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Complex and Trigonometric Identities

The shortest path between two truths in the real domain passes through the complex domain. Jacques Hadamard Simplicity in linearity

• In , we know that the states: • a(b + c) = ab + ac • But why is this even true to begin with? • Here is a visual proof where we can think of the real values representing the lengths of rectangles and their products the area of their associated rectangles.

• Even the proof for natural numbers takes effort. • Since is just + + + , repeated times. Then by using the : + = + = + + + 𝑚𝑚 ⋅ 𝑛𝑛 𝑛𝑛 𝑛𝑛 ⋯ 𝑛𝑛 𝑚𝑚 ( + + + )+ ( + + 𝑎𝑎 𝑏𝑏+ )𝑐𝑐= 𝑏𝑏 +𝑐𝑐 𝑎𝑎 =𝑎𝑎 𝑎𝑎+ ⋯ 𝑎𝑎 𝑏𝑏+𝑐𝑐 𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡 𝑎𝑎 𝑎𝑎 ⋯ 𝑎𝑎 𝑎𝑎 𝑎𝑎 ⋯ 𝑎𝑎 𝑏𝑏 ⋅ 𝑎𝑎 𝑐𝑐 ⋅ 𝑎𝑎 𝑎𝑎𝑎𝑎 𝑏𝑏𝑏𝑏 https://math.stackexchange.com/questions/786066/prove𝑏𝑏 𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡 𝑐𝑐 𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡𝑡 -the-distributive-law-abc-abac-for-real-numbers Simplicity in linearity Its definitively ALIVE!!!

• Previous show how you will see in 1 how the of two functions does behave linearly. • What other mathematical objects have this nice linear property? • Lets take another result from calc 1, the definite Simplicity in Linearity

• Linearity property of the definite integral As expected…

Lets go beyond calculus, and go into theory. Expect to see this in a statistics class (Math 120).

The expected value of a random , intuitively, is the long-run average value of repetitions of the experiment it represents.

Discrete case:

[ ] = 𝑘𝑘 = + + + ( )

𝐸𝐸 𝑋𝑋 � 𝑥𝑥𝑖𝑖𝑝𝑝 𝑥𝑥𝑖𝑖 𝑥𝑥1𝑝𝑝 𝑥𝑥1 𝑥𝑥2𝑝𝑝 𝑥𝑥2 ⋯ 𝑥𝑥𝑘𝑘𝑝𝑝 𝑥𝑥𝑘𝑘 𝑖𝑖=1 Continuous case:

= ( )

𝐸𝐸 𝑋𝑋 � 𝑥𝑥𝑥𝑥 𝑥𝑥 𝑑𝑑𝑑𝑑 ℝ As expected… a proof

• For discrete random variables X and Y. By the basic definition of expected value,

• Note that we have never used any properties of independence in this proof, and thus linearity of expectation holds for all random variables! • For continuous random variables, the proof is essentially the same except that the are replaced by . https://brilliant.org/wiki/linearity-of-expectation/ Linear Transformations https://en.wikipedia.org/wiki/Linear_map http://mathworld.wolfram.com/LinearTransformation.html

• A Linear Transformation (or linear map) is a special type of where: . F(u + v) = F(u) + F(v) and . F(cv) = cF(v) for a /scalar c.

These functions are extensively studied in (Math 200) and get their name by always mapping a into a line.

The function f: The function is additive: It doesn't The function is homogeneous: It with f(x,y)=(2x,y) is2 a linear2 matter whether first vectors are doesn't matter whether a vector is map. This functionℝ scales→ ℝ added and then mapped or whether first scaled and then mapped or the x component of a vector by they are mapped and finally added: first mapped and then the factor 2. f(u+v)=f(u)+f(v) scaled: f(cv)=cf(v) Is everything linear?

• Can we apply this procedure universally, just because its easy? • Lets consider a “freshman sum“ from math students, when requested to add fractions • + = Right!! 2 3 5 • 7In reality5 12 this “mistake” leads us to interesting area and study of numbers called the Mediant + = . 𝑎𝑎 𝑐𝑐 𝑎𝑎+𝑐𝑐 • IF we do allow this new interesting𝑏𝑏 𝑑𝑑 relationships𝑏𝑏+𝑑𝑑 can occur

https://www.nctm.org/Publications/Mathematics-Teacher/2016/Vol110/Issue1/mt2016-08-18a/ .https://en.wikipedia.org/wiki/Mediant_(mathematics) More on mediant

• Not todays topic, but want to entice your math curiosity, look at: • Farey sequences

https://en.wikipedia.org/wiki/Farey_sequence

• Stern-Brocot tree

https://en.wikipedia.org/wiki/Stern%E2%80%93Brocot_tree Fundamental Tragedy of algebra • That sinister bug has raised his head, • And like a germ he is starting to spread. • + + Distributing exponents is the sign, 2 2 2 • • 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • That this bug is on the climb. • + + • Look at that student over there, • 2 2 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • Distributing exponents without a care. • + / + • Please listen to your maker, • 2 2 1 2 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • Distributing exponents will bring the undertaker. • + + • Dear Lord please open your gates. −1 −1 −1 • 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • Being a math student was not his fate. • + • Distributing exponents was his only sin. −1 −1 1 • 𝑎𝑎 𝑏𝑏 ≠ − 𝑎𝑎+𝑏𝑏 • But that’s enough to do an algebra student in. • + + • An example, his demise should serve, 3 • 3 3 • For other students who haven’t heard, 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • + + • Distributing exponents is a sin. • 3 3 3 • It’s enough to do an algebra student in. 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • + + • • 4 4 4 • Donald E. Brook 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 • + + • Mt. San Antonio College 2 𝑎𝑎 𝑏𝑏 ≠ 𝑎𝑎 𝑏𝑏 Fundamental Tragedy of linearity

• Linear breakdowns in other areas of mathematics: . Algebra: logb(x) + logb(y) ≠ logb(x + y) y . Recall logb x=y ↔b =x . Correct logb(x) + logb(y) = logb(xy), Proof:

A B A B A+B . Let b =x and b =y, then logb(xy)=logb(b b )=logb(b )=A+B= logb(x) + logb(y)

