Published June 15, 2006
| Version v1
Journal article
Structure formation in the quasispherical Szekeres model
Creators
- 1. Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Bartycka 18, 00-716 Warsaw (Poland)
Description
Structure formation in the Szekeres model is investigated. Since the Szekeres model is an inhomogeneous model with no symmetries, it is possible to examine the interaction of neighboring structures and its impact on the growth of a density contrast. It has been found that the mass flow from voids to clusters enhances the growth of the density contrast. In the model presented here, the growth of the density contrast is almost 8 times faster than in the linear approach
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.73.123508;
- arXiv
- arXiv:astro-ph/0604490v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 73
- Journal Issue
- 12
- Journal Page Range
- p. 123508-123508.8
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37078431
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- COSMOLOGY; DENSITY; EINSTEIN FIELD EQUATIONS; GALAXY CLUSTERS; MASS; SPACE-TIME; SYMMETRY
- Descriptors DEC
- EQUATIONS; FIELD EQUATIONS; PHYSICAL PROPERTIES
Optional Information
- Notes
- (c) 2006 The American Physical Society