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© ABCC Australia 2015 new-physics.com
IN CAME EULER
PM [B010]
© ABCC Australia 2015 new-physics.com
Leonhard Euler
The French mathematician
Leonhard Euler (1707-1783) was
fascinated by the similarity of these
last three formulas.
He ingeniously solved the problem
by introducing the imaginary
number 𝑖𝑖 in the equations.
He had worked it out in a way
different from what we are doing
now. It was more analytic and
harder to work out.
Neither did he leave an equation
exactly the same as we have now.
But the credit of finding the solution
was accredited to him.
© ABCC Australia 2015 new-physics.com
Expansion of 𝑒𝑒𝑖𝑖𝑥𝑥
By the Maclaurin method, the vector 𝑒𝑒𝑖𝑖𝑥𝑥
can also be expanded into a similar infinite
series:
𝑒𝑒 𝑥𝑥
= 1 + 𝑥𝑥 +
𝑥𝑥2
2!
+
𝑥𝑥3
3!
+
𝑥𝑥4
4!
+
𝑥𝑥5
5!
+
𝑥𝑥6
6!
+
𝑥𝑥7
7!
+ · · ·
𝑒𝑒𝑖𝑖𝑥𝑥
= 1 + 𝑖𝑖𝑖𝑖 −
𝑥𝑥2
2!
−
𝑖𝑖𝑥𝑥3
3!
−
𝑥𝑥4
4!
+
𝑖𝑖𝑥𝑥5
5!
−
𝑥𝑥6
6!
− 𝑖𝑖
𝑥𝑥7
7!
+ · · ·
𝑒𝑒 𝑥𝑥
→ 𝑒𝑒𝑖𝑖𝑥𝑥
© ABCC Australia 2015 new-physics.com
Shuffling the Terms
Rearranging the terms into two groups:
𝑒𝑒𝑖𝑖𝑖𝑖
= 1 + 𝑖𝑖𝑖𝑖 −
𝑥𝑥2
2!
−
𝑖𝑖𝑥𝑥3
3!
−
𝑥𝑥4
4!
+
𝑖𝑖𝑥𝑥5
5!
−
𝑥𝑥6
6!
− 𝑖𝑖
𝑥𝑥7
7!
+ · · ·
𝑒𝑒𝑖𝑖𝑖𝑖
= 1 −
𝑥𝑥2
2!
−
𝑥𝑥4
4!
−
𝑥𝑥6
6!
+ · · · + 𝑖𝑖 𝑥𝑥 −
𝑥𝑥3
3!
+
𝑥𝑥5
5!
−
𝑥𝑥7
7!
+ · · ·
© ABCC Australia 2015 new-physics.com
The 𝑖𝑖 does it
Compare this:
𝑒𝑒𝑖𝑖 𝑖𝑖
= 1 −
𝑥𝑥2
2!
−
𝑥𝑥4
4!
−
𝑥𝑥6
6!
+ · · · + 𝑖𝑖 𝑥𝑥 −
𝑥𝑥3
3!
+
𝑥𝑥5
5!
−
𝑥𝑥7
7!
+ · · ·
With the cosine and sine equations again:
𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 = 1 −
𝑥𝑥2
2!
+
𝑥𝑥4
4!
−
𝑥𝑥6
6!
+ · · ·
𝑖𝑖 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 𝑖𝑖 𝑥𝑥 −
𝑥𝑥3
3!
+
𝑥𝑥5
5!
−
𝑥𝑥7
7!
+ · · ·
It is not hard to see that:
𝑒𝑒𝑖𝑖𝑖𝑖 = 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 + 𝑖𝑖 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥
© ABCC Australia 2015 new-physics.com
𝒙𝒙 → 𝜽𝜽
Now, it’s time for the medusa to
come in. She connects the linear
world with the circular universe
but in a slightly different way
from the centaur. She links up
the arc with the radius:
𝜃𝜃 =
𝑠𝑠
𝑟𝑟
She is a hybrid and easily slip
into the equation which
becomes:
𝑒𝑒𝑖𝑖 𝜃𝜃 = 𝑐𝑐𝑐𝑐𝑐𝑐 𝜃𝜃 + 𝑖𝑖 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃
𝜃𝜃
© ABCC Australia 2015 new-physics.com
Where is the Centaur?
But this is not the famous Euler
equation - it is only the origin of the
Euler equation.
When the vector rotates to the
other side of the real axis, that is, to
where −1 is, the angle becomes 𝜋𝜋
(in radian measure).
