Vlasov Perturbation Theory applied to $Λ$CDM
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arXiv
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| Format: | Preprint |
| Publié: |
2025
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| _version_ | 1866913820943843328 |
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| author | Garny, Mathias Laxhuber, Dominik Scoccimarro, Roman |
| author_facet | Garny, Mathias Laxhuber, Dominik Scoccimarro, Roman |
| contents | We apply the framework of Vlasov Perturbation Theory (VPT) to the two-loop matter power spectrum within $Λ$CDM cosmologies. The main difference to Standard Perturbation Theory (SPT) arises from taking the velocity dispersion tensor into account, and the resulting screening of the backreaction of UV modes renders loop integrals cutoff-independent. VPT is informed about non-perturbative small scale dynamics via the average value of the dispersion generated by shell-crossing, which impacts the evolution of perturbations on weakly non-linear scales. When using an average dispersion from halo models, the VPT power spectrum agrees with the one from the simulation, up to differences from missing three-loop contributions. Alternatively, treating the average dispersion as free parameter we find a remarkably stable prediction of the matter power spectrum from collisionless dynamics at percent level for a wide range of the dispersion scale. We quantify the impact of truncating the Vlasov hierarchy for the cumulants of the phase-space distribution function, finding that the two-loop matter power spectrum is robust to neglecting third and higher cumulants. Finally, we introduce and validate a simplified fast scheme fVPT that can be easily incorporated into existing codes and is as numerically efficient as SPT. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_02907 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Vlasov Perturbation Theory applied to $Λ$CDM Garny, Mathias Laxhuber, Dominik Scoccimarro, Roman Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology We apply the framework of Vlasov Perturbation Theory (VPT) to the two-loop matter power spectrum within $Λ$CDM cosmologies. The main difference to Standard Perturbation Theory (SPT) arises from taking the velocity dispersion tensor into account, and the resulting screening of the backreaction of UV modes renders loop integrals cutoff-independent. VPT is informed about non-perturbative small scale dynamics via the average value of the dispersion generated by shell-crossing, which impacts the evolution of perturbations on weakly non-linear scales. When using an average dispersion from halo models, the VPT power spectrum agrees with the one from the simulation, up to differences from missing three-loop contributions. Alternatively, treating the average dispersion as free parameter we find a remarkably stable prediction of the matter power spectrum from collisionless dynamics at percent level for a wide range of the dispersion scale. We quantify the impact of truncating the Vlasov hierarchy for the cumulants of the phase-space distribution function, finding that the two-loop matter power spectrum is robust to neglecting third and higher cumulants. Finally, we introduce and validate a simplified fast scheme fVPT that can be easily incorporated into existing codes and is as numerically efficient as SPT. |
| title | Vlasov Perturbation Theory applied to $Λ$CDM |
| topic | Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology |
| url | https://arxiv.org/abs/2505.02907 |