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3 Contents 1 Introduction 5 Means 11.1 Greek means Definition and properties of means Comparison of means Weak relations and symmetric angular relations Weighted Greek means Angular relations Operations with means Invariant and complementary means Partial derivatives of means Double sequences Measurement of the circle Heron s method of extracting square roots Lagrange and the definition of the AGM Elliptic integrals Gaussian double sequences Determination of G-compound means Rate of convergence of G-compound means Archimedean double sequences References 81 3

4 4 CONTENTS

5 Chapter 1 Introduction Our goal in writing this book was twofold. First of all we make a short incursion in the history of mathematics. The subjects in which we are interested means and double sequences are related to names like those of Pythagoras Archimedes Heron Lagrange and Gauss for giving the most famous of them. The second aim was to give the present stage of development of the problems we are dealing with. Of course we insist on our own results which are published in Romanian journals with limited distribution and so they are less known. Here as in the rest of the book for referring to a paper or on a book we indicate in brackets the name of the author(s) and the year of publication. If an author is present in the references with more papers published in the same year we add a small letter after the corresponding year. Pappus of Alexandria presented in his books in the fourth century AD the main mathematical contributions of the ancient Greeks (see [Pappus 193]). Among them we can find the means defined by the Pytagorean school: four well known means the arithmetic mean defined by the geometric mean given by A(a b) = a + b a b > 0 G(a b) = ab a b > 0 the harmonic mean with the expression H(a b) = ab a b > 0 a + b 5

6 6 CHAPTER 1. INTRODUCTION the contraharmonic mean defined by C(a b) = a + b a b > 0 a + b and six unnamed means. These means are the only ten means which can be defined using the method of proportions which is attributed to Pythagoras of Samos ( BC) (see [C. Gini 1958; C. Antoine 1998]) but also to Eudoxus (see [P. Eymard J.-P. Lafon 004]). Having no access to original sources we must content ourselves to present such controversies without taking any adherent position. The method may be described as follows. Consider a set of three numbers with the property that two of their differences are in the same ratio as two of the initial numbers. More exactly if the numbers are a m b > 0 the first member of the proportion can be one of the ratios while the second member must be a m a b a b m b or a m m b a a a b b a a m m a b m or m b. Thus we have twenty one proportions. Such a proportion defines a mean if a > b > 0 implies a > m > b. Namely the value of m represents the mean of a and b. As it is stated in [C. Gini 1958] we get only ten means the Greek means. We will define these means in the first part of the book. We give some of their properties and relations as they are presented in [Silvia Toader G. Toader 00]. A special attention is devoted to the determination of all complementaries of a Greek mean with respect to another which was done in [G. Toader 004; Silvia Toader G. Toader a]. The importance of this problem for the determination of the common limit of some double sequences will be presented a few lines later. A last subject developed in this part is devoted to the weighted Greek means which were defined in [G. Toader 005]. For doing this the first member of the proportions was multiplied by the report λ/(λ 1) where λ (0 1) is a parameter. The weighted variants of the arithmetic harmonic and contraharmonic means are those well known for long time. For the geometric mean is obtained a

