Addressing Dipole Tension via Clustering in ΛCDM and Beyond
The dipole in the angular distribution of the cosmic microwave background (CMB) is attributed to the Doppler effect and our motion relative to the CMB rest frame. It is expected that observations of large-scale structures (LSSs) would also exhibit a related kinematic dipole. However, numerous studie...
-д хадгалсан:
| Үндсэн зохиолчид: | , , , |
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| Формат: | Artigo |
| Хэл сонгох: | Inglês |
| Хэвлэсэн: |
IOP Publishing
2026-01-01
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| Цуврал: | The Astrophysical Journal |
| Нөхцлүүд: | |
| Онлайн хандалт: | https://doi.org/10.3847/1538-4357/ae3a8e |
| Шошгууд: |
Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!
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