Split Dirac supersymmetry: An ultraviolet completion of Higgsino dark matter

Fox, Patrick J.; Kribs, Graham D.; Martin, Adam

doi:10.1103/PhysRevD.90.075006

Title: Split Dirac supersymmetry: An ultraviolet completion of Higgsino dark matter

Journal Article · Tue Oct 07 00:00:00 EDT 2014 · Physical Review. D, Particles, Fields, Gravitation and Cosmology

DOI:https://doi.org/10.1103/PhysRevD.90.075006· OSTI ID:1601483

Fox, Patrick J. ^[1]; Kribs, Graham D. ^[2]; Martin, Adam ^[3]

Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States).
Institute for Advanced Study, Princeton, NJ (United States); Univ. of Oregon, Eugene, OR (United States)
Univ. of Notre Dame, IN (United States)

Motivated by the observation that the Higgs quartic coupling runs to zero at an intermediate scale, we propose a new framework for models of split supersymmetry, in which gauginos acquire intermediate scale Dirac masses of $$\sim 10^{8-11}$$ GeV. Scalar masses arise from one-loop finite contributions as well as direct gravity-mediated contributions. Like split supersymmetry, one Higgs doublet is fine-tuned to be light. The scale at which the Dirac gauginos are introduced to make the Higgs quartic zero is the same as is necessary for gauge coupling unification. Thus, gauge coupling unification persists (nontrivially, due to adjoint multiplets), though with a somewhat higher unification scale $$\gtrsim 10^{17}$$ GeV. The $$\mu$$-term is naturally at the weak scale, and provides an opportunity for experimental verification. We present two manifestations of Split Dirac Supersymmetry. In the "Pure Dirac" model, the lightest Higgsino must decay through R-parity violating couplings, leading to an array of interesting signals in colliders. In the "Hypercharge Impure" model, the bino acquires a Majorana mass that is one-loop suppressed compared with the Dirac gluino and wino. This leads to weak scale Higgsino dark matter whose overall mass scale, as well as the mass splitting between the neutral components, is naturally generated from the same UV dynamics. We outline the challenges to discovering pseudo-Dirac Higgsino dark matter in collider and dark matter detection experiments.

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Research Organization:: Univ. of Oregon, Eugene, OR (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

Grant/Contract Number:: SC0011640; FG02-96ER40969; AC02-07CH11359

OSTI ID:: 1601483

Alternate ID(s):: OSTI ID: 1180682; OSTI ID: 1333176

Report Number(s):: FERMILAB-PUB-14-124-T; arXiv:1405.3692; PRVDAQ; TRN: US2103668

Journal Information:: Physical Review. D, Particles, Fields, Gravitation and Cosmology, Vol. 90, Issue 7; ISSN 1550-7998

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 32 works

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