cp's OEIS Frontend

This is a front-end for the Online Encyclopedia of Integer Sequences, made by Christian Perfect. The idea is to provide OEIS entries in non-ancient HTML, and then to think about how they're presented visually. The source code is on GitHub.

A209079 Integer part of sigma(m)*phi(m)/m for colossally abundant numbers m.

Original entry on oeis.org

1, 4, 9, 44, 96, 312, 2139, 4421, 48234, 623336, 1266781, 3897787, 20138571, 341171088, 6464294306, 148397712765, 299150944780, 8665061848812, 268337399189042, 1911903969221925, 5783509506896323, 213833540687410017
Offset: 1

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Author

Alexei Kourbatov, Mar 04 2012

Keywords

Comments

The sequence is increasing about as fast as the sequence of colossally abundant (CA) numbers (A004490).
We have two results:
(1) sigma(m)*phi(m)/m ~ m as m tends to infinity.
Here gamma is the Euler-Mascheroni constant 0.5772156649... (A001620).
Formula (1) follows from these known facts for CA numbers m:
(A) sigma(m)/m ~ exp(gamma) * log(log(m))
(B) m/phi(m) ~ exp(gamma) * log(log(m))
Dividing (A) by (B) we get sigma(m)*phi(m)/(m^2) ~ 1, hence (1) is true.
(2) 6m/(pi^2) < sigma(m)*phi(m)/m < m, which follows from Theorem 329 (Hardy and Wright, p. 352).
Ramanujan was the first to establish (A) for CA numbers m (see equation 383 in Ramanujan's paper; note that he used a different name for CA numbers: generalized superior highly composite numbers). Once we have (A) for an increasing sequence of numbers m (including, but not limited to CA numbers m), then (B) easily follows from (A) because, for large m, sigma(m)/m < m/phi(m) < exp(gamma) log(log(m)) + 0.6/(log(log(m))) (see Robin, 1984, p. 206).

Examples

			1 = [3*1/2]
4 = [12*2/6]
9 = [28*4/12]
44 = [168*16/60]
96 = [360*32/120]
312 = [1170*96/360]
2139 = [9360*576/2520]
4421 = [19344*1152/5040]
48234 = [232128*11520/55440]
623336 = [3249792*138240/720720]
1266781 = [6604416*276480/1441440]
3897787 = [20321280*829440/4324320]
20138571 = [104993280*4147200/21621600]
341171088 = [1889879040*66355200/367567200]
6464294306 = [37797580800*1194393600/6983776800]
148397712765 = [907141939200*26276659200/160626866400]
299150944780 = [1828682956800*52553318400/321253732800]
8665061848812 = [54860488704000*1471492915200/9316358251200]
268337399189042 = [1755535638528000*44144787456000/288807105787200]
1911903969221925 = [12508191424512000*309013512192000/2021649740510400]
5783509506896323 = [37837279059148800*927040536576000/6064949221531200]
		

References

  • G. H. Hardy and E. M. Wright, An introduction to the theory of numbers, 6th edition, Oxford University Press (2008), 350-353.
  • G. Robin, Grandes valeurs de la fonction somme des diviseurs et hypothèse de Riemann. J. Math. Pures Appl. 63 (1984), 187-213.

Crossrefs

Cf. A004490 (colossally abundant numbers), A001620, A073751, A185339.