Gravitational critical phenomena in the realm of the galaxies and Ising magnets

被引:13
作者
Hochberg, D
PerezMercader, J
机构
[1] Lab. de Astrofis. Espacial y Fis. F., 28080 Madrid
关键词
galaxy-to-galaxy correlation function;
D O I
10.1007/BF02113772
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the non-relativistic and quasi-static limit, it is possible to map exactly the system of galaxies in the observable universe onto an Ising magnet. Techniques from the theory of critical phenomena as applied to magnets can then be employed to calculate rigorously the galaxy-to-galaxy correlation function, whose critical exponent is predicted to be between 1.530 to 1.862, to be compared to the empirical/observational value of 1.6 to 1.8.
引用
收藏
页码:1427 / 1432
页数:6
相关论文
共 10 条
[1]  
Amit D. J., 1984, FIELD THEORY RENORMA
[2]  
BARBER MN, 1977, PHYS REP, V29, P1
[3]  
Binney J. J., 1992, The theory of critical phenomena, an introduction to the Renormalization Group
[4]  
CHAIKIN PM, 1995, PRINCIPLES CONDENSED, P483
[5]   THEORY OF DYNAMIC CRITICAL PHENOMENA [J].
HOHENBERG, PC ;
HALPERIN, BI .
REVIEWS OF MODERN PHYSICS, 1977, 49 (03) :435-479
[6]   GALAXY CORRELATIONS ON LARGE SCALES [J].
MADDOX, SJ ;
EFSTATHIOU, G ;
SUTHERLAND, WJ ;
LOVEDAY, J .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1990, 242 (02) :P43-&
[7]  
PEEBLES PJE, 1993, PRINCIPLES PHYSICAL
[8]  
PEREZMERCADER J, 1995, LAUR951055
[9]  
SHANE CD, 1967, PUB LICK OBS 1, V22
[10]   NON-LAGRANGIAN MODELS OF CURRENT ALGEBRA [J].
WILSON, KG .
PHYSICAL REVIEW, 1969, 179 (05) :1499-&