7 weighted mean which is different from the classical known variant. The other six weighted means are new. The second part of the book is devoted to double sequences. First of all we present some classical examples. The oldest was given by Archimedes of Syracuse (87-1 BC) in his book Measurement of the Circle. His problem was the evaluation of the number π defined as the ratio of the perimeter of a circle to its diameter. Consider a circle of radius 1 and denote by p n and P n the half of the perimeters of the inscribed and circumscribed regular polygons with n sides respectively. As p n < π < P n n 3 to get an estimation with any accuracy Archimedes passes from a given n to n proving his famous inequalities < < p 96 < π < P 96 < < The procedure was so defined as a tongs method. But as was shown in [G. M. Phillips 1981] it can be presented also as a double sequence. Denoting P k n = a k and p k n = b k he proved that the sequences (a k ) k 0 and (b k ) k 0 are given step by step by the relations a k+1 = H(a n b n ) b k+1 = G(a n+1 b n ) k 0 for some initial values a 0 and b 0. Also it is shown that these sequences are monotonously convergent to a common limit which for 0 < b 0 < a 0 has the value a 0 b 0 arccos b 0. a 0 b a 0 0 In Archimedes case as a 0 = P 3 = 3 3 and b 0 = p 3 = 3 3/ the common limit is π. The second example of double sequences is furnished by Heron s method of extracting square roots. To compute the geometric root of two numbers a and b Heron used the arithmetic mean and the harmonic mean. Putting a 0 = a and b 0 = b define a k+1 = H(a n b n ) b k+1 = A(a n b n ) k 0. 7

8 8 CHAPTER 1. INTRODUCTION It is proved that the sequences (a k ) k 0 and (b k ) k 0 are monotonously convergent to the common limit ab. Of course the procedure was also used only as a tongs method the notion of limit being unknown in Heron s time (fl. c. 60 as it is given in [P. S. Bullen 003]). The third example is Lagrange s method of determination of some irrational integrals. In [J. -L. Lagrange ] for the evaluation of an integral of the form N(y )dy (1 + p y )(1 + q y ) where N is a rational function is defined an iterative method which leads to the rationalization of the function. It is based on the double sequence defined by a 0 = p b 0 = q and a k+1 = A(a n b n ) b k+1 = G(a n b n ) k 0. The same double sequence was defined in [C. F. Gauss 1800] which was published only many years later. For a 0 = and b 0 = 1 he remarked that a 4 and b 4 have the same first eleven decimals as those determined in [L. Euler 178] for the integral 1 0 z dz 1 z 4. In fact the sequences (a k ) k 0 and (b k ) k 0 are monotonously convergent to a common limit which is now known under the name of arithmetic-geometric mean and it is denoted by A G(a b). Later Gauss was able to represent it using an elliptic integral by A G(a b) = π [ π/ 0 dθ a cos θ + b sin θ ] 1. Of course the result is used for the numerical evaluation of the elliptic integral. After presenting some results related to these special double sequences we pass to the general definition of double sequences that is the special means A G or H which appear in the definition of these examples are replaced by arbitrary means M and N. Before doing this we have to remark that the

9 9 essential difference between the first example and the other examples is the use of a k+1 in the definition of b k+1. So we can define double sequences of type a k+1 = M(a n b n ) b k+1 = N(a n+1 b n ) k 0 which are called in [G. M. Phillips 1981] Archimedean double sequences or of the type a k+1 = M(a n b n ) b k+1 = N(a n b n ) k 0 named in [D. M. E. Foster G. M. Phillips 1984] Gaussian double sequences. It is easy to see that an Archimedean double sequence can be written as a Gaussian one by changing the mean N. So in what follows we can content ourself to discuss only this last case. The first problem which was studied related to a given double sequence is that of the convergence of the sequences (a k ) k 0 and (b k ) k 0 to a common limit. In this case it is proved that the common limit defines a mean denoted by M N and called the compound mean of M and N. We give in References a lot of papers which deal with this problem. We mention here only a few of them [D. M. E. Foster G. M. Phillips 1985; G. Toader ; Iulia Costin G. Toader a] in which one looks after minimal conditions on the means M and N that assure that their compound mean exists. The second main problem was that of the determination of M N. Using the idea by which Gauss was able to give the representation of A G in [J. M. Borwein P. B. Borwein 1987] is proved the following Invariance Principle: if M N exists and is continuous then it is the unique mean P satisfying P (M(a b) N(a b)) = P (a b) a b > 0. In this case the mean P is called (M N) invariant. As we can see in the case of A G it is not at all easy to determine a mean invariant with respect to two given means. Thus becomes important the change of the point of view as it is done in [G. Toader 1991]. Given the means M and P if the previous relation is satisfied the mean N is named complementary of M with respect to P. As we saw before we have determined all the complementaries of a Greek mean with respect to another. On this way we are able to construct ninety double sequences with known limits. Among them we get only eight cases in which by composing two Greek means we get again a Greek mean. Of course Heron s example is one of them.

