The Origin of Power and Acceleration of High-Redshift Galaxies in the Unicentric Model of the Universe
- 1 IWR, University of Heidelberg, Heidelberg, Germany
Abstract
Recently, a unicentric model of our observable universe was proposed. Accordingly, the big bang was neither a singular event nor invoked by external forces, but rather a frequent event in cosmic life cycles that occur sequentially or in parallel at the same and/or in different locations of our infinitely large, flat, homogeneous, and isotropic parent universe. The progenitor of our big bang is predicted to have been of a measurable size and happened to be in our neighbourhood. Based on theoretical arguments and general relativistic numerical calculations, it is argued that: 1) The surface of the progenitor is most appropriate for the hadron flash to run away; 2) The structure of the progenitor is immune to self-collapse into a hyper-massive black hole; and 3) The power and acceleration of high-redshift galaxies may be connected to the BB-explosion. We conclude that the currently observed high-redshift galaxies must have been old and inactive in older times, but turned into life through matter and momentum transfer from the fireball and the collision of the locally curved spacetime embedding the galaxy with the expanding one embedding the fireball. With the present scenario, the origin of the monstrous black hole candidates with M BH ≥10 9 M e , that are believed to have resided at the centre of galaxies when the observable universe was 400 Myr old, could be straightforwardly explained. This implies that QSOs with ever higher redshifts should exist, though their detection becomes increasingly harder.
- Mann, A. (2020) The Golden Age of Neutron-Star Physics Has Arrived. Nature, 579, 20-22. https://doi.org/10.1038/d41586-020-00590-8
- Glendenning, N.K. (2007) Special and General Relativity. Springer, New York. https://doi.org/10.1007/978-0-387-47109-9
- Camenzind, M. (2007) Compact Objects in Astrophysics. Springer, Berlin.
- Hujeirat, A.A. and Samtaney, R. (2019) Glitching Pulsars: Unraveling the Interactions of General Relativistic and Quantum Fields in the Strong Field Regimes. Journal of Modern Physics, 10, 1696-1712. https://doi.org/10.4236/jmp.2019.1014111
- Fan, X., Wang, F., Jinyi Yang, J., et al. (2019) The Discovery of a Gravitationally Lensed Quasar at z = 6.51. The Astrophysical Journal Letters, 870, L11 https://doi.org/10.3847/2041-8213/aaeffe
- Hujeirat, A.A. (2021) Does Our Universe Conform with the Existence of a Universal Maximum Energy-Density p max uni Journal of Modern Physics, 12, 937-958. https://doi.org/10.4236/jmp.2021.127057
- Laporte, N., Meyer, R.A., Ellis, R.S., et al. (2021) Probing Cosmic Dawn: Ages and Star Formation Histories of Candidate z ≥ 9 Galaxies. Monthly Notices of the Royal Astronomical Society, 505, 3336-3346. https://doi.org/10.1093/mnras/stab1239
- Oesch, P.A., et al. (2016) A Remarkably Luminous Galaxy at Z = 11.1 Measured with Hubble Space Telescope Grism Spectroscopy. The Astrophysical Journal, 819, Article No. 129. https://doi.org/10.3847/0004-637X/819/2/129
- Yang, J., Wang, F., Fan, X., et al. (2020) Pōniuā’ena: A Luminous z = 7.5 Quasar Hosting a 1.5 Billion Solar Mass Black Hole. The Astrophysical Journal Letters, 897, L14. https://doi.org/10.3847/2041-8213/ab9c26
- Shao, Y. (2022) On the Neutron Star/Black Hole Mass Gap and Black Hole Searches. Research in Astronomy and Astrophysics, 22, Article ID: 122002. https://doi.org/10.1088/1674-4527/ac995e
- Haensel, P., Potekhin, A.Y. and Yakovlev, D.G. (2007) Neutron Stars 1. Springer, New York. https://doi.org/10.1007/978-0-387-47301-7
- Eskola, K.J. (2019) Nearly Perfect Quark-Gluon Fluid. Nature Physics, 15, 1111-1112. https://doi.org/10.1038/s41567-019-0643-0
- Abbott, B.P., et al. (2017) Multi-Messenger Observations of a Binary Neutron Star Merger. The Astrophysical Journal Letters, 848, L12. https://doi.org/10.3847/2041-8213/aa91c9
- Piro, L., Troja, E., Zhang, B., et al. (2019) A Long-Lived Neutron Star Merger Remnant in GW170817: Constraints and Clues from X-Ray Observation. Monthly Notices of the Royal Astronomical Society, 483, 1912-1921. https://doi.org/10.1093/mnras/sty3047