Relevant bibliographies by topics / Einstein general relativity

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Einstein general relativity'

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Published: 10 March 2023

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Journal articles on the topic "Einstein general relativity"

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Barukčić, Ilija. "Anti Einstein – Refutation of Einstein’s General Theory of Relativity." International Journal of Applied Physics and Mathematics 5, no. 1 (2015): 18–28. http://dx.doi.org/10.17706/ijapm.2015.5.1.18-28.

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Lo, C. Y. "The Development of Relativity and Einstein." JOURNAL OF ADVANCES IN PHYSICS 10, no. 3 (October 6, 2015): 2874–85. http://dx.doi.org/10.24297/jap.v10i3.1327.

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There are errors in general relativity that must be rectified. As Zhou pointed out, Einstein’s covariance principle is proven to be invalid by explicit examples. Linearization is conditionally valid. Pauli's version of the equivalence principle is impossible in mathematics. Einstein's adaptation of the distance in Riemannian geometry is invalid in physics as pointed out by Whitehead. Moreover, it is inconsistent with the calculation on the bending of light, for which a Euclidean-like framework is necessary. Thus, the interpretation of the Hubble redshifts as due to receding velocities of stars is invalid. The Einstein equation has no dynamic solutions just as Gullstrand suspected. All claims on the existence of dynamic solutions for the Einstein equation are due to mistakes in non-linear mathematics. For the existence of a dynamic solution, the Einstein equation must be modified to the Lorentz-Levy-Einstein equation that have additionally a gravitational energy-stress tensor with an anti-gravity coupling. The existence of photons is a consequence of general relativity. Thus, the space-time singularity theorems of Hawking and Penrose are actually irrelevant to physics because their energy conditions cannot be satisfied. The positive mass theorem of Schoen and Yau is misleading because invalid implicit assumptions are used as Hawking and Penrose did. There are three experiments that show formula E = mc2 is invalid, and a piece of heated-up metal has reduced weight just as a charged capacitor. Thus, the weight is temperature dependent. It is found, due to the repulsive charge-mass interaction, gravity is not always attractive to mass. Since the assumption that gravity is always attractive to mass is not valid, the existence of black holes are questionable. Because of the repulsive charge-mass interaction, the theoretical framework of general relativity must be extended to a five-dimensional relativity of Lo, Goldstein & Napier. Thus Einstein's conjecture of unification is valid. Moreover, the repulsive gravitational force from a charged capacitor is incompatible with the notion of a four-dimensional space. In Quantum theory, currently the charge-mass interaction is neglected. Thus, quantum theory is not a final theory as Einstein claims.
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Heller, Michael. "Einstein algebras and general relativity." International Journal of Theoretical Physics 31, no. 2 (February 1992): 277–88. http://dx.doi.org/10.1007/bf00673258.

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Heller, Michael, Tomasz Miller, Leszek Pysiak, and Wiesław Sasin. "Generalized derivations and general relativity." Canadian Journal of Physics 91, no. 10 (October 2013): 757–63. http://dx.doi.org/10.1139/cjp-2013-0186.

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We construct differential geometry (connection, curvature, etc.) based on generalized derivations of an algebra [Formula: see text]. Such a derivation, introduced by Brešar in 1991, is given by a linear mapping [Formula: see text] such that there exists a usual derivation, d, of [Formula: see text] satisfying the generalized Leibniz rule u(ab) = u(a)b + ad(b) for all [Formula: see text]. The generalized geometry “is tested” in the case of the algebra of smooth functions on a manifold. We then apply this machinery to study generalized general relativity. We define the Einstein–Hilbert action and deduce from it Einstein’s field equations. We show that for a special class of metrics containing, besides the usual metric components, only one nonzero term, the action reduces to the O’Hanlon action that is the Brans–Dicke action with potential and with the parameter ω equal to zero. We also show that the generalized Einstein equations (with zero energy–stress tensor) are equivalent to those of the Kaluza–Klein theory satisfying a “modified cylinder condition” and having a noncompact extra dimension. This opens a possibility to consider Kaluza–Klein models with a noncompact extra dimension that remains invisible for a macroscopic observer. In our approach, this extra dimension is not an additional physical space–time dimension but appears because of the generalization of the derivation concept.
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Ni, Wei-Tou. "Genesis of general relativity — A concise exposition." International Journal of Modern Physics D 25, no. 14 (December 2016): 1630004. http://dx.doi.org/10.1142/s0218271816300044.