. Logic: ¬(p q)≠ ¬p ¬q, likewise ¬(p q)≠ ¬p ¬q

p q ∧ p q ∧¬(p q) ¬p ¬q ¬p ¬q∨ ∨ p q p q ¬(p q) ¬p ¬q ¬p ¬q F F ∧F T∧ ∧T ∨T F F F∧ T ∨ T ∨ T ∧ F T F T F T F T F F T F T F F T F T T F F F T F T T T F F F T T T F F F

. Rather by DeMorgans law ¬(p q)= ¬p ¬q likewise ¬(p q)= ¬p ¬q

∧ ∨ ∨ ∧ Fundamental Tragedy of linearity

• Linear breakdowns in other areas of mathematics: . Sets: ( ) likewise ( )

. Rather𝐴𝐴 by∩ DeMorgans𝐵𝐵 ′ ≠ 𝐴𝐴� ∩ 𝐵𝐵law� ( )𝐴𝐴 ∪ 𝐵𝐵 ′ ≠ 𝐴𝐴, proof� ∪ 𝐵𝐵� below. . Likewise = . Try proving this second version. ′ 𝐴𝐴 ∩ 𝐵𝐵 ′ ≠ 𝐴𝐴� ∪ 𝐵𝐵� 𝐴𝐴 ∪ 𝐵𝐵 𝐴𝐴� ∩ 𝐵𝐵� Attempt at Linearity

What should cos + and sin + be? Do these behave linearly? 𝑥𝑥 𝑦𝑦 𝑥𝑥 𝑦𝑦 Is cos + = cos + cos and sin + = sin + sin ?

Try with𝑥𝑥 some𝑦𝑦 known𝑥𝑥 values: 𝑦𝑦 𝑥𝑥 𝑦𝑦 𝑦𝑦 𝑦𝑦

cos + = cos + cos sin + = sin + sin 6 3 6 3 6 3 6 3 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 3 3 cos = cos + cos sin = sin + sin 6 6 3 6 6 3 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 𝜋𝜋 3 1 1 3 cos = + sin = + 2 2 2 2 2 2 𝜋𝜋 𝜋𝜋 0 = ? 1 = ? 1+ 3 1+ 3 2 2 So that failed… let’s try distance!

Find cos based on the unit .

𝑥𝑥 − 𝑦𝑦 So that failed… let’s try distance! Find cos based on the . Label the coordinates of each point.

𝑥𝑥 − 𝑦𝑦 (cos (x – y), sin (x – y)) (cos x, sin x) (cos y, sin y)

x y x – y (1, 0)

Figure 1 Figure 2 Find cos based on the unit circle.

Distance between𝑥𝑥 the− two𝑦𝑦 labeled points in Figure 1.

= + = 2 + + 2 2 + 𝑑𝑑 𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 − 𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 𝑠𝑠𝑖𝑖𝑖𝑖𝑥𝑥 − 𝑠𝑠𝑠𝑠𝑠𝑠𝑦𝑦 = 2 + + 2+ 2 2 𝑑𝑑 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 − 2𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 𝑐𝑐𝑐𝑐𝑐𝑐 𝑦𝑦 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 − 𝑠𝑠𝑠𝑠𝑠𝑠𝑥𝑥𝑠𝑠𝑠𝑠𝑠𝑠𝑦𝑦 𝑠𝑠𝑠𝑠𝑠𝑠 𝑦𝑦 = 1 + 12 2 2 2 𝑑𝑑 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 𝑐𝑐𝑐𝑐𝑐𝑐 𝑦𝑦 𝑠𝑠𝑠𝑠𝑠𝑠 𝑦𝑦 − 2𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 − 2𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 = 2 𝑑𝑑 − 2𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 − 2𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 = 2 2 + 𝑑𝑑 − 2𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 − 2𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 𝑑𝑑 − 𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 Keep this in mind as we move to the next part. Find cos based on the unit circle. Distance between the two labeled points in Figure 2.

= 𝑥𝑥1 −+ 𝑦𝑦 0 = 2 + 1 + 2 𝑑𝑑 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 − 𝑦𝑦 − 𝑠𝑠𝑖𝑖𝑖𝑖 𝑥𝑥 − 𝑦𝑦 − 2 2 𝑑𝑑 = 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 − 𝑦𝑦 −+2𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 − 𝑦𝑦 + 1 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 − 𝑦𝑦 2 2 𝑑𝑑 = 1𝑐𝑐𝑐𝑐𝑐𝑐+ 1 𝑥𝑥 − 𝑦𝑦 𝑠𝑠𝑠𝑠𝑠𝑠 =𝑥𝑥 − 2𝑦𝑦 − 2𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 − 𝑦𝑦

Now𝑑𝑑 compare− this2𝑐𝑐𝑐𝑐𝑐𝑐 to 𝑥𝑥the− previous𝑦𝑦 distance:− 2𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 −=𝑦𝑦 2 2 +

Since the distances must be the same, we conclude𝑑𝑑 that:− 𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 = +

Want𝒄𝒄𝒄𝒄𝒄𝒄 𝒙𝒙 − 𝒚𝒚 𝒄𝒄𝒄𝒄𝒄𝒄, then𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄 just𝒄𝒄 check𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔 the𝒔𝒔𝒔𝒔 𝒔𝒔complement ( Identity): = = = 𝑠𝑠𝑖𝑖𝑖𝑖 𝑥𝑥 − 𝑦𝑦 2 2 𝜋𝜋 𝜋𝜋 cos𝒔𝒔𝒔𝒔𝒔𝒔 𝒙𝒙 − 𝒚𝒚 cos𝑐𝑐𝑐𝑐𝑐𝑐 +−sin𝑥𝑥 − 𝑦𝑦 sin𝑐𝑐𝑐𝑐𝑐𝑐( ) =− 𝑥𝑥 − −𝑦𝑦 2 2 𝜋𝜋 𝜋𝜋 − 𝑥𝑥 −𝑦𝑦 − 𝑥𝑥 −𝑦𝑦 𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔𝒔 − 𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄𝒄 What about the other ones?

You can use a similar picture to graph , but in this case, you’ll need to think of a clockwise rotation of an , so one angle will be negative.

