Galaxy dynamics tracing quantum cosmology beyond ACDM below the de Sitter scale of acceleration

被引:2
作者
van Putten, Maurice H. P. M. [1 ,2 ]
机构
[1] Sejong Univ, Phys & Astron, 209 Neungdong ro, Seoul, South Korea
[2] INAF, OAS Bologna, via P Gobetti,101, I-40129 Bologna, Italy
基金
新加坡国家研究基金会;
关键词
Galaxy dynamics - cosmology; SUPERMASSIVE BLACK-HOLE; DARK-MATTER; LAMBDA-CDM; TELESCOPE; CONSTANT; WAVE;
D O I
10.1016/j.cjph.2024.07.040
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It is proposed that the baryonic Tully-Fisher relation (bTFR) and JWST 'Impossible galaxies' at cosmic dawn are unified in weak gravity by the trace J of the Schouten tensor below the Sitter scale of acceleration a(dS )= cH, where c is the velocity of light and H is the Hubble parameter. Across a(dS), J parametrizes short-period galaxy rotation curves and fast gravitational collapse beyond the predictions of Lambda CDM. The sensitivity of weak gravitation to J=16R is derived in infrared gravitation from a consistent limit of quantum gravity, reducing to general relativity in the limit of a small Planck constant, where R is Ricci scalar tensor. For the first time, it identifies the exact relation a(0 )= c(2 )root J/2 pi of the Milgrom parameter across all redshifts, accounting for the bTFR and early galaxy formation accelerated by a factor similar to J(1/8). It predicts a ' 0(0)<0 at the present epoch.
引用
收藏
页码:377 / 381
页数:5
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