Peccei-Quinn Symmetric Pure Gravity Mediation - INSPIRE

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Peccei-Quinn Symmetric Pure Gravity Mediation

Jason L. Evans
(
- Minnesota U., Theor. Phys. Inst.
)
,
Masahiro Ibe
(
- Tokyo U., ICRR and
- Tokyo U., IPMU
)
,
Keith A. Olive
(
- Minnesota U., Theor. Phys. Inst.
)
,
Tsutomu T. Yanagida
(
- Tokyo U., IPMU
)

Feb 24, 2014

18 pages

Published in:

Eur.Phys.J.C 74 (2014) 2931

Published: Jul 1, 2014

e-Print:

1402.5989 [hep-ph]

DOI:

10.1140/epjc/s10052-014-2931-2

View in:

ADS Abstract Service

reference search10 citations

Citations per year

Abstract: (arXiv)

Successful models of Pure Gravity Mediation (PGM) with radiative electroweak symmetry breaking can be expressed with as few as two free parameters which can be taken as the gravitino mass and

\tan \beta

. These models easily support a 125-126 GeV Higgs mass at the expense of a scalar spectrum in the multi-TeV range and a much lighter wino as the lightest supersymmetric particle. In these models, it is also quite generic that the Higgs mixing mass parameter,

\mu

, which is determined by the minimization of the Higgs potential is also in the multi-TeV range. For

\mu > 0

, the thermal relic density of winos is too small to account for the dark matter. The same is true for

\mu < 0

unless the gravitino mass is of order 500 TeV. Here, we consider the origin of a multi-TeV

\mu

parameter arising from the breakdown of a Peccei-Quinn (PQ) symmetry. A coupling of the PQ-symmetry breaking field,

P

, to the MSSM Higgs doublets, naturally leads to a value of

\mu \sim \langle P \rangle^2 /M_P \sim \mathcal{O}(100)

TeV and of order that is required in PGM models. In this case, axions make up the dark matter or some fraction of the dark matter with the remainder made up from thermal or non-thermal winos. We also provide solutions to the problem of isocurvature fluctuations with axion dark matter in this context.

Note:

17 pages, 7 figures

new physics
supersymmetry: symmetry breaking
supersymmetry: dark matter
minimal supersymmetric standard model
mediation: gravitation
symmetry: Peccei-Quinn
axion: dark matter
axion: relic density
gravitino: mass
Higgs particle: mass

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