Summary: ± =

𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 𝑦𝑦 𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 ∓ 𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 ± = ±

𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 𝑦𝑦 𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠𝑠 𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐 Deriving sum identity using SOHCAHTOA, and without the Unit circle.

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

• Consider the small right in the figure above, which gives

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

• Now, the usual trigonometric definitions applied to the large give

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

• Solving these two simultaneously for the variables sin(α+β) and cos(α +β) then immediately gives

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Deriving sum identity using SOHCAHTOA, and without the Unit circle.

• These can be put into the familiar forms with the aid of the trigonometric identities

• which can be verified by direct . • Plugging these back to the equations in the previous slide gives:

http://mathworld.wolfram.com/TrigonometricAdditionFormulas.html Other pictures My eyes hurt

• Is there another way, that does not involve the unit circle with distance formula or ‘weird’ pictures.

• Is there a way that doesn’t require long , memorizing or remembering some picture, or remembering some method to create a picture that would work?

• Lets enter an imaginary word of opportunities. [1707-1783]

• Euler is considered the most prolific mathematician in history. (What about Erdős?) • His contemporaries called him “analysis incarnate.” • “He calculated without effort, just as men breathe or as eagles sustain themselves in the air.”

The Saga of Mathematics: A Brief History http://math.widulski.net/ 33 Leonhard Euler [1707-1783]

•Euler was born in Basel, Switzerland, on April 15, 1707. •He received his first schooling from his father Paul, a Calvinist minister, who had studied mathematics under Jacob Bernoulli. •Euler's father wanted his son to follow in his footsteps and, in 1720 at the age of 14, sent him to the University of Basel to prepare for the ministry.

The Saga of Mathematics: A Brief History http://math.widulski.net/ 34 Leonhard Euler [1707-1783]

• At the age of 15, he received his Bachelor’s . • In 1723 at the age of 16, Euler completed his Master's degree in philosophy having compared and contrasted the philosophical ideas of Descartes and Newton. • His father demanded he study theology and he did, but eventually through the persuading of Johann Bernoulli, Jacob’s brother, Euler switched to mathematics.

The Saga of Mathematics: A Brief History http://math.widulski.net/ 35 Leonhard Euler [1707-1783]

• Euler completed his studies at the University of Basel in 1726. • He had studied many mathematical works including those by Varignon, Descartes, Newton, Galileo, von Schooten, Jacob Bernoulli, Hermann, Taylor and Wallis. • By 1727, he had already published a couple of articles on isochronous and submitted an entry for the 1727 Grand Prize of the French Academy on the optimum placement of masts on a ship.

The Saga of Mathematics: A Brief History http://math.widulski.net/ 36 Leonhard Euler [1707-1783]

• Euler did not win but instead received an honorable mention. • He eventually would recoup from this loss by winning the prize 12 times. • What is interesting is that Euler had never been on a ship having come from landlocked Switzerland. • The strength of his work was in the analysis.

The Saga of Mathematics: A Brief History http://math.widulski.net/ 37 Leonhard Euler [1707-1783]

• Euler was in a sense the creator of modern mathematical expression. • In terms of , Euler was the person who gave us: • π for •i for √−1 •∆y for the change in y •f(x) for a function • Σ for

The Saga of Mathematics: A Brief History http://math.widulski.net/ 38 Leonhard Euler [1707-1783]

• To get an idea of the of Euler’s work it is worth noting that: • Euler wrote more than 500 books and papers during his lifetime – about 800 pages per year. • After Euler’s death, it took over forty years for the backlog of his work to appear in print. • Approximately 400 more publications.

The Saga of Mathematics: A Brief History http://math.widulski.net/ 39 Leonhard Euler [1707-1783]

• He published so many mathematics articles that his collected works Opera Omnia already fill 73 large volumes – tens of thousands of pages – with more volumes still to come. • More than half of the volumes of Opera Omnia deal with applications of mathematics – acoustics, engineering, mechanics, astronomy, and optical devices (telescopes and microscopes).

The Saga of Mathematics: A Brief History http://math.widulski.net/ 40 The number e and compound interest

“Compound interest is the most • Invest $1 = 1 + powerful force in the universe.” 𝑛𝑛𝑡𝑡 • Interest rate 100% 𝑟𝑟 Albert Einstein. 𝐴𝐴 𝑃𝑃 𝑛𝑛 Interest applied each Sum at end of the year

Year $2.00000

Half-year $2.25000

Quarter $2.44141

Month $2.61304

Week $2.69260

Day $2.71457

Hour $2.71813

Minute $2.71828

Second $2.71828 What about ‘continuous’ compounding? The number e as a limit

1 = lim 1 + 𝑛𝑛 = 2.7182818284590452353602874...

𝑒𝑒 𝑛𝑛→∞ So for continuous compounding,𝑛𝑛 let x=n/r we would get 1 1 = lim 1 + = lim 1 + = lim 1 + 𝑟𝑟𝑟𝑟 = 𝑛𝑛𝑡𝑡 𝑥𝑥𝑥𝑥𝑡𝑡 𝑥𝑥 𝑟𝑟 𝑟𝑟𝑟𝑟 𝐴𝐴 𝑛𝑛→∞ 𝑃𝑃 𝑃𝑃 ⋅ 𝑥𝑥→∞ 𝑃𝑃 𝑥𝑥→∞ 𝑃𝑃𝑒𝑒 https://en.wikipedia.org/wiki/E_(mathematical_constant)𝑛𝑛 𝑥𝑥 𝑥𝑥 Euler on complex numbers

Of such numbers we may truly assert that they are neither nothing, nor greater than nothing, nor less than nothing, which necessarily constitutes them imaginary or impossible. Complex Numbers William Rowan Hamilton 1805 - 1865

We define a as a pair (a, b) of real numbers.

https://www.quantamagazine.org/the-imaginary-numbers-at-the-edge-of-reality-20181025/ http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials Complex Numbers William Rowan Hamilton 1805 - 1865

We define a complex number as a pair (a, b) of real numbers.

They are added as follows: (a, b) + (c, d) = (a + c, b + d);

(1, 2) + (3, 4) = (4, 6)

https://www.quantamagazine.org/the-imaginary-numbers-at-the-edge-of-reality-20181025/ http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials Complex Numbers William Rowan Hamilton 1805 - 1865

We define a complex number as a pair (a, b) of real numbers.

