Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation
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arXiv
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| Autori principali: | , , , , , , , , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866914964444282880 |
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| author | Caprini, Chiara Jinno, Ryusuke Lewicki, Marek Madge, Eric Merchand, Marco Nardini, Germano Pieroni, Mauro Pol, Alberto Roper Vaskonen, Ville |
| author_facet | Caprini, Chiara Jinno, Ryusuke Lewicki, Marek Madge, Eric Merchand, Marco Nardini, Germano Pieroni, Mauro Pol, Alberto Roper Vaskonen, Ville |
| contents | We develop a tool for the analysis of stochastic gravitational wave backgrounds from cosmological first-order phase transitions with LISA: we initiate a template databank for these signals, prototype their searches, and forecast their reconstruction. The templates encompass the gravitational wave signals sourced by bubble collisions, sound waves and turbulence. Accounting for Galactic and extra-Galactic foregrounds, we forecast the region of the parameter space that LISA will reconstruct with better than $\sim 10\,\%$ accuracy, if certain experimental and theoretical uncertainties are solved by the time LISA flies. We illustrate the accuracy with which LISA can reconstruct the parameters on a few benchmark signals, both in terms of the template parameters and the phase transition ones. To show the impact of the forecasts on physics beyond the Standard Model, we map the reconstructed benchmark measurements into the parameter spaces of the singlet extension of the Standard Model and of the classically conformal invariant $U(1)_{B-L}$ model. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_03723 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation Caprini, Chiara Jinno, Ryusuke Lewicki, Marek Madge, Eric Merchand, Marco Nardini, Germano Pieroni, Mauro Pol, Alberto Roper Vaskonen, Ville Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology We develop a tool for the analysis of stochastic gravitational wave backgrounds from cosmological first-order phase transitions with LISA: we initiate a template databank for these signals, prototype their searches, and forecast their reconstruction. The templates encompass the gravitational wave signals sourced by bubble collisions, sound waves and turbulence. Accounting for Galactic and extra-Galactic foregrounds, we forecast the region of the parameter space that LISA will reconstruct with better than $\sim 10\,\%$ accuracy, if certain experimental and theoretical uncertainties are solved by the time LISA flies. We illustrate the accuracy with which LISA can reconstruct the parameters on a few benchmark signals, both in terms of the template parameters and the phase transition ones. To show the impact of the forecasts on physics beyond the Standard Model, we map the reconstructed benchmark measurements into the parameter spaces of the singlet extension of the Standard Model and of the classically conformal invariant $U(1)_{B-L}$ model. |
| title | Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation |
| topic | Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2403.03723 |