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This short exposition starts with a brief discussion of situation before the completion of special relativity (Le Verrier’s discovery of the Mercury perihelion advance anomaly, Michelson–Morley experiment, Eötvös experiment, Newcomb’s improved observation of Mercury perihelion advance, the proposals of various new gravity theories and the development of tensor analysis and differential geometry) and accounts for the main conceptual developments leading to the completion of the general relativity (CGR): gravity has finite velocity of propagation; energy also gravitates; Einstein proposed his equivalence principle and deduced the gravitational redshift; Minkowski formulated the special relativity in four-dimentional spacetime and derived the four-dimensional electromagnetic stress–energy tensor; Einstein derived the gravitational deflection from his equivalence principle; Laue extended Minkowski’s method of constructing electromagnetic stress-energy tensor to stressed bodies, dust and relativistic fluids; Abraham, Einstein, and Nordström proposed their versions of scalar theories of gravity in 1911–13; Einstein and Grossmann first used metric as the basic gravitational entity and proposed a “tensor” theory of gravity (the “Entwurf” theory, 1913); Einstein proposed a theory of gravity with Ricci tensor proportional to stress–energy tensor (1915); Einstein, based on 1913 Besso–Einstein collaboration, correctly derived the relativistic perihelion advance formula of his new theory which agreed with observation (1915); Hilbert discovered the Lagrangian for electromagnetic stress–energy tensor and the Lagrangian for the gravitational field (1915), and stated the Hilbert variational principle; Einstein equation of GR was proposed (1915); Einstein published his foundation paper (1916). Subsequent developments and applications in the next two years included Schwarzschild solution (1916), gravitational waves and the quadrupole formula of gravitational radiation (1916, 1918), cosmology and the proposal of cosmological constant (1917), de Sitter solution (1917), Lense–Thirring effect (1918).
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DUPRÉ, MAURICE J., and FRANK J. TIPLER. "GENERAL RELATIVITY AS AN ÆTHER THEORY." International Journal of Modern Physics D 21, no. 02 (February 2012): 1250011. http://dx.doi.org/10.1142/s0218271812500113.

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Most early twentieth century relativists — Lorentz, Einstein, Eddington, for examples — claimed that general relativity was merely a theory of the æther. We shall confirm this claim by deriving the Einstein equations using æther theory. We shall use a combination of Lorentz's and Kelvin's conception of the æther. Our derivation of the Einstein equations will not use the vanishing of the covariant divergence of the stress–energy tensor, but instead equate the Ricci tensor to the sum of the usual stress–energy tensor and a stress–energy tensor for the æther, a tensor based on Kelvin's æther theory. A crucial first step is generalizing the Cartan formalism of Newtonian gravity to allow spatial curvature, as conjectured by Gauss and Riemann. In essence, we shall show that the Einstein equations are a special case of Newtonian gravity coupled to a particular type of luminiferous æther. Our derivation of general relativity is simple, and it emphasizes how inevitable general relativity is, given the truth of Newtonian gravity and the Maxwell equations.
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Eisinger, Josef. "Thoughts on Einstein and general relativity." Physics Today 69, no. 10 (October 2016): 12. http://dx.doi.org/10.1063/pt.3.3312.

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Klainerman, Sergiu. "General Relativity and the Einstein Equations." Classical and Quantum Gravity 27, no. 1 (December 16, 2009): 019001. http://dx.doi.org/10.1088/0264-9381/27/1/019001.

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von Borzeszkowski, H. H., and H. J. Treder. "Mach-Einstein doctrine and general relativity." Foundations of Physics 26, no. 7 (July 1996): 929–42. http://dx.doi.org/10.1007/bf02148835.

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Kox, A. J. "Einstein, Lorentz, Leiden and general relativity." Classical and Quantum Gravity 10, S (December 1, 1993): S187—S191. http://dx.doi.org/10.1088/0264-9381/10/s/020.

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Dissertations / Theses on the topic "Einstein general relativity"

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Maidens, Anna Victoria. "The hole argument : substantivalism and determinism in general relativity." Thesis, University of Cambridge, 1993. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.309205.