They are added as follows: (a, b) + (c, d) = (a + c, b + d);

They are multiplied as follows: (a, b) x (c, d) = (ac - bd, ad + bc);

(1, 2) × (3, 4) = (3 – 8, 4 + 6) = (-5, 10)

https://www.quantamagazine.org/the-imaginary-numbers-at-the-edge-of-reality-20181025/ http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials Complex Numbers William Rowan Hamilton 1805 - 1865

We define a complex number as a pair (a, b) of real numbers.

They are added as follows: (a, b) + (c, d) = (a + c, b + d);

They are multiplied as follows: (a, b) x (c, d) = (ac - bd, ad + bc);

The pair (a, 0) then corresponds to the a

the pair (0, 1) corresponds to the i

https://www.quantamagazine.org/the-imaginary-numbers-at-the-edge-of-reality-20181025/ http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials Complex Numbers William Rowan Hamilton 1805 - 1865

We define a complex number as a pair (a, b) of real numbers.

They are added as follows: (a, b) + (c, d) = (a + c, b + d);

They are multiplied as follows: (a, b) x (c, d) = (ac - bd, ad + bc);

The pair (a, 0) then corresponds to the real number a

the pair (0, 1) corresponds to the imaginary number i

Then (0, 1) x (0, 1) = (-1, 0), which corresponds to the relation i x i = i 2= - 1. Representing Complex numbers geometrically Caspar Wessel in 1799 In this representation, called the complex , two axes are drawn at right – the real axis and the imaginary axis – and the complex number a + b 1 is represented by the point at a distance a in the direction− of the real axis and at height b in the direction of the imaginary axis.

https://en.wikipedia.org/wiki/Complex_number https://www.quantamagazine.org/the-octonion-math-that-could-underpin-physics-20180720/ Complicated Extensions

https://www.quantamagazine.org/the-imaginary-numbers-at-the-edge-of-reality-20181025/ https://en.wikipedia.org/wiki/Quaternion https://en.wikipedia.org/wiki/Octonion Powers of the complex expression (1+iπ/n)n

• We can approximate numerically these complex powers without evaluating trigonometric functions

https://www.desmos.com/calculator/qtqlhrazd4

The ez can be defined as the limit of (1 + z/n)n, as n approaches , and thus eiπ is the limit of (1 + iπ/n)n. In this animation n takes various increasing values from 1 to 100. The computation of (1 + iπ/n)n is displayed as the combined effect of n repeated in the , with the final point being the actual value of (1 + iπ/n)n. As n gets larger (1 + iπ/n)n approaches a limit of −1.

https://www.youtube.com/watch?v=-dhHrg-KbJ0 http://demonstrations.wolfram.com/ComplexPowerPlot/ This animation depicts points moving along the graphs of the function (in blue) and the cosine function (in green) corresponding to a point moving around the unit circle

Source: http://www2.seminolestate.edu/lvosbury/AnimationsForTrigonometry.htm = cos + sin 𝑖𝑖𝑖𝑖 Three𝑒𝑒 -dimensional𝑥𝑥 visualization𝑖𝑖 𝑥𝑥of Euler's formula. See also circular polarization.

https://betterexplained.com/articles/intuitive- understanding-of-eulers-formula/ Tailor made for math

Borrowing results from calculus we can find the Taylor expansions for the transcendental functions: cos = 1 - + - + - + + ⋅⋅⋅ 2! 4! 6! 8! 10! 12! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 2 4 6 8 10 12 sin = - + - + - + + ⋅⋅⋅ 3! 5! 7! 9! 11! 13! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 3 5 7 9 11 13 The exponential =1 + + + + + + + + + ⋅⋅⋅ x 2! 3! 4! 5! 6! 7! 8! function e (in blue), 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 and the sum of the 𝑒𝑒 𝑥𝑥 2 3 4 5 6 7 8 first n + 1 terms of its at 0 (in is measured in red). https://www.desmos.com/calculator/8ksvin4rua 𝑥𝑥 https://en.wikipedia.org/wiki/Taylor_series = cos + sin 𝑖𝑖𝑖𝑖 cos𝑒𝑒 = 1 - 𝑥𝑥+ 𝑖𝑖- +𝑥𝑥 - + + ⋅⋅⋅ 2! 4! 6! 8! 10! 12! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 2 4 6 8 10 12 sin = - + - + - + + ⋅⋅⋅ 3! 5! 7! 9! 11! 13! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑖𝑖 𝑥𝑥 𝑖𝑖𝑥𝑥 𝑖𝑖 3 𝑖𝑖 5 𝑖𝑖 7 𝑖𝑖 9 𝑖𝑖 11 𝑖𝑖 13

http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials = cos + sin 𝑖𝑖𝑖𝑖 cos𝑒𝑒 = 1 - 𝑥𝑥+ 𝑖𝑖- +𝑥𝑥 - + + ⋅⋅⋅ 2! 4! 6! 8! 10! 12! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 2 4 6 8 10 12 sin = - + - + - + + ⋅⋅⋅ 3! 5! 7! 9! 11! 13! Add to get 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑖𝑖 𝑥𝑥 𝑖𝑖𝑥𝑥 𝑖𝑖 3 𝑖𝑖 5 𝑖𝑖 7 𝑖𝑖 9 𝑖𝑖 11 𝑖𝑖 13 1 + - - + + - - + + ⋅⋅⋅ 2! 3! 4! 5! 6! 7! 8! 9! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑖𝑖𝑥𝑥 2 𝑖𝑖 3 4 𝑖𝑖 5 6 𝑖𝑖 7 8 𝑖𝑖 9

