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Poplawski, N. (2009) Classical Physics: Spacetime and Fields. arXiv: 0911.0334.
https://doi.org/10.48550/arXiv.0911.0334

has been cited by the following article:

• TITLE: How Relic Black Holes, in the Early Universe in Terms of a Quantum Number n as Specified Are Linked to Torsion, Cosmological Constant and Also Adding Quantum Hair to Quantum Black Holes

  AUTHORS: Andrew Walcott Beckwith

  KEYWORDS: Inflation, Gravitational Waves, Penrose CCC

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.10 No.4, September 24, 2024

  ABSTRACT: Our idea is to state that a particular set of values and reformulation of initial conditions for relic black holes, as stated in this manuscript, will enable using the idea of Torsion to formulate a cosmological constant and resultant Dark Energy. Relic Planck sized black holes will allow for a spin density term which presents an opportunity to modify a brilliant argument given as to cancelling Torsion as given by de Sabbata and Sirvaram, Erice 1990. Meantime speculation given by Corda replaces traditional firewalls in relic Black holes with a different formulation are included with a quantum number, n. In addition and most important, we have that there may be a solution to showing the incompleteness of the black holes have no hair theorem, for reasons which require quantum number, n, and also BEC representation of Black holes in primordial conditions.