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Math 132. Sigma Notation. Stewart §4.1, Part 2. Notation for sums. In Notes §4.1, we define the integral ∫ b a f(x)dx as a limit of approximations. That is ...
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Notation for sums. In Notes §4.1, we define the integral
∫ (^) b a f^ (x)^ dx^ as a limit of approximations. That is, we split the interval x ∈ [a, b] into n increments of size ∆x = b−n a, we choose sample points x 1 , x 2 ,... , xn, and we take:
∫ (^) b
a
f (x) dx = lim ∆x→ 0
f (x 1 )∆x + f (x 2 )∆x + · · · + f (xn)∆x.
The sum which appears on the right is called a Riemann sum. Similar sums appear frequently in mathematics, and we define a special notation to handle them. In the most general situation, we have a sequence of numbers q 0 , q 1 , q 2 , q 3 ,... so that for any i = 0, 1 , 2 ,... we have a number qi. We consider an interval of integers i = m, m+1, m+2,... , n, and we introduce a notation for the sum of all the qi for i = m to n:
∑^ n
i=m
qi = qm + qm+1 + qm+2 + · · · + qn.
The summation symbol Σ is capital sigma, the Greek letter S, standing for “sum”. The variable i is called the index of summation. Note: In the WebWork problems, a sequence is denoted f (i) instead of qi. This is because we can consider the sequence of qi’s as a function with input i (an integer) and output qi (a specified number).
Examples
i, we have q 0 = 0, q 1 = 1, q 2 =
2, q 3 =
3, etc., and taking the interval of integers i = 2, 3 , 4 , 5, we have:
∑^5
i=
i =
i=1 1 = 1 + 1 +︸ ︷︷^ · · · + 1︸ 10 terms
i=
i^2.
i=
(2i−1).
Notes by Peter Magyar [email protected]
Another way would be to consider the terms as qi = 2i+1:
i=
(2i+1).
1 + 3 + 5 + · · · + (2n−1) =
∑^ n
i=
(2i−1).
f (x 1 )∆x + f (x 2 )∆x + · · · + f (xn)∆x =
∑^ n
i=
f (xi)∆x.
Summation Rules. As for limits and derivatives, we can sometimes compute summations by starting with known Basic Summations, and combining them by Summation Rules.
∑^ n
i=m
(qi+pi) =
∑^ n
i=m
qi +
∑^ n
i=m
pi.
∑^ n
i=m
(qi−pi) =
∑^ n
i=m
qi −
∑^ n
i=m
pi.
∑^ n
i=m
C qi = C ·
∑^ n
i=m
qi , where C does not depend on i.
Like all facts about summations, these formulas can be understood by writing out the terms in dot-dot-dot (ellipsis) notation:
∑^ n
i=m
(qi+pi) = (qm+pm) + (qm+1+pm+1) + · · · + (qn+pn)
= (qm + qm+1 + · · · + qn) + (pm + pm+1 + · · · + pn)
∑^ n
i=m
qi +
∑^ n
i=m
pi.
Similarly for the other two rules. Note that n is a constant not depending on i, so we may factor it out of a summation:
∑n i=1 ni
(^2) = n ∑n i=1 i
(^2). This gives a separate formula for each n: for
n = 3 it means 3(1^2 )+3(2^2 )+3(3^2 ) = 3(1^2 +2^2 +3^2 ). However, the variable i has no meaning outside the summation, and cannot be factored out:
i=1 i^2
i (^) =?? i ∑^3 i=1 2
i
is nonsense, because the left side means 1(2^1 ) + 2(2^2 ) + 3(2^3 ), but the right side would mean some constant “i” times 2^1 +2^2 +2^3 , but i is not a constant. Warning: the summation of a product
qipi is NOT equal to the product of summations (
qi)(
pi). For example: 1 · 1 + 2 · 2 + 3 · 3 6 = (1+2+3)(1+2+3).
Direct Evaluation of Integrals. We can use the above rules to simplify Rie- mann sums and find integrals exactly. For example, consider:
∫ (^3)
1
5 x dx = lim ∆x→ 0
∑^ n
i=
5 xi ∆x.
On the right side, we divide the interval [1, 3] into n increments of length ∆x = 3 − 1 n =^
2 n , with dividing points:
1 < 1+∆x < 1+2∆x < 1+3∆x < · · · < 1+n∆x = 3.
In the ith^ increment, we arbitrarily choose the sample point xi to be the right endpoint, that is xi = 1 + i ∆x = 1 + (^2) n i. Thus:
∑^ n
i=
5 xi ∆x =
∑^ n
i=
n
i
n
n
∑^ n
i=
n^2
∑^ n
i=
i
n
· n +
n^2
n(n+1)
n
(Here n is a fixed number not depending on i, such as n = 100 or n = 1000, and we can factor it out of the
.) Finally, we let ∆x → 0 or equivalently n → ∞: ∫ (^3)
1
5 x dx = lim ∆x→ 0
∑^ n
i=
5 xi ∆x = (^) nlim→∞ 20 +
n
We computed this to show in principle that Riemann sums can be evaluated directly, but this is far from the easiest way to compute an integral. Geometrically, the integral equals the trapezoid area below the graph y = 5x and above the interval [1, 3] on the x-axis. Since (trapezoid area) = (width)×(average height),
we get that the integral is A = (3−1)( 5(1)+5(3) 2 ) = 20.
Physically, if v(t) = 5t is a velocity, then the integral
1 v(t)^ dt^ is the distance traveled from t = 1 to t = 3. Since the position s(t) is an antiderivative, we must have s(t) = 52 t^2 + C, so the distance traveled is s(3) − s(1) = 52 (3^2 ) − 52 (1^2 ) = 20.