http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials = cos + sin 𝑖𝑖𝑖𝑖 cos𝑒𝑒 = 1 - 𝑥𝑥+ 𝑖𝑖- +𝑥𝑥 - + + ⋅⋅⋅ 2! 4! 6! 8! 10! 12! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 2 4 6 8 10 12 sin = - + - + - + + ⋅⋅⋅ 3! 5! 7! 9! 11! 13! Add to get 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑖𝑖 𝑥𝑥 𝑖𝑖𝑥𝑥 𝑖𝑖 3 𝑖𝑖 5 𝑖𝑖 7 𝑖𝑖 9 𝑖𝑖 11 𝑖𝑖 13 1 + - - + + - - + + ⋅⋅⋅ 2! 3! 4! 5! 6! 7! 8! 9! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 Lets compare it with 𝑖𝑖𝑥𝑥 2 𝑖𝑖 3 4 𝑖𝑖 5 6 𝑖𝑖 7 8 𝑖𝑖 9 ( ) ( ) ( ) ( ) ( ) ( ) = 1+ + + + + + + + ⋅⋅⋅ ! ! 2 ! 3 ! 4 ! 5 ! 6 ! 7 𝑖𝑖𝑥𝑥 𝑖𝑖𝑥𝑥 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑒𝑒 1 2 3 4 5 6 7

http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials = cos + sin 𝑖𝑖𝑖𝑖 𝑒𝑒 𝑥𝑥 Note:𝑖𝑖 𝑥𝑥2 = -1 3 = - 4 = 1 𝑖𝑖 𝑖𝑖5 = 𝑖𝑖and so on Add to get 𝑖𝑖 1 + - - +𝑖𝑖 +𝑖𝑖 - - + + ⋅⋅⋅ 2! 3! 4! 5! 6! 7! 8! 9! which is𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑖𝑖𝑥𝑥 2 𝑖𝑖 3 4 𝑖𝑖 5 6 𝑖𝑖 7 8 𝑖𝑖 9 ( ) ( ) ( ) ( ) ( ) ( ) = 1+ + + + + + + + ⋅⋅⋅ ! ! 2 ! 3 ! 4 ! 5 ! 6 ! 7 𝑖𝑖𝑥𝑥 𝑖𝑖𝑥𝑥 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 1 2 3 4 5 6 7 𝑒𝑒 http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials Euler’s formula in Introductio, 1748

From which it can be worked out in what way the exponentials of imaginary quantities can be reduced to the and cosines of real arcs

http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials = cos + sin 𝑖𝑖𝑖𝑖 Now𝑒𝑒 that we have the𝑥𝑥 basics,𝑖𝑖 let’s𝑥𝑥 check how it works: = cos + sin = + • 𝜋𝜋 . 𝑖𝑖 3 𝜋𝜋 𝜋𝜋 1 3 • 𝑒𝑒This corresponds3 to𝑖𝑖 the point3 2 , 2 𝑖𝑖on the unit circle. 1 3 2 2 Now if we equal to π π = cos π+ sin π 𝑥𝑥 and use cos π = -1 and sin π = 0 giving𝑖𝑖 𝑒𝑒 𝑖𝑖

= -1 𝑖𝑖πor 𝑒𝑒 + 1 = 0 http://www.gresham.ac.uk/lectures𝒊𝒊𝝅𝝅 -and-events/eulers-exponentials 𝒆𝒆 + 1 = 0

This𝑖𝑖𝜋𝜋 links five of the most important constants in mathematics: 𝑒𝑒 • 0 is the additive identity, which when added to any number leaves the number unchanged

• 1 is the multiplicative identity, which multiplied by any number leaves the number unchanged

• e of the exponential function which we have defined before and base of the natural

• which is the ratio of a circle’s circumference to its diameter

• i𝜋𝜋is the , which is the root of -1

, an incredibly famous physicist, claimed this was the jewel of mathematics. Some have written that because of the innate beauty and simplicity of this , that Euler used it as a proof that god must exist. = cos + sin 𝑖𝑖𝑖𝑖 Futher unexpected results: if we raise the imaginary unit to itself as a power, the answer𝑒𝑒 is a REAL number𝑥𝑥 𝑖𝑖 . 𝑥𝑥

Set equal to π/2 and use cos π/2 = 0 and sin π/2 = 1 Then raise both sides to the power of i. 𝑥𝑥 = ( ( / )) = / = / = 𝑖𝑖 𝑖𝑖 𝜋𝜋 2 𝑖𝑖 𝑖𝑖∗𝑖𝑖𝜋𝜋 2 −𝜋𝜋 2 𝑖𝑖 𝑒𝑒 𝑒𝑒 𝑒𝑒 / = =0.207879576350… 𝜋𝜋 −1 2 1 𝜋𝜋 𝑒𝑒 𝑒𝑒 https://www.youtube.com/watch?v=9tlHQOKMHGA

http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials = cos + sin 𝑖𝑖𝑖𝑖 𝑒𝑒 𝑥𝑥 𝑖𝑖 𝑥𝑥

Set equal to π/2 and use cos π/2 = 0 and sin π/2 = 1 Then raise both sides to the power of i. 𝑥𝑥 = =0.207879576350… 𝑖𝑖 1 “… we have not the slightest idea of what𝜋𝜋 this equation means , but we may be 𝑖𝑖 𝑒𝑒 certain that it means something very important” Benjamin Peirce

http://www.gresham.ac.uk/lectures-and-events/eulers-exponentials Why is this formula so powerful?

= cos + + sin + (1) 𝑖𝑖 𝑥𝑥+𝑦𝑦 𝑒𝑒 = 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑥𝑥+𝑦𝑦 𝑖𝑖𝑥𝑥 𝑖𝑖𝑖𝑖 𝑒𝑒 = 𝑒𝑒cos𝑒𝑒 + sin cos + sin 𝑖𝑖 𝑥𝑥+𝑦𝑦 𝑒𝑒 𝑥𝑥 𝑖𝑖 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑦𝑦 = cos cos + sin cos + sin cos + sin sin 𝑖𝑖 𝑥𝑥+𝑦𝑦 2 𝑒𝑒 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑦𝑦 𝑥𝑥 𝑖𝑖 𝑥𝑥 𝑦𝑦

= cos cos + sin cos + sin cos sin sin 𝑖𝑖 𝑥𝑥+𝑦𝑦 𝑒𝑒 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑦𝑦 𝑥𝑥 − 𝑥𝑥 𝑦𝑦 = cos cos sin sin + sin cos + sin cos (2) 𝑖𝑖 𝑥𝑥+𝑦𝑦 𝑒𝑒 𝑥𝑥 𝑦𝑦 − 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑥𝑥 𝑦𝑦 𝑦𝑦 𝑥𝑥 At this point, we will need to equate the real parts and the imaginary parts of the two equations. Why is this formula so powerful?

