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Impact of the relative motion between the dark matter and baryons on the first stars: semi-analytical modelling

Fialkov, Anastasia and Barkana, Rennan and Tseliakhovich, Dmitriy and Hirata, Christopher M. (2012) Impact of the relative motion between the dark matter and baryons on the first stars: semi-analytical modelling. Monthly Notices of the Royal Astronomical Society, 424 (2). pp. 1335-1345. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20120813-085311872

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Abstract

Recently the initial supersonic relative velocity between the dark matter and baryons was shown to have an important effect on galaxy formation at high redshift. We study the impact of this relative motion on the distribution of the star-forming haloes and on the formation redshift of the very first star. We include a new aspect of the relative velocity effect found in recent simulations by fitting their results to obtain the spatially varying minimum halo mass needed for molecular cooling. Thus, the relative velocities have three separate effects: suppression of the halo abundance, suppression of the gas content within each halo and boosting of the minimum cooling mass. We show that the two suppressions (of gas content and of halo abundance) are the primary effects on the small minihaloes that cannot form stars, while the cooling mass boost combines with the abundance suppression to produce order unity fluctuations in stellar density. We quantify the large-scale inhomogeneity of galaxies, finding that 68 per cent of the star formation (averaged on a 3 Mpc scale) is confined to 35 per cent of the volume at z= 20 (and just 18 per cent at z= 40). In addition, we estimate the first observable star to be formed at redshift z= 65 (t∼ 33 Myr) which includes a delay of Δz∼ 5 (Δt∼ 3.6 Myr) due to the relative velocity.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1111/j.1365-2966.2012.21318.x DOIUNSPECIFIED
http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2012.21318.x/abstractPublisherUNSPECIFIED
Additional Information:© 2012 The Authors. Monthly Notices of the Royal Astronomical Society © 2012 RAS. Accepted 2012 May 15. Received 2012 May 15; in original form 2011 October 11. Article first published online: 19 Jun 2012. This work was supported in part by European Research Council grant 203247 (for AF) and by Israel Science Foundation grant 823/09 (for RB). DT and CMH were supported by the National Science Foundation (AST-0807337) and the US Department of Energy (DE-FG03-92-ER40701). CMH was also supported by the David and Lucile Packard Foundation.
Group:TAPIR
Funders:
Funding AgencyGrant Number
European Research Council grant203247
Israel Science Foundation (ISF) 823/09
NSFAST-0807337
Department of Energy (DOE)DE-FG03-92-ER40701
David and Lucile Packard FoundationUNSPECIFIED
Subject Keywords: galaxies: formation; galaxies: high-redshift; cosmology: theory
Record Number:CaltechAUTHORS:20120813-085311872
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20120813-085311872
Official Citation:Fialkov, A., Barkana, R., Tseliakhovich, D. and Hirata, C. M. (2012), Impact of the relative motion between the dark matter and baryons on the first stars: semi-analytical modelling. Monthly Notices of the Royal Astronomical Society, 424: 1335–1345. doi: 10.1111/j.1365-2966.2012.21318.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:33112
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:13 Aug 2012 16:08
Last Modified:26 Mar 2014 01:00

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