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	<entry>
		<id>https://en.formulasearchengine.com/index.php?title=Dissipation_factor&amp;diff=5917</id>
		<title>Dissipation factor</title>
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		<updated>2014-01-03T05:14:31Z</updated>

		<summary type="html">&lt;p&gt;46.226.190.2: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In [[geometric group theory]], &#039;&#039;&#039;Gromov&#039;s theorem on groups of polynomial growth&#039;&#039;&#039;, named for [[Mikhail Gromov (mathematician)|Mikhail Gromov]], characterizes finitely generated [[Group (mathematics)|groups]] of &#039;&#039;polynomial&#039;&#039; growth, as those groups which have [[nilpotent group|nilpotent]] subgroups of finite [[index of a subgroup|index]]. &lt;br /&gt;
&lt;br /&gt;
The [[Growth rate (group theory)|growth rate]] of a group is a [[well-defined]] notion from [[asymptotic analysis]]. To say that a finitely generated group has &#039;&#039;&#039;polynomial growth&#039;&#039;&#039; means the number of elements of [[length]] (relative to a symmetric generating set) at most &#039;&#039;n&#039;&#039; is bounded above by a [[polynomial]] function &#039;&#039;p&#039;&#039;(&#039;&#039;n&#039;&#039;). The &#039;&#039;order of growth&#039;&#039; is then the least degree of any such polynomial function &#039;&#039;p&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;nilpotent&#039;&#039; group &#039;&#039;G&#039;&#039; is a group with a [[lower central series]] terminating in the identity subgroup. &lt;br /&gt;
&lt;br /&gt;
Gromov&#039;s theorem states that a finitely generated group has polynomial growth if and only if it has a nilpotent subgroup that is of finite index.&lt;br /&gt;
&lt;br /&gt;
There is a vast literature on growth rates, leading up to Gromov&#039;s theorem. An earlier result of [[Joseph A. Wolf]] showed that if &#039;&#039;G&#039;&#039; is a finitely generated nilpotent group, then the group has polynomial growth. [[Yves Guivarc&#039;h]] and independently [[Hyman Bass]] (with different proofs) computed the exact order of polynomial growth. Let &#039;&#039;G&#039;&#039; be a finitely generated nilpotent group with lower central series&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; G = G_1 \supseteq G_2 \supseteq \ldots. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In particular, the quotient group &#039;&#039;G&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;k&#039;&#039;&amp;lt;/sub&amp;gt;/&#039;&#039;G&#039;&#039;&amp;lt;sub&amp;gt;&#039;&#039;k&#039;&#039;+1&amp;lt;/sub&amp;gt; is a finitely generated abelian group. &lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;The Bass&amp;amp;ndash;Guivarc&#039;h formula&#039;&#039;&#039; states that the order of polynomial growth of &#039;&#039;G&#039;&#039; is&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; d(G) = \sum_{k \geq 1} k \ \operatorname{rank}(G_k/G_{k+1}) &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where:&lt;br /&gt;
:&#039;&#039;rank&#039;&#039; denotes the [[rank of an abelian group]], i.e. the largest number of independent and torsion-free elements of the abelian group.&lt;br /&gt;
&lt;br /&gt;
In particular, Gromov&#039;s theorem and the Bass&amp;amp;ndash;Guivarch formula imply that the order of polynomial growth of a finitely generated group is always either an integer or infinity (excluding for example, fractional powers).&lt;br /&gt;
&lt;br /&gt;
In order to prove this theorem Gromov introduced a convergence for metric spaces. This convergence, now called  the [[Gromov&amp;amp;ndash;Hausdorff convergence]], is currently widely used in geometry.&lt;br /&gt;
&lt;br /&gt;
