TY - JOUR
T1 - Natural little hierarchy for SUSY from radiative breaking of the Peccei-Quinn symmetry
AU - Bae, Kyu Jung
AU - Baer, Howard
AU - Serce, Hasan
N1 - Publisher Copyright:
© 2015 American Physical Society.
PY - 2015/1/6
Y1 - 2015/1/6
N2 - While LHC8 Higgs mass and sparticle search constraints favor a multi-TeV value of soft SUSY breaking terms, electroweak naturalness favors a superpotential Higgsino mass μ∼100-200GeV: the mismatch results in an apparent little hierarchy characterized by μ msoft (with msoft∼m3/2 in gravity mediation). It has been suggested that the little hierarchy arises from a mismatch between Peccei-Quinn (PQ) and hidden sector intermediate scales vPQ mhidden. We examine the Murayama-Suzuki-Yanagida model of radiatively driven PQ symmetry breaking which not only generates a weak scale value of μ but also produces intermediate scale Majorana masses for right-hand neutrinos. For this model, we show ranges of parameter choices with multi-TeV values of m3/2 which can easily generate values of μ∼100-200GeV so that the apparent little hierarchy suggested from data emerges quite naturally. In such a scenario, dark matter would be comprised of an axion plus a Higgsino-like weakly-interacting massive particle admixture where the axion mass and Higgsino masses are linked by the value of the PQ scale. The required light Higgsinos should ultimately be detected at a linear e+e- collider with s>2m(Higgsino).
AB - While LHC8 Higgs mass and sparticle search constraints favor a multi-TeV value of soft SUSY breaking terms, electroweak naturalness favors a superpotential Higgsino mass μ∼100-200GeV: the mismatch results in an apparent little hierarchy characterized by μ msoft (with msoft∼m3/2 in gravity mediation). It has been suggested that the little hierarchy arises from a mismatch between Peccei-Quinn (PQ) and hidden sector intermediate scales vPQ mhidden. We examine the Murayama-Suzuki-Yanagida model of radiatively driven PQ symmetry breaking which not only generates a weak scale value of μ but also produces intermediate scale Majorana masses for right-hand neutrinos. For this model, we show ranges of parameter choices with multi-TeV values of m3/2 which can easily generate values of μ∼100-200GeV so that the apparent little hierarchy suggested from data emerges quite naturally. In such a scenario, dark matter would be comprised of an axion plus a Higgsino-like weakly-interacting massive particle admixture where the axion mass and Higgsino masses are linked by the value of the PQ scale. The required light Higgsinos should ultimately be detected at a linear e+e- collider with s>2m(Higgsino).
UR - http://www.scopus.com/inward/record.url?scp=84920885317&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.91.015003
DO - 10.1103/PhysRevD.91.015003
M3 - Article
AN - SCOPUS:84920885317
SN - 1550-7998
VL - 91
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 1
M1 - 015003
ER -