{"paper":{"title":"Gravitational Wave Signatures from Domain Wall and Strong First-Order Phase Transitions in a Two Complex Scalar extension of the Standard Model","arxiv_id":"2010.03439","primary_cat":"hep-ph","submitted_at":"2020-10-07T14:32:00+00:00","version_compiled":"v2"},"notice":"Every quoted sentence is the authors' text from the arXiv listing abstract. Labels and probabilities are the outputs of classifier-1.13.0 on the question bank abstract-p1-20260923, exactly as returned. 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spontaneously.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.53,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.17,"role_probabilities":{"gap":0.0,"method":0.73,"result":0.0,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.26,"interpretation":0.0}},{"i":2,"p":0.45,"id":"s2","own":true,"role":"method","text":"The real (CP even) parts of the complex scalars mix with the SM Higgs and give three physical mass eigenstates.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.58,"main_claim_p":0.03,"quantitative":false,"quantitative_p":0.48,"role_probabilities":{"gap":0.0,"method":0.45,"result":0.27,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.26,"interpretation":0.01}},{"i":3,"p":0.74,"id":"s3","own":true,"role":"result","text":"One of these physical mass eigenstates is attributed to the SM like Higgs boson with mass 125.09 GeV.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.52,"main_claim_p":0.04,"quantitative":true,"quantitative_p":0.98,"role_probabilities":{"gap":0.0,"method":0.1,"result":0.74,"background":0.05,"limitation":0.0,"future_work":0.0,"contribution":0.08,"interpretation":0.03}},{"i":4,"p":0.41,"id":"s4","own":false,"role":"contribution","text":"In the present scenario, domain walls are formed in the early Universe due to the breaking of discrete $\\mathcal{Z}_2 \\times \\mathcal{Z}^{\\prime}_2$ symmetry.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.45,"main_claim_p":0.07,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.13,"result":0.4,"background":0.05,"limitation":0.0,"future_work":0.0,"contribution":0.41,"interpretation":0.01}},{"i":5,"p":0.84,"id":"s5","own":true,"role":"method","text":"In order to ensure the unstability of the domain wall this discrete symmetry is also explicitly broken by adding a bias potential to the Lagrangian.","hedge":{"p":0.98,"label":"asserted"},"own_p":0.77,"main_claim_p":0.04,"quantitative":false,"quantitative_p":0.04,"role_probabilities":{"gap":0.0,"method":0.84,"result":0.0,"background":0.01,"limitation":0.0,"future_work":0.0,"contribution":0.15,"interpretation":0.0}},{"i":6,"p":0.87,"id":"s6","own":true,"role":"result","text":"The unstable annihilating domain walls produce a significant amount of gravitational waves (GWs).","hedge":{"p":1.0,"label":"asserted"},"own_p":0.5,"main_claim_p":0.3,"quantitative":false,"quantitative_p":0.13,"role_probabilities":{"gap":0.0,"method":0.02,"result":0.87,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.09,"interpretation":0.02}},{"i":7,"p":0.99,"id":"s7","own":true,"role":"contribution","text":"In addition, we also explore the possibility of the production of GW emission from the strong first-order phase transition.","hedge":{"p":0.99,"label":"hedged_possibility"},"own_p":0.62,"main_claim_p":0.06,"quantitative":false,"quantitative_p":0.06,"role_probabilities":{"gap":0.0,"method":0.01,"result":0.0,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.99,"interpretation":0.0}},{"i":8,"p":0.75,"id":"s8","own":true,"role":"contribution","text":"We calculate the intensities and frequencies of each of such gravitational waves originating from two different phenomena of the early Universe namely annihilating domain walls and strong first-order phase transition.","hedge":{"p":1.0,"label":"asserted"},"own_p":0.95,"main_claim_p":0.17,"quantitative":false,"quantitative_p":0.4,"role_probabilities":{"gap":0.0,"method":0.22,"result":0.03,"background":0.0,"limitation":0.0,"future_work":0.0,"contribution":0.75,"interpretation":0.0}},{"i":9,"p":0.81,"id":"s9","own":true,"role":"contribution","text":"Finally, we investigate the observational signatures from these GWs at the future GW detectors such as ALIA, BBO, DECIGO, LISA, TianQin, Taiji, aLIGO, aLIGO+ and pulsar timing arrays such as SKA, IPTA, EPTA, PPTA, NANOGrav11 and NANOGrav12.5.","hedge":{"p":0.93,"label":"asserted"},"own_p":0.84,"main_claim_p":0.18,"quantitative":false,"quantitative_p":0.07,"role_probabilities":{"gap":0.0,"method":0.09,"result":0.06,"background":0.0,"limitation":0.0,"future_work":0.01,"contribution":0.81,"interpretation":0.02}}]},"compiled":{"main_claim":{"p":0.6,"text":"The unstable annihilating domain walls produce a significant amount of gravitational waves (GWs).","location":"abstract s6","hedge_strength":{"p":1.0,"label":"asserted"}},"provenance":{"route":{"via":"TypeSafe API","model":"classifier-1.13.0","endpoint":"https://api.typesafe.ai/v1/systemone","provider":"TypeSafe"},"packing":"one request per 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