10 10 CHAPTER 1. INTRODUCTION Finally the rate of convergence of the sequences to the common limit is also studied. In our cases it is quadratic and even faster as suggest the numerical examples. We hope that this book will contribute to the spreading of the ancient Greek mathematical knowledge about the means. We underline also the modern possibilities of development of the subject first of all related to the work of C. F. Gauss on double sequences.

11 Chapter Means This part is devoted to the study of Greek means. We remind first the method of proportions used by the Pytagorean school for the definition of means. We present the ten means constructed on this way the Greek means. Then we study some of their properties define more relations that hold among them and determine all the complementaries of a Greek mean with respect to another. Finally we present weighted variants of the Greek means..1 Greek means As many other important Greek mathematical contributions the means defined by the Pytagorean school were presented by Pappus of Alexandria in his books (see[pappus 193]). Some indications about them can be found in the books [C. Gini 1958; J. M. Borwein P. B. Borwein 1986; C. Antoine 1998]. We present here a variant of the original construction of the means but also their modern transcriptions. We select some properties of these means and some relations among them as they are given in [Silvia Toader G. Toader 00]. Pythagoras of Samos ( BC) already knew the arithmetic mean A the geometric mean G and the harmonic mean H. To construct them he used the method of proportions: he considered a set of three numbers with the property that two of their differences are in the same ratio as two of the initial numbers. More exactly let a > m > b > 0. Then m represents: 11

12 1 CHAPTER. MEANS 1. the arithmetic mean of a and b if a m m b = a a ;. the geometric mean of a and b if a m m b = a m = m b ; 3. the harmonic mean of a and b if a m m b = a b ; Following [C. Antoine 1998] three other means including the contraharmonic mean C were defined by Eudoxus and finally other four means by Temnoides and Euphranor. In [C. Gini1958] all these seven means are attributed to Nicomah. Only three of these new means have a name: 4. the contraharmonic mean of a and b defined by a m m b = b a ; 5. the first contrageometric mean of a and b defined by a m m b = b m ; 6. the second contrageometric mean of a and b defined by the proportion a m m b = m a ; The rest of four no-named means are defined by the relations: 7. a m a b = b a ; 8. a m a b = m a ; 9. a b m b = a b ;

13 .1. GREEK MEANS a b m b = m b. As it is remarked in [C. Gini 1958] we can consider more such proportions. In fact the first member can be one of the ratios while the second member must be a m a b a b m b or a m m b a a a b b a a m m a b m or m b. Thus we have twenty one proportions but we get no other nontrivial mean. Solving each of the above relations as an equation with unknown term m we get the analytic expressions M(a b) of the means. For the first four means we use the classical notations. For the other six we accept the neutral symbols proposed in [J. M. Borwein P. B. Borwein 1986]. We get so in order the following means: 1. A(a b) = a + b ;. G(a b) = ab ; H(a b) = ab a + b ; C(a b) = a + b a + b ; F 5 (a b) = a b + (a b) + 4b F 6 (a b) = b a + (a b) + 4a F 7 (a b) = a ab + b ; a ; ;

14 14 CHAPTER. MEANS F 8 (a b) = F 9 (a b) = a a b ; b(a b) a F 10 (a b) = b + b(4a 3b). Sometimes it is convenient to refer to all means by the neutral notation considering that F 1 = A F = G F 3 = H and F 4 = C. The first four expressions of the Greek means are symmetric that is we can use them also to define the corresponding means for a < b. For the other six expressions we have to replace a with b to define the means on a < b. ;. Definition and properties of means There are more definitions of means as we can see in the book [C. Gini 1958]. The most used definition may be found in the book [G. H. Hardy J. E. Littlewood G. Pòlya 1934] but it was suggested even by Cauchy (as it is stated in [C. Gini 1958]). Definition 1 A mean is defined as a function M : R + R + which has the property a b M(a b) a b a b > 0 (.1) where a b = min(a b) and a b = max(a b). Regarding the properties of means of course each mean is reflexive that is M(a a) = a a > 0 which will be used also as definition of M(a a) if it is necessary. A mean can have additional properties.

