Search: id:A004394 Results 1-1 of 1 results found. %I A004394 %S A004394 1,2,4,6,12,24,36,48,60,120,180,240,360,720,840,1260,1680,2520,5040, %T A004394 10080,15120,25200,27720,55440,110880,166320,277200,332640,554400,665280, %U A004394 720720,1441440,2162160,3603600,4324320,7207200,8648640,10810800 %N A004394 Superabundant [or super-abundant] numbers: n such that sigma(n)/n > sigma(m)/ m for all m sigma_{-1}(m) for all m < n, where sigma_{-1}(n) is the sum of the reciprocals of the divisors of n. - Matthew Vandermast (ghodges14(AT)comcast.net), Jun 09 2004 %C A004394 Alaoglu and Erdos show that: (1) n is superabundant => n=2^{e_2} * 3^{e_3} * ...* p^{e_p}, with e_2>=e_3>=...>=e_p (and e_p is 1 unless n=4 or n=36); (2) if qTable of n, a(n) for n=0..2000 (Extends to n=8436 in the comments.) %H A004394 Matthew M. Conroy, Home page (listed instead of email address) %H A004394 P. Erdos & J.-L. Nicolas, Repartition des nombres superabondants (Text in French) %H A004394 J. C. Lagarias, An elementary problem equivalent to the Riemann hypothesis, Am. Math. Monthly 109 (#6, 2002), 534-543. %H A004394 Walter Nissen, Abundancy : Some Resources %H A004394 T. D. Noe, First 500 superabundant numbers %H A004394 T. D. Noe, First 1000000 superabundant numbers (21 MB, zipped) [From T. D. Noe (noe(AT)sspectra.com), Oct 15 2009] %H A004394 Eric Weisstein's World of Mathematics, Superabundant Number %H A004394 Wikipedia, Superabundant number %t A004394 a=0; Do[b=DivisorSigma[1, n]/n; If[b>a, a=b; Print[n]], {n, 1, 10^7}] %Y A004394 Cf. A002182, A002093; colossally abundant numbers: A004490. %Y A004394 A023199 is a subsequence. Almost same as A077006. %Y A004394 Cf. A112974 (number of superabundant numbers between colossally abundant numbers). %Y A004394 Sequence in context: A094348 A002182 A077006 this_sequence A166981 A137425 A141320 %Y A004394 Adjacent sequences: A004391 A004392 A004393 this_sequence A004395 A004396 A004397 %K A004394 nonn,nice %O A004394 1,2 %A A004394 Matthew Conroy %E A004394 Matthew Conroy points out that these are different from the highly composite numbers - see A002182. Jul 10 1996. Search completed in 0.002 seconds