Heavier <math display="inline"><mi>W</mi></math> boson, dark matter, and gravitational waves from strings in an SO(10) axion model - INSPIRE

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Heavier $W$ boson, dark matter, and gravitational waves from strings in an SO(10) axion model

May 10, 2022

20 pages

Published in:

Phys.Rev.D 106 (2022) 5, 055009

Published: Sep 1, 2022

e-Print:

2205.04824 [hep-ph]

DOI:

10.1103/PhysRevD.106.055009 (publication)

View in:

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Abstract: (APS)

Inspired by the recent determination of the

W

-boson mass by the CDF collaboration, we revisit an

S O (10)

axion model in which a scalar

S U (2)_{L}

triplet field with zero hypercharge is known to acquire a nonzero vacuum expectation value (VEV) through its mixing with the Standard Model Higgs doublet. The triplet VEV provides a sizable contribution to the

W

mass, which helps in significantly lowering the

7 σ

discrepancy between the Standard Model prediction and the higher CDF value for

m_{W}

. We show that the relatively light triplet mass (

\sim (1 - 50) TeV

) is compatible with gauge coupling unification and observable proton decay. An unbroken

Z_{2}

gauge symmetry, coupled with the presence of two fermionic 10-plets required to resolve the axion domain wall problem means that both axions and a stable intermediate mass (

\sim 10^{9} - 10^{10} GeV

) fermion are plausible dark matter candidates. We also display the gravitational wave spectrum from the intermediate scale topologically stable cosmic strings predicted by the model.

Note:

20 pages, 6 figures, published version

model: axion
symmetry: gauge
gravitational radiation: spectrum
W: mass
cosmic string: stability
p: decay
coupling: gauge
Higgs particle: doublet
axion: domain wall
triplet

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