Relative baryon-dark matter velocities in cosmological zoom simulations

Author:

Conaboy Luke12ORCID,Iliev Ilian T1ORCID,Fialkov Anastasia34,Dixon Keri L56ORCID,Sullivan David1ORCID

Affiliation:

1. Astronomy Centre, Department of Physics and Astronomy, University of Sussex , Brighton, BN1 9QH , UK

2. School of Physics and Astronomy, University of Nottingham, University Park , Nottingham, NG7 2RD , UK

3. Institute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB3 0HA , UK

4. Kavli Institute for Cosmology, University of Cambridge , Madingley Road, Cambridge CB3 0HA , UK

5. New York University Abu Dhabi , PO Box 129188, Saadiyat Island, Abu Dhabi , United Arab Emirates

6. Center for Astro, Particle and Planetary Physics (CAP3), New York University Abu Dhabi , PO Box 129188, Saadiyat Island, Abu Dhabi , United Arab Emirates

Abstract

ABSTRACT Supersonic relative motion between baryons and dark matter due to the decoupling of baryons from the primordial plasma after recombination affects the growth of the first small-scale structures. Large box sizes (greater than a few hundred Mpc) are required to sample the full range of scales pertinent to the relative velocity, while the effect of the relative velocity is strongest on small scales (less than a few hundred kpc). This separation of scales naturally lends itself to the use of ‘zoom’ simulations, and here we present our methodology to self-consistently incorporate the relative velocity in zoom simulations, including its cumulative effect from recombination through to the start time of the simulation. We apply our methodology to a large-scale cosmological zoom simulation, finding that the inclusion of relative velocities suppresses the halo baryon fraction by 46–23 per cent between z = 13.6 and 11.2, in qualitative agreement with previous works. In addition, we find that including the relative velocity delays the formation of star particles by ∼20 Myr on average (of the order of the lifetime of a ∼9 M⊙ Population III star) and suppresses the final stellar mass by as much as 79 per cent at z = 11.2.

Funder

Science and Technology Facilities Council

Royal Society

BEIS

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3