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© ABCC Australia 2015 new-physics.com
THE TRIGO COMPANIONS
PM [B09]
© ABCC Australia 2015 new-physics.com
The ordinary vector
Let us come back to the oldie
vector to review what we have
started with.
It is the nice and simple vector
𝑶𝑶𝑶𝑶 in the common Cartesian
coordinates making an angle 𝜃𝜃
with the 𝑥𝑥-axis.
Here angular measure is used.
𝑂𝑂
𝐴𝐴
𝑥𝑥
𝜃𝜃
𝜋𝜋
2
=90°
𝑃𝑃
𝑦𝑦
𝑀𝑀
For the time
being, this is true
angular measure,
not radian
measure.
© ABCC Australia 2015 new-physics.com
Vector Components
This vector will generates two
projections, one on the 𝑥𝑥-axis as
OP and the other on the 𝑦𝑦-axis
as OM.
Projectors
𝑂𝑂
A
𝑥𝑥
𝜃𝜃 90°
𝑃𝑃
𝑦𝑦
Projectionon𝑦𝑦-axis
Projection on 𝑥𝑥-axis
𝑀𝑀
© ABCC Australia 2015 new-physics.com
Cos 𝜽𝜽 & sin 𝜽𝜽
These projection have a relation
with the initial position 𝑶𝑶𝑶𝑶
represented by the ratio of its
projection on the original
direction to the original length:
𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅1 =
|𝑶𝑶𝑶𝑶|
|𝑶𝑶𝑶𝑶|
& 𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅2 =
|𝑨𝑨𝑷𝑷|
|𝑶𝑶𝑶𝑶|
In trigonometry these ratios are
called the cosine (cos) and sine
(sin) of the angle 𝜃𝜃:
cos 𝜃𝜃 =
𝑂𝑂𝑂𝑂
𝑂𝑂𝑂𝑂
& 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 =
𝐴𝐴𝑃𝑃
𝑂𝑂𝑂𝑂
O
A
x
θ
P
y
Projectionon𝑦𝑦-axis
Projection on 𝑥𝑥-axis
M
cos 𝜃𝜃 =
𝑂𝑂𝑂𝑂
𝑂𝑂𝑂𝑂
𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 =
𝐴𝐴𝐴𝐴
𝑂𝑂𝑂𝑂
© ABCC Australia 2015 new-physics.com
A Normal Vector
In the normal Cartesian
coordinate systems, the vector
OA of length 𝑟𝑟 is written in
terms of its cosine and sine
components as:
𝑶𝑶𝑶𝑶 = 𝑟𝑟 𝑐𝑐𝑐𝑐𝑐𝑐 𝜃𝜃 �𝒙𝒙 + 𝑟𝑟 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 �𝒚𝒚
Where �𝒙𝒙 and �𝒚𝒚 are the unit
vectors on the 𝑥𝑥 and 𝑦𝑦 axes
respectively.
𝑂𝑂
𝐴𝐴
𝑥𝑥
𝜃𝜃
𝑃𝑃
𝑦𝑦
𝑶𝑶𝑷𝑷 = 𝑟𝑟 𝑐𝑐𝑐𝑐𝑐𝑐 𝜃𝜃
𝑀𝑀
𝑶𝑶𝑨𝑨 = 𝑟𝑟 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃
© ABCC Australia 2015 new-physics.com
POWER SERIES
Some functions of the variable 𝜃𝜃
such as cos 𝑥𝑥, ln 𝑥𝑥, √𝑥𝑥 etc., are
commonly occurring functions
and their values are found in the
familiar mathematical tables.
However unlike the other
simpler rational functions of 𝑥𝑥,
these values cannot be arrived
at by simple arithmetical
operations such as addition,
subtraction, multiplication, and
division. To obtain these values
as we see them in the tables, we
have to stretch them by using
power series.
© ABCC Australia 2015 new-physics.com
Maclaurin's series
In mathematics, a power series
is a sequence of variables in
different values of power,
generally in a properly arrange
order.
One of the power series of
relevant interest in our study is
the Maclaurin's series.
