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We explore the role of redshift-space galaxy clustering data in constraining non-gravitational interactions between dark energy (DE) and dark matter (DM), for which state-of-the-art limits have so far been obtained from late-time background measurements.
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Closest in time.
H. Gil-Marín, (2022), arXiv:2203.05581 [astro-ph.CO]
2022
Closest in time.
G. S. Farren, O. H. E. Philcox, and B. D. Sherwin, Phys. Rev. D 105
2022
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R. K. Sharma, K. L. Pandey, and S. Das, (2022), arXiv:2202.01749 [astro-ph.CO]
2022
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2022
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J.-Q. Jiang and Y.-S. Piao, (2022), arXiv:2202.13379 [astro-ph.CO]
2022
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T. Rudelius, (2022), arXiv:2203.05575 [hep-th]
2022
Closest in time.