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Longobardi, Agata. "On the formulation of Einstein general relativity in a phisycal reference system." Doctoral thesis, Universita degli studi di Salerno, 2012. http://hdl.handle.net/10556/347.

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2010 - 2011
The research deals with the breaking of the evolution problem of a reversible material system in two different problems, the initial data problem and the restricted evolution problem. This breaking, intrinsically formulated, permits to study of the evolution of a perfect fluid which produces a spherically symmetric 4--manifold. By using different systems of coordinates adapted to the world-lines of this fluid, such as curvature coordinates, gaussian coordinates, gaussian polar coordinates and harmonic coordinates, different exact solutions are obtained. In particular, in gaussian coordinates, I have obtained two solutions already deduced, in a different way, by Wesson and Gutman, showing that they are physically equivalent. In addition, by considering the frames of reference associated to isotropic coordinates and spherical symmetry, I have obtained that the restricted evolution problem gives dynamic models non different from Einstein--deSitter or Friedman--Robertson--Walker or Wyman models; moreover, if the distribution of the fluid is initially regular in the symmetry center, and the Hubble parameter is constant, all the configurations of the fluid are demonstrated to be Euclidean hypersurfaces. Finally, I have studied the geometrical and physical characteristics of the class of reference frames associated to harmonic coordinates. Precisely, I express in relative form the harmonicity conditions and consider the so called “spatially harmonicity" of a reference frame in spherical symmetry. The initial data problem is then analyzed in polar coordinates and the obtained results are applied to special cases of exact solutions. [edited by author]
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Hajj-Boutros, Joseph. "Détermination des nouvelles solutions exactes d’Einstein dans le cas intérieur." Paris 6, 1987. http://www.theses.fr/1987PA066421.

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Ensemble de travaux réalisé dans le cadre de la théorie de la relativité générale. La métrique de l'espace-temps adoptée est à symétrie bien précise pour simplifier dans la mesure du possible les équations du champ d’Einstein. Dans le cadre de la symétrie sphérique statique et non statique, nous avons obtenu de nouvelles solutions des équations du champ (cas intérieur). Dans le cas de la symétrie plane, nous avons pu engendrer plusieurs nouvelles solutions statiques et non statiques. Nous avons mis au point de nouvelles solutions du type cosmologique. L'espace-temps utilise étant essentiellement homogène, nous avons pu étudier le caractère non isotropique de la singularité initiale. Les conditions physiques ont été respectées. Dans le cas des solutions cosmologiques nous avons pu construire un modèle rendant compte de l'évolution possible de notre univers depuis son état initial radiatif et singulier jusqu'à son état actuel. Nous avons trouvé une solution globalement régulière dans le cadre de la symétrie cylindrique. La technique du calcul utilise a consisté dans la plupart des cas à linéariser les équations du champ.
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Ames, Ellery. "Singular Symmetric Hyperbolic Systems and Cosmological Solutions to the Einstein Equations." Thesis, University of Oregon, 2014. http://hdl.handle.net/1794/17905.

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Characterizing the long-time behavior of solutions to the Einstein field equations remains an active area of research today. In certain types of coordinates the Einstein equations form a coupled system of quasilinear wave equations. The investigation of the nature and properties of solutions to these equations lies in the field of geometric analysis. We make several contributions to the study of solution dynamics near singularities. While singularities are known to occur quite generally in solutions to the Einstein equations, the singular behavior of solutions is not well-understood. A valuable tool in this program has been to prove the existence of families of solutions which are so-called asymptotically velocity term dominated (AVTD). It turns out that a method, known as the Fuchsian method, is well-suited to proving the existence of families of such solutions. We formulate and prove a Fuchsian-type theorem for a class of quasilinear hyperbolic partial differential equations and show that the Einstein equations can be formulated as such a Fuchsian system in certain gauges, notably wave gauges. This formulation of Einstein equations provides a convenient general framework with which to study solutions within particular symmetry classes. The theorem mentioned above is applied to the class of solutions with two spatial symmetries -- both in the polarized and in the Gowdy cases -- in order to prove the existence of families of AVTD solutions. In the polarized case we find families of solutions in the smooth and Sobolev regularity classes in the areal gauge. In the Gowdy case we find a family of wave gauges, which contain the areal gauge, such that there exists a family of smooth AVTD solutions in each gauge.
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Stark, Elizabeth. "Gravitoelectromagnetism and the question of stability in general relativity." Monash University, School of Mathematical Sciences, 2004. http://arrow.monash.edu.au/hdl/1959.1/9509.