= cos + + sin + 𝑖𝑖 𝑥𝑥+𝑦𝑦 = cos cos 𝑒𝑒 sin sin𝑥𝑥 𝑦𝑦+ 𝑖𝑖sin 𝑥𝑥cos 𝑦𝑦 + sin cos 𝑖𝑖 𝑥𝑥+𝑦𝑦 𝑒𝑒 𝑥𝑥 𝑦𝑦 − 𝑥𝑥 𝑦𝑦 𝑖𝑖 𝑥𝑥 𝑦𝑦 𝑦𝑦 𝑥𝑥

Once you do this, you can see two identities with just one quick expansion of the distributive property: • Red (Real): cos + = cos cos sin sin • Green (Imaginary): sin + = sin cos + sin cos 𝑥𝑥 𝑦𝑦 𝑥𝑥 𝑦𝑦 − 𝑥𝑥 𝑦𝑦 𝑥𝑥 𝑦𝑦 𝑥𝑥 𝑦𝑦 𝑦𝑦 𝑥𝑥 You could continue doing this with as well; no pictures needed, and very little algebra. As a bonus, the derivation𝑖𝑖 𝑥𝑥− 𝑦𝑦is extremely quick, and you get two formulas each time! 𝑒𝑒 Why is this formula so powerful?

What about other identities? Maybe Even/Odd? = cos + sin 1 1 𝑖𝑖 −𝑥𝑥 = = = 𝑒𝑒 −𝑥𝑥 𝑖𝑖 cos−𝑥𝑥 + sin 𝑖𝑖 −𝑥𝑥 −𝑖𝑖𝑖𝑖 𝑒𝑒Multiply by𝑒𝑒 the complex𝑖𝑖𝑖𝑖 conjugate. 1 𝑒𝑒 cos 𝑥𝑥 sin𝑖𝑖 𝑥𝑥 cos + sin cos sin 𝑥𝑥 − 𝑖𝑖 𝑥𝑥 = = cos + sin 𝑥𝑥 𝑖𝑖 𝑥𝑥 𝑥𝑥 − 𝑖𝑖 𝑥𝑥 cos 𝑥𝑥 −𝑖𝑖 sin 𝑥𝑥 2 2 cos 𝑥𝑥 + sin 𝑥𝑥 𝑥𝑥 𝑖𝑖 − 𝑥𝑥 So this means that cos = cos and sin = sin

−𝑥𝑥 𝑥𝑥 −𝑥𝑥 − 𝑥𝑥 No pictures… just a little algebra! Application to Trigonometric Identities

What about other identities?

= cos 2 + sin 2 𝑖𝑖�𝑖𝑖 On𝑒𝑒 the other𝜃𝜃hand𝑖𝑖 , 𝜃𝜃 = = cos + sin =𝑖𝑖�cos𝑖𝑖 𝑖𝑖𝑖𝑖 sin2 + 2 cos sin 2 𝑒𝑒 2 𝑒𝑒 2 𝜃𝜃 𝑖𝑖 𝜃𝜃 Equating𝜃𝜃 −real and𝜃𝜃 imaginary𝑖𝑖 𝜃𝜃 parts𝜃𝜃 of the two expressions yield identities:

𝑡𝑡ℎ𝑒𝑒 𝑑𝑑𝑑𝑑𝑑𝑑𝑑𝑑𝑑𝑑𝑑𝑑 𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎𝑎 cos 2 = cos sin sin 2 = 2 cos2 sin 2 𝜃𝜃 𝜃𝜃 − 𝜃𝜃 𝜃𝜃 𝜃𝜃 𝜃𝜃

69 Application to Trigonometric Identities (cont.)

In general, = cos + sin = = cos + sin 𝑖𝑖𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝑛𝑛 𝑛𝑛 , 𝑒𝑒 𝑛𝑛 𝜃𝜃 𝑖𝑖 𝑛𝑛 𝜃𝜃 𝑒𝑒 𝜃𝜃 𝑖𝑖 𝜃𝜃 Expand using . then equate real and imaginary parts to obtain new identities = cos + sin 𝑖𝑖𝑖𝑖 = cos sin 𝑒𝑒−𝑖𝑖𝑖𝑖 𝑧𝑧 𝑖𝑖+ 𝑧𝑧 cos = , sin = 𝑒𝑒 𝑧𝑧𝑖𝑖𝑖𝑖− 2𝑖𝑖 −𝑖𝑖𝑧𝑧𝑖𝑖 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 𝑒𝑒 𝑒𝑒 𝑒𝑒 − 𝑒𝑒 ⇒ 𝑧𝑧 𝑧𝑧 2𝑖𝑖 + cos = = cosh , sin = = sinh 𝑧𝑧 2 −𝑧𝑧 𝑧𝑧 −𝑧𝑧 𝑒𝑒 𝑒𝑒 𝑒𝑒 − 𝑒𝑒 ⇒ 𝑖𝑖𝑖𝑖 𝑧𝑧 𝑖𝑖𝑖𝑖 − 𝑖𝑖 𝑧𝑧 Connecting them to the hyperbolic cosine and hyperbolic2𝑖𝑖 sine https://en.wikipedia.org/wiki/Hyperbolic_function 70 DeMoivre’s Theorem

= = = cos + sin = 𝑛𝑛 𝑖𝑖𝑖𝑖 𝑛𝑛 𝑛𝑛 𝑖𝑖𝑖𝑖𝑖𝑖 𝑛𝑛 𝑛𝑛 𝑧𝑧 𝑟𝑟𝑒𝑒 𝑟𝑟 𝑒𝑒 𝑟𝑟 𝑛𝑛 𝜃𝜃 𝑖𝑖 𝑛𝑛 𝜃𝜃 𝑟𝑟 ∠𝑛𝑛𝑛𝑛

y z z θ

x θπ+ 2 k θπ− 2 k

https://en.wikipedia.org/wiki/De_Moivre%27s_formula 71 Roots of a Complex Number

= = = cos + sin = ( Theorem) 𝑛𝑛 𝑖𝑖𝑖𝑖 𝑛𝑛 𝑛𝑛 𝑖𝑖𝑖𝑖𝑖𝑖 𝑛𝑛 𝑛𝑛 𝑧𝑧Applies𝑟𝑟𝑒𝑒also for 𝑟𝑟 not𝑒𝑒 an 𝑟𝑟 , but𝑛𝑛 𝜃𝜃 in𝑖𝑖this𝑛𝑛case𝜃𝜃 , the𝑟𝑟 result∠𝑛𝑛𝑛𝑛 DeMoivre′s

