Τριγωνομετρική Ταυτότης

- Ένα είδος μαθηματικών ταυτοτήτων.

## Ετυμολογία

Η ονομασία "Τριγωνομετρική" σχετίζεται ετυμολογικά με την λέξη " Τριγωνομετρία".

## Εισαγωγή

In mathematics, trigonometric identities are equalities that involve trigonometric functions and are true for every single value of the occurring variables. Geometrically, these are identities involving certain functions of one or more angles. They are distinct from triangle identities, which are identities involving both angles and side lengths of a triangle. Only the former are covered in this article.

These identities are useful whenever expressions involving trigonometric functions need to be simplified. An important application is the integration of non-trigonometric functions: a common technique involves first using the substitution rule with a trigonometric function, and then simplifying the resulting integral with a trigonometric identity.

## Notation

### Angles

This article uses Greek letters such as alpha (α), beta (β), gamma (γ), and theta (θ) to represent angles. Several different units of angle measure are widely used, including degrees, radians, and grads:

1 full circle  = 360 degrees = 2 radians  =  400 grads.

The following table shows the conversions for some common angles:

Unless otherwise specified, all angles in this article are assumed to be in radians, though angles ending in a degree symbol (°) are in degrees.

### Trigonometric functions

The primary trigonometric functions are the sine and cosine of an angle. These are sometimes abbreviated sin(θ) and cos(θ), respectively, where θ is the angle, but the parentheses around the angle are often omitted, e.g., sin θ and cos θ.

The tangent (tan) of an angle is the ratio of the sine to the cosine:

Finally, the reciprocal functions secant (sec), cosecant (csc), and cotangent (cot) are the reciprocals of the cosine, sine, and tangent:

These definitions are sometimes referred to as ratio identities.

### Inverse functions

Πρότυπο:Main The inverse trigonometric functions are partial inverse functions for the trigonometric functions. For example, the inverse function for the sine, known as the inverse sine (sin−1) or arcsine (arcsin or asin), satisfies

and

 Function Inverse sin cos tan sec csc cot arcsin arccos arctan arcsec arccsc arccot

## Pythagorean identity

The basic relationship between the sine and the cosine is the Pythagorean trigonometric identity:

where cos2 θ means (cos(θ))2 and sin2 θ means (sin(θ))2.

This can be viewed as a version of the Pythagorean theorem, and follows from the equation x2 + y2 = 1 for the unit circle. This equation can be solved for either the sine or the cosine:

### Related identities

Dividing the Pythagorean identity through by either cos2 θ or sin2 θ yields two other identities:

Using these identities together with the ratio identities, it is possible to express any trigonometric function in terms of any other (up to a plus or minus sign):

Each trigonometric function in terms of the other five.[1]
in terms of

## Historic shorthands

The versine, coversine, haversine, and exsecant were used in navigation. For example the haversine formula was used to calculate the distance between two points on a sphere. They are rarely used today.

Name(s) Abbreviation(s) Value[2]
versed sine, versine

versed cosine, vercosine
coversed sine, coversine
coversed cosine, covercosine
half versed sine, haversine
half versed cosine, havercosine
half coversed sine, hacoversine
cohaversine
half coversed cosine, hacovercosine
cohavercosine
exterior secant, exsecant
exterior cosecant, excosecant
chord

## Symmetry, shifts, and periodicity

By examining the unit circle, the following properties of the trigonometric functions can be established.

### Symmetry

When the trigonometric functions are reflected from certain angles, the result is often one of the other trigonometric functions. This leads to the following identities:

Reflected in [3] Reflected in
(co-function identities)[4]
Reflected in

### Shifts and periodicity

By shifting the function round by certain angles, it is often possible to find different trigonometric functions that express the result more simply. Some examples of this are shown by shifting functions round by π/2, π and 2π radians. Because the periods of these functions are either π or 2π, there are cases where the new function is exactly the same as the old function without the shift.

Shift by π/2 Shift by π
Period for tan and cot[5]
Shift by 2π
Period for sin, cos, csc and sec[6]

## Angle sum and difference identities

These are also known as the addition and subtraction theorems or formulæ. They were originally established by the 10th century Persian mathematician Abū al-Wafā' Būzjānī. One method of proving these identities is to apply Euler's formula. The use of the symbols and is described in the article plus-minus sign.

Sine [7][8] [8][9] [8][10] [11] [12] [13]

### Matrix form

The sum and difference formulae for sine and cosine can be written in matrix form as:

This shows that these matrices form a representation of the rotation group in the plane (technically, the special orthogonal group SO(2)), since the composition law is fulfilled: subsequent multiplications of a vector with these two matrices yields the same result as the rotation by the sum of the angles.

