Scrutinizing the primordial black hole interpretation of PTA gravitational waves and JWST early galaxies

被引:15
作者
Gouttenoire, Yann [1 ]
Trifinopoulos, Sokratis [2 ]
Valogiannis, Georgios [3 ]
Vanvlasselaer, Miguel [4 ,5 ]
机构
[1] Tel Aviv Univ, Sch Phys & Astron, IL-69978 Tel Aviv, Israel
[2] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA
[3] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[4] Vrije Univ Brussel, Theoret Natuurkunde & IIHE ELEM, Pleinlaan 2, B-1050 Brussels, Belgium
[5] Int Solvay Inst, Pleinlaan 2, B-1050 Brussels, Belgium
基金
瑞士国家科学基金会;
关键词
UV LUMINOSITY FUNCTIONS; HUBBLE FRONTIER FIELDS; WARM DARK-MATTER; SIMILAR-TO; 6; MASSIVE GALAXIES; POWER SPECTRUM; POINT MASSES; CONSTRAINTS; REIONIZATION; BINARIES;
D O I
10.1103/PhysRevD.109.123002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent observations have granted to us two unique insights into the early Universe: the presence of a low-frequency stochastic gravitational wave background detected by the NANOGrav and Pulsar Timing Array (PTA) experiments and the emergence of unusually massive galaxy candidates at high redshifts reported by the James Webb Space Telescope (JWST). In this paper, we consider the possibility that both observations have a common origin, namely primordial black holes (PBHs) in the mass range between 106M circle dot and 1013M circle dot. While superheavy PBHs act as seeds for accelerated galaxy formation capable of explaining the JWST extreme galaxies, they can also form binary mergers that source gravitational waves which can be potentially identified as the PTA signal. The analysis is performed taking into account the constraints on the relevant region of the PBH parameter space including the novel bound imposed by the ultraviolet luminosity function of galaxies observed by the Hubble Space Telescope. We conclude that PTA's and JWST's interpretations in terms of PBH binary mergers and Poissonian gas of PBHs, respectively, are strongly excluded.
引用
收藏
页数:14
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