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PreprintarXiv licencearXiv

Two-peak gravitational wave spectra from supercooled two-field phase transitions

Abstract

We study the gravitational wave (GW) spectrum generated by supercooled first-order phase transitions in two-field conformal models. We construct three representative toy models that capture the essential features of these models, derive analytical criteria for the existence of two-step transitions, and show how the two-field dynamics generate a genuine two-peak GW spectrum. We identify regions of parameter space in which two-peak GW spectra are observable at LISA and the Einstein Telescope. By way of illustration, we apply our analysis to a realistic conformal dark SU(3) model.

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BibTeX
@misc{araujo2026twopeak,
  title = {{Two-peak gravitational wave spectra from supercooled two-field phase transitions}},
  author = {Daniel Araújo and João Gonçalves and Danny Marfatia},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.40354},
  eprint = {2610.40354},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.40354},
}
RIS
TY  - UNPB
TI  - Two-peak gravitational wave spectra from supercooled two-field phase transitions
AU  - Daniel Araújo
AU  - João Gonçalves
AU  - Danny Marfatia
PY  - 2026
DA  - 2026/10/29
PB  - arXiv
DO  - 10.48550/arxiv.2610.40354
UR  - https://arxiv.org/abs/2610.40354
AB  - We study the gravitational wave (GW) spectrum generated by supercooled first-order phase transitions in two-field conformal models. We construct three representative toy models that capture the essential features of these models, derive analytical criteria for the existence of two-step transitions, and show how the two-field dynamics generate a genuine two-peak GW spectrum. We identify regions of parameter space in which two-peak GW spectra are observable at LISA and the Einstein Telescope. By way of illustration, we apply our analysis to a realistic conformal dark SU(3) model.
ER  -