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Title: Note on structure formation from cosmic string wakes

Abstract

The search for cosmic strings has been of renewed interest with the advent of precision cosmology. In this note we give a quantitative description of the nonlinear matter density fluctuations that can form from a scaling network of cosmic string wakes. Specifically, we compute the distribution of dark matter halos. These halos would possess strong correlations in position space that should have survived until today. We also discuss the challenges involved in their detection due to their small size and the complex dynamics of their formation.

Authors:
;  [1]
  1. Physics Department, McGill University, 3600 University Street, Montreal, QC, H3A 2T8 (Canada)
Publication Date:
OSTI Identifier:
22282846
Resource Type:
Journal Article
Journal Name:
Journal of Cosmology and Astroparticle Physics
Additional Journal Information:
Journal Volume: 2013; Journal Issue: 04; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 1475-7516
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; ACCURACY; ASTROPHYSICS; CORRELATIONS; COSMOLOGY; DENSITY; FLUCTUATIONS; NONLINEAR PROBLEMS; NONLUMINOUS MATTER; SPACE; STRING MODELS

Citation Formats

Duplessis, Francis, and Brandenberger, Robert. Note on structure formation from cosmic string wakes. United States: N. p., 2013. Web. doi:10.1088/1475-7516/2013/04/045.
Duplessis, Francis, & Brandenberger, Robert. Note on structure formation from cosmic string wakes. United States. https://doi.org/10.1088/1475-7516/2013/04/045
Duplessis, Francis, and Brandenberger, Robert. 2013. "Note on structure formation from cosmic string wakes". United States. https://doi.org/10.1088/1475-7516/2013/04/045.
@article{osti_22282846,
title = {Note on structure formation from cosmic string wakes},
author = {Duplessis, Francis and Brandenberger, Robert},
abstractNote = {The search for cosmic strings has been of renewed interest with the advent of precision cosmology. In this note we give a quantitative description of the nonlinear matter density fluctuations that can form from a scaling network of cosmic string wakes. Specifically, we compute the distribution of dark matter halos. These halos would possess strong correlations in position space that should have survived until today. We also discuss the challenges involved in their detection due to their small size and the complex dynamics of their formation.},
doi = {10.1088/1475-7516/2013/04/045},
url = {https://www.osti.gov/biblio/22282846}, journal = {Journal of Cosmology and Astroparticle Physics},
issn = {1475-7516},
number = 04,
volume = 2013,
place = {United States},
year = {Mon Apr 01 00:00:00 EDT 2013},
month = {Mon Apr 01 00:00:00 EDT 2013}
}