Published November 18, 2022 | Version v1
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The Dialectic Epistemological Possibility of Objects related to Dark Energy and Dark Matter: Supplementary Study to the Epistemic Justification of Whole-Reason

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  • 1. No

Description

The study takes up the notion expounded in recent research that the modern disciplines of epistemology and science are implicitly engaged in a constant reciprocal dialectic, and then such a dialectic as has been historically characterized by the incognizant usage of an epistemically unjustified form of reasoning that connects, directs and delimits the respective discourses of these disciplines in conceptually problematic ways. Upon the newly formulated epistemology of reason the current discourse gives demonstration to how the identified dialectic can be explicitly utilized over the use of an epistemically justified form of reasoning to develop more sophisticated scientific knowledges of investigated objects. Here the cosmological phenomena related to the hypotheses of respectively dark energy and dark matter will be theoretically reflected through the logico-semantic structuring of the ‘whole’ form of reason, and thus rationally developed into a novel scientific formulation of potentially testable object knowledge.     

Notes

An early version of the basic argument of the presented cosmological principle/dynamic was originally proposed as part of a book first published in 2013 by the same author. Book title: The Premise of Non-locality.

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Is supplement to
Journal article: 10.1007/s11406-021-00399-3 (DOI)

References

  • Arbey, A., & Mahmoudi, F. (2021). Dark matter and the early universe: a review. Progress in Particle and Nuclear Physics, 119, 103865. Arun, K., Gudennavar, S. B., & Sivaram, C. (2017). Dark matter, dark energy, and alternate models: a review. Advances in Space Research, 60(1), 166-186. Bidin, C. M., Carraro, G., Mendez, R. A., & van Altena, W. F. (2010). No evidence for dark matter disk within 4 kpc from galactic plane. The Astrophysical Journal Letters, 724, L122-L126. Bidin, C. M., Carraro, G., Mendez, R. A., & Smith, R. (2012). Kinematical and chemical vertical structure of the galactic thick disk. II. A lack of dark matter in the solar neighbourhood. The Astrophysical Journal Letters, 751, 30-44. Bidin, C. M., Carraro, G., Mendez, R. A., & Moyano, M. (2014). On the local dark matter density. Astronomy and Astrophysics, 573, A91. Chadha-Day, F., Ellis, J., & Marsh, D. J. E. (2022). Axion dark matter: what is it and why now? Science Advances, 8(8), eabj3618. Dreyer, V.M. (2022). The epistemology and science of justified reason. Philosophia, 50, 503- 532. Hauser, J., & Dröscher, W. (2017). Gravity beyond Einstein? Part I: physics and the trouble with experiments, Z. Naturforsch, 72(6)a, 493-525. Markevitch, M., Gonzalez, A. H., Clowe, D., Vikhlinin, A., Forman, W., Jones, C., Murray, S., & Tucker, W. (2004). Direct constraints on the dark matter self-interaction cross section from the merging galaxy cluster 1E 0657-56. Astrophys. J., 606, 819-824. Nicolson, I. (2007). Dark side of the universe: dark matter, dark energy, and the fate of the cosmos. Baltimore: The Johns Hopkins University Press. Peebles, P. J. E., & Ratra, B. (2003). The cosmological constant and dark energy. Rev. Mod. Phys., 75, 559. Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D.E., & Hook, I. M. (1999). Measurements of Ω and Λ from 42 high-redshift supernovae. The Astrophysical Journal, 517(2), 565. Pooley, O. (2008). Space and time. In C. Martin, & P. Stathis (Eds.), The Routledge companion to philosophy of science (pp. 452-467). New York: Routledge. Popper, K. R. (2002). The logic of scientific discovery. London: Routledge. Riess, A. G., Filippenko, A. V., Challis, P., Clocchiatti, A., Diercks, A., Garnavich, P. M., Gilliland, R.L., Hogan, C.J., Jha, S., Kirshner, R.P. and Leibundgut, B.R.U.N.O., (1998). Observational evidence from supernovae for an accelerating universe and a cosmological constant. The Astronomical Journal, 116(3), 1009. Rubin, V. C., & Ford Jr., W. K. (1970). Rotation of the Andromeda nebula from a spectroscopic survey of emission regions. Astrophys. J. 159, 379-403. Rubin, V.C., Ford Jr., W.K., & Thonnard, N. (1980). Rotational properties of 21 SC galaxies with a large range of luminosities and radii, from NGC 4605 /R = 4kpc/ to UGC 2885 /R =122 kpc/. Astrophys. J., 238, 471-487. Sanders, R. H. (2010). The dark matter problem: a historical perspective. Cambridge: Cambridge University Press. Sivaram, C. (1994). Mond, dark matter and the cosmological constant. Astrophys. Space Sci. 219, 135-141. Sivaram, C. (1999). A non-anthropic origin for a small cosmological constant. Mod. Phys. Lett. A 14, 2363-2366. Vagnozzi, S., Visinelli, L., Brax, P., Davis, A-C., & Sakstein, J. (2021). Direct detection of dark energy: the XENON1T excess and future prospects. Physical Review D, 104, 063023. Wang, B., Abdalla, E., Atrio-Barandela, F., & Pavon, D. (2016). Dark matter and dark energy interactions: theoretical challenges, cosmological implications and observational signatures. Reports on Progress in Physics, 79(9), 096901. Zwicky, F. (1937). On the masses of nebulae and of clusters of nebulae. The Astrophysical Journal, 86, 217.