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Taylor, Stephen M. "On Stability and Evolution of Solutions in General Relativity." Diss., CLICK HERE for online access, 2007. http://contentdm.lib.byu.edu/ETD/image/etd2033.pdf.

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Dilts, James. "The Einstein Constraint Equations on Asymptotically Euclidean Manifolds." Thesis, University of Oregon, 2015. http://hdl.handle.net/1794/19237.

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In this dissertation, we prove a number of results regarding the conformal method of finding solutions to the Einstein constraint equations. These results include necessary and sufficient conditions for the Lichnerowicz equation to have solutions, global supersolutions which guarantee solutions to the conformal constraint equations for near-constant-mean-curvature (near-CMC) data as well as for far-from-CMC data, a proof of the limit equation criterion in the near-CMC case, as well as a model problem on the relationship between the asymptotic constants of solutions and the ADM mass. We also prove a characterization of the Yamabe classes on asymptotically Euclidean manifolds and resolve the (conformally) prescribed scalar curvature problem on asymptotically Euclidean manifolds for the case of nonpositive scalar curvatures. This dissertation includes previously published coauthored material.
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Gasperin, Garcia. "Applications of conformal methods to the analysis of global properties of solutions to the Einstein field equations." Thesis, Queen Mary, University of London, 2017. http://qmro.qmul.ac.uk/xmlui/handle/123456789/25820.

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Although the study of the initial value problem in General Relativity started in the decade of 1950 with the work of Foures-Bruhat, addressing the problem of global non-linear stability of solutions to the Einstein field equations is in general a hard problem. The first non-linear global stability result in General Relativity was obtained for the de-Sitter spacetime by means of the so-called conformal Einstein field equations introduced by H. Friedrich in the decade of 1980. The latter constitutes the main conceptual and technical tool for the results discussed in this thesis. In Chapter 1 the physical and geometrical motivation for these equations is discussed. In Chapter 2 the conformal Einstein equations are presented and first order hyperbolic reduction strategies are discussed. Chapter 3 contains the first result of this work; a second order hyperbolic reduction of the spinorial formulation of the conformal Einstein field equations. Chapter 4 makes use of the latter equations to give a discussion of the non-linear stability of the Milne universe. Chapter 5 is devoted to the analysis of perturbations of the Schwarzschild-de Sitter spacetime via suitably posed asymptotic initial value problems. Chapter 6 gives a partial generalisation of the results of Chapter 5. Finally a result relating the Newman-Penrose constants at future and past null infinity for spin-1 and spin-2 fields propagating on Minkowski spacetime close to spatial infinity is discussed in Chapter 7 exploiting the framework of the cylinder at spatial in nity. Collectively, these results show how the conformal Einstein field equations and more generally conformal methods can be employed for analysing perturbations of spacetimes of interest and extract information about their conformal structure.
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Machado, Ramos Maria da Peidade. "Invariant differential operators and the equivalence problem of algebraically special spacetimes." Thesis, University of Southampton, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.241986.

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Bredberg, Irene. "The Einstein and the Navier-Stokes Equations: Connecting the Two." Thesis, Harvard University, 2012. http://dissertations.umi.com/gsas.harvard:10214.

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This thesis establishes a precise mathematical connection between the Einstein equations of general relativity and the incompressible Navier-Stokes equation of fluid dynamics. We carry out a holographic analysis which relates solutions to the Einstein equations to the behaviour of a dual fluid living in one fewer dimensions. Gravitational systems are found to exhibit Navier-Stokes behaviour when we study the dynamics of the region near an event horizon. Thus, we find non-linear deformations of Einstein solutions which, after taking a suitable near horizon limit and imposing our particular choice of boundary conditions, turn out to be precisely characterised by solutions to the incompressible Navier-Stokes equation. In other words, for any solution to the Navier-Stokes equation, the set-up we present provides a solution to the Einstein equations near a horizon. We consider the cases of fluids flowing on the plane and on the sphere. Fluid dynamics on the plane is analysed foremost in the context of a flat background geometry whilst the spherical analysis is undertaken for Schwarzschild black holes and the static patch of four-dimensional de Sitter space.
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Books on the topic "Einstein general relativity"

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General relativity and the Einstein equations. Oxford: Oxford University Press, 2009.

