Electroweak Phase Transition, Gravitational Waves and Dark Matter in Two Scalar Singlet Extension of Standard Model. (arXiv:1811.09807v1 [hep-ph])
<a href="http://arxiv.org/find/hep-ph/1/au:+Shajiee_V/0/1/0/all/0/1">Vahid Reza Shajiee</a>, <a href="http://arxiv.org/find/hep-ph/1/au:+Tofighi_A/0/1/0/all/0/1">Ali Tofighi</a>
In this paper, the electroweak phase transition, the gravitational waves and
the dark matter issues are investigated in two scalar singlet extension of the
standard model. The detectability of the gravitational wave signals are
discussed by comparing the results with the sensitivity curves of
$mathbf{eLISA}$, $mathbf{LISA}$, $mathbf{ALIA}$, $mathbf{DECIGO}$ and
$mathbf{BBO}$ detectors. It is shown that the results support the recent
reports on the dark matter relic density by $mathbf{Plack}$ $mathbf{2018}$
collaboration and the direct detection experiment by $mathbf{LUX}$
collaboration.
In this paper, the electroweak phase transition, the gravitational waves and
the dark matter issues are investigated in two scalar singlet extension of the
standard model. The detectability of the gravitational wave signals are
discussed by comparing the results with the sensitivity curves of
$mathbf{eLISA}$, $mathbf{LISA}$, $mathbf{ALIA}$, $mathbf{DECIGO}$ and
$mathbf{BBO}$ detectors. It is shown that the results support the recent
reports on the dark matter relic density by $mathbf{Plack}$ $mathbf{2018}$
collaboration and the direct detection experiment by $mathbf{LUX}$
collaboration.
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