Abstract
AbstractWe consider a particle dark matter model by extending the Standard Model (SM) of particle physics by an extra Higgs doublet and a real singlet scalar. The added Higgs doublet is attributed to be an inert doublet and the lightest inert particle acts as a viable candidate of dark matter. We consider a finite temperature effective potential to explore the first-order phase transition (FOPT) within the framework of the model. We also discuss the possible production mechanisms of gravitational waves (GWs) from the strong FOPT. Finally, we calculate the intensities and frequencies of such GWs and investigate their detection possibilities at the future space-based detectors such as eLISA, ALIA, BBO, DECIGO, U-DECIGO, and ground-based detector aLIGO.KeywordsDark matterGravitational wavePhase transition
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