Example: 𝑛𝑛th root of a complex number:

𝑛𝑛

72 Roots of a Complex Number (cont.)

/ / y = = v 1 3 1 3 z 𝑤𝑤 𝑧𝑧 = +−8𝑖𝑖 w

𝑤𝑤 𝑢𝑢 𝑖𝑖𝑖𝑖 3 , x u = , 1 3 3− 𝑖𝑖 −8i −8𝑖𝑖 � 2𝑖𝑖 − − 𝑖𝑖 Im Note that the th root of can also be expressed in terms 1∠° 120

𝑛𝑛 𝑧𝑧 10∠° Re

Cube root 1∠° 240 of unity

73 Could we do more?

Heck yes! We could use this to find the sum to product formulas, but they require the ability to remember a substitution in the middle of the problem. These types of substitutions do come up in calculus, but we’ll leave them off for now.

What kind of substitutions?

When you look at , you probably don’t immediately think = + 0.

𝑥𝑥 𝑥𝑥 𝑥𝑥 Further, you probably don’t think + 0 = + , right? 𝑦𝑦 𝑦𝑦 𝑥𝑥 𝑥𝑥 2 − 2 Oh, and once you do think about these, do you immediately think: + = + + = + + = + .  𝑦𝑦 𝑦𝑦 𝑥𝑥 𝑥𝑥 𝑦𝑦 𝑦𝑦 𝑥𝑥 𝑦𝑦 𝑥𝑥 𝑦𝑦 𝑥𝑥+𝑦𝑦 𝑥𝑥−𝑦𝑦 𝑥𝑥 2 − 2 2 2 2 − 2 2 2 2 − 2 2 2 Well, those are the types of substitutions needed for the sum-to-product formulas. Why use it?

Euler’s formula is a tool you can use, but don’t have to. Like many things in math, it is extremely useful at times and not as useful in other situations.

Try it out. As you get comfortable with it, you may find some very interesting results! Bonus, this opens up a whole new world. Indeed, if = 1, which we confirmed that it did on an earlier slide, then we could𝑖𝑖𝜋𝜋 rewrite this using logarithms: = 1 1 = 𝑒𝑒 − 𝑖𝑖𝜋𝜋 𝑒𝑒 − ↔ 𝑙𝑙𝑙𝑙 − 𝑖𝑖𝑖𝑖 So logarithms could be defined over negative and even complex numbers if we allowed complex number outputs. Test this on your calculator in complex mode to see the result. Back when covering logarithms, the domain was restricted to all non-negative real numbers… but that was needed to get the result to be a real number. Expanding our definition/domain will allow us to do MORE, not less. Now, go explore for yourselves!

https://math.stackexchange.com/questions/2089690/log-of-a-negative-number https://en.wikipedia.org/wiki/Complex_logarithm How Important are the Addition Formulas?

Back in the 1950s, Professor Hans Rademacher* showed that all of could be developed with just two functions that he called “C” and “S” where:

1. = + 2. = 𝐶𝐶 𝑥𝑥 − 𝑦𝑦 𝐶𝐶 𝑥𝑥 𝐶𝐶 𝑦𝑦 𝑆𝑆 𝑥𝑥 𝑆𝑆 𝑦𝑦 3. lim = 1 𝑆𝑆 𝑥𝑥 −𝑆𝑆 𝑦𝑦𝑥𝑥 𝑆𝑆 𝑥𝑥 𝐶𝐶 𝑦𝑦 − 𝑆𝑆 𝑥𝑥 𝐶𝐶 𝑦𝑦 + 𝑥𝑥→0 𝑥𝑥 Those of you who have taken calculus may recognize (3) as one of the most important limits in calculus, necessary for the formulation of trigonometric . *Mathematics Teacher Vol L (January 1957) pp. 45-48. Calc link (power reduction)

+ 1 = 2 2 𝑐𝑐𝑐𝑐𝑐𝑐 2𝑥𝑥 � 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 𝑑𝑑𝑑𝑑 � 𝑑𝑑𝑑𝑑 = cos + sin 𝑖𝑖𝑖𝑖 = cos sin 𝑒𝑒−𝑖𝑖𝑖𝑖 𝑥𝑥 𝑖𝑖 𝑥𝑥 So + = 2cos which means cos = 𝑒𝑒 𝑥𝑥 − 𝑖𝑖 𝑥𝑥 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 𝑒𝑒 +𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑥𝑥 𝑥𝑥 2 This means = = = = 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 2 𝑖𝑖�𝑖𝑖 −𝑖𝑖�𝑖𝑖 2 𝑒𝑒 +𝑒𝑒 𝑒𝑒 +2+𝑒𝑒 2𝑐𝑐𝑐𝑐𝑐𝑐 2𝑥𝑥 +2 𝑐𝑐𝑐𝑐𝑐𝑐 2𝑥𝑥 +1 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 2 4 4 2 Calc link (power reduction)

Expanding the technique from the previous page, we can even do something like this:

+ + + 20 = 64 6 2𝑐𝑐𝑐𝑐𝑐𝑐 6𝑥𝑥 12𝑐𝑐𝑐𝑐𝑐𝑐 4𝑥𝑥 30𝑐𝑐𝑐𝑐𝑐𝑐 2𝑥𝑥 It helps to� 𝑐𝑐𝑐𝑐𝑐𝑐remember𝑥𝑥 𝑑𝑑𝑑𝑑 Pascal’s� triangle: 𝑑𝑑𝑑𝑑