A relatively simple proof of the theorem was found by [[Bruce Kleiner]]. Later, [[Terence Tao]] and [[Yehuda Shalom]] modified Kleiner&#039;s proof to make an essentially elementary proof as well as a version of the theorem with explicit bounds.&amp;lt;ref&amp;gt;http://terrytao.wordpress.com/2010/02/18/a-proof-of-gromovs-theorem/&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{cite arxiv |eprint=0910.4148 |author1=Yehuda Shalom |author2=Terence Tao |title=A finitary version of Gromov&#039;s polynomial growth theorem |class=math.GR |year=2009}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&amp;lt;references/&amp;gt;&lt;br /&gt;
* H. Bass, The degree of polynomial growth of finitely generated nilpotent groups, &#039;&#039;Proceedings London Mathematical Society&#039;&#039;, vol 25(4), 1972&lt;br /&gt;
* M. Gromov, Groups of Polynomial growth and Expanding Maps, [http://www.numdam.org/numdam-bin/feuilleter?id=PMIHES_1981__53_ &#039;&#039;Publications mathematiques I.H.É.S.&#039;&#039;, 53, 1981]&lt;br /&gt;
* Y. Guivarc&#039;h, Groupes de Lie à croissance polynomiale, C. R. Acad. Sci. Paris Sér. A&amp;amp;ndash;B 272 (1971). [http://www.numdam.org/item?id=BSMF_1973__101__333_0]&lt;br /&gt;
* {{Cite arxiv | last1=Kleiner | first1=Bruce | year=2007  | title=A new proof of Gromov&#039;s theorem on groups of polynomial growth | arxiv=0710.4593}}&lt;br /&gt;
* J. A. Wolf,  Growth of finitely generated solvable groups and curvature of Riemannian manifolds, &#039;&#039;Journal of Differential Geometry&#039;&#039;, vol 2, 1968&lt;br /&gt;
&lt;br /&gt;
[[Category:Theorems in group theory]]&lt;br /&gt;
[[Category:Nilpotent groups]]&lt;br /&gt;
[[Category:Infinite group theory]]&lt;br /&gt;
[[Category:Metric geometry]]&lt;br /&gt;
[[Category:Geometric group theory]]&lt;/div&gt;</summary>
		<author><name>46.226.190.2</name></author>
	</entry>
	<entry>
		<id>https://en.formulasearchengine.com/index.php?title=Continuously_variable_slope_delta_modulation&amp;diff=5939</id>
		<title>Continuously variable slope delta modulation</title>
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		<updated>2013-12-26T00:53:07Z</updated>

		<summary type="html">&lt;p&gt;46.226.190.2: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In [[recreational mathematics]], a &#039;&#039;&#039;Harshad number&#039;&#039;&#039; (or &#039;&#039;&#039;Niven number&#039;&#039;&#039;) in a given [[number base]], is an [[integer]] that is divisible by the [[digit sum|sum of its digits]] when written in that base.&lt;br /&gt;
Harshad numbers in base &#039;&#039;n&#039;&#039; are also known as &#039;&#039;&#039;&#039;&#039;n&#039;&#039;-Harshad&#039;&#039;&#039; (or &#039;&#039;&#039;&#039;&#039;n&#039;&#039;-Niven&#039;&#039;&#039;) numbers.&lt;br /&gt;
Harshad numbers were defined by [[D. R. Kaprekar]], a [[mathematician]] from [[India]]. The word &amp;quot;Harshad&amp;quot; comes from the [[Sanskrit]] &#039;&#039;{{IAST|harṣa}}&#039;&#039; (joy) + &#039;&#039;{{IAST|da}}&#039;&#039; (give), meaning joy-giver. The term “Niven number” arose from a paper delivered by [[Ivan M. Niven]] at a conference on [[number theory]] in 1977. All integers between [[0 (number)|zero]] and &#039;&#039;n&#039;&#039; are &#039;&#039;n&#039;&#039;-Harshad numbers.&lt;br /&gt;
To date there appear to be no applications for Harshad numbers, not even within pure mathematics.&lt;br /&gt;
&lt;br /&gt;
