DIFFERENTIALS OF FUNCTIONS OF A SINGLE VARIABLE.

2019 ◽  
pp. 17-20
Author(s):  
Dennis M. Cates
Keyword(s):  
2019 ◽  
Vol 141 ◽  
pp. 41-46 ◽  
Author(s):  
F. Rahbarizadeh ◽  
D. Ahmadvand ◽  
S.M. Moghimi

1981 ◽  
Vol 34 (2) ◽  
pp. 383-389 ◽  
Author(s):  
PH. DELSARTE ◽  
Y. GENIN ◽  
Y. KAMP
Keyword(s):  

1980 ◽  
pp. 447-456
Author(s):  
David E. Hunt
Keyword(s):  

1970 ◽  
Vol 26 (3) ◽  
pp. 975-984
Author(s):  
Mary Juhan Larsen ◽  
Jerry C. Allen

Item performance on the Stanford-Binet by a sample ( n = 289) of Georgia children (CA = 5) and by equivalent-aged children used in the test standardization was compared in terms of 5 subject variables: race, sex, socioeconomic status, intelligence level, and community size. The Georgia Sample's performance exceeded ( p < .01) the norm group's performance on 62% of the items. The five subject variables were associated with these differences: among levels of the variables, variations occurred in the presence and direction of item performance differences; generally, more than one subject variable influenced item performance. These data affirm that certain variables confound intelligence test performance and that norms based on a single variable, like race, do not eliminate test biases.


2018 ◽  
Vol 15 (12) ◽  
pp. 1850212 ◽  
Author(s):  
K. Kleidis ◽  
V. K. Oikonomou

In this paper we will study the cosmological dynamical system of an [Formula: see text] gravity in the presence of a canonical scalar field [Formula: see text] with an exponential potential by constructing the dynamical system in a way that it is rendered autonomous. This feature is controlled by a single variable [Formula: see text], which when it is constant, the dynamical system is autonomous. We focus on the [Formula: see text] case which, as we demonstrate by using a numerical analysis approach, leads to an unstable de Sitter attractor, which occurs after [Formula: see text] [Formula: see text]-foldings. This instability can be viewed as a graceful exit from inflation, which is inherent to the dynamics of de Sitter attractors.


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