Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Smith–Volterra–Cantor set
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
{{Short description|Set of real numbers in mathematics}} [[Image:Smith-Volterra set.png|thumb|right|256px|After black intervals have been removed, the white points which remain are a nowhere dense set of measure 1/2.]] In [[mathematics]], the '''Smith–Volterra–Cantor set''' ('''SVC'''), '''ε-Cantor set''',<ref>Aliprantis and Burkinshaw (1981), Principles of Real Analysis</ref> or '''fat Cantor set''' is an example of a set of points on the [[real line]] that is [[nowhere dense]] (in particular it contains no [[interval (mathematics)|interval]]s), yet has positive [[measure (mathematics)|measure]]. The Smith–Volterra–Cantor set is named after the [[mathematician]]s [[Henry John Stephen Smith|Henry Smith]], [[Vito Volterra]] and [[Georg Cantor]]. In an 1875 paper, Smith discussed a nowhere-dense set of positive measure on the real line,<ref>[[Henry John Stephen Smith|Smith, Henry J.S.]] (1874). "[https://babel.hathitrust.org/cgi/pt?id=ucm.5324906759;view=1up;seq=148 On the integration of discontinuous functions]". Proceedings of the London Mathematical Society. First series. 6: 140–153 </ref> and Volterra introduced a similar example in 1881.<ref>{{Cite journal |last1=Ponce Campuzano |first1=Juan |last2=Maldonado |first2=Miguel |date=2015 |title=Vito Volterra's construction of a nonconstant function with a bounded, non Riemann integrable derivative |journal=BSHM Bulletin Journal of the British Society for the History of Mathematics |volume=30 |issue=2 |pages=143–152 |doi=10.1080/17498430.2015.1010771|s2cid=34546093 }}</ref> The Cantor set as we know it today followed in 1883. The Smith–Volterra–Cantor set is [[Homeomorphism|topologically equivalent]] to the [[Cantor set|middle-thirds Cantor set]].
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)