Interacting dark sector within ETHOS: Cosmological constraints from SPT cluster abundance with des and HST weak lensing data

Mazoun, A.; Bocquet, S.; Mohr, J. J.; Garny, M.; Rubira, H.; Klein, M.; Bleem, L. E.; Grandis, S.; Schrabback, T.; Aguena, M.; Allam, S.; Allen, S. W.; Alves, O.; Andrade-Oliveira, F.; Brooks, D.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Costanzi, M.; Da Costa, L. N.; Davis, T. M.; Desai, S.; De Vicente, J.; Diehl, H. T.; Dodelson, S.; Doel, P.; Everett, S.; Flaugher, B.; Frieman, J.; Garcia-Bellido, J.; Gassis, R.; Giannini, G.; Grun, D.; Gutierrez, G.; Hinton, S. R.; Hollowood, D. L.; James, D. J.; Kuehn, K.; Lahav, O.; Lee, S.; Lima, M.; Mahler, G.; Marshall, J. L.; Miquel, R.; Myles, J.; Ogando, R. L. C.; Pereira, M. E. S.; Pieres, A.; Plazas Malagon, A. A.; Porredon, A.; Reichardt, C. L.; Romer, A. K.; Samuroff, S.; Sanchez, E.; Sanchez Cid, D.; Sevilla-Noarbe, I.; Schubnell, M.; Smith, M.; Suchyta, E.; Swanson, M. E. C.; Tamosiunas, A.; Tarle, G.; Tucker, D. L.; Vikram, V.; Weaverdyck, N.; Weller, J.; Wiseman, P.

doi:10.1103/PhysRevD.111.083543

We use galaxy cluster abundance measurements from the South Pole Telescope enhanced by multicomponent matched filter confirmation and complemented with mass information obtained using weak-lensing data from Dark Energy Survey Year 3 (DES Y3) and targeted Hubble Space Telescope observations for probing deviations from the cold dark matter paradigm. Concretely, we consider a class of dark sector models featuring interactions between dark matter (DM) and a dark radiation (DR) component within the framework of the effective theory of structure formation (ETHOS). We focus on scenarios that lead to power suppression over a wide range of scales, and thus can be tested with data sensitive to large scales, as realized, for example, for DM-DR interactions following from an unbroken non-Abelian SU(N) gauge theory (interaction rate with power-law index n=0 within the ETHOS parametrization). Cluster abundance measurements are mostly sensitive to the amount of DR interacting with DM, parametrized by the ratio of DR temperature to the cosmic microwave background (CMB) temperature, ζDR=TDR/TCMB. We find an upper limit ζDR<17% at 95% credibility. When the cluster data are combined with Planck 2018 CMB data along with baryon acoustic oscillation (BAO) measurements we find ζDR<10%, corresponding to a limit on the abundance of interacting DR that is around 3 times tighter than that from CMB + BAO data alone. We also discuss the complementarity of weak lensing informed cluster abundance studies with probes sensitive to smaller scales, explore the impact on our analysis of massive neutrinos, and comment on a slight preference for the presence of a nonzero interacting DR abundance, which enables a physical solution to the S8 tension.

Interacting dark sector within ETHOS: Cosmological constraints from SPT cluster abundance with des and HST weak lensing data / Mazoun, A.; Bocquet, S.; Mohr, J. J.; Garny, M.; Rubira, H.; Klein, M.; Bleem, L. E.; Grandis, S.; Schrabback, T.; Aguena, M.; Allam, S.; Allen, S. W.; Alves, O.; Andrade-Oliveira, F.; Brooks, D.; Carnero Rosell, A.; Carrasco Kind, M.; Carretero, J.; Costanzi, M.; Da Costa, L. N.; Davis, T. M.; Desai, S.; De Vicente, J.; Diehl, H. T.; Dodelson, S.; Doel, P.; Everett, S.; Flaugher, B.; Frieman, J.; Garcia-Bellido, J.; Gassis, R.; Giannini, G.; Grun, D.; Gutierrez, G.; Hinton, S. R.; Hollowood, D. L.; James, D. J.; Kuehn, K.; Lahav, O.; Lee, S.; Lima, M.; Mahler, G.; Marshall, J. L.; Miquel, R.; Myles, J.; Ogando, R. L. C.; Pereira, M. E. S.; Pieres, A.; Plazas Malagon, A. A.; Porredon, A.; Reichardt, C. L.; Romer, A. K.; Samuroff, S.; Sanchez, E.; Sanchez Cid, D.; Sevilla-Noarbe, I.; Schubnell, M.; Smith, M.; Suchyta, E.; Swanson, M. E. C.; Tamosiunas, A.; Tarle, G.; Tucker, D. L.; Vikram, V.; Weaverdyck, N.; Weller, J.; Wiseman, P.. - In: PHYSICAL REVIEW D. - ISSN 2470-0010. - 111:8(2025), pp. 083543.--083543.-. [10.1103/PhysRevD.111.083543]