Farrah, D., Petty, S., Croker, K.S., Tarlé, G., Zevin, M., Hatziminaoglou, E., Shankar, F., Wang, L., Clements, D.L., Efstathiou, A., Lacy, M., Nishimura, K.A., Afonso, J., Pearson, C. and Pitchford, L.K. (2023) A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z ≤ 2. ApJ, 943, 133.
https://doi.org/10.3847/1538-4357/acac2e

has been cited by the following article:

• TITLE: Part II: Explaining Black Hole Growth due to Universal Expansion: Probabilistic Spacetime versus GEODEs

  AUTHORS: Dennis M. Doren, James Harasymiw

  KEYWORDS: Probabilistic Spacetime, GEODE, Cosmological Coupling, Universal Expansion, Black Holes

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.9 No.2, April 18, 2023

  ABSTRACT: Recent research indicates that black holes can grow based on the expansion of the universe and not just through accretion and mergers. Two different models independently predicted that finding. One model, describing the relevant massive star remnants as “generic objects of dark energy”, rejects the traditional view of black holes while hypothesizing that dark energy causes the cosmologically coupled growth of these objects. The other model, based on the probabilistic spacetime theory, indicates the growth of black holes is based on the same spacetime mechanism underlying all universal expansion, and does so while leaving the traditional black hole conceptualization essentially intact. The fact these two models predicted this observational finding but did so from different perspectives suggests more can be learned by further study of their differences. This paper explores similarities and differences in the two models’ explanations for massive star remnants’ growth, concluding with suggestions for research testing their relative veracity. An exploration of the relative utility and parsimony of the two models is also described.