15 .. DEFINITION AND PROPERTIES OF MEANS 15 Definition The mean M is called: a) symmetric if b) homogeneous (of degree one) if c) (strictly) isotone if for a b > 0 are (strictly) increasing; d) strict at the left if strict at the right if M(a b) = M(b a) a b > 0 ; (.) M(ta tb) = t M(a b) t a b > 0 ; (.3) M(a.) and M(. b) M(a b) = a a = b (.4) M(a b) = b a = b (.5) and strict if is strict at the left and strict at the right. In what follows we shall use the following obvious Lemma 3 A mean M is isotone if and only if M(a b) M(a b ) for all a a b b. (.6) Example 4 Of course and are also means. We can consider them as trivial Greek means defined by the proportions a b a m = a a respectively a b m b = a a. They are symmetric homogeneous and isotone but are not strict neither at the left nor at the right.

16 16 CHAPTER. MEANS Remark 5 In [J. M. Borwein P. B. Borwein 1986] are used these means for the definition of the Greek means. Namely a is replaced by a b and b by a b. So we get expressions of the following type M(a b a b). With this construction any mean becomes symmetric. Remark 6 Simple examples of non symmetric means may be given by the projections Π 1 and Π defined respectively by Π 1 (a b) = a Π (a b) = b a b > 0. Of course Π 1 is strict only at the right while Π is strict only at the left. They cannot be defined by the method of proportions. Remark 7 In [Silvia Toader G. Toader 00] is proved that all the functions F i i = are means. We shall give this proof later but we refer at them always as means. All the Greek means are homogeneous and strict. The monotony of the above means is also studied in [Silvia Toader G. Toader 00]. We have the following results. Theorem 8 For a > b > 0 the Greek means have the following monotonicities: 1) All the means are increasing with respect to a on (b ). ) The means A G H F 6 F 8 F 9 and F 10 are increasing with respect to b on (0 a) thus they are isotone. 3) For each of the means C F 5 and F 7 there is a number 0 < p < 1 such that the mean is decreasing with respect to b on the interval (0 p a) and increasing on (p a a). These means have the values M(a 0) = M(a a) = a and M(a pa) = qa respectively. The values of the constants p q are given in the following table: M C F 5 F 7 p 1 /5 1/ q ( 1) 4/5 3/4

17 .3. COMPARISON OF MEANS 17.3 Comparison of means Before proving that all of the above functions are means we give some inequalities among them. We write to denote M N M(a b) < N(a b) a b > 0. We say that M is comparable to N if M N or N M. In [Silvia Toader G. Toader 00] is proved the following Theorem 9 Among the Greek means we have only the following inequalities: H G A F 6 F 5 C and H F 9 F 10 F 8 F 7 F 5 C F 8 A F 6 F 5 C G F 10. These inequalities are easy to prove. In the next paragraph will be studied other relations among the Greek means. They are more complicated. Corollary 10 The functions F k k = are means. It is enough to prove that H F 8 C and F 10 which are simple computations. Given two means M and N we can define the means M N and M N by M N(a b) = max{m(a b) N(a b)} respectively M N(a b) = min{m(a b) N(a b)}.

