Effect of small-scale structure on the dynamics of cosmic strings

1990 ◽  
Vol 41 (10) ◽  
pp. 3038-3040 ◽  
Author(s):  
Alexander Vilenkin
Keyword(s):  
Cosmic Strings ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

Evolution of small-scale structure on cosmic strings

1991 ◽  
Vol T36 ◽  
pp. 153-166 ◽  
Author(s):  
T W B Kibble ◽  
E Copeland
Keyword(s):  
Cosmic Strings ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

Small-scale structure on cosmic strings

1993 ◽  
Vol 48 (8) ◽  
pp. R3422-R3426 ◽  
Author(s):  
Daren Austin
Keyword(s):  
Cosmic Strings ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

scholarly journals Models for small-scale structure on cosmic strings. II. Scaling and its stability

2016 ◽  
Vol 94 (9) ◽  
Author(s):  
J. P. P. Vieira ◽  
C. J. A. P. Martins ◽  
E. P. S. Shellard
Keyword(s):  
Cosmic Strings ◽  
Scale Structure ◽  
Small Scale ◽  
Small Scale Structure

scholarly journals ACCRETION OF HOT DARK MATTER ONTO SLOWLY MOVING COSMIC STRINGS

1995 ◽  
Vol 04 (06) ◽  
pp. 711-721 ◽  
Author(s):  
ANTHONY N. AGUIRRE ◽  
ROBERT H. BRANDENBERGER
Keyword(s):  
Dark Matter ◽  
Line Source ◽  
Cosmic Strings ◽  
Unit Length ◽  
String Tension ◽  
Scale Structure ◽  
Coarse Grained ◽  
Small Scale ◽  
Translational Velocity ◽  
Small Scale Structure

Cosmic strings with small-scale structure have a coarse-grained mass per unit length μ which is larger than the string tension. This leads to an effective Newtonian gravitational line source and to a characteristic translational velocity which is smaller than for strings without small-scale structure. Here, the accretion of hot dark matter onto such strings is studied by means of the Zel’dovich approximation. We find that clustering is greatly enhanced by the Newtonian line source. In the limit of vanishing translational velocity, the first nonlinear filaments form at a redshift of greater than 100 for standard values of μ.

Sign in / Sign up

Export Citation Format

Share Document