Monte Carlo simulation of texture formation
- 15 December 1991
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 44 (12) , 3749-3759
- https://doi.org/10.1103/physrevd.44.3749
Abstract
The formation of global texture in both two and three spatial dimensions is studied using Monte Carlo techniques. We calculate the probability of texture formation for critical windings in the range [½, 1], finding for three dimensions average values per correlation volume in the range [0.017, 0.045], which is in good agreement with previous dynamical simulations. We discuss cosmological structures seeded by texture collapse.Keywords
This publication has 21 references indexed in Scilit:
- Clustering of cosmological defects at the time of formationPhysics Letters B, 1991
- Large-scale structure in a texture-seeded cold dark matter cosmogonyThe Astrophysical Journal, 1991
- Initial conditions for global texturePhysics Letters B, 1991
- Importance of boundary conditions for topological production of textures and SkyrmionsPhysical Review D, 1991
- Global texture and the microwave backgroundPhysical Review Letters, 1990
- The large-scale structure of the universe: Turbulence, intermittency, structures in a self-gravitating mediumReviews of Modern Physics, 1989
- Projection contamination in cluster catalogs - Are the Abell redshift sample correlations significant?The Astrophysical Journal, 1989
- Cosmic texture and the microwave backgroundPhysical Review D, 1987
- Texture: A cosmological topological defectPhysical Review D, 1987
- THE FUNCTIONS OF SCHLÄFLI AND LOBATSCHEFSKYThe Quarterly Journal of Mathematics, 1935