18 18 CHAPTER. MEANS Of course if M < N then M N = M M N = N but generally we get the inequalities M N M M N and M N N M N. Remark 11 As it is well known (see [P. S. Bullen 003]) now are known much more means (of course defined by other methods). We mention here two families of means which will be used later: the power means defined by ( ) a n + b n 1 n P n (a b) = n 0 and the generalized contraharmonic means (or Lehmer means) defined by C n (a b) = an + b n a n 1 + b n 1. Of course P 1 = A P 1 = H C = C and usually P 0 = G is also taken. It is known that these families of means are increasing with respect to the parameter n that is P n P m and C n C m for n m..4 Weak relations and symmetric angular relations In [I. J. Schoenberg 198; D. M. E. Foster G. M. Phillips 1985] a comparability of means on a subset was considered. Definition 1 The means M and N are in the relation where D R + if M D N M(a b) N(a b) (a b) D.

19 .4. WEAK RELATIONS AND SYMMETRIC ANGULAR RELATIONS19 If the last inequality is strict for a b we write M < D N. If M < D N and N D M where D = R + \ D we write M D N. Remark 13 If the means M and N are symmetric and M D N then D has a kind of symmetry namely: (a b) D (b a) D. For non-symmetric means in [G. Toader 1987] was given the following Definition 14 The means M and N are in the weak relation M N if M D N for D = { (x y) R +; x < y }. The comparison of homogeneous means can be done only on special sets. Definition 15 The set D R is called starshaped if (a b) D t > 0 (ta tb) D. It is easy to prove the following property. Lemma 16 If the means M and N are homogeneous and M D N then the set D is starshaped. The simplest relation of this kind was given in [Silvia Toader G. Toader 00]. Let m > 1. Definition 17 The means M and N are in the symmetric angular relation M m N if M D N for D = { (x y) R +; y/m < x < my }.

20 0 CHAPTER. MEANS Theorem 18 Let s1 = s = + s3 = and t1 t t3 t4 respectively t5 be the greatest roots of the equations t 3 t + t 1 = 0 t 3 t t + 1 = 0 t 3 t t 1 = 0 t 3 3t + t 1 = 0 t 3 5t + 4t 1 = 0. We have the following angular relations between the Greek means: F 5 F 10 F 8 H F 7 A A F 9 A 3 F 10 F 7 s1 H C s1 F 9 F 5 s F 9 F 8 s3 G G s3 F 9 F 7 t1 G F 6 t F 9 C t3 F 10 F 7 t4 F 6 F 6 t4 F 10 and F 8 t5 F 10. Remark 19 The approximate values of the above numbers are: s1 = s = t1 = t = t3 = t4 = s3 = t5 = Corollary 0 For each fixed b the interval (b ) divides into eleven subintervals such that on each of them the Greek means are completely ordered. Let us present here the table of these intervals and orders. (b s1 b) F 8 F 7 H G A F 6 F 5 C F 9 F 10 (s1 b s b) F 8 H F 7 G A F 6 F 5 F 9 C F 10 (s b t1 b) F 8 H F 7 G A F 6 F 9 F 5 C F 10 (t1 b t b) F 8 H G F 7 A F 6 F 9 F 5 C F 10 (t b t3 b) F 8 H G F 7 A F 9 F 6 F 5 C F 10 (t3 b b) F 8 H G F 7 A F 9 F 6 F 5 F 10 C (b t4 b) H F 8 G F 9 A F 7 F 6 F 10 F 5 C (t4 b s3 b) H F 8 G F 9 A F 10 F 6 F 7 F 5 C (s3 b 3b) H F 9 G F 8 A F 10 F 6 F 7 F 5 C (3b t5 b) H F 9 G F 8 F 10 A F 6 F 7 F 5 C (t5 b ) H F 9 G F 10 F 8 A F 6 F 7 F 5 C Remark 1 We can give a similar table for each fixed a with b running in the interval (0 a). We have only to replace each interval (sb tb) with the interval (a/t a/s) by keeping the order of the means. Of course the order of the intervals must be reversed. Thus the first interval will be (0 a/t5).