### Sines and cosines of sums of infinitely many terms

In these two identities an asymmetry appears that is not seen in the case of sums of finitely many terms: in each product, there are only finitely many sine factors and cofinitely many cosine factors.

If only finitely many of the terms θi are nonzero, then only finitely many of the terms on the right side will be nonzero because sine factors will vanish, and in each term, all but finitely many of the cosine factors will be unity.

### Tangents of sums of finitely many terms

Let ek (for k ∈ {0, ..., n}) be the kth-degree elementary symmetric polynomial in the variables

for i ∈ {0, ..., n}, i.e.,

Then

the number of terms depending on n.

For example:

and so on. The general case can be proved by mathematical induction.[14]

### Secants and cosecants of sums of finitely many terms

where ek is the kth-degree elementary symmetric polynomial in the n variables xi = tan θi, i = 1, ..., n, and the number of terms in the denominator depends on n.

For example,

## Multiple-angle formulae

Tn is the nth Chebyshev polynomial [15] [16]

This function of x is called the Dirichlet kernel. This is one of Lagrange's trigonometric identities.

### Double-, triple-, and half-angle formulae

Πρότυπο:See also These can be shown by using either the sum and difference identities or the multiple-angle formulae.

Double-angle formulae[17][18]
Triple-angle formulae[15][19]
Half-angle formulae[20][21]

The fact that the triple-angle formula for sine and cosine only involves powers of a single function allows one to relate the geometric problem of a compass and straightedge construction of angle trisection to the algebraic problem of solving a cubic equation, which allows one to prove that this is in general impossible, by field theory.

A formula for computing the trigonometric identities for the third-angle exists, but it requires finding the zeroes of the cubic equation , where x is the value of the sine function at some angle and d is the known value of the sine function at the triple angle. However, the discriminant of this equation is negative, so this equation has three real roots (of which only one is the solution within the correct third-circle) but none of these solutions is reducible to a real algebraic expression, as they use intermediate complex numbers under the cube roots, (which may be expressed in terms of real-only functions only if using hyperbolic functions).

### Sine, cosine, and tangent of multiple angles

For specific multiples, these follow from the angle addition formulas, while the general formula was given by 16th century French mathematician Vieta.

In each of these two equations, the first parenthesized term is a binomial coefficient, and the final trigonometric function equals one or minus one or zero so that half the entries in each of the sums are removed. Tan  can be written in terms of tan θ using the recurrence relation:

cot  can be written in terms of cot θ using the recurrence relation:

### Chebyshev method

The Chebyshev method is a recursive algorithm for finding the nth multiple angle formula knowing the (n − 1)th and (n − 2)th formulae.[22]

The cosine for nx can be computed from the cosine of (n − 1) and (n − 2) as follows:

Similarly sin(nx) can be computed from the sines of (n − 1)x and (n − 2)x

For the tangent, we have:

where H/K = tan(n − 1)x.

### Tangent of an average

Setting either α or β to 0 gives the usual tangent half-angle formulæ.

## Power-reduction formula

Obtained by solving the second and third versions of the cosine double-angle formula.

Sine Cosine Other

and in general terms of powers of sin θ or cos θ the following is true, and can be deduced using De Moivre's formula, Euler's formula and binomial theorem.

Cosine Sine

## Product-to-sum and sum-to-product identities

The product-to-sum identities or prosthaphaeresis formulas can be proven by expanding their right-hand sides using the angle addition theorems. See beat (acoustics) for an application of the sum-to-product formulæ.

Product-to-sum[23]
Sum-to-product[24]

### Other related identities

If x, y, and z are the three angles of any triangle, or in other words

(If any of x, y, z is a right angle, one should take both sides to be ∞. This is neither +∞ nor −∞; for present purposes it makes sense to add just one point at infinity to the real line, that is approached by tan(θ) as tan(θ) either increases through positive values or decreases through negative values. This is a one-point compactification of the real line.)

### Hermite's cotangent identity

Πρότυπο:Main

Charles Hermite demonstrated the following identity.[25] Suppose a1, ..., an are complex numbers, no two of which differ by an integer multiple of π. Let

(in particular, A1,1, being an empty product, is 1). Then

The simplest non-trivial example is the case n = 2:

### Ptolemy's theorem

(The first three equalities are trivial; the fourth is the substance of this identity.) Essentially this is Ptolemy's theorem adapted to the language of modern trigonometry.

## Linear combinations

For some purposes it is important to know that any linear combination of sine waves of the same period or frequency but different phase shifts is also a sine wave with the same period or frequency, but a different phase shift. In the case of a non-zero linear combination of a sine and cosine wave[26] (which is just a sine wave with a phase shift of π/2), we have

where

or equivalently

or even

More generally, for an arbitrary phase shift, we have

where

and

For the most general case, see Phasor addition.

