Formation and growth of the first supermassive black holes in MOG

被引：2

作者：

Haghighi, Mohammad H. Zhoolideh ^{[1
,2
,3
]}

Moffat, John ^{[3
,4
]}

机构：

[1] KN Toosi Univ Technol, Dept Phys, POB 15875-4416, Tehran, Iran

[2] Inst Res Fundamental Sci IPM, Sch Astron, Tehran 193955746, Iran

[3] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada

[4] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada

来源：

EUROPEAN PHYSICAL JOURNAL C | 2024年 / 84卷 / 03期

关键词：

WEAK-FIELD APPROXIMATION; DIGITAL SKY SURVEY; OBSERVATIONAL TEST; ACCRETION; REDSHIFT; QUASARS; DISCOVERY; EVOLUTION; UNIVERSE;

D O I：

10.1140/epjc/s10052-024-12612-0

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The emergence of supermassive black holes (SMBHs) in the early universe remains a topic of profound interest and debate. In this paper, we investigate the formation and growth of the first SMBHs within the framework of Modified Gravity (MOG), where gravity exhibits increased strength. We explore how MOG, as an alternative to the standard model, may offer novel insights into the emergence of SMBHs and potentially reconcile the discrepancies observed in the accretion and growth processes. We examine the dynamics of gas and matter in this modified gravitational framework, shedding light on the unique interplay between gravity and the formation of SMBHs.

引用

页数：9

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