative of the inverse function g is determined by the derivative of f at the location of g:

$$ g'(x) = {1\over f'(g(x))}$$

Using this formula for $f(x) = x^2$, you learn that

$$ {d\over dx} \sqrt{x} = {1\over 2\sqrt{x}}$$

again, the same pattern $k x^{k-1}$, except now with half-integer powers! You can now prove this in general by using inverse functions for 1/n and continuity.

The summation theorem becomes more breathtaking:

$$ \int_a^b f'(x) dx = f(b) - f(a) $$

Where the integral simply means the sum of all values of f on the lattice, multiplied by the lattice spacing.

$$ \int f(x) dx = \sum_x f(x) \epsilon $$

Where the sum is over x in the interval a,b in steps of $\epsilon$ beginning at a. This has the interpretation on the graph of f as the area under the curve of f.

Further, for a general function, you expect that if

$$f(0) = g(0)$$ $$f'(0) = g'(0)$$ $$f''(0)=g''(0)$$

and so on, you will have f(x)=g(x). This is not true, but it is true for a class of functions of high importance, which are called "analytic functions". The analytic functions obey the analog of the Gregory series:

$$ f(x) = f(0) + f'(0)x + f''(0) {x^2\over 2} + f'''(0) { x^3\over 3!} ... $$

Which is usually called a Taylor series, but was already known to Newton and contemporaries (who were familiar with Gregory series already).

So you see that the calculus is simply a method of defining a limiting calculation method for finite differences where all the arbitrariness and ugliness of the finite differences go away. It is essential for motion, because it tells you what "velocity" means at any one time. It is essential for physics, because it describes how quantities change continuously, the same way that the finite difference business describes how quantities change discretely.

For a good book, I would recommend Lang's calculus, although it is good to learn everything that appears in every book (there isn't that much).

share|improve this answer
add comment

There isn't a simple answer to your question. The sort of basic calculus you need to understand the equations of motion isn't especially hard maths, but it takes a while to get comfortable with it. Your profile says you're 16, so I'd guess that if you do Physics and Maths at school you'll soon be learning calculus. In the UK you learn it as part of your A-level course, which is from age 16 to 18.

If you want to have a go now, I'd say find a reasonably friendly book on calculus. I would look for a book aimed at physicists as maths books on calculus tend to have a somewhat different emphasis. I can't recommend a book because it's 35 years (!!) since I started learning calculus and I've long since forgotten which books I used. I had a quick scan through the preview of "The Complete Idiot's Guide to Calculus" on amazon.com and that seemed reasonably friendly. I'd get a copy of that and see how you get on. Be warned though, it isn't something you're going to learn in an afternoon.

"Cycles of Time" is a slightly odd book as it can't decide if it's a popular science book along the lines of "A Brief History of Time" or a proper scientific book. I think it's managed to be neither. Despite what Penrose may have told you, understanding everything in the book is likely to be way beyond you even after you've mastered basic calculus.

share|improve this answer
    
Thanks, why would he publish a book that's way beyond most Physicists? –  Olly Price May 22 '12 at 17:58
    
It's not way beyond most physicists - the high reputation guys hereabouts would consider it light reading! However parts of it are way beyond 16 year olds just starting to learn calculus. How far have you got with it? You could probably get a lot out of it knowing no calculus at all. –  John Rennie May 22 '12 at 18:01
    
Oh yeah I understand the basic concept of the whole idea and everything (although it took quite some time as you can imagine) because there's only calculus in the Appendix as a reference, but yeah, when I've done my Physics degrees, have strong knowledge of calculus and am just generally more intelligent I'll be sure to read it again to gain really deep knowledge of the idea. –  Olly Price May 22 '12 at 18:04
    
(I didn't realise by you saying "after you've mastered basic calculus" you meant if I was to study it now, my mistake). –  Olly Price May 22 '12 at 18:05
    
do you think that Khan Academy would be a good online 'place' for me to take a course in calculus? khanacademy.org/math/calculus –  Olly Price May 22 '12 at 19:24
show 3 more comments

Perhaps the simplest and most grandiose way of describing calculus is: 'the mathematical study of change'. In practice, and simply, this general means integrals and derivates of functions.

If a given function corresponds to some value of interest $f$ which is a function of a parameter $x$, then the derivative of that function describes the change of $f$ with respect to (e.g.) $x$. If instead, $f$ represents itself some amount of change, then the integral of $f$ describes the total amount of change.

Without calculus, you can only consider each level independently.... i.e. you can consider the quantity, or you can consider the change in that quantity, but you cannot relate the two.

For example, velocity is the change-in (derivative of) position. Or alternately, the position is the accumulated difference (integral) of the velocity. Relating position to velocity requires calculus. For instance, the fundamental equation 'velocity equals distance over time' ($v=d/t$) is a result of calculus---althought it is certainly simple enough to arrive at it by reasoning alone.

Understanding the connection between a quantity and the change in that quantity underlies the fundamental dynamic nature of physics. All velocities are changes in position. All forces can be described as resulting from differences in potentials; which then produce accelerations which are changes in velocity. Calculus provides the tools to quantitatively analyze these relationships.

share|improve this answer
add comment

Very briefly... I'm following the advice of others here by presenting a short list of the resources I hunted for a couple of questions back!

  • Fairly light and significantly incomplete, constantly update, though:

Wikibook on Calculus

  • A bit disconnected between lessons but fairly thorough and the videos are marvelous!

MIT OpenCourseWare

  • Basically, a near approximation of your upcoming two-year curricula in Math with all the calculus usually there:

Siyavula Grades 10-12 Math Books | The Free Learning for All Project

That's not all... But that was all I could find in my bookmarks right now. Others would do a better job than me in recommending professional, commercial books.

share|improve this answer
add comment

Your Answer

 
discard

By posting your answer, you agree to the privacy policy and terms of service.

Not the answer you're looking for? Browse other questions tagged or ask your own question.