ETHOS-an effective theory of structure formation: From dark particle physics to the matter distribution of the Universe

被引:176
作者
Cyr-Racine, Francis-Yan [1 ,2 ]
Sigurdson, Kris [3 ,4 ]
Zavala, Jesus [5 ]
Bringmann, Torsten [6 ]
Vogelsberger, Mark [7 ]
Pfrommer, Christoph [8 ]
机构
[1] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[2] CALTECH, Pasadena, CA 91125 USA
[3] Inst Adv Study, Sch Nat Sci, Olden Lane, Princeton, NJ 08540 USA
[4] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[5] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
[6] Univ Oslo, Dept Phys, Box 1048, NO-0316 Oslo, Norway
[7] MIT, Dept Phys, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
[8] Heidelberg Inst Theoret Studies, Schloss Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany
基金
加拿大自然科学与工程研究理事会; 新加坡国家研究基金会;
关键词
LARGE-SCALE STRUCTURE; COSMOLOGICAL SIMULATIONS; GALAXIES; CONSTRAINTS; PERTURBATIONS; EVOLUTION; CORES; MILKY; CDM;
D O I
10.1103/PhysRevD.93.123527
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We formulate an effective theory of structure formation (ETHOS) that enables cosmological structure formation to be computed in almost any microphysical model of dark matter physics. This framework maps the detailed microphysical theories of particle dark matter interactions into the physical effective parameters that shape the linear matter power spectrum and the self-interaction transfer cross section of nonrelativistic dark matter. These are the input to structure formation simulations, which follow the evolution of the cosmological and galactic dark matter distributions. Models with similar effective parameters in ETHOS but with different dark particle physics would nevertheless result in similar dark matter distributions. We present a general method to map an ultraviolet complete or effective field theory of low-energy dark matter physics into parameters that affect the linear matter power spectrum and carry out this mapping for several representative particle models. We further propose a simple but useful choice for characterizing the dark matter self-interaction transfer cross section that parametrizes self-scattering in structure formation simulations. Taken together, these effective parameters in ETHOS allow the classification of dark matter theories according to their structure formation properties rather than their intrinsic particle properties, paving the way for future simulations to span the space of viable dark matter physics relevant for structure formation.
引用
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页数:27
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