infinite series of the reciprocals of the positive integers From Wikipedia, the free encyclopedia
In mathematics, the harmonic series is the divergent infinite series:
Divergent means that as you add more terms the sum never stops getting bigger. It does not go towards a single finite value.
Infinite means that you can always add another term. There is no final term to the series.
Its name comes from the idea of harmonics in music: the wavelengths of the overtones of a vibrating string are , , , etc., of the string's fundamental wavelength. Apart from the first term, every term of the series is the harmonic mean of the terms either side of it. The phrase harmonic mean also comes from music.
The fact that the harmonic series diverges was first proven in the 14th century by Nicole Oresme,[1] but was forgotten. Proofs were given in the 17th century by Pietro Mengoli,[2] Johann Bernoulli,[3] and Jacob Bernoulli.[4][5]
Harmonic sequences have been used by architects. In the Baroque period architects used them in the proportions of floor plans, elevations, and in the relationships between architectural details of churches and palaces.[6]
There are several well-known proofs of the divergence of the harmonic series. A few of them are given below.
One way to prove divergence is to compare the harmonic series with another divergent series, where each denominator is replaced with the next-largest power of two:
Each term of the harmonic series is greater than or equal to the corresponding term of the second series, and therefore the sum of the harmonic series must be greater than or equal to the sum of the second series. However, the sum of the second series is infinite:
It follows (by the comparison test) that the sum of the harmonic series must be infinite as well. More precisely, the comparison above proves that
This proof, proposed by Nicole Oresme in around 1350, is considered to be a high point of medieval mathematics. It is still a standard proof taught in mathematics classes today.
It is possible to prove that the harmonic series diverges by comparing its sum with an improper integral. Consider the arrangement of rectangles shown in the figure to the right. Each rectangle is 1 unit wide and units high, so the total area of the infinite number of rectangles is the sum of the harmonic series:
The total area under the curve from 1 to infinity is given by a divergent improper integral:
Since this area is entirely contained within the rectangles, the total area of the rectangles must be infinite as well. This proves that
The generalization of this argument is known as the integral test.
The harmonic series diverges very slowly. For example, the sum of the first 1043 terms is less than 100.[7] This is because the partial sums of the series have logarithmic growth. In particular,
where is the Euler–Mascheroni constant and which approaches 0 as goes to infinity. Leonhard Euler proved both this and also that the sum which includes only the sum of the reciprocals of the primes diverges also diverges, that is:
Partial sum of the harmonic series, | ||||
---|---|---|---|---|
expressed as a fraction | decimal | relative size | ||
1 | 1 | 1 | ||
2 | 3 | /2 | 1.5 | |
3 | 11 | /6 | ~1.83333 | |
4 | 25 | /12 | ~2.08333 | |
5 | 137 | /60 | ~2.28333 | |
6 | 49 | /20 | 2.45 | |
7 | 363 | /140 | ~2.59286 | |
8 | 761 | /280 | ~2.71786 | |
9 | 7129 | /2520 | ~2.82897 | |
10 | 7381 | /2520 | ~2.92897 | |
11 | 83711 | /27720 | ~3.01988 | |
12 | 86021 | /27720 | ~3.10321 | |
13 | 1145993 | /360360 | ~3.18013 | |
14 | 1171733 | /360360 | ~3.25156 | |
15 | 1195757 | /360360 | ~3.31823 | |
16 | 2436559 | /720720 | ~3.38073 | |
17 | 42142223 | /12252240 | ~3.43955 | |
18 | 14274301 | /4084080 | ~3.49511 | |
19 | 275295799 | /77597520 | ~3.54774 | |
20 | 55835135 | /15519504 | ~3.59774 | |
21 | 18858053 | /5173168 | ~3.64536 | |
22 | 19093197 | /5173168 | ~3.69081 | |
23 | 444316699 | /118982864 | ~3.73429 | |
24 | 1347822955 | /356948592 | ~3.77596 | |
25 | 34052522467 | /8923714800 | ~3.81596 | |
26 | 34395742267 | /8923714800 | ~3.85442 | |
27 | 312536252003 | /80313433200 | ~3.89146 | |
28 | 315404588903 | /80313433200 | ~3.92717 | |
29 | 9227046511387 | /2329089562800 | ~3.96165 | |
30 | 9304682830147 | /2329089562800 | ~3.99499 |
The finite partial sums of the diverging harmonic series,
are called harmonic numbers.
The difference between and converges to the Euler–Mascheroni constant. The difference between any two harmonic numbers is never an integer. No harmonic numbers are integers, except for .[8]: p. 24 [9]: Thm. 1
The series
is known as the alternating harmonic series. This series converges by the alternating series test. In particular, the sum is equal to the natural logarithm of 2:
The alternating harmonic series, while conditionally convergent, is not absolutely convergent: if the terms in the series are systematically rearranged, in general the sum becomes different and, dependent on the rearrangement, possibly even infinite.
The alternating harmonic series formula is a special case of the Mercator series, the Taylor series for the natural logarithm.
A related series can be derived from the Taylor series for the arctangent:
This is known as the Leibniz series.
The general harmonic series is of the form
where and are real numbers, and is not zero or a negative integer.
By the limit comparison test with the harmonic series, all general harmonic series also diverge.
A generalization of the harmonic series is the -series (or hyperharmonic series), defined as
for any real number . When , the -series is the harmonic series, which diverges. Either the integral test or the Cauchy condensation test shows that the -series converges for all (in which case it is called the over-harmonic series) and diverges for all . If then the sum of the -series is , i.e., the Riemann zeta function evaluated at .
The problem of finding the sum for is called the Basel problem; Leonhard Euler showed it is . The value of the sum for is called Apéry's constant, since Roger Apéry proved that it is an irrational number.
Related to the -series is the ln-series, defined as
for any positive real number . This can be shown by the integral test to diverge for but converge for all .
For any convex, real-valued function such that
the series
is convergent.[source?]
The random harmonic series
where the are independent, identically distributed random variables taking the values +1 and −1 with equal probability , is a well-known example in probability theory for a series of random variables that converges with probability 1. The fact of this convergence is an easy consequence of either the Kolmogorov three-series theorem or of the closely related Kolmogorov maximal inequality. Byron Schmuland of the University of Alberta further examined[10] the properties of the random harmonic series, and showed that the convergent series is a random variable with some interesting properties. In particular, the probability density function of this random variable evaluated at +2 or at −2 takes on the value 0.124999999999999999999999999999999999999999764..., differing from by less than 10−42. Schmuland's paper explains why this probability is so close to, but not exactly, . The exact value of this probability is given by the infinite cosine product integral [11] divided by π.
The depleted harmonic series where all of the terms in which the digit 9 appears anywhere in the denominator are removed can be shown to converge and its value is less than 80.[12] In fact, when all the terms containing any particular string of digits (in any base) are removed the series converges.
The harmonic series can be counterintuitive. This is because it is a divergent series even though the terms of the series get smaller and go towards zero. The divergence of the harmonic series is the source of some paradoxes.
Because the series gets arbitrarily large as becomes larger, eventually this ratio must exceed 1, which implies that the worm reaches the end of the rubber band. However, the value of at which this occurs must be extremely large: approximately , a number exceeding 1043 minutes (1037 years). Although the harmonic series does diverge, it does so very slowly.
Calculating the sum shows that the time required to get to the speed of light is only 97 seconds.
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