𝑒𝑒𝑖𝑖 𝜋𝜋
= 𝑐𝑐𝑐𝑐𝑐𝑐 𝜋𝜋 + 𝑖𝑖 sin 𝜋𝜋
= −1 + 0
= −1
𝑒𝑒𝑖𝑖 𝜋𝜋 + 1 = 0
Reputed to be the most ‘beautiful’
equation in science and
mathematics.
𝑂𝑂
𝐴𝐴
𝜃𝜃 = 𝜋𝜋
𝜋𝜋
© ABCC Australia 2015 new-physics.com
The Beauty of Equation
Now, maybe you’ve never
thought of math equations
as “beautiful,” but look at
that result:
It combines the five most
fundamental numbers in
math − 0, 1, e, 𝑖𝑖, and 𝜋𝜋 −
𝑖𝑖𝑖𝑖 a relation of irreducible
simplicity.
Lee Simmons@actual_self
𝜋𝜋
𝑖𝑖
𝑒𝑒
𝜃𝜃
© ABCC Australia 2015 new-physics.com
The beautiful Equation
Even more astonishing if you slog
through the proof, which involves
infinite sums, factorials, and
fractions nested within fractions
within fractions like matryoshka
dolls. And remember, e and 𝜋𝜋 are
infinitely long decimals with
seemingly nothing in common;
they’re the ultimate jigsaw puzzle
pieces. Yet they fit together
perfectly—not to a few places, or a
hundred, or a million, but all the way
to forever.
Lee Simmons@actual_self
𝑒𝑒𝑖𝑖 𝜋𝜋
© ABCC Australia 2015 new-physics.com
The Most Beautiful Equation
But the weirdest thing about Euler’s
formula—given that it relies on
imaginary numbers—is that it’s so
immensely useful in the real world.
By translating one type of motion
into another, it lets engineers convert
messy trigonometric problems into
more tractable algebra—like a
wormhole between separate
branches of math.
It’s the secret sauce in Fourier
transforms used to digitize music,
and it tames all manner of wavy
things in quantum mechanics,
electronics, and signal processing;
without it, computers might not
exist. Lee Simmons@actual_self
𝑒𝑒𝑖𝑖 𝜃𝜃
© ABCC Australia 2015 new-physics.com
To be continued on PM [011]
ABCC

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PM [B10] In comes Euler

  • 1. © ABCC Australia 2015 new-physics.com IN CAME EULER PM [B010]
  • 2. © ABCC Australia 2015 new-physics.com Leonhard Euler The French mathematician Leonhard Euler (1707-1783) was fascinated by the similarity of these last three formulas. He ingeniously solved the problem by introducing the imaginary number 𝑖𝑖 in the equations. He had worked it out in a way different from what we are doing now. It was more analytic and harder to work out. Neither did he leave an equation exactly the same as we have now. But the credit of finding the solution was accredited to him.
  • 3. © ABCC Australia 2015 new-physics.com Expansion of 𝑒𝑒𝑖𝑖𝑥𝑥 By the Maclaurin method, the vector 𝑒𝑒𝑖𝑖𝑥𝑥 can also be expanded into a similar infinite series: 𝑒𝑒 𝑥𝑥 = 1 + 𝑥𝑥 + 𝑥𝑥2 2! + 𝑥𝑥3 3! + 𝑥𝑥4 4! + 𝑥𝑥5 5! + 𝑥𝑥6 6! + 𝑥𝑥7 7! + · · · 𝑒𝑒𝑖𝑖𝑥𝑥 = 1 + 𝑖𝑖𝑖𝑖 − 𝑥𝑥2 2! − 𝑖𝑖𝑥𝑥3 3! − 𝑥𝑥4 4! + 𝑖𝑖𝑥𝑥5 5! − 𝑥𝑥6 6! − 𝑖𝑖 𝑥𝑥7 7! + · · · 𝑒𝑒 𝑥𝑥 → 𝑒𝑒𝑖𝑖𝑥𝑥
  • 4. © ABCC Australia 2015 new-physics.com Shuffling the Terms Rearranging the terms into two groups: 𝑒𝑒𝑖𝑖𝑖𝑖 = 1 + 𝑖𝑖𝑖𝑖 − 𝑥𝑥2 2! − 𝑖𝑖𝑥𝑥3 3! − 𝑥𝑥4 4! + 𝑖𝑖𝑥𝑥5 5! − 𝑥𝑥6 6! − 𝑖𝑖 𝑥𝑥7 7! + · · · 𝑒𝑒𝑖𝑖𝑖𝑖 = 1 − 𝑥𝑥2 2! − 𝑥𝑥4 4! − 𝑥𝑥6 6! + · · · + 𝑖𝑖 𝑥𝑥 − 𝑥𝑥3 3! + 𝑥𝑥5 5! − 𝑥𝑥7 7! + · · ·
