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Higgs and dark matter hints of an oasis in the desert

Cheung, Clifford and Papucci, Michele and Zurek, Kathryn M. (2012) Higgs and dark matter hints of an oasis in the desert. Journal of High Energy Physics, 2012 (7). Art. No. 105. ISSN 1029-8479. doi:10.1007/jhep07(2012)105. https://resolver.caltech.edu/CaltechAUTHORS:20190613-164147888

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Abstract

Recent LHC results suggest a standard model (SM)-like Higgs boson in the vicinity of 125 GeV with no clear indications yet of physics beyond the SM. At the same time, the SM is incomplete, since additional dynamics are required to accommodate cosmological dark matter (DM). In this paper we show that interactions between weak scale DM and the Higgs which are strong enough to yield a thermal relic abundance consistent with observation can easily destabilize the electroweak vacuum or drive the theory into a non-perturbative regime at a low scale. As a consequence, new physics — beyond the DM itself — must enter at a cutoff well below the Planck scale and in some cases as low as O(10-1000 TeV), a range relevant to indirect probes of flavor and CP violation. In addition, this cutoff is correlated with the DM mass and scattering cross-section in a parameter space which will be probed experimentally in the near term. Specifically, we consider the SM plus additional spin 0 or 1/2 states with singlet, triplet, or doublet electroweak quantum numbers and quartic or Yukawa couplings to the Higgs boson. We derive explicit expressions for the full two-loop RGEs and one-loop threshold corrections for these theories.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/jhep07(2012)105DOIArticle
https://arxiv.org/abs/1203.5106arXivDiscussion Paper
ORCID:
AuthorORCID
Papucci, Michele0000-0003-0810-0017
Zurek, Kathryn M.0000-0002-2629-337X
Additional Information:© SISSA, Trieste, Italy 2012. Received: May 13, 2012. Accepted: July 6, 2012. Published: July 17, 2012. C.C. and M.P. are supported in part by the Director, Office of Science, Office of High Energy and Nuclear Physics, of the US Department of Energy under Contract DE-AC02-05CH11231. C.C. is also supported in part by the National Science Foundation under grant PHY-0855653. K.Z. is supported by NSF CAREER award PHY1049896 and NASA Astrophysics Theory grant NNX11AI17G. K.Z. thanks the Berkeley theory group for hospitality where this work was initiated.
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)DE-AC02-05CH11231
NSFPHY-0855653
NSFPHY-1049896
NASANNX11AI17G
Subject Keywords:Higgs Physics, Beyond Standard Model, Standard Model
Issue or Number:7
DOI:10.1007/jhep07(2012)105
Record Number:CaltechAUTHORS:20190613-164147888
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190613-164147888
Official Citation:Cheung, C., Papucci, M. & Zurek, K.M. J. High Energ. Phys. (2012) 2012: 105. https://doi.org/10.1007/JHEP07(2012)105
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96401
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:17 Jun 2019 15:44
Last Modified:16 Nov 2021 17:20

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