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Density functions for prime and relatively prime numbers
Authors:Paul Erdös  Ian Richards
Institution:(1) Hungarian National Academy, Budapest, Hungary;(2) Department of Mathematics, University of Minnesota, 55455 Minneapolis, MN, U.S.A.;(3) Mathematisches Institut der Universität, Strudlhofgasse 4, A-1090 Wien, Austria
Abstract:Letr *(x) denote the maximum number of pairwiserelatively prime integers which can exist in an interval (y,y+x] of lengthx, and let rhov*(x) denote the maximum number ofprime integers in any interval (y,y+x] whereygex. Throughout this paper we assume the ldquoprimek-tuples hypothesis.rdquo (This hypothesis could be avoided by using an alternative sievetheoretic definition of rhov*(x); cf. the beginning of Section 1.) We investigate the differencer *(x)—rhov*(x): that is we ask how many more relatively prime integers can exist on an interval of lengthx than the maximum possible number of prime integers. As a lower bound we obtainr *(x)—rhov*(x)<x c for somec>0 (whenxrarrinfin). This improves the previous lower bound of logx. As an upper bound we getr *(x)—rhov*(x)=ox/(logx)2]. It is known that rhov*(x)—pgr(x)>const.x/(logx)2];.; thus the difference betweenr *(x) and rhov*(x) is negligible compared to rhov*(x)—pgr(x). The results mentioned so far involve the ldquoupper boundrdquo or ldquomaximizingrdquo sieve. In Section 2, similar comparisons are made between two types of ldquominimumrdquo sieves. One of these is the ldquoerasingrdquo sieve, which completely eliminates an interval of lengthx; and the other, introduced by Erdös and Selfridge 1], involves a kind of ldquominimaxrdquo for sets of pairwise relatively prime numbers. Again these two sieving methods produce functions which are found to be closely related.
Keywords:
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