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Allais, Maurice. Albert Einstein: Un extraordinaire paradoxe. Paris: C. Juglar, 2005.

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Allais, Maurice. Albert Einstein: Un extraordinaire paradoxe. Paris: C. Juglar, 2005.

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Was Einstein right?: Putting general relativity to the test. 2nd ed. Oxford: Oxford University Press, 1995.

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Will, Clifford M. Was Einstein right?: Putting general relativity to the test. Oxford: Oxford University Press, 1988.

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Thibault, Damour, ed. Einstein, 1905-2005: Poincaré Seminar 2005. Boston: Birkhäuser Verlag, 2006.

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Einstein: A hundred years of relativity. New York: Harry N. Abrams, 2005.

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1956-, Renn Jürgen, Janssen M, and Schemmel Matthias, eds. The genesis of general relativity. Dordrecht: Springer, 2007.

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1956-, Renn Jürgen, Janssen M, and Schemmel Matthias, eds. The genesis of general relativity. Dordrecht: Springer, 2007.

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Was Einstein right?: Putting general relativity to the test. 2nd ed. New York, NY: BasicBooks, 1993.

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Book chapters on the topic "Einstein general relativity"

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Ryckman, Thomas. "General relativity." In Einstein, 196–246. 1 [edition]. | New York : Routledge, 2017. | Series: Routledge philosophers: Routledge, 2017. http://dx.doi.org/10.4324/9781315175829-7.

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Solomon, Adam Ross. "Gravity Beyond General Relativity." In Cosmology Beyond Einstein, 21–51. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-46621-7_2.

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Shapira, Yair. "General Relativity: Einstein Equations." In Linear Algebra and Group Theory for Physicists and Engineers, 403–17. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-17856-7_15.

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Weatherall, James Owen. "Geometry and Motion in General Relativity." In Einstein Studies, 207–26. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-47782-0_10.

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Ferrari, Valeria, Leonardo Gualtieri, and Paolo Pani. "The Einstein equations." In General Relativity and its Applications, 109–20. Boca Raton: CRC Press, 2020.: CRC Press, 2020. http://dx.doi.org/10.1201/9780429491405-6.

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Miller, James, and Connie J. Weeks. "Einstein Field Equations." In General Relativity for Planetary Navigation, 1–30. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-77546-9_1.

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Barbour, Julian B. "Einstein and Mach's Principle." In The Genesis of General Relativity, 1492–527. Dordrecht: Springer Netherlands, 2007. http://dx.doi.org/10.1007/978-1-4020-4000-9_32.

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Adler, Ronald J. "The Einstein Field Equations for Cosmology." In General Relativity and Cosmology, 193–201. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-61574-1_12.

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Fletcher, Samuel C. "Approximate Local Poincaré Spacetime Symmetry in General Relativity." In Einstein Studies, 247–67. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-47782-0_12.

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Norton, John D. "Einstein’s Conflicting Heuristics: The Discovery of General Relativity." In Einstein Studies, 17–48. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-47782-0_2.

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Conference papers on the topic "Einstein general relativity"

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Polarski, David. "Dark Energy: beyond General Relativity?" In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399692.

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Flin, Piotr, and Hilmar W. Duerbeck. "Silberstein, General Relativity and Cosmology." In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399704.

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Poltorak, A. "General Relativity in Metric-Affine Space." In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399608.

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LÜCK, H. "THE EINSTEIN TELESCOPE ET." In Proceedings of the MG12 Meeting on General Relativity. WORLD SCIENTIFIC, 2012. http://dx.doi.org/10.1142/9789814374552_0299.

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COLEY, ALAN, PATRICK SANDIN, and BASSEMAH ALHULAIMI. "EINSTEIN-AETHER COSMOLOGICAL MODELS." In Proceedings of the MG13 Meeting on General Relativity. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814623995_0136.

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Werner, Marcus C. "The Struble–Einstein correspondence." In Proceedings of the MG15 Meeting on General Relativity. WORLD SCIENTIFIC, 2022. http://dx.doi.org/10.1142/9789811258251_0261.

