Abstract

We study the gravitational-wave signal stemming from strongly coupled models featuring both, dark chiral and confinement phase transitions. We therefore identify strongly coupled theories that can feature a first-order phase transition. Employing the Polyakov-Nambu-Jona-Lasinio model, we focus our attention on SU(3) Yang-Mills theories featuring fermions in fundamental, adjoint, and two-index symmetric representations. We discover that for the gravitational-wave signals analysis, there are significant differences between the various representations. Interestingly we also observe that the two-index symmetric representation leads to the strongest first-order phase transition and therefore to a higher chance of being detected by the Big Bang Observer experiment. Our study of the confinement and chiral phase transitions is further applicable to extensions of the Standard Model featuring composite dynamics.

Details

Title
Dark confinement and chiral phase transitions: gravitational waves vs matter representations
Author
Reichert, Manuel 1   VIAFID ORCID Logo  ; Sannino, Francesco 2   VIAFID ORCID Logo  ; Zhi-Wei, Wang 3   VIAFID ORCID Logo  ; Zhang, Chen 4   VIAFID ORCID Logo 

 University of Sussex, Department of Physics and Astronomy, Brighton, UK (GRID:grid.12082.39) (ISNI:0000 0004 1936 7590) 
 Scuola Superiore Meridionale, Napoli, Italy (GRID:grid.508348.2); University of Southern Denmark, CP3-Origins, Odense M, Denmark (GRID:grid.10825.3e) (ISNI:0000 0001 0728 0170); Dipartimento di Fisica “E. Pancini”, Università di Napoli Federico II | INFN sezione di Napoli, Napoli, Italy (GRID:grid.470211.1) (ISNI:0000 0004 8343 7696) 
 University of Southern Denmark, CP3-Origins, Odense M, Denmark (GRID:grid.10825.3e) (ISNI:0000 0001 0728 0170); Lund University, Department of Astronomy and Theoretical Physics, Lund, Sweden (GRID:grid.4514.4) (ISNI:0000 0001 0930 2361) 
 INFN Sezione di Firenze, Sesto Fiorentino, Italy (GRID:grid.470204.5) (ISNI:Q30265285) 
Publication year
2022
Publication date
Jan 2022
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2616478458
Copyright
© The Author(s) 2022. This work is published under CC-BY 4.0 (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.