25–28 Mar 2020
UCLA
US/Pacific timezone

Gravity safe, electroweak natural axionic\\ solution to strong $CP$ and SUSY $\mu$ problems

Not scheduled
15m
PAB- 1-425 (UCLA)

PAB- 1-425

UCLA

UCLA Department of Physics and Astronomy 475 Portola Plaza, Los Angeles, CA 90095
Talk Dark matter theory

Speaker

Howard Baer (University of Oklahoma)

Description

Particle physics models with Peccei-Quinn (PQ) symmetry breaking
as a consequence of supersymmetry (SUSY) breaking are attractive in that
they solve the strong CP problem with a SUSY DFSZ-like axion,
link the SUSY breaking and PQ breaking intermediate mass scales
and can resolve the SUSY $\mu$ problem with a naturalness-required
weak scale $\mu$ term whilst soft SUSY breaking terms inhabit the
multi-TeV regime as required by LHC sparticle mass limits and
the Higgs mass measurement.
On the negative ledger, models based on global
symmetries suffer a generic gravity spoliation problem.
We present two models based on the discrete $R$-symmetry
${\bf Z}_{24}^R$-- which may emerge
from compactification of 10-d Lorentzian spacetime in string theory--
where the $\mu$ term and dangerous proton decay and $R$-parity
violating operators are either suppressed or forbidden
while a gravity-safe PQ symmetry emerges as an accidental approximate
global symmetry leading to a solution to the strong CP problem
and a weak-scale/natural value for the $\mu$ term.

Author

Howard Baer (University of Oklahoma)

Presentation materials

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