Stated mathematically, let &#039;&#039;X&#039;&#039; be a positive integer with &#039;&#039;m&#039;&#039; digits when written in base &#039;&#039;n&#039;&#039;, and let the digits be &#039;&#039;a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&#039;&#039; (&#039;&#039;i&#039;&#039; = 0, 1, ..., &#039;&#039;m&#039;&#039;&amp;amp;nbsp;&amp;amp;minus;&amp;amp;nbsp;1). (It follows that &#039;&#039;a&amp;lt;sub&amp;gt;i&amp;lt;/sub&amp;gt;&#039;&#039; must be either zero or a positive integer up to &#039;&#039;n&#039;&#039;&amp;amp;nbsp;&amp;amp;minus;&amp;amp;nbsp;1.) &#039;&#039;X&#039;&#039; can be expressed as&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;X=\sum_{i=0}^{m-1} a_i n^i.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If there exists an integer &#039;&#039;A&#039;&#039; such that the following holds, then &#039;&#039;X&#039;&#039; is a Harshad number in base &#039;&#039;n&#039;&#039;:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;X=A\sum_{i=0}^{m-1} a_i.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Harshad numbers in [[base 10]] form the sequence:&lt;br /&gt;
&lt;br /&gt;
: [[1 (number)|1]], [[2 (number)|2]], [[3 (number)|3]], [[4 (number)|4]], [[5 (number)|5]], [[6 (number)|6]], [[7 (number)|7]], [[8 (number)|8]], [[9 (number)|9]], [[10 (number)|10]], [[12 (number)|12]], [[18 (number)|18]], [[20 (number)|20]], [[21 (number)|21]], [[24 (number)|24]], [[27 (number)|27]], [[30 (number)|30]], [[36 (number)|36]], [[40 (number)|40]], [[42 (number)|42]], [[45 (number)|45]], [[48 (number)|48]], [[50 (number)|50]], [[54 (number)|54]], [[60 (number)|60]], [[63 (number)|63]], [[70 (number)|70]], [[72 (number)|72]], [[80 (number)|80]], [[81 (number)|81]], [[84 (number)|84]], [[90 (number)|90]], [[100 (number)|100]], [[102 (number)|102]], [[108 (number)|108]], [[110 (number)|110]], [[111 (number)|111]], [[112 (number)|112]], [[114 (number)|114]], [[117 (number)|117]], [[120 (number)|120]], [[126 (number)|126]], [[132 (number)|132]], [[133 (number)|133]], [[135 (number)|135]], [[140 (number)|140]], [[144 (number)|144]], [[150 (number)|150]], [[152 (number)|152]], [[153 (number)|153]], [[156 (number)|156]], [[162 (number)|162]], [[171 (number)|171]], [[180 (number)|180]], [[190 (number)|190]], [[192 (number)|192]], [[195 (number)|195]], [[198 (number)|198]], [[200 (number)|200]], [[201 (number)|201]], ...  {{OEIS|id=A005349}}&lt;br /&gt;
&lt;br /&gt;
A number which is a Harshad number in any number base is called an &#039;&#039;&#039;all-Harshad number&#039;&#039;&#039;, or an &#039;&#039;&#039;all-Niven number&#039;&#039;&#039;. There are only four all-Harshad numbers: [[1 (number)|1]], [[2 (number)|2]], [[4 (number)|4]], and [[6 (number)|6]].&lt;br /&gt;
&lt;br /&gt;
== What numbers can be Harshad numbers? ==&lt;br /&gt;
&lt;br /&gt;
Given the [[divisibility test]] for [[9 (number)|9]], one might be tempted to generalize that all numbers divisible by 9 are also Harshad numbers. But for the purpose of determining  the Harshadness of &#039;&#039;n&#039;&#039;, the digits of &#039;&#039;n&#039;&#039; can only be added up once and &#039;&#039;n&#039;&#039; must be divisible by that sum; otherwise, it is not a Harshad number. For example, [[99 (number)|99]] is not a Harshad number, since 9 + 9 = 18, and 99 is not divisible by 18.&lt;br /&gt;
&lt;br /&gt;
The base number (and furthermore, its powers) will always be a Harshad number in its own base, since it will be represented as &amp;quot;10&amp;quot; and 1 + 0 = 1.&lt;br /&gt;
&lt;br /&gt;
For a [[prime number]] to also be a Harshad number it must be less than or equal to the base number. Otherwise, the digits of the prime will add up to a number that is more than 1 but less than the prime and, obviously, it will not be divisible. For example: 11 is not Harshad in base 10 because the sum of its digits &amp;quot;11&amp;quot; is 1+1=2 and 11 is not divisible by 2, while in [[hexadecimal]] the number 11 may be represented as &amp;quot;B&amp;quot;, the sum of whose digits is also B and clearly B is divisible by B, ergo it is Harshad in base 16. &lt;br /&gt;
