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Stern polynomialsKlavžar, Sandi ; Milutinović, Uroš ; Petr, CirilSternovi polinomi ▫$B_k(t)$▫, ▫$k \ge 0$▫, ▫$t \in \RR$▫, so vpeljani na naslednji način: ▫$B_0(t) = 0$▫, ▫$B_1(t) = 1$▫, ▫$B_{2n}(t) = tB_n(t)$▫ in ▫$B_{2n+1}(t) = B_{n+1}(t) + B_n(t)$▫. Pokazano ... je, da ima ▫$B_n(t)$▫ enostavno eksplicitno reprezentacijo s hiperebinarnimi reprezentacijami ▫$n-1$▫ in da je odvod ▫$B'_{2n-1}(0)$▫ enak številu enic v standardni Grayjevi kodi za ▫$n-1$▫. Dokazano je tudi, da je stopnja polinoma ▫$B_n(t)$▫ enaka razliki med dolžino in težo nesosednje predstavitve števila ▫$n$▫.Source: Preprint series. - ISSN 1318-4865 (Vol. 43, št. 994, 2005, str. 1-11)Type of material - article, component partPublish date - 2005Language - englishCOBISS.SI-ID - 13805913
Author
Klavžar, Sandi |
Milutinović, Uroš |
Petr, Ciril
Topics
matematika |
Sternovo (dvoatomsko) zaporedje |
Sternovi polinomi |
hiperbinarna reprezentacija |
standardna Grayjeva koda |
nesosednja predstavitev |
mathematics |
Stern (diatomic) sequence |
Stern polynomials |
hyperbinary representation |
standard Gray code |
non-adjacent form
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Database name | Field | Year |
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Klavžar, Sandi | 05949 |
Milutinović, Uroš | 08727 |
Petr, Ciril | 16013 |
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