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The warped dark sector

Brax, Philippe and Fichet, Sylvain and Tanedo, Philip (2019) The warped dark sector. Physics Letters B, 798 . Art. No. 135012. ISSN 0370-2693. https://resolver.caltech.edu/CaltechAUTHORS:20191011-110521505

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Abstract

Five-dimensional braneworld constructions in anti-de Sitter space naturally lead to dark sector scenarios in which parts of the dark sector vanish at high 4d momentum or temperature. In the language of modified gravity, such feature implies a new mechanism for hiding light scalars, as well as the possibility of UV-completing chameleon-like effective theories. In the language of dark matter phenomenology, the high-energy behavior of the mediator sector changes dark matter observational complementarity. A multitude of signatures—including exotic ones—are present from laboratory to cosmological scales, including long-range forces with non-integer behavior, periodic signals at colliders, “soft bombs” events well-known from conformal theories, as well as a dark phase transition and a typically small amount of dark radiation.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1016/j.physletb.2019.135012DOIArticle
https://arxiv.org/abs/1906.02199arXivDiscussion Paper
Additional Information:© 2019 Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3. Received 9 July 2019, Revised 5 September 2019, Accepted 5 October 2019, Available online 11 October 2019. We thank Nathaniel Craig, Csaba Csáki, Gabriel Lee, Hai-Bo Yu, Stefania Gori, Gordan Krnjaic, Mark Wise, Prashant Saraswat, Eric Perlmutter and David Poland for discussions. PT is supported by the DOE grant DE-SC/0008541. PT thanks the Kavli Institute for Theoretical Physics (Grant No. NSF PHY-1748958) for its hospitality during the completion of this work. SF is supported by the São Paulo Research Foundation (FAPESP) under grants #2011/11973, #2014/21477-2 and #2018/11721-4. SF thanks Orsay University for hospitality and funding. This work is supported in part by the EU Horizon 2020 research and innovation programme under the Marie-Sklodowska grant No. 690575. This article is based upon work related to the COST Action CA15117 (CANTATA) supported by COST (European Cooperation in Science and Technology).
Group:Walter Burke Institute for Theoretical Physics
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-SC/0008541
NSFPHY-1748958
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)2011/11973
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)2014/21477-2
Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)2018/11721-4
Orsay UniversityUNSPECIFIED
Marie Curie Fellowship690575
European Cooperation in Science and TechnologyCA15117
SCOAP3UNSPECIFIED
Record Number:CaltechAUTHORS:20191011-110521505
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191011-110521505
Official Citation:Philippe Brax, Sylvain Fichet, Philip Tanedo, The warped dark sector, Physics Letters B, Volume 798, 2019, 135012, ISSN 0370-2693, https://doi.org/10.1016/j.physletb.2019.135012. (http://www.sciencedirect.com/science/article/pii/S0370269319307348)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99238
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 Oct 2019 18:15
Last Modified:15 Oct 2019 16:37

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