Wino-Higgsino dark matter in MSSM from the g − 2 anomaly - INSPIRE

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Wino-Higgsino dark matter in MSSM from the g − 2 anomaly

Sho Iwamoto
(
- Eotvos U.
)
,
Tsutomu T. Yanagida
(
- Tsung-Dao Lee Inst., Shanghai and
- Tokyo U., IPMU
)
,
Norimi Yokozaki
(
- Zhejiang U., Inst. Mod. Phys. and
- Zhejiang U.
)

Apr 7, 2021

13 pages

Published in:

Phys.Lett.B 823 (2021) 136768

Published: Dec 10, 2021

e-Print:

2104.03223 [hep-ph]

DOI:

10.1016/j.physletb.2021.136768 (publication)

View in:

ADS Abstract Service

reference search41 citations

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Abstract: (Elsevier B.V.)

In this letter, we show that the wino-Higgsino dark matter (DM) is detectable in near future DM direct detection experiments for almost all consistent parameter space in the spontaneously broken supergravity (SUGRA) if the muon

g - 2

anomaly is explained by the wino-Higgsino loop diagrams. We also point out that the present and future LHC experiments can exclude or confirm this SUGRA explanation of the observed muon

g - 2

anomaly.

Note:

Figures and benchmark point for tanb=40 added, typos corrected

magnetic moment: anomaly
muon: magnetic moment
supergravity: spontaneous symmetry breaking
dark matter: direct detection
minimal supersymmetric standard model
interpretation of experiments: CERN LHC Coll

References(43)

Figures(7)

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