## Other sums of trigonometric functions

Sum of sines and cosines with arguments in arithmetic progression[27]:

For any a and b:

where atan2(y, x) is the generalization of arctan(y/x) that covers the entire circular range.

The above identity is sometimes convenient to know when thinking about the Gudermannian function, which relates the circular and hyperbolic trigonometric functions without resorting to complex numbers.

If x, y, and z are the three angles of any triangle, i.e. if x + y + z = π, then

## Certain linear fractional transformations

If ƒ(x) is given by the linear fractional transformation

and similarly

then

More tersely stated, if for all α we let ƒα be what we called ƒ above, then

If x is the slope of a line, then ƒ(x) is the slope of its rotation through an angle of −α.

## Relation to the complex exponential function

[28] (Euler's formula),
(Euler's identity),
[29]
[30]

and hence the corollary:

where .

## Infinite product formulae

For applications to special functions, the following infinite product formulae for trigonometric functions are useful:[31][32] Πρότυπο:Col-start Πρότυπο:Col-2

Πρότυπο:Col-2

Πρότυπο:Col-end

## Identities without variables

The curious identity

is a special case of an identity that contains one variable:

For example

A similar-looking identity is

Similarly:

The following is perhaps not as readily generalized to an identity containing variables (but see explanation below):

Degree measure ceases to be more felicitous than radian measure when we consider this identity with 21 in the denominators:

The factors 1, 2, 4, 5, 8, 10 may start to make the pattern clear: they are those integers less than 21/2 that are relatively prime to (or have no prime factors in common with) 21. The last several examples are corollaries of a basic fact about the irreducible cyclotomic polynomials: the cosines are the real parts of the zeroes of those polynomials; the sum of the zeroes is the Möbius function evaluated at (in the very last case above) 21; only half of the zeroes are present above. The two identities preceding this last one arise in the same fashion with 21 replaced by 10 and 15, respectively.

A lot of those curious identities stem from more general facts like the following[33]:

and

Combining these gives us

If n is an odd number (n = 2m + 1) we can make use of the symmetries to get

### Computing π

An efficient way to compute π is based on the following identity without variables, due to Machin:

or, alternatively, by using an identity of Leonhard Euler:

### A useful mnemonic for certain values of sines and cosines

For certain simple angles, the sines and cosines take the form for 0 ≤ n ≤ 4, which makes them easy to remember.

### Miscellany

With the golden ratio φ:

Also see exact trigonometric constants.

### An identity of Euclid

Euclid showed in Book XIII, Proposition 10 of his Elements that the area of the square on the side of a regular pentagon inscribed in a circle is equal to the sum of the areas of the squares on the sides of the regular hexagon and the regular decagon inscribed in the same circle. In the language of modern trigonometry, this says:

Ptolemy used this proposition to compute some angles in his table of chords.

## Calculus

In calculus the relations stated below require angles to be measured in radians; the relations would become more complicated if angles were measured in another unit such as degrees. If the trigonometric functions are defined in terms of geometry, their derivatives can be found by verifying two limits. The first is:

verified using the unit circle and squeeze theorem. The second limit is:

verified using the identity tan(x/2) = (1 − cos x)/sin x. Having established these two limits, one can use the limit definition of the derivative and the addition theorems to show that (sin x)′ = cos x and (cos x)′ = −sin x. If the sine and cosine functions are defined by their Taylor series, then the derivatives can be found by differentiating the power series term-by-term.

The rest of the trigonometric functions can be differentiated using the above identities and the rules of differentiation:[34][35][36]

The integral identities can be found in "list of integrals of trigonometric functions". Some generic forms are listed below.

### Implications

The fact that the differentiation of trigonometric functions (sine and cosine) results in linear combinations of the same two functions is of fundamental importance to many fields of mathematics, including differential equations and Fourier transforms.

## Exponential definitions

Function Inverse function[37]

## Miscellaneous

### Dirichlet kernel

The Dirichlet kernel Dn(x) is the function occurring on both sides of the next identity:

The convolution of any integrable function of period 2π with the Dirichlet kernel coincides with the function's nth-degree Fourier approximation. The same holds for any measure or generalized function.

### Weierstrass substitution

Πρότυπο:Main

If we set

then[38]

where eix = cos(x) + i sin(x), sometimes abbreviated to cis(x).

When this substitution of t for tan(x/2) is used in calculus, it follows that sin(x) is replaced by 2t/(1 + t2), cos(x) is replaced by (1 − t2)/(1 + t2) and the differential dx is replaced by (2 dt)/(1 + t2). Thereby one converts rational functions of sin(x) and cos(x) to rational functions of t in order to find their antiderivatives.