21 .5. WEIGHTED GREEK MEANS 1.5 Weighted Greek means There are also known weighted generalizations of some means (see [P. S. Bullen 003]). The most important example is that of the weighted power means P nλ defined by P n;λ (a b) = { [λ a n + (1 λ) b n ] 1/n n 0 a λ b 1 λ n = 0 with λ [0 1] fixed. Of course for λ = 0 or λ = 1 we have P n;0 = Π respectively P n;1 = Π 1 n R. For n = 1 0 or 1 we have the weighted arithmetic mean A λ the weighted geometric mean G λ and the weighted harmonic mean H λ. Weighted generalized contraharmonic means are defined by C n;λ (a b) = λ an + (1 λ) b n λ a n 1 + (1 λ) b n 1. So for the first four Greek means we have weighted variants. But how to define such variants of the last six Greek means? In [G. Toader 005] an answer to this question was given. We remark that in the case of the geometric mean is obtained a weighted variant which is completely different from P 0;λ (a b) = a λ b 1 λ. Consider a set of three numbers a > m > b > 0. Remember that the arithmetic mean is defined by the proportion a m m b = a a. Take λ (0 1) and multiply the first member of the proportion by λ/(1 λ). Now m will give the weighted arithmetic mean of a and b. We shall proceed like this in the first six cases getting successively: 1. the equality λ 1 λ a m m b = a a

22 CHAPTER. MEANS gives the weighted arithmetic mean of a and b defined as above by A λ (a b) = λ a + (1 λ) b ;. the equality λ 1 λ a m m b = a m gives the weighted geometric mean of a and b defined by G λ (a b) = 1 [ ] (1 λ) a λ + 4λ (1 λ) ab (1 λ) a ; 3. the equality λ 1 λ a m m b = a b gives the weighted harmonic mean of a and b defined by H λ (a b) = ab λ b + (1 λ) a ; 4. the equality λ 1 λ a m m b = b a gives the weighted contraharmonic mean of a and b defined by C λ (a b) = λ a + (1 λ) b λ a + (1 λ) b 5. the equality λ 1 λ a m m b = b m ; gives the first weighted contrageometric mean of a and b defined by F 5λ (a b) = 1 [λa (1 λ) b + ] λ λ a λ (1 λ) ab + (1 λ) (1 + 3λ) b ; 6. the equality λ 1 λ a m m b = m a gives the second weighted contrageometric mean of a and b defined by [ ] 1 F 6λ (a b) = (1 λ) b λa + λ (4 3λ) a (1 λ) λ (1 λ) ab + (1 λ) b.

23 .5. WEIGHTED GREEK MEANS 3 Remark To define the means on a < b we replace a with b and λ with 1 λ. So A λ H λ and C λ preserve their expressions but the other do not. Of course for λ = 1/ we get the usual Greek means. To prove that all of the above functions represent means some relations among them are useful. Theorem 3 For each λ (0 1) the following inequalities and are valid. H λ G λ A λ F 5λ C λ A λ F 6λ C λ Proof. All the relations can be proved by direct calculation. For example the inequality A(a b) F 5λ (a b) for a > b > 0 is equivalent with λ a λ (1 λ) ab + (1 λ) (1 + 3λ) b λ [λa + (1 λ)b] λa + (1 λ)b which after raising to the second power and collecting the like terms becomes which is certainly true. 4λ 3 (1 λ) (a b) 0 Corollary 4 The functions A λ G λ H λ C λ F 5λ and F 6λ define means for each λ (0 1). Proof. We have only to prove that H λ and C λ is true. This can be easily verified.