&lt;br /&gt;
Although the sequence of [[factorial]]s starts with Harshad numbers in base 10, not all factorials are Harshad numbers. 432! is the first that is not.&lt;br /&gt;
&lt;br /&gt;
== Consecutive Harshad numbers ==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== Maximal runs of consecutive Harshad numbers ===&lt;br /&gt;
Cooper and Kennedy proved in 1993 that no 21 consecutive integers are all Harshad numbers in base 10.&amp;lt;ref&amp;gt;{{citation | zbl=0776.11003 | last1=Cooper | first1=Curtis | last2=Kennedy | first2=Robert E. | title=On consecutive Niven numbers | journal=[[Fibonacci Quarterly]] | volume=31 | number=2 | pages=146–151 | year=1993 | issn=0015-0517 |url=http://www.fq.math.ca/Scanned/31-2/cooper.pdf}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=HBII382&amp;gt;{{cite book | last1=Sándor | first1=Jozsef | last2=Crstici | first2=Borislav | title=Handbook of number theory II | location=Dordrecht | publisher=Kluwer Academic | year=2004 | isbn=1-4020-2546-7 | zbl=1079.11001|page=382}}&amp;lt;/ref&amp;gt; They also constructed infinitely many 20-tuples of consecutive integers that are all 10-Harshad numbers, the smallest of which exceeds 10&amp;lt;sup&amp;gt;44363342786&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
{{harvs|authorlink=Helen G. Grundman|first=H. G.|last=Grundman|year=1994|txt}} extended the Cooper and Kennedy result to show that there are 2&#039;&#039;b&#039;&#039; but not 2&#039;&#039;b&#039;&#039;+1 consecutive &#039;&#039;b&#039;&#039;-Harshad numbers.&amp;lt;ref name=HBII382/&amp;gt;&amp;lt;ref&amp;gt;{{citation | last = Grundman | first = H. G. | authorlink=Helen G. Grundman | title = Sequences of consecutive &#039;&#039;n&#039;&#039;-Niven numbers | journal = [[Fibonacci Quarterly]] | volume = 32 | issue = 2 | year=1994 | pages = 174–175 | zbl=0796.11002 | issn=0015-0517 |url=http://www.fq.math.ca/Scanned/32-2/grundman.pdf}}&amp;lt;/ref&amp;gt; &lt;br /&gt;
This result was strengthened to show that there are infinitely many runs of 2&#039;&#039;b&#039;&#039; consecutive &#039;&#039;b&#039;&#039;-Harshad numbers for &#039;&#039;b&#039;&#039; = 2 or 3 by {{harvs|authorlink=T. Tony Cai|first=T.|last=Cai|year=1996|txt}}&amp;lt;ref name=HBII382/&amp;gt; and for arbitrary &#039;&#039;b&#039;&#039; by [[Brad Wilson (mathematician)|Brad Wilson]] in 1997.&amp;lt;ref&amp;gt;{{citation | last1=Wilson | first1=Brad | title=Construction of 2&#039;&#039;n&#039;&#039; consecutive &#039;&#039;n&#039;&#039;-Niven numbers | journal=[[Fibonacci Quarterly]] | volume=35 | pages=122–128 | year=1997 | issn=0015-0517 |url=http://www.fq.math.ca/Scanned/35-2/wilson.pdf}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In [[binary numeral system|binary]], there are thus infinitely many runs of four consecutive Harshad numbers and in [[ternary numeral system|ternary]] infinitely many runs of six.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
In general, such maximal sequences run from &#039;&#039;N · b&amp;lt;sup&amp;gt;k&amp;lt;/sup&amp;gt; - b&#039;&#039; to &#039;&#039;N · b&amp;lt;sup&amp;gt;k&amp;lt;/sup&amp;gt;&#039;&#039; + (&#039;&#039;b&#039;&#039;-1) , where &#039;&#039;b&#039;&#039; is the base, &#039;&#039;k&#039;&#039; is a relatively large power, and &#039;&#039;N&#039;&#039; is a constant.&lt;br /&gt;
Given one such suitably chosen sequence we can convert it to a larger one as follows:&lt;br /&gt;
* Inserting zeroes into &#039;&#039;N&#039;&#039; will not change the sequence of digital sums (just as 21, 201 and 2001 are all 10-Harshad numbers).&lt;br /&gt;