## Υποσημειώσεις

1. Abramowitz and Stegun, p. 73, 4.3.45
2. Abramowitz and Stegun, p. 78, 4.3.147
3. Abramowitz and Stegun, p. 72, 4.3.13–15
4. The Elementary Identities
5. Abramowitz and Stegun, p. 72, 4.3.9
6. Abramowitz and Stegun, p. 72, 4.3.7–8
7. Abramowitz and Stegun, p. 72, 4.3.16
8. Πρότυπο:MathWorld
9. Abramowitz and Stegun, p. 72, 4.3.17
10. Abramowitz and Stegun, p. 72, 4.3.18
11. Abramowitz and Stegun, p. 80, 4.4.42
12. Abramowitz and Stegun, p. 80, 4.4.43
13. Abramowitz and Stegun, p. 80, 4.4.36
14. Bronstein, Manual (1989). "Simplification of Real Elementary Functions". Proceedings of the ACM-SIGSAM 1989 international symposium on Symbolic and algebraic computation: 211.
15. Πρότυπο:MathWorld
16. Abramowitz and Stegun, p. 74, 4.3.48
17. Abramowitz and Stegun, p. 72, 4.3.24–26
18. Πρότυπο:MathWorld
19. Abramowitz and Stegun, p. 72, 4.3.27–28
20. Abramowitz and Stegun, p. 72, 4.3.20–22
21. Πρότυπο:MathWorld
22. Ken Ward's Mathematics Pages, http://www.trans4mind.com/personal_development/mathematics/trigonometry/multipleAnglesRecursiveFormula.htm
23. Abramowitz and Stegun, p. 72, 4.3.31–33
24. Abramowitz and Stegun, p. 72, 4.3.34–39
25. Warren P. Johnson, "Trigonometric Identities à la Hermite", American Mathematical Monthly, volume 117, number 4, April 2010, pages 311–327
26. Michael P. Knapp, Sines and Cosines of Angles in Arithmetic Progression
27. Abramowitz and Stegun, p. 74, 4.3.47
28. Abramowitz and Stegun, p. 71, 4.3.2
29. Abramowitz and Stegun, p. 71, 4.3.1
30. Abramowitz and Stegun, p. 75, 4.3.89–90
31. Abramowitz and Stegun, p. 85, 4.5.68–69
32. Weisstein, Eric W., "Sine" from MathWorld
33. Abramowitz and Stegun, p. 77, 4.3.105–110
34. Abramowitz and Stegun, p. 82, 4.4.52–57
35. Finney, Ross (2003). Calculus : Graphical, Numerical, Algebraic. Glenview, Illinois: Prentice Hall. σελ. 159–161. ISBN 0-13-063131-0.
36. Abramowitz and Stegun, p. 80, 4.4.26–31
37. Abramowitz and Stegun, p. 72, 4.3.23

## Ιστογραφία

Κίνδυνοι Χρήσης

Αν και θα βρείτε εξακριβωμένες πληροφορίες
σε αυτήν την εγκυκλοπαίδεια
ωστόσο, παρακαλούμε να λάβετε σοβαρά υπ' όψη ότι
η "Sciencepedia" δεν μπορεί να εγγυηθεί, από καμιά άποψη,
την εγκυρότητα των πληροφοριών που περιλαμβάνει.

"Οι πληροφορίες αυτές μπορεί πρόσφατα
να έχουν αλλοιωθεί, βανδαλισθεί ή μεταβληθεί από κάποιο άτομο,
η άποψη του οποίου δεν συνάδει με το "επίπεδο γνώσης"
του ιδιαίτερου γνωστικού τομέα που σας ενδιαφέρει."

Πρέπει να λάβετε υπ' όψη ότι
όλα τα άρθρα μπορεί να είναι ακριβή, γενικώς,
και για μακρά χρονική περίοδο,
αλλά να υποστούν κάποιο βανδαλισμό ή ακατάλληλη επεξεργασία,
ελάχιστο χρονικό διάστημα, πριν τα δείτε.

Επίσης,
(όχι μόνον, της Sciencepedia
αλλά και κάθε διαδικτυακού ιστότοπου (ή αλλιώς site)),
αν και άκρως απαραίτητοι,
είναι αδύνατον να ελεγχθούν
(λόγω της ρευστής φύσης του Web),
και επομένως είναι ενδεχόμενο να οδηγήσουν
σε παραπλανητικό, κακόβουλο ή άσεμνο περιεχόμενο.
Ο αναγνώστης πρέπει να είναι
εξαιρετικά προσεκτικός όταν τους χρησιμοποιεί.

- Μην κάνετε χρήση του περιεχομένου της παρούσας εγκυκλοπαίδειας
αν διαφωνείτε με όσα αναγράφονται σε αυτήν

>>Διαμαρτυρία προς την wikia<<

- Όχι, στις διαφημίσεις που περιέχουν απαράδεκτο περιεχόμενο (άσεμνες εικόνες, ροζ αγγελίες κλπ.)