24 4 CHAPTER. MEANS Remark 5 Passing at limit for λ 0 we get the value b while for λ 1 we have the value a. So we can extend the definition of the above weighted means by considering them equal with Π for λ = 0 and with Π 1 for λ = 1. Let again the set of three numbers a > m > b > 0 and a parameter λ (0 1). Continuing as before we want to find the rest of four weighted Greek means. 7. the relation λ 1 λ a m a b = b a gives for m the value gives gives gives 8. the relation 9. the relation 10. the relation F 7λ (a b) = λ a + b (b a) (1 λ) λ a λ 1 λ a m a b = m a F 8λ (a b) = λ a a (1 λ) b ; λ 1 λ m b a b = b a F 9λ (a b) = b (a + λ b b) λ a λ 1 λ m b a b = b m F 10λ (a b) = λ b + λ b [λ b + 4 (1 λ) (a b)] λ Remark 6 Passing to limit for λ 0 in F kλ k = we get the values 0 respectively. This shows that they cannot be used to define means for all the values of λ. In fact each of them has the property F kλ (a b) b for a > b if and only if λ [1/ 1). To define them on a < b we replace a with b (we cannot replace also λ with 1 λ). We extend the ; ;.

25 .5. WEIGHTED GREEK MEANS 5 definition of the above weighted means for λ = 1 (passing at limit for λ): F 7λ and F 8λ equal with while F 9λ and F 10λ equal with. Also we define the means for λ [0 1/) by F kλ = F k1 λ k = (only to avoid this restriction on λ). Some properties of the weighted means were also studied in [G. Toader 005]. All the weighted Greek means are homogeneous. Relative to the monotony of the above means are given the following results. Theorem 7 For a > b > 0 the weighted Greek means have the following monotonicities: 1) All the means are increasing with respect to a on (b ). ) The means A λ G λ H λ F 6λ F 8λ F 9λ and F 10λ are increasing with respect to b on (0 a). 3) The means C λ F 5λ and F 7λ are decreasing with respect to b on the interval (0 p λ a) and increasing on (p λ a a). These means have the values M(a 0) = M(a a) = a respectively M(a p λ a) = q λ a. The values of the constants p λ q λ are given in the following table: M C λ F 5λ F 7λ p λ λ 1+ λ λ 1+3λ 4 5λ q λ p λ p λ 1. 4(1 λ) λ 5λ 1 λ 1 4λ Proof. All the results can be verified by the study of the sign of the partial derivatives of the corresponding means. For example in the case of the mean C λ we have C λ b = (1 λ) [ λ a + λ ab + (1 λ) b ] [λ a + (1 λ) b] and it is positive if and only if [ ( ) ] [ ( ) ] λ a λ 1 b λ a λ + 1 b < 0. As the first factor is positive we get the equivalent condition 1 Similarly we have b > λ 1 + λ a.

26 6 CHAPTER. MEANS Theorem 8 For b > a > 0 the weighted Greek means have the following monotonicities: 1) All the means are increasing with respect to b on (a ). ) The means A λ G λ H λ F 6λ F 8λ F 9λ and F 10λ are increasing with respect to a on (0 b). 3) The means C λ F 5λ and F 7λ are decreasing with respect to a on the interval (0 p λ b) and increasing on (p λ b b). These means have the values M(0 b) = M(b b) = b respectively M(p λ b b) = q λ b. The values of the constants p λ q λ are given in the following table: M C λ F 5λ F 7λ p λ 1 λ 1+ 1 λ (1 λ) 4 3λ q λ p λ p λ 1 4 5λ 4(1 λ) λ 1 5λ 1 4λ λ 1 As concerns the asymptotic behavior of the given means is proved the following. Theorem 9 For a fixed value of following asymptotes: b the weighted Greek means have the i) the mean H λ has a horizontal asymptote of equation y = b 1 λ ii) the mean F 9λ has a horizontal asymptote of equation: y = { b 1 λ if λ 1 b λ if λ 1 ; iii) the means G λ and F 10λ have asymptotic directions 0; iv) the mean F 8λ has the inclined asymptote with equation: y = { (1 λ) (a + λ b) if λ 1 λ [a + (1 λ) b] if λ 1 ; v) the mean F 6λ has the inclined asymptote with equation y = 4λ 3λ λ ( ) a 1 λ + b ; 4λ 3λ

