Decay (Expansion) of the Universe and Stabilized Solar System in a Fundamental Quantum Description

  • Hans-Peter Morsch HOFF
Keywords: comparison of decay velocities with supernovae 1a observation, boundary conditions for a stabilized Solar system, Dynamic Potentials and Velocities of the uiverse in a fundamental quantum description

Abstract

The expanding (decaying) universe is discussed in the framework of a local quantum field theory, based on a Lagrangian, in which all fermion operators are coupled to bosons. In this formalism the initial phase of the universe has been explained by creation of particles out of the vacuum, accumulation of a system of large mass and immense radius dominated by (e- p+) and (e+ p-) pairs, followed by a chirally triggered collapse and annihilation of all (e+ p-) pairs (antimatter).
The subsequent decay of the remaining (e- p+) pairs (matter) shows a velocity, which increases exponentially towards large radii. This gives rise to a good description of velocity-distance data from supernovae 1a observation by adjusting the position of the Solar system to a radius of the universe of about 1300 Mpc. Of importance, at this radius the repulsive and attractive forces compensate each other, giving rise to a boundary condition for a stabilized Solar system. Combined with a calculation of its mass, this yields surprising evidence for the existence of stable cosmic systems, which do not follow the general expansion of the universe.
No evidence is found for (not understood) dark energy contributions as deduced from cosmological models.

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References

see e.g. P.J.E. Peebles, Principles of physical cosmology, Princeton University Press (1993)

A. Einstein, Die Feldgleichungen der Gravitation, Sitzungsber. Preuss. Akad. Wiss. Berlin, 1915: 844; see also

textbooks on Classical Field Theory, as e.g. L.D. Landau and E.M. Lifshitz, Akademie Verlag Berlin (1966)

A. Guth, In atory universe: A possible solution to the horizon and atness problems, Phys. Rev. D 23, 347

(1981); A. Linde and A.D. Linde, Particle Physics and In atory Cosmology, Harwood (1990)

A.G. Ries et al., Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116, 1009 (1998)

S. Perlmutter et al., Measuement of and from 42 high-redshift supernovae, Astrophys. J. 517, 565 (1999)

G. Hinshaw et al., Nine year WMAP observations: Cosmological parameter results, Astrophys. J. Supp. 208, 19

(2013) and refs. therein

H.P. Morsch, Origin of gravitation and description of galaxy rotation in a fundamental bound state approach,

Global J. Sci