- - - - - - - -
Colin Maclaurin (1698 –1746) a
Scottish mathematician who
made important contributions to
geometry and algebra.[The
Maclaurin series, a special case
of the Taylor series, is named
after him.
© ABCC Australia 2015 new-physics.com
MACLAURIN'S SERIES
The Maclaurin's series is written as:
ƒ 𝑥𝑥 stands for the function of 𝑥𝑥.
The superscripts (′), ("), etc. stand for
the respective derivatives.
“!” stands for: 2! = 2 × 1; 5! = 5 ×
4 × 3 × 2 × 1.
ƒ(𝑥𝑥) = ƒ(0) + ƒ′(0)/1! 𝑥𝑥 + ƒ"(0)/2! 𝑥𝑥2
+ . . . . + 𝑓𝑓 𝑛𝑛
(0)/n! 𝑥𝑥 𝑛𝑛
+ . . .
© ABCC Australia 2015 new-physics.com
Maclaurin Series of sine and cosine
With the methodology of Maclaurin’s Series, the trigonometric
functions cos 𝑥𝑥 and sin 𝑥𝑥 can be expanded into the following
infinite series:
𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 = 1 −
𝑥𝑥2
2!
+
𝑥𝑥4
4!
−
𝑥𝑥6
6!
+ · · ·
𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 𝑥𝑥 −
𝑥𝑥3
3!
+
𝑥𝑥5
5!
−
𝑥𝑥7
7!
+ · · ·
3! = 3 × 2 × 1 5! = 5 × 4 × 3 × 2 × 1.
© ABCC Australia 2015 new-physics.com
Expansion of 𝑒𝑒 𝑥𝑥
Now we come back to our exponential friend 𝑒𝑒 𝑥𝑥
. It happened
that for 𝑒𝑒 raised to a variable power 𝑥𝑥 into 𝑒𝑒 𝑥𝑥
, there is also
an infinite series expression:
𝑒𝑒 𝑥𝑥
= 1 + 𝑥𝑥 +
𝑥𝑥2
2!
+
𝑥𝑥3
3!
+
𝑥𝑥4
4!
+
𝑥𝑥5
5!
+ · · ·
© ABCC Australia 2015 new-physics.com
Similarity
This is quite intriguing.
The functions of cosine and sine
are equations from the
trigonometry of right triangles.
On the other hand 𝑒𝑒 is an
exponentials that is related to
logarithms.
They are usually considered
totally separate and unrelated
areas in mathematics.
How can they be so similar in
these expressions?
Trigonometric:
𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 = 1 −
𝑥𝑥2
2!
+
𝑥𝑥4
4!
−
𝑥𝑥6
6!
+ · · ·
𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 𝑥𝑥 −
𝑥𝑥3
3!
+
𝑥𝑥5
5!
−
𝑥𝑥7
7!
+ · · ·
Exponential:
𝑒𝑒 𝑥𝑥
= 1 + 𝑥𝑥 +
𝑥𝑥2
2!
+
𝑥𝑥3
3!
+
𝑥𝑥4
4!
+
𝑥𝑥5
5!
+ · · ·
© ABCC Australia 2015 new-physics.com
More Striking Similarity
If we add the first two formulas, we get:
𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 + 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 1 + 𝑥𝑥 −
𝑥𝑥2
2!
−
𝑥𝑥3
3!
+
𝑥𝑥4
4!
+
𝑥𝑥5
5!
−
𝑥𝑥6
6!
−
𝑥𝑥7
7!
+ · · ·
Compare with the expansion of 𝑒𝑒:
𝑒𝑒 𝑥𝑥
= 1 + 𝑥𝑥 +
𝑥𝑥2
2!
+
𝑥𝑥3
3!
+
𝑥𝑥4
4!
+
𝑥𝑥5
5!
+
𝑥𝑥6
6!
+
𝑥𝑥7
7!
+ · · ·
The similarity are more pronounced.
