We consider dark matter self-interactions mediated by ultralight scalars. We show that effectively massless mediators lead to an enhancement of the matter power spectrum, while heavier mediators lead to a suppression, together with a feature around their Jeans scale.We derive the strongest present constraints by combining Planck and BOSS data. The recent DESI measurements of baryon acoustic oscillations exhibit a mild 2σ preference for long-range self-interactions, as strong as 4 per mille of the gravitational coupling. Full-shape analyses of forthcoming DESI and Euclid data will confirm or disprove such a hint.
From 100 kpc to 10 Gpc: Dark matter self-interactions before and after DESI observations / S. Bottaro, E. Castorina, M. Costa, D. Redigolo, E. Salvioni. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 112:2(2025 Jul 15), pp. 023525.1-023525.12. [10.1103/gc78-96l5]
From 100 kpc to 10 Gpc: Dark matter self-interactions before and after DESI observations
E. CastorinaSecondo
;
2025
Abstract
We consider dark matter self-interactions mediated by ultralight scalars. We show that effectively massless mediators lead to an enhancement of the matter power spectrum, while heavier mediators lead to a suppression, together with a feature around their Jeans scale.We derive the strongest present constraints by combining Planck and BOSS data. The recent DESI measurements of baryon acoustic oscillations exhibit a mild 2σ preference for long-range self-interactions, as strong as 4 per mille of the gravitational coupling. Full-shape analyses of forthcoming DESI and Euclid data will confirm or disprove such a hint.| File | Dimensione | Formato | |
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gc78-96l5.pdf
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