AI 中文总结
该研究回应Pantheon+超新星相关的暗能量辩论，指出Ray等人混淆坐标搞错CMB偶极子方向，其否定SRS26各向异性论点的结论无依据。
AI 中文摘要
Ray等人[1]声称，从Pantheon+星表的Ia型超新星推断出的哈勃膨胀率加速度“在CMB偶极子（$q_m = +1.45$）和反偶极子半球（+1.55）中同样强烈，直接与SRS26各向异性论点矛盾”。此处SRS26指我们的分析[2]，该分析显示“局部$q_0$具有与 bulk flow 大致对齐的强偶极各向异性，且在超过数百兆秒差距的距离上仅剩下小的单极分量”。我们发现这些作者混淆了赤道坐标与银道坐标，从而搞错了CMB偶极子方向，因此他们的结论是无根据的。
英文摘要
Ray et al. [1] have claimed that the acceleration of the Hubble expansion rate inferred from Type Ia supernovae in the Pantheon+ catalogue "is equally strong in the CMB dipole ($q_m = + 1.45$) and anti-dipole hemispheres ($+ 1.55$), directly contradicting the SRS26 anisotropy argument". Here SRS26 refers to our analysis [2] which showed that "locally $q_0$ has a strong dipole anisotropy aligned approximately with the bulk flow, and only a small monopole component remains at distances exceeding a few hundred Mpc". We find that these authors confused Equatorial with Galactic coordinates, thereby getting the CMB dipole direction wrong. Hence their conclusion is baseless.
Comments1 page; Comment on arXiv:2607.20570v1
