铁砧 发表于 2025-3-28 18:22:10
http://reply.papertrans.cn/103/10220/1021959/1021959_41.png侵蚀 发表于 2025-3-28 19:42:01
Massive Neutrinos Meet Inflation,e values inferred for . might be sensitive to the assumptions I make when introducing . into the picture, or to the very fact that I introduced . in first place. Recall, in fact, that in the baseline .CDM model, . is not a free parameter, but is fixed to ., the minimum value allowed by oscillations data.摘要记录 发表于 2025-3-29 02:58:19
Massive Neutrinos Meet Inflation,e values inferred for . might be sensitive to the assumptions I make when introducing . into the picture, or to the very fact that I introduced . in first place. Recall, in fact, that in the baseline .CDM model, . is not a free parameter, but is fixed to ., the minimum value allowed by oscillations data.新娘 发表于 2025-3-29 04:33:05
Scale-Dependent Galaxy Bias and CMB Lensing-Galaxy Cross-Correlations,However, naïvely comparing the constraining power of .(.) versus BAO measurements revealed that improvements are needed in order to fully harness the constraining power of the former, especially in terms of getting a better handle on the galaxy bias.Fantasy 发表于 2025-3-29 09:38:04
Scale-Dependent Galaxy Bias and CMB Lensing-Galaxy Cross-Correlations,However, naïvely comparing the constraining power of .(.) versus BAO measurements revealed that improvements are needed in order to fully harness the constraining power of the former, especially in terms of getting a better handle on the galaxy bias.捏造 发表于 2025-3-29 14:56:45
http://reply.papertrans.cn/103/10220/1021959/1021959_46.png1分开 发表于 2025-3-29 17:56:31
http://reply.papertrans.cn/103/10220/1021959/1021959_47.pngPalpate 发表于 2025-3-29 20:52:44
Overview of Physical Cosmology,ic, and correspondingly the Friedmann equations, Eqs. (2.4) and (2.5). In this Chapter, I will provide a more detailed (but still rather brief) picture of physical cosmology and the (thermal) history of the Universe, starting from the equations we have seen in Sect. 2.2 and elementary notions of theconcise 发表于 2025-3-30 03:43:05
Overview of Physical Cosmology,ic, and correspondingly the Friedmann equations, Eqs. (2.4) and (2.5). In this Chapter, I will provide a more detailed (but still rather brief) picture of physical cosmology and the (thermal) history of the Universe, starting from the equations we have seen in Sect. 2.2 and elementary notions of the天真 发表于 2025-3-30 06:15:41
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