{"total":11,"items":[{"citing_arxiv_id":"2607.02505","ref_index":151,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A critical look at low-scale cosmological phase transitions in the PTA era","primary_cat":"hep-ph","submitted_at":"2026-07-02T17:58:57+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Precision study of dark sector phase transitions finds PTA-favored parameters near EFT breakdown with disfavored GW signals after higher-order corrections.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"and bubble profiles with multiple fields,Comput. Phys. Commun.183(2012) 2006 [1109.4189]. [149] V. Guada, M. Nemevˇ sek, and M. Pintar,FindBounce: Package for multi-field bounce actions, Comput. Phys. Commun.256(2020) 107480 [2002.00881]. [150] L. Bian, H. Wang, Y. Xiao, J.-C. Yang, J. M. Yang, and Y. Zhang,Enhancing Phase Transition Calculations with Fitting and Neural Network,[2510.10667]. [151] S. Pascoli, S. Rosauro-Alcaraz, and M. Zandi,Cosmological phase transitions: from particle physics to gravitational waves, semi-analytically,[2602.02829]. [152] C. Capriniet al.,Detecting gravitational waves from cosmological phase transitions with LISA: an update,JCAP03(2020) 024 [1910.13125]. [153] P. Athron, L. Morris, and Z. Xu,How robust are gravitational wave predictions from cosmological"},{"citing_arxiv_id":"2607.01697","ref_index":90,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Gravitational Waves from Multiple First-Order Phase Transitions in a Scenario with Early Matter Domination","primary_cat":"hep-ph","submitted_at":"2026-07-02T04:41:30+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Early matter domination with time-dependent decay rates produces multiple first-order phase transitions whose gravitational wave signatures encode the transition and reheating temperatures.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.19425","ref_index":45,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"LeWRON: Agentic Analysis of Electroweak Phase Transitions","primary_cat":"hep-ph","submitted_at":"2026-06-17T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"LeWRON is a new agentic framework that automates construction, auditing, and exploration of finite-temperature effective potentials and gravitational-wave predictions for electroweak phase transitions starting from an input Lagrangian.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13514","ref_index":125,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Electroweak First-Order Phase Transition Triggered by Non-Gaussian Fluctuations of a $\\mathbb{Z}_2$-Symmetric Spectator Scalar","primary_cat":"hep-ph","submitted_at":"2026-06-11T16:00:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Non-Gaussian primordial fluctuations of a Z2-symmetric spectator scalar trigger a strong first-order electroweak phase transition, with the field serving as cold dark matter and generating a stochastic gravitational wave background in the 10^{-3}-10^{-1} Hz band.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03758","ref_index":72,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Dark Matter Production from Bubble Collisions during a First-Order Phase Transition at the End of Inflation","primary_cat":"hep-ph","submitted_at":"2026-05-05T13:42:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Bubble collisions during a first-order phase transition at the end of inflation can generate the observed dark matter abundance in a restricted region of parameter space via direct production and spectator decays.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Universe and the Grand Unification Scale,Phys. 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