* If we insert &#039;&#039;n&#039;&#039; zeroes after the first digit, α (worth α&#039;&#039;b&amp;lt;sup&amp;gt;i&amp;lt;/sup&amp;gt;&#039;&#039;), we increase the value of &#039;&#039;N&#039;&#039; by α&#039;&#039;b&amp;lt;sup&amp;gt;i&amp;lt;/sup&amp;gt;(b&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; - 1)&#039;&#039; .&lt;br /&gt;
* If we can ensure that &#039;&#039;b&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; - 1&#039;&#039; is divisible by all digit sums in the sequence, then the divisibility by those sums is maintained.&lt;br /&gt;
* If our initial sequence is chosen so that the digit sums are [[coprime]] to &#039;&#039;b&#039;&#039;, we can solve &#039;&#039;b&amp;lt;sup&amp;gt;n&amp;lt;/sup&amp;gt; = 1&#039;&#039; modulo all those sums.&lt;br /&gt;
* If that is not so, but the part of each digit sum not coprime to &#039;&#039;b&#039;&#039; divides α&#039;&#039;b&amp;lt;sup&amp;gt;i&amp;lt;/sup&amp;gt;&#039;&#039;, then divisibility is still maintained.&lt;br /&gt;
* &#039;&#039;(Unproven)&#039;&#039; The initial sequence is so chosen.&lt;br /&gt;
Thus &amp;lt;!-- any solution implies --&amp;gt; our initial sequence yields an infinite set of solutions.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=== First runs of exactly &#039;&#039;n&#039;&#039; consecutive 10-Harshad numbers ===&lt;br /&gt;
The smallest naturals starting runs of &amp;lt;u&amp;gt;exactly&amp;lt;/u&amp;gt; &#039;&#039;n&#039;&#039; consecutive 10-Harshad numbers (i.e., smallest &#039;&#039;x&#039;&#039; such that &#039;&#039;x&#039;&#039;, &#039;&#039;x&#039;&#039;+1, ..., &#039;&#039;x&#039;&#039;+&#039;&#039;n&#039;&#039;-1 are Harshad numbers but &#039;&#039;x&#039;&#039;-1 and &#039;&#039;x&#039;&#039;+&#039;&#039;n&#039;&#039; are not) are as follows {{OEIS|id=A060159}}:&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|-&lt;br /&gt;
! &#039;&#039;n&#039;&#039;: !! 1 !! 2 !! 3 !! 4 !! 5 !! 6 !! 7 !! 8 !! 9 !! 10&lt;br /&gt;
|-&lt;br /&gt;
| &#039;&#039;x&#039;&#039;: || 12 || 20 || 110 || 510 || 131052 || 12751220 || 10000095 || 2162049150 || 124324220 || 1&lt;br /&gt;
|-&lt;br /&gt;
| &#039;&#039;&#039;&#039;&#039;n&#039;&#039;&#039;&#039;&#039;: || &#039;&#039;&#039;11&#039;&#039;&#039; || &#039;&#039;&#039;12&#039;&#039;&#039; || &#039;&#039;&#039;13&#039;&#039;&#039; || &#039;&#039;&#039;14&#039;&#039;&#039; || &#039;&#039;&#039;15&#039;&#039;&#039; || &#039;&#039;&#039;16&#039;&#039;&#039; || &#039;&#039;&#039;17&#039;&#039;&#039; || &#039;&#039;&#039;18&#039;&#039;&#039; || &#039;&#039;&#039;19&#039;&#039;&#039; || &#039;&#039;&#039;20&#039;&#039;&#039;&lt;br /&gt;
|-&lt;br /&gt;
| &#039;&#039;x&#039;&#039;: || &amp;lt;small&amp;gt;920067411130599&amp;lt;/small&amp;gt; || &amp;lt;small&amp;gt;43494229746440272890&amp;lt;/small&amp;gt; || &amp;lt;small&amp;gt;121003242000074550107423034⋅10&amp;lt;sup&amp;gt;20&amp;lt;/sup&amp;gt;&amp;amp;nbsp;-&amp;amp;nbsp;10&amp;lt;/small&amp;gt; || &amp;lt;small&amp;gt;420142032871116091607294⋅10&amp;lt;sup&amp;gt;40&amp;lt;/sup&amp;gt;&amp;amp;nbsp;-&amp;amp;nbsp;04&amp;lt;/small&amp;gt; || ? || &amp;lt;small&amp;gt;50757686696033684694106416498959861492⋅10&amp;lt;sup&amp;gt;280&amp;lt;/sup&amp;gt;&amp;amp;nbsp;-&amp;amp;nbsp;9&amp;lt;/small&amp;gt; || &amp;lt;small&amp;gt;14107593985876801556467795907102490773681⋅10&amp;lt;sup&amp;gt;280&amp;lt;/sup&amp;gt;&amp;amp;nbsp;-&amp;amp;nbsp;10&amp;lt;/small&amp;gt; || ? || ? || ?&lt;br /&gt;
|}&lt;br /&gt;
By the previous section, no such &#039;&#039;x&#039;&#039; exists for &#039;&#039;n&#039;&#039; &amp;gt; 20.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Estimating the density of Harshad numbers ==&lt;br /&gt;