1 1 1 1 2 1 1 3 3 1 1 4 6 4 1 1 5 10 10 5 1 1 6 15 20 15 6 1 Calc link (power reduction) cos = , which means + = 2cos . 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 𝑒𝑒 +𝑒𝑒 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 𝑥𝑥 2 𝑒𝑒 𝑒𝑒 𝑥𝑥 + + cos = = 𝑖𝑖𝑖𝑖 2 −𝑖𝑖𝑖𝑖 6 𝑖𝑖𝑖𝑖 2 −𝑖𝑖𝑖𝑖 6 6 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑥𝑥 6 Using Pascal’s Triangle for coefficients: + = + 6 + 15 + 20 +15 + + 6 6 5 4 2 3 3 2 4 5 6 𝑎𝑎 𝑏𝑏 𝑎𝑎 𝑎𝑎 𝑏𝑏 𝑎𝑎 𝑏𝑏 𝑎𝑎 𝑏𝑏 𝑎𝑎 𝑏𝑏 6𝑎𝑎𝑏𝑏 𝑏𝑏 Expanding the binomial: + = + 6 + 15 + 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 206 𝑖𝑖𝑖𝑖 6 +𝑖𝑖𝑖𝑖155 −𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖+ 64 −𝑖𝑖𝑖𝑖 2 + 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑖𝑖𝑖𝑖 3 −𝑖𝑖𝑖𝑖 3 𝑖𝑖𝑖𝑖 2 −𝑖𝑖𝑖𝑖 4 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 5 −𝑖𝑖𝑖𝑖 6 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 Simplifying exponents: + = + 6 + 15 + 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 6 20𝑖𝑖6𝑥𝑥 𝑖𝑖5𝑥𝑥 +−𝑖𝑖𝑖𝑖15 𝑖𝑖4𝑥𝑥 −+𝑖𝑖26𝑥𝑥 + 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑖𝑖3𝑥𝑥 𝑒𝑒−𝑖𝑖3𝑥𝑥 𝑒𝑒 𝑖𝑖2𝑥𝑥 𝑒𝑒−𝑖𝑖4𝑥𝑥𝑒𝑒 𝑖𝑖𝑖𝑖 −𝑖𝑖5𝑥𝑥 −𝑖𝑖6𝑥𝑥 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 Calc link (power reduction) Simplifying exponents: + = + + 6 + 6 + 15 + 15 + 20 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 6 𝑖𝑖6𝑥𝑥 −𝑖𝑖6𝑥𝑥 𝑖𝑖4𝑥𝑥 −𝑖𝑖4𝑥𝑥 𝑖𝑖2𝑥𝑥 −𝑖𝑖2𝑥𝑥 𝑖𝑖0𝑥𝑥 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 Grouping like objects: + = + + 6 + + 15 + 15 + 20 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 6 𝑖𝑖6𝑥𝑥 −𝑖𝑖6𝑥𝑥 𝑖𝑖4𝑥𝑥 −𝑖𝑖4𝑥𝑥 𝑖𝑖2𝑥𝑥 −𝑖𝑖2𝑥𝑥 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 𝑒𝑒 Euler’s formula then substitutes since + = 2cos : + = + 6 𝑖𝑖𝑖𝑖+ 15 −𝑖𝑖𝑖𝑖 2 + 20 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 6 𝑒𝑒 𝑒𝑒 𝑥𝑥 𝑒𝑒 𝑒𝑒 2𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐� 2𝑐𝑐𝑐𝑐𝑐𝑐𝑐𝑐� 2𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 This shows why = . 6 2𝑐𝑐𝑐𝑐𝑐𝑐 6𝑥𝑥 +12𝑐𝑐𝑐𝑐𝑐𝑐 4𝑥𝑥 +30𝑐𝑐𝑐𝑐𝑐𝑐 2𝑥𝑥 +20 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 64 And now you can do the integration in calculus II much quicker:

+ + + 20 = 64 6 2𝑐𝑐𝑐𝑐𝑐𝑐 6𝑥𝑥 12𝑐𝑐𝑐𝑐𝑐𝑐 4𝑥𝑥 30𝑐𝑐𝑐𝑐𝑐𝑐 2𝑥𝑥 � 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 𝑑𝑑𝑑𝑑 � 𝑑𝑑𝑑𝑑 Lets raise the roof!

Recall:

= 1 + + + + = ∞ 22! 33! 𝑛𝑛! 𝑥𝑥 𝑥𝑥 𝑥𝑥 𝑥𝑥 Define𝑒𝑒 extension𝑥𝑥 to complex⋯ variable� ( = + ): 𝑛𝑛=0 𝑛𝑛

1 + + + + = ∞ (converges𝑥𝑥 → 𝑧𝑧 𝑥𝑥for all𝑖𝑖𝑖𝑖 ) 22! 33! 𝑛𝑛! 𝑧𝑧 𝑧𝑧 𝑧𝑧 𝑧𝑧 𝑒𝑒 ≡ 𝑧𝑧 ⋯ � 𝑧𝑧 𝑛𝑛=0 𝑛𝑛 = ∞ = 1 + + + ! 𝑛𝑛 22! 44! 33! 55! 𝑖𝑖𝑖𝑖 𝑖𝑖𝑖𝑖 𝜃𝜃 𝜃𝜃 𝜃𝜃 𝜃𝜃 ⇒= cos𝑒𝑒 +�sin − − ⋯ 𝑖𝑖 𝜃𝜃 − − ⋯ 𝑛𝑛=0 𝑛𝑛 = cos + sin = cos sin 𝜃𝜃 𝑖𝑖 𝜃𝜃 𝑖𝑖𝑖𝑖 −𝑖𝑖𝑖𝑖 ⇒ 𝑒𝑒 𝜃𝜃 𝑖𝑖 𝜃𝜃 𝑒𝑒 𝜃𝜃 − 𝑖𝑖 𝜃𝜃

http://mathworld.wolfram.com/ComplexExponentiation.html https://brilliant.org/wiki/complex-exponentiation/ 81 Further connections

In Calculus 2 (Math 141) you will see Taylor and McLaurin series. Used to confirm Euler’s formula = cos + sin . 𝑖𝑖𝑖𝑖 𝑒𝑒 𝑥𝑥 𝑖𝑖 𝑥𝑥 In Discrete Math (Math 245) you can prove that the previous formulas are true for all values of n, using formal mathematical induction.

Calc I and II (Math 140 and 141) often must substitute in power reduction formulas for powers of trigonometric functions.

http://spikedmath.com/297.html