  • 5. © ABCC Australia 2015 new-physics.com The 𝑖𝑖 does it Compare this: 𝑒𝑒𝑖𝑖 𝑖𝑖 = 1 − 𝑥𝑥2 2! − 𝑥𝑥4 4! − 𝑥𝑥6 6! + · · · + 𝑖𝑖 𝑥𝑥 − 𝑥𝑥3 3! + 𝑥𝑥5 5! − 𝑥𝑥7 7! + · · · With the cosine and sine equations again: 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 = 1 − 𝑥𝑥2 2! + 𝑥𝑥4 4! − 𝑥𝑥6 6! + · · · 𝑖𝑖 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 𝑖𝑖 𝑥𝑥 − 𝑥𝑥3 3! + 𝑥𝑥5 5! − 𝑥𝑥7 7! + · · · It is not hard to see that: 𝑒𝑒𝑖𝑖𝑖𝑖 = 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 + 𝑖𝑖 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥
  • 6. © ABCC Australia 2015 new-physics.com 𝒙𝒙 → 𝜽𝜽 Now, it’s time for the medusa to come in. She connects the linear world with the circular universe but in a slightly different way from the centaur. She links up the arc with the radius: 𝜃𝜃 = 𝑠𝑠 𝑟𝑟 She is a hybrid and easily slip into the equation which becomes: 𝑒𝑒𝑖𝑖 𝜃𝜃 = 𝑐𝑐𝑐𝑐𝑐𝑐 𝜃𝜃 + 𝑖𝑖 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 𝜃𝜃
  • 7. © ABCC Australia 2015 new-physics.com Where is the Centaur? But this is not the famous Euler equation - it is only the origin of the Euler equation. When the vector rotates to the other side of the real axis, that is, to where −1 is, the angle becomes 𝜋𝜋 (in radian measure). 𝑒𝑒𝑖𝑖 𝜋𝜋 = 𝑐𝑐𝑐𝑐𝑐𝑐 𝜋𝜋 + 𝑖𝑖 sin 𝜋𝜋 = −1 + 0 = −1 𝑒𝑒𝑖𝑖 𝜋𝜋 + 1 = 0 Reputed to be the most ‘beautiful’ equation in science and mathematics. 𝑂𝑂 𝐴𝐴 𝜃𝜃 = 𝜋𝜋 𝜋𝜋
  • 8. © ABCC Australia 2015 new-physics.com The Beauty of Equation Now, maybe you’ve never thought of math equations as “beautiful,” but look at that result: It combines the five most fundamental numbers in math − 0, 1, e, 𝑖𝑖, and 𝜋𝜋 − 𝑖𝑖𝑖𝑖 a relation of irreducible simplicity. Lee Simmons@actual_self 𝜋𝜋 𝑖𝑖 𝑒𝑒 𝜃𝜃
  • 9. © ABCC Australia 2015 new-physics.com The beautiful Equation Even more astonishing if you slog through the proof, which involves infinite sums, factorials, and fractions nested within fractions within fractions like matryoshka dolls. And remember, e and 𝜋𝜋 are infinitely long decimals with seemingly nothing in common; they’re the ultimate jigsaw puzzle pieces. Yet they fit together perfectly—not to a few places, or a hundred, or a million, but all the way to forever. Lee Simmons@actual_self 𝑒𝑒𝑖𝑖 𝜋𝜋
  • 10. © ABCC Australia 2015 new-physics.com The Most Beautiful Equation But the weirdest thing about Euler’s formula—given that it relies on imaginary numbers—is that it’s so immensely useful in the real world. By translating one type of motion into another, it lets engineers convert messy trigonometric problems into more tractable algebra—like a wormhole between separate branches of math. It’s the secret sauce in Fourier transforms used to digitize music, and it tames all manner of wavy things in quantum mechanics, electronics, and signal processing; without it, computers might not exist. Lee Simmons@actual_self 𝑒𝑒𝑖𝑖 𝜃𝜃
  • 11. © ABCC Australia 2015 new-physics.com To be continued on PM [011] ABCC