27 .6. ANGULAR RELATIONS 7 vi) the means C λ and F 5λ have the inclined asymptote with equation y = a 1 λ λ b ; vi) the mean F 7λ has the inclined asymptote with equation y = { a λ 1 λ b if λ 1 a 1 λ λ b if λ 1. Proof. Let us prove this statement for the mean F 5λ. We have F 5λ (a b) lim a a and then lim [F 5λ(a b) a] = λ 1 b. a λ Looking after new relations among the weighted Greek means we get only two global relations. = 1 Theorem 30 For every λ (0 1) the inequalities and hold. F 9λ F 10λ F 8λ F 7λ Proof. For λ 1/ and a > b each of the above inequalities is equivalent with the relation λa (1 λ)b. Corollary 31 The functions F kλ are means for k = and Angular relations To give the relation between F 5λ and F 6λ in [G. Toader 005] was defined a new notion which is more general than the symmetric angular relation.

28 8 CHAPTER. MEANS Definition 3 For m n 0 consider the set D mn = {(a b) R + : min(m n) a b max(m n) a }. We say that the means M and N are in the angular relation M mn N if M Dmn N. Theorem 33 For every λ (0 1) holds the angular inequality F 5λ 1m F 6λ where m = λ 1 λ. Proof. The inequality F 6λ (a b) > F 5λ (a b) is equivalent with the relation (a b) (m a b) < 0. For λ > 1/ as m > 1 we have no solution with a > b thus F 5λ (a b) F 6λ (a b) if and only if a b m a. For λ = 1/ we have m = 1 thus which is equivalent with F 6λ F 5λ F 5λ 11 F 6λ. Finally for λ < 1/ as m < 1 we have F 5λ (a b) F 6λ (a b) if and only if m a b a. To present the next results we allow angular relations for infinite value of the parameters m or n. Also we denote by β = the inverse of the golden section. 5 1

29 .6. ANGULAR RELATIONS 9 Theorem 34 Among the weighted Greek means we have the angular inequalities M mn N with m 1 λ ( ] 0 1 m = m λ ( 1 λ (0 1 β] 1 β) n = n λ ( ) 1 β 1 1 λ [β 1) n 3 λ [ 1 1) where the value of m 1 and m are given in the following table: while n 1 and n are: M N m 1 m λ 1 H λ F 9λ 0 λ(1 λ) λ 1 A λ F 8λ 0 λ(1 λ) λ A λ F 9λ 1 λ 1 λ 1 λ λ A λ F 3 10λ λ C λ F 5λ 8λ+4 λ 9λ (1 λ) λ G λ F 5λ 8λ+4 9λ λ 1 F 5λ F 4λ 3 4λ +1 9λ λ (1 λ) (1+λ) λ( 5 1) (1 λ) 1+λ (1 λ) 5 (1 λ) 1 1 λ 1 λ M N n n 3 λ(1 λ) H λ F 9λ λ 1 λ(1 λ) A λ F 8λ λ 1 λ 1 A λ F 9λ (1 λ) λ λ A λ F ( λ) 1+λ 10λ (1 λ) 3 λ C λ F 9λ λ (1 λ)( 5 1) G λ F 9λ λ λ λ 5 F 5λ F 9λ λ 1 λ λ 5λ λ+1 1+λ (1 λ) 1+λ 1 λ+5λ (1 λ) 1 1 4λ+8λ 4λ 3. Proof. Consider the inequality F 9λ (a b) H λ (a b). It is easy to verify it for a b and λ (0 1/] as well as for a < b and λ [1/ 1). For a b and λ (1/ 1) the inequality is equivalent with the relation (1 λ)a + λ(1 λ)b 0. This cannot hold if λ 1 β.

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