Elastic properties of anisotropic domain wall lattices

被引:17
作者
Battye, Richard A. [1 ]
Chachoua, Elie
Moss, Adam
机构
[1] Univ Manchester, Sch Phys & Astron, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[2] Observ Paris, LuTh, F-92195 Meudon, France
来源
PHYSICAL REVIEW D | 2006年 / 73卷 / 12期
关键词
D O I
10.1103/PhysRevD.73.123528
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Interest in the elastic properties of regular lattices constructed from domain walls has recently been motivated by cosmological applications as solid dark energy. This work investigates the particularly simple examples of triangular, hexagonal, and square lattices in two dimensions and a variety of more complicated lattices in three dimensions which have cubic symmetry. The relevant rigidity coefficients are computed taking into account nonaffine perturbations where necessary, and these are used to evaluate the propagation velocity for any macroscopic scale perturbation mode. Using this information we assess the stability of the various configurations. It is found that triangular lattices are isotropic and stable, whereas hexagonal lattices are unstable. It is argued that the simple orthonormal cases of a square in two dimensions and the cube in three are stable, except to perturbations of infinite extent. We also find that the more complicated case of a rhombic dodecahedral lattice is stable, except to the existence of transverse modes in certain directions, whereas a lattice formed from truncated octahedra is unstable.
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页数:12
相关论文
共 15 条
[1]  
BATTYE AR, 2005, J COSMOL ASTROPART P, P1
[2]   Rigidity and stability of cold dark solid universe model [J].
Battye, RA ;
Carter, B ;
Chachoua, E ;
Moss, A .
PHYSICAL REVIEW D, 2005, 72 (02) :1-6
[3]  
BATTYE RA, ASTROPH9908047
[4]  
BATTYE RA, UNPUB STABILITY DOMA, P5005
[5]  
Brakke K., 1992, EXP MATH, V1, P141, DOI DOI 10.1080/10586458.1992.10504253
[6]   Is the dark matter a solid? art. no. 043505 [J].
Bucher, M ;
Spergel, D .
PHYSICAL REVIEW D, 1999, 60 (04)
[7]   Covariant Newtonian and relativistic dynamics of (magneto)-elastic solid model for neutron star crust [J].
Carter, B ;
Chachoua, E ;
Chamel, N .
GENERAL RELATIVITY AND GRAVITATION, 2006, 38 (01) :83-119
[8]   SPEED OF SOUND IN A HIGH-PRESSURE GENERAL-RELATIVISTIC SOLID [J].
CARTER, B .
PHYSICAL REVIEW D, 1973, 7 (06) :1590-1593
[9]   FOUNDATIONS OF GENERAL RELATIVISTIC HIGH-PRESSURE ELASTICITY THEORY [J].
CARTER, B ;
QUINTANA, H .
PROCEEDINGS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL AND PHYSICAL SCIENCES, 1972, 331 (1584) :57-&
[10]  
CARTER B, 1983, P GRAV RAD HOUCH SUM, P455