© ABCC Australia 2015 new-physics.com
IN CAME EULER
To be continued on PM [B010]:
ABCC

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PM [B09] The Trigo Companions

  • 1. © ABCC Australia 2015 new-physics.com THE TRIGO COMPANIONS PM [B09]
  • 2. © ABCC Australia 2015 new-physics.com The ordinary vector Let us come back to the oldie vector to review what we have started with. It is the nice and simple vector 𝑶𝑶𝑶𝑶 in the common Cartesian coordinates making an angle 𝜃𝜃 with the 𝑥𝑥-axis. Here angular measure is used. 𝑂𝑂 𝐴𝐴 𝑥𝑥 𝜃𝜃 𝜋𝜋 2 =90° 𝑃𝑃 𝑦𝑦 𝑀𝑀 For the time being, this is true angular measure, not radian measure.
  • 3. © ABCC Australia 2015 new-physics.com Vector Components This vector will generates two projections, one on the 𝑥𝑥-axis as OP and the other on the 𝑦𝑦-axis as OM. Projectors 𝑂𝑂 A 𝑥𝑥 𝜃𝜃 90° 𝑃𝑃 𝑦𝑦 Projectionon𝑦𝑦-axis Projection on 𝑥𝑥-axis 𝑀𝑀
  • 4. © ABCC Australia 2015 new-physics.com Cos 𝜽𝜽 & sin 𝜽𝜽 These projection have a relation with the initial position 𝑶𝑶𝑶𝑶 represented by the ratio of its projection on the original direction to the original length: 𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅1 = |𝑶𝑶𝑶𝑶| |𝑶𝑶𝑶𝑶| & 𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅𝑅2 = |𝑨𝑨𝑷𝑷| |𝑶𝑶𝑶𝑶| In trigonometry these ratios are called the cosine (cos) and sine (sin) of the angle 𝜃𝜃: cos 𝜃𝜃 = 𝑂𝑂𝑂𝑂 𝑂𝑂𝑂𝑂 & 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 = 𝐴𝐴𝑃𝑃 𝑂𝑂𝑂𝑂 O A x θ P y Projectionon𝑦𝑦-axis Projection on 𝑥𝑥-axis M cos 𝜃𝜃 = 𝑂𝑂𝑂𝑂 𝑂𝑂𝑂𝑂 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 = 𝐴𝐴𝐴𝐴 𝑂𝑂𝑂𝑂
  • 5. © ABCC Australia 2015 new-physics.com A Normal Vector In the normal Cartesian coordinate systems, the vector OA of length 𝑟𝑟 is written in terms of its cosine and sine components as: 𝑶𝑶𝑶𝑶 = 𝑟𝑟 𝑐𝑐𝑐𝑐𝑐𝑐 𝜃𝜃 �𝒙𝒙 + 𝑟𝑟 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃 �𝒚𝒚 Where �𝒙𝒙 and �𝒚𝒚 are the unit vectors on the 𝑥𝑥 and 𝑦𝑦 axes respectively. 𝑂𝑂 𝐴𝐴 𝑥𝑥 𝜃𝜃 𝑃𝑃 𝑦𝑦 𝑶𝑶𝑷𝑷 = 𝑟𝑟 𝑐𝑐𝑐𝑐𝑐𝑐 𝜃𝜃 𝑀𝑀 𝑶𝑶𝑨𝑨 = 𝑟𝑟 𝑠𝑠𝑠𝑠𝑠𝑠 𝜃𝜃
  • 6. © ABCC Australia 2015 new-physics.com POWER SERIES Some functions of the variable 𝜃𝜃 such as cos 𝑥𝑥, ln 𝑥𝑥, √𝑥𝑥 etc., are commonly occurring functions and their values are found in the familiar mathematical tables. However unlike the other simpler rational functions of 𝑥𝑥, these values cannot be arrived at by simple arithmetical operations such as addition, subtraction, multiplication, and division. To obtain these values as we see them in the tables, we have to stretch them by using power series.
