Russian Presidential Academy of National Economy and Public Administration, Stolypin Volga Region Institute, Saratov, Russia
* Author to whom correspondence should be addressed
2023.2(2); https://doi.org/10.58396/gges020203
Received: 28 Mar 2024 / Accepted:16 Apr 2024 / Published: 29 Apr 2024
more >
Calling for papers-GGES
2023-12-21
Cosmological constant, virtual particles, neutron, neutron cluster, Planck length, Planck mass.
[1] Weinberg, C. S. The cosmological constant problem (Moris Loeb lectures inphysics, Harvard University. May 2, 3, 5, and 10, 1988): UTTG_12_88
[2] Rindler, W. Relativity Special, General and Cosmological. 2nd Ed, (2006) Oxford Univ. Press.
[3] Zel’dovich, Ya. B. The cosmological constant and the theory of elementary particles,Sov. Phys. Uspekhi (1968) 11, PP. 381–393.
[4] Zayko, Y.N. The Dynamics of the Neutron Complexes: From Neutron Star to Black Hole, Int. J. of Astrophysics and Space Science (2019), V. 7 (4); PP 45-49, DOI: 0.11648/j.ijass.20190704.11
[5] The Demystification of the Mystery of the Cosmological Constant,in the book: YuriyZayko, General Relativity in Applications. Hypercomputations. Cosmology. Particles, LAP Lambert Academic Publishing (2023) ISBN: 978-620-6-84329-0.
[6] Zayko, Y.N. Calculation of the Effective Gravitational Charge using the Newton-Schrödinger Equations, International Journal of Scientific and Innovative Mathematical Research (2019) V. 7 (6), PP 17-22, DOI: http://dx.doi.org/10.20431/2347-3142.0706003
[7] Moroz, I.M., Penrose, R., Tod, P. Spherically-symmetric solutions of theSchrōdinger–Newton equations, Class. Quantum Grav. (1998) 15,2733–2742.
[8] Harrison, R., Moroz, I., Tod, K. P. A numerical study of the Schrōdinger-Newton equation, 1: Perturbing the spherically-symmetric stationary states, arXiv:math-ph/0208045v1 30 Aug 2002
[9] Harrison, R., Moroz, I., Tod, K. P. A numerical study of the Schrōdinger-Newton equation, 2: the time-dependent problem, arXiv:math-ph/0208046v1 30 Aug 2002
[10] Polyanin, A.D., Zaitsev. V. F. (2003) Handbook of Nonlinear Partial Differential Equations, (Handbooks of Mathematical Equations), 2nd Edition, Chapman and Hall/CRC, Boca Raton.
[11] Feynman, R. P., Morinigo, F.P., Wagner, W.G. 1995, Feynman Lectures on Gravitation, Ed. By B. Hartfield, Addison-Wesley Publishing Co.
[12] Zayko, Y.N. Spiral Galaxy Model Free of Dark Matter, Theoretical Physics Letters (2020) 06 (06) pp. 94 – 100, https://www.wikipt.org/tphysicsletters, DOI: 10.1490/ptl.dxdoi.com/08-01tpl-sci; Available from: https://www.researchgate.net/ publication/347258981_Spiral_Galaxy_Model_Free_of_Dark_Matter
[13] ВоhrА., МоttеlsопВ. R., Pines D., Possible analogy betweenthe excitation spectra of nuclei and those ofthe superconducting metals slate (1958) Phys. Rev., 110, № 4, p. 9.
[14] Lifshitz, E. M.; Pitaevskii, L. P. (1980). Statistical Physics, Part 2: Theory of the Condensed State. Vol. 9 (1st ed.). Butterworth-Heinemann..
[15] Wondrak, M.F., van Suijlekom, W, D., Falcke, H. Gravitational Pair Production and Black Hole Evaporation,arXiv: 2305.18521v1 [gr-qc] 29 May 2023.
[16] Wang, Q., Zhen Zhu, Z., Unruh, W.G., How the huge energy of quantum vacuum gravitates to drive the slow accelerating expansion of the Universe, arXiv: 1703.00543v2 [gr-qc] 11 May 2017.
[17] Gamow, G. Expanding Universe and the Origin of Elements (1946) Phys. Rev., 70, 572-575.