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{{Short description|Function from the limited hyperreal to the real numbers}}
In [[
The standard part function was first defined by [[Abraham Robinson]] who used the notation <math>{}^{\circ}x</math> for the standard part of a hyperreal <math>x</math> (see Robinson 1974). This concept plays a key role in defining the concepts of the calculus, such as continuity, the derivative, and the integral, in [[nonstandard analysis]]. The latter theory is a rigorous formalization of calculations with [[infinitesimal]]s. The standard part of ''x'' is sometimes referred to as its '''shadow'''.<ref>{{cite journal |last1=Bascelli |first1=Tiziana |last2=Bottazzi |first2=Emanuele |last3=Herzberg |first3=Frederik |last4=Kanovei |first4=Vladimir |last5=Katz |first5=Karin U. |last6=Katz |first6=Mikhail G. |last7=Nowik |first7=Tahl |last8=Sherry |first8=David |last9=Shnider |first9=Steven |title=Fermat, Leibniz, Euler, and the Gang: The True History of the Concepts of Limit and Shadow |journal=Notices of the American Mathematical Society |date=1 September 2014 |volume=61 |issue=8 |pages=848 |doi=10.1090/noti1149 |url=https://community.ams.org/journals/notices/201408/rnoti-p848.pdf}}</ref>
==Definition==
[[File:Standard part function with two continua.
Nonstandard analysis deals primarily with the pair <math>\R \subseteq {}^*\R</math>, where the [[hyperreal number|hyperreal]]s
▲Nonstandard analysis deals primarily with the [[hyperreal number|hyperreal]] line. The hyperreal line is an extension of the real line, containing infinitesimals, in addition to the reals. In the hyperreal line every real number has a collection of numbers (called a [[monad (mathematics)|monad]]) of hyperreals infinitely close to it. The standard part function associates to a [[Wikt:finite|finite]] [[hyperreal number|hyperreal]] ''x'', the unique standard real number ''x<sub>0</sub>'' which is infinitely close to it. The relationship is expressed symbolically by writing
The standard part of any [[infinitesimal]] is 0. Thus if ''N'' is an infinite [[hypernatural]], then
▲:<math>\,\mathrm{st}(x)=x_0.</math>
▲The standard part of any [[infinitesimal]] is 0. Thus if ''N'' is an infinite [[hypernatural]], then 1/''N'' is infinitesimal, and st(1/''N'') = 0.
If a hyperreal <math>u</math> is represented by a Cauchy sequence <math>\langle u_n:n\in\mathbb{N} \rangle</math> in the [[ultrapower]] construction, then
:<math>\
More generally, each finite <math>u \in {}^*\R</math> defines a [[Dedekind cut]] on the subset <math>\R\subseteq{}^*\R</math> (via the total order on <math>{}^{\ast}\R</math>) and the corresponding real number is the standard part of ''u''.
==Not internal==
The standard part function "st" is not defined by an [[internal set]]. There are several ways of explaining this. Perhaps the simplest is that its ___domain L, which is the collection of limited (i.e. finite) hyperreals, is not an internal set. Namely, since L is bounded (by any infinite hypernatural, for instance), L would have to have a least upper bound if L were internal, but L doesn't have a least upper bound. Alternatively, the range of "st" is <math>\
==Applications==
All the traditional notions of calculus can be expressed in terms of the standard part function, as follows.
The standard part function is used to define the derivative of a function ''f''. If ''f'' is a real function, and ''h'' is infinitesimal, and if ''f''′(''x'') exists, then▼
===Derivative===
▲The standard part function is used to define the derivative of a function ''f''. If ''f'' is a real function, and ''h'' is infinitesimal, and if ''f''
:<math>f'(x) = \operatorname{st}\left(\frac {f(x+h)-f(x)}h\right).</math>
Alternatively, if <math>y=f(x)</math>, one takes an infinitesimal increment <math>\Delta x</math>, and computes the corresponding <math>\Delta y=f(x+\Delta x)-f(x)</math>. One forms the ratio <math display="inline">\frac{\Delta y}{\Delta x}</math>. The derivative is then defined as the standard part of the ratio:
:<math>\frac{dy}{dx}=\operatorname{st}\left( \frac{\Delta y}{\Delta x} \right) .</math>
==
Given a function <math>f</math> on <math>[a,b]</math>, one defines the integral <math display="inline">\int_a^b f(x)\,dx</math> as the standard part of an infinite Riemann sum <math>S(f,a,b,\Delta x)</math> when the value of <math>\Delta x</math> is taken to be infinitesimal, exploiting a [[hyperfinite set|hyperfinite]] partition of the interval [''a'',''b''].
{{Reflist}}▼
===Limit===
Given a sequence <math>(u_n)</math>, its limit is defined by <math display="inline">\lim_{n\to\infty} u_n = \operatorname{st}(u_H)</math> where <math>H \in {}^*\N \setminus \N</math> is an infinite index. Here the limit is said to exist if the standard part is the same regardless of the infinite index chosen.
===Continuity===
A real function <math>f</math> is continuous at a real point <math>x</math> if and only if the composition <math>\operatorname{st}\circ f</math> is ''constant'' on the [[halo (mathematics)|halo]] of <math>x</math>. See [[microcontinuity]] for more details.
==See also==
*[[Adequality]]
*[[
==
▲{{Reflist}}
*[[H. Jerome Keisler]]: ''[[Elementary Calculus: An Infinitesimal Approach]]''. First edition 1976; 2nd edition 1986. (This book is now out of print. The publisher has reverted the copyright to the author, who has made available the 2nd edition in .pdf format available for downloading at http://www.math.wisc.edu/~keisler/calc.html.)▼
==Further reading==
▲*[[H. Jerome Keisler]]
*[[Abraham Robinson]]. Non-standard analysis. Reprint of the second (1974) edition. With a foreword by [[Wilhelmus A. J. Luxemburg]]. Princeton Landmarks in Mathematics. Princeton University Press, Princeton, NJ, 1996. xx+293 pp. {{isbn|0-691-04490-2}}
{{Infinitesimals}}
[[Category:Calculus]]
[[Category:
[[Category:Real closed field]]
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