CaltechAUTHORS
  A Caltech Library Service

Dark Matter Interactions, Helium, and the Cosmic Microwave Background

de Putter, Roland and Doré, Olivier and Gleyzes, Jérôme and Green, Daniel and Meyers, Joel (2019) Dark Matter Interactions, Helium, and the Cosmic Microwave Background. Physical Review Letters, 122 (4). Art. No. 041301. ISSN 0031-9007. https://resolver.caltech.edu/CaltechAUTHORS:20190129-155840930

[img] PDF - Published Version
See Usage Policy.

320Kb
[img] PDF - Submitted Version
See Usage Policy.

725Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190129-155840930

Abstract

The cosmic microwave background (CMB) places a variety of model-independent constraints on the strength interactions of the dominant component of dark matter with the standard model. Percent-level subcomponents of the dark matter can evade the most stringent CMB bounds by mimicking the behavior of baryons, allowing for larger couplings and novel experimental signatures. However, in this Letter, we will show that such tightly coupled subcomponents leave a measurable imprint on the CMB that is well approximated by a change to the helium fraction, Y_(He). Using the existing CMB constraint on Y_(He), we derive a new upper limit on the fraction of tightly coupled dark matter, f_(TCDM), of f_(TCDM) < 0.006 (95% C.I.). We show that future CMB experiments can reach f_(TCDM) < 0.001 (95% C.I.) and confirm that the bounds derived in this way agree with the results of a complete analysis. These bounds provide an example of how CMB constraints on Y_(He) have applications beyond studying big bang nucleosynthesis, since tightly coupled dark matter plays no direct role in the formation of light nuclei. We briefly comment on the implications for model building, including millicharged dark matter.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/physrevlett.122.041301DOIArticle
https://arxiv.org/abs/1805.11616arXivDiscussion Paper
ORCID:
AuthorORCID
Doré, Olivier0000-0002-5009-7563
Additional Information:© 2019 American Physical Society. Received 1 June 2018; revised manuscript received 12 December 2018; published 29 January 2019. We thank Yacine Ali-Haïmoud, Kimberly Boddy, and Surjeet Rajendran for helpful conversations. We acknowledge the use of camb [25], class [26], and CosmoMC [31]. R. d. P. and O. D. acknowledge the generous support from the Heising-Simons Foundation.
Funders:
Funding AgencyGrant Number
Heising-Simons FoundationUNSPECIFIED
Issue or Number:4
Record Number:CaltechAUTHORS:20190129-155840930
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190129-155840930
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:92512
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:30 Jan 2019 00:08
Last Modified:03 Oct 2019 20:45

Repository Staff Only: item control page