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Lee, Hayoung. "The Einstein-Vlasov System with a scalar field." In GENERAL RELATIVITY AND GRAVITATIONAL PHYSICS: 16th SIGRAV Conference on General Relativity and Gravitational Physics. AIP, 2005. http://dx.doi.org/10.1063/1.1891557.

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Davidson, Aharon, and Ilya Gurwich. "Einstein Corpuscles and Dark Core Black Holes in Spontaneously induced General Relativity." In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399630.

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Dimmelmeier, H., P. Cerdá-Durán, A. Marek, and G. Faye. "New Methods for Approximating General Relativity in Numerical Simulations of Stellar Core Collapse." In ALBERT EINSTEIN CENTURY INTERNATIONAL CONFERENCE. AIP, 2006. http://dx.doi.org/10.1063/1.2399631.

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KLEINERT, H. "MULTIVALUED FIELDS AND EINSTEIN-CARTAN GEOMETRY." In Proceedings of the MG13 Meeting on General Relativity. WORLD SCIENTIFIC, 2015. http://dx.doi.org/10.1142/9789814623995_0488.

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Reports on the topic "Einstein general relativity"

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GENERAL THEORY OF THE WHOLE PHYSICAL WORLD. SIB-Expertise, August 2022. http://dx.doi.org/10.12731/er0599.29072022.

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THE WORK CONSISTS IN COMBINING NEWTON'S CLASSICAL MECHANICS DESCRIBED BY EUCLIDIAN GEOMETRY, EINSTEIN'S GENERAL THEORY OF RELATIVITY, QUANTUM MECHANICS, THE THEORY OF SUPERSYMMETRY AND INFLATION THEORY ON THE BASIS OF THE BASIC LAW OF ECONOMIC HEALTH. THE PROPOSED THEORY, INCLUDING ALLOWS TO GIVE ANSWERS TO THE GLOBAL QUESTIONS OF TODAY'S COSMOLOGY AND ASTROPHYSICS: "WHAT WAS BEFORE THE BIG BANG?"; "WHAT IS DARK MATTER?"; "WHAT IS DARK ENERGY?"; “HOW TO UNDERSTAND PARALLEL WORLDS AND MULTI UNIVERSE''. THE WORK WILL SHOW A STRICT CORRELATION OF ALL INTERACTIONS (GRAVITATIONAL, ELECTROMAGNETIC, WEAK AND STRONG) BETWEEN PARTICLES OF MATTER, BOTH ON THE SCALE OF THE GALACTIC SYSTEM AND AT THE LEVEL OF NUCLEI OF ATOMS AND UNSTABLE OUTSIDE ATOMIC NUCLEI OF SUBATOMIC NUCLEI. THESE INTERACTIONS FORMED THE OBSERVABLE PICTURE OF THE WORLD.
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GENERAL THEORY OF THE WHOLE PHYSICAL WORLD. SIB-Expertise, August 2022. http://dx.doi.org/10.12731/er0599.10082022.

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THE WORK CONSISTS IN COMBINING NEWTON'S CLASSICAL MECHANICS DESCRIBED BY EUCLIDIAN GEOMETRY, EINSTEIN'S GENERAL THEORY OF RELATIVITY, QUANTUM MECHANICS, THE THEORY OF SUPERSYMMETRY AND INFLATION THEORY ON THE BASIS OF THE BASIC LAW OF ECONOMIC HEALTH. THE PROPOSED THEORY, INCLUDING ALLOWS TO GIVE ANSWERS TO THE GLOBAL QUESTIONS OF TODAY'S COSMOLOGY AND ASTROPHYSICS: "WHAT WAS BEFORE THE BIG BANG?"; "WHAT IS DARK MATTER?"; "WHAT IS DARK ENERGY?"; “HOW TO UNDERSTAND PARALLEL WORLDS AND MULTI UNIVERSE''. THE WORK WILL SHOW A STRICT CORRELATION OF ALL INTERACTIONS (GRAVITATIONAL, ELECTROMAGNETIC, WEAK AND STRONG) BETWEEN PARTICLES OF MATTER, BOTH ON THE SCALE OF THE GALACTIC SYSTEM AND AT THE LEVEL OF NUCLEI OF ATOMS AND UNSTABLE OUTSIDE ATOMIC NUCLEI OF SUBATOMIC NUCLEI. THESE INTERACTIONS FORMED THE OBSERVABLE PICTURE OF THE WORLD.
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