Statistical bootstrap duality

1976 ◽  
Vol 14 (5) ◽  
pp. 1420-1424 ◽  
Author(s):  
S. Kogitz ◽  
R. K. Logan ◽  
S. Tanaka
1974 ◽  
Vol 63 ◽  
pp. 195-210
Author(s):  
Robert V. Wagoner

The results of improved calculations of the abundances of the nuclei produced in big-bang models of the early universe are presented. In addition to the standard model, other possible universes are considered, including the recent statistical bootstrap theory of Carlitz, Frautschi, and Nahm. Some conclusions which can be drawn about the nature of the early universe, depending upon whether the observed deuterium and helium are of galactic or cosmological origin, are presented.


2000 ◽  
Vol 38 (9) ◽  
pp. 3498-3501 ◽  
Author(s):  
J. Z. Zhang ◽  
M. Y. Fan ◽  
Y. M. Wu ◽  
P. E. Fournier ◽  
V. Roux ◽  
...  

To determine the phylogenetic position of two new rickettsial strains isolated from ticks in China, 16S ribosomal DNA,gltA, and ompA (apart from the tandem repeat units) genes were amplified by PCR and sequenced. The phylogenetic relationships between these strains and other rickettsiae were inferred from the comparison of sequences of the three genes by the parsimony, neighbor-joining, and maximum-likelihood methods. The results demonstrated that the 054 strain, a rickettsia pathogenic in humans, and the HL-93 strain were related and clustered together withRickettsia japonica. Significant statistical bootstrap values (100 and 92%) supported the nodes in this cluster. Based on previous genotypic and antigenic data and the phylogenetic analysis presented here, the 054 and HL-93 strains should be considered as new species, and we formally propose that they be named “Rickettsia heilongjiangii” and “Rickettsia hulinii,” respectively.


1997 ◽  
Vol 23 (12) ◽  
pp. 1921-1931 ◽  
Author(s):  
A S Kapoyannis ◽  
C N Ktorides ◽  
A D Panagiotou

1974 ◽  
Vol 76 (3) ◽  
pp. 453-476 ◽  
Author(s):  
M.I. Gorenstein ◽  
V.A. Miransky ◽  
V.P. Shelest ◽  
G.M. Zinovjev ◽  
H. Satz

1972 ◽  
Vol 5 (5) ◽  
pp. 1235-1235 ◽  
Author(s):  
C. J. Hamer ◽  
S. C. Frautschi

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