&lt;br /&gt;
If we let &#039;&#039;N&#039;&#039;(&#039;&#039;x&#039;&#039;) denote the number of Harshad numbers ≤ x, then for any given ε &amp;gt; 0,&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;x^{1-\varepsilon} \ll N(x) \ll \frac{x\log\log x}{\log x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
as shown by [[Jean-Marie De Koninck]] and Nicolas Doyon;&amp;lt;ref&amp;gt;{{citation|first1=Jean-Marie|last1=De Koninck|first2=Nicolas|last2=Doyon|title=On the number of Niven numbers up to &#039;&#039;x&#039;&#039;|journal=[[Fibonacci Quarterly]]|volume=41|issue=5|date=November 2003|pages=431–440}}.&amp;lt;/ref&amp;gt; furthermore, De Koninck, Doyon and Kátai&amp;lt;ref&amp;gt;{{citation|first1=Jean-Marie|last1=De Koninck|first2=Nicolas|last2=Doyon|first3=I.|last3=Katái|title=On the counting function for the Niven numbers|journal=[[Acta Arithmetica]]|volume=106|year=2003|pages=265–275}}.&amp;lt;/ref&amp;gt; proved that&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;N(x)=(c+o(1))\frac{x}{\log x}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &#039;&#039;c&#039;&#039; = (14/27)  log 10 ≈ 1.1939.&lt;br /&gt;
&lt;br /&gt;
== Nivenmorphic numbers ==&lt;br /&gt;
&lt;br /&gt;
A &#039;&#039;&#039;Nivenmorphic number&#039;&#039;&#039; or &#039;&#039;&#039;Harshadmorphic number&#039;&#039;&#039; for a given number base is an integer &#039;&#039;t&#039;&#039; such that there exists some Harshad number &#039;&#039;N&#039;&#039; whose [[digit sum]] is &#039;&#039;t&#039;&#039;, and &#039;&#039;t&#039;&#039;, written in that base, terminates &#039;&#039;N&#039;&#039; written in the same base.&lt;br /&gt;
&lt;br /&gt;
For example, 18 is a Nivenmorphic number for base 10:&lt;br /&gt;
&lt;br /&gt;
  16218 is a Harshad number&lt;br /&gt;
  16218 has 18 as digit sum&lt;br /&gt;
     18 terminates 16218&lt;br /&gt;
&lt;br /&gt;
Sandro Boscaro determined that for base 10 all positive integers are Nivenmorphic numbers except [[11 (number)|11]].&amp;lt;ref&amp;gt;{{citation|first=Sandro|last=Boscaro|title=Nivenmorphic integers|journal=[[Journal of Recreational Mathematics]]|volume=28|issue=3|year=1996–1997|pages=201–205}}.&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Multiple Harshad numbers ==&lt;br /&gt;
{{harvtxt|Bloem|2005}} defines a &#039;&#039;multiple Harshad number&#039;&#039; as a Harshad number that, when divided by the sum of its digits, produces another Harshad number.&amp;lt;ref&amp;gt;{{citation|first=E.|last=Bloem|year=2005|title=Harshad numbers|journal=[[Journal of Recreational Mathematics]]|volume=34|issue=2|page=128}}.&amp;lt;/ref&amp;gt;  He states that 6804 is &amp;quot;MHN-3&amp;quot; on the grounds that&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;&lt;br /&gt;
\begin{array}{l}&lt;br /&gt;
6804/18=378\\&lt;br /&gt;
378/18=21\\&lt;br /&gt;
21/3=7&lt;br /&gt;
\end{array}&lt;br /&gt;
&amp;lt;/math&amp;gt; &lt;br /&gt;
&lt;br /&gt;
and went on to show that 2016502858579884466176 is MHN-12. The number 10080000000000 = 1008·10&amp;lt;sup&amp;gt;10&amp;lt;/sup&amp;gt;, which is smaller, is also MHN-12. In general, 1008·10&amp;lt;sup&amp;gt;&#039;&#039;n&#039;&#039;&amp;lt;/sup&amp;gt; is MHN-(&#039;&#039;n&#039;&#039;+2).&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
== External links ==&lt;br /&gt;
* [http://www.harshad-numbers.com/en/ Harshad Numbers]&lt;br /&gt;
* [http://www.numbers-of-harshad.com/ Numbers of Harshad]&lt;br /&gt;
&lt;br /&gt;
{{Classes of natural numbers}}&lt;br /&gt;
[[Category:Base-dependent integer sequences]]&lt;/div&gt;</summary>
		<author><name>46.226.190.2</name></author>
	</entry>
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