Gravitational waves from walls bounded by strings in SO(10) model of pseudo-Goldstone dark matter - INSPIRE

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Gravitational waves from walls bounded by strings in SO(10) model of pseudo-Goldstone dark matter

Rinku Maji
(
- Jeonbuk Natl. U.
)
,
Wan-Il Park
(
- Chonbuk Natl. U. and
- Valencia U., IFIC and
- Valencia U.
)
,
Qaisar Shafi
(
- Delaware U.
)

May 19, 2023

8 pages

Published in:

Phys.Lett.B 845 (2023) 138127

Published: Aug 19, 2023

e-Print:

2305.11775 [hep-ph]

DOI:

10.1016/j.physletb.2023.138127 (publication)

View in:

ADS Abstract Service

reference search16 citations

Citations per year

Abstract: (Elsevier B.V.)

We explore the gravitational wave spectrum generated by string-wall structures in an

S O (10)

(

S p i n (10)

) based scenario of pseudo-Goldstone boson dark matter (pGDM) particle. This dark matter candidate is a linear combination of the Standard Model (SM) singlets present in the 126 and 16 dimensional Higgs fields. The Higgs 126-plet vacuum expectation value (VEV)

〈 126_{H} 〉

leaves unbroken the

Z_{2}

subgroup of

Z_{4}

, the center of

S O (10)

. Among other things, this yields topologically stable cosmic strings with a string tension

μ \sim {〈 126_{H} 〉}^{2}

. The subsequent (spontaneous) breaking of

Z_{2}

at a significantly lower scale by the 16-plet VEV

〈 16_{H} 〉

leads to the appearance of domain walls bounded by the strings produced earlier. We display the gravitational wave spectrum for Gμ values varying between

10^{- 15}

and

10^{- 9}

(

〈 126_{H} 〉 \sim 10^{11}

- 10¹⁴ GeV), and

〈 16_{H} 〉 \sim 0.1

- 10² TeV range (G denotes Newton's constant.) These predictions can be tested, as we show, by a variety of (proposed) experiments including LISA, ET, CE and others.

Note:

8 pages, 3 figures, version published in PLB

gravitational radiation: spectrum
boson: dark matter
gravitation: fundamental constant
cosmic string: stability
SO(10)
Goldstone particle
string
GeV
Spin(10)
domain wall

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