  • 7. © ABCC Australia 2015 new-physics.com Maclaurin's series In mathematics, a power series is a sequence of variables in different values of power, generally in a properly arrange order. One of the power series of relevant interest in our study is the Maclaurin's series. - - - - - - - - Colin Maclaurin (1698 –1746) a Scottish mathematician who made important contributions to geometry and algebra.[The Maclaurin series, a special case of the Taylor series, is named after him.
  • 8. © ABCC Australia 2015 new-physics.com MACLAURIN'S SERIES The Maclaurin's series is written as: ƒ 𝑥𝑥 stands for the function of 𝑥𝑥. The superscripts (′), ("), etc. stand for the respective derivatives. “!” stands for: 2! = 2 × 1; 5! = 5 × 4 × 3 × 2 × 1. ƒ(𝑥𝑥) = ƒ(0) + ƒ′(0)/1! 𝑥𝑥 + ƒ"(0)/2! 𝑥𝑥2 + . . . . + 𝑓𝑓 𝑛𝑛 (0)/n! 𝑥𝑥 𝑛𝑛 + . . .
  • 9. © ABCC Australia 2015 new-physics.com Maclaurin Series of sine and cosine With the methodology of Maclaurin’s Series, the trigonometric functions cos 𝑥𝑥 and sin 𝑥𝑥 can be expanded into the following infinite series: 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 = 1 − 𝑥𝑥2 2! + 𝑥𝑥4 4! − 𝑥𝑥6 6! + · · · 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 𝑥𝑥 − 𝑥𝑥3 3! + 𝑥𝑥5 5! − 𝑥𝑥7 7! + · · · 3! = 3 × 2 × 1 5! = 5 × 4 × 3 × 2 × 1.
  • 10. © ABCC Australia 2015 new-physics.com Expansion of 𝑒𝑒 𝑥𝑥 Now we come back to our exponential friend 𝑒𝑒 𝑥𝑥 . It happened that for 𝑒𝑒 raised to a variable power 𝑥𝑥 into 𝑒𝑒 𝑥𝑥 , there is also an infinite series expression: 𝑒𝑒 𝑥𝑥 = 1 + 𝑥𝑥 + 𝑥𝑥2 2! + 𝑥𝑥3 3! + 𝑥𝑥4 4! + 𝑥𝑥5 5! + · · ·
  • 11. © ABCC Australia 2015 new-physics.com Similarity This is quite intriguing. The functions of cosine and sine are equations from the trigonometry of right triangles. On the other hand 𝑒𝑒 is an exponentials that is related to logarithms. They are usually considered totally separate and unrelated areas in mathematics. How can they be so similar in these expressions? Trigonometric: 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 = 1 − 𝑥𝑥2 2! + 𝑥𝑥4 4! − 𝑥𝑥6 6! + · · · 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 𝑥𝑥 − 𝑥𝑥3 3! + 𝑥𝑥5 5! − 𝑥𝑥7 7! + · · · Exponential: 𝑒𝑒 𝑥𝑥 = 1 + 𝑥𝑥 + 𝑥𝑥2 2! + 𝑥𝑥3 3! + 𝑥𝑥4 4! + 𝑥𝑥5 5! + · · ·
  • 12. © ABCC Australia 2015 new-physics.com More Striking Similarity If we add the first two formulas, we get: 𝑐𝑐𝑐𝑐𝑐𝑐 𝑥𝑥 + 𝑠𝑠𝑠𝑠𝑠𝑠 𝑥𝑥 = 1 + 𝑥𝑥 − 𝑥𝑥2 2! − 𝑥𝑥3 3! + 𝑥𝑥4 4! + 𝑥𝑥5 5! − 𝑥𝑥6 6! − 𝑥𝑥7 7! + · · · Compare with the expansion of 𝑒𝑒: 𝑒𝑒 𝑥𝑥 = 1 + 𝑥𝑥 + 𝑥𝑥2 2! + 𝑥𝑥3 3! + 𝑥𝑥4 4! + 𝑥𝑥5 5! + 𝑥𝑥6 6! + 𝑥𝑥7 7! + · · · The similarity are more pronounced.
  • 13. © ABCC Australia 2015 new-physics.com IN CAME EULER To be continued on PM [B010]: ABCC