Early growth of massive black holes in dynamical dark energy models with negative cosmological constant
Context. Recent results from combined cosmological probes indicate that the dark energy component of the Universe could be dynamical. The simplest explanation envisages the presence of a quintessence field rolling into a potential, where the dark energy density parameter ΩDE = ΩΛ + Ωx results from t...
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| Asıl Yazarlar: | , , , , , , |
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| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
EDP Sciences
2026-03-01
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| Seri Bilgileri: | Astronomy & Astrophysics |
| Konular: | |
| Online Erişim: | https://www.aanda.org/articles/aa/full_html/2026/03/aa58610-25/aa58610-25.html |
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