Results 1  10
of
2,587
Integermagic spectra of amalgamations of stars and cycles
 Ars Combin
, 2003
"... Abstract. For any positive integer k, a graph G = (V, E) is said to be Zkmagic if there exists a labeling l: E(G) − → Zk − {0} such that the induced vertex set labeling l +: V (G) − → Zk defined by l + (v) = � { l(uv) : uv ∈ E(G)} is a constant map. For a given graph G, the set of all h ∈ Z+ for ..."
Abstract

Cited by 8 (2 self)
 Add to MetaCart
+ for which G is Zhmagic is called the integermagic spectrum of G and is denoted by IM(G). In this paper, we will determine the integermagic spectra of the graphs which are formed by the amalgamation of stars and cycles. In particular, we will provide examples of graphs that for a given n> 2
IntegerMagic Spectra of Functional Extensions of Graphs
"... For any kEN, a graph G = (V, E) is said to be;:z kmagic if there exists a labeling Z: E(G)+;:z k {OJ such that the induced vertex set labeling Z+: V (G)+;:z k defined by Z+(v) = L Z(uv) uvEE(G) is a constant map. For a given graph G, the set of all kEN for which G is;:z kmagic is called the i ..."
Abstract

Cited by 1 (1 self)
 Add to MetaCart
the integermagic spectrum of G and is denoted by IM(G). In this paper we will consider the functional extensions of Pn (n = 2,3,4) and will determine their integermagic spectra.
Time Discounting and Time Preference: A Critical Review
 Journal of Economic Literature
, 2002
"... www.people.cornell.edu/pages/edo1/. ..."
Wireless Communications
, 2005
"... Copyright c ○ 2005 by Cambridge University Press. This material is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University ..."
Abstract

Cited by 1129 (32 self)
 Add to MetaCart
Copyright c ○ 2005 by Cambridge University Press. This material is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University
Functional Phonology  Formalizing the interactions between articulatory and perceptual drives
, 1998
"... ..."
3D Sound for Virtual Reality and Multimedia
, 2000
"... This paper gives HRTF magnitude data in numerical form for 43 frequencies between 0.212 kHz, the average of 12 studies representing 100 different subjects. However, no phase data is included in the tables; group delay simulation would need to be included in order to account for ITD. In 3D sound ..."
Abstract

Cited by 282 (5 self)
 Add to MetaCart
This paper gives HRTF magnitude data in numerical form for 43 frequencies between 0.212 kHz, the average of 12 studies representing 100 different subjects. However, no phase data is included in the tables; group delay simulation would need to be included in order to account for ITD. In 3D sound applications intended for many users, we want might want to use HRTFs that represent the common features of a number of individuals. But another approach might be to use the features of a person who has desirable HRTFs, based on some criteria. (One can sense a future 3D sound system where the pinnae of various famous musicians are simulated.) A set of HRTFs from a good localizer (discussed in Chapter 2) could be used if the criterion were localization performance. If the localization ability of the person is relatively accurate or more accurate than average, it might be reasonable to use these HRTF measurements for other individuals. The Convolvotron 3D audio system (Wenzel, Wightman, and Foster, 1988) has used such sets particularly because elevation accuracy is affected negatively when listening through a bad localizers ears (see Wenzel, et al., 1988). It is best when any single nonindividualized HRTF set is psychoacoustically validated using a 113 statistical sample of the intended user population, as shown in Chapter 2. Otherwise, the use of one HRTF set over another is a purely subjective judgment based on criteria other than localization performance. The technique used by Wightman and Kistler (1989a) exemplifies a laboratorybased HRTF measurement procedure where accuracy and replicability of results were deemed crucial. A comparison of their techniques with those described in Blauert (1983), Shaw (1974), Mehrgardt and Mellert (1977), Middlebrooks, Makous, and Gree...
Particle dark matter: Evidence, candidates and constraints
, 2005
"... In this review article, we discuss the current status of particle dark matter, including experimental evidence and theoretical motivations. We discuss a wide array of candidates for particle dark matter, but focus on neutralinos in models of supersymmetry and KaluzaKlein dark matter in models of un ..."
Abstract

Cited by 201 (2 self)
 Add to MetaCart
In this review article, we discuss the current status of particle dark matter, including experimental evidence and theoretical motivations. We discuss a wide array of candidates for particle dark matter, but focus on neutralinos in models of supersymmetry and KaluzaKlein dark matter in models of universal extra dimensions. We devote much of our attention to direct and indirect detection techniques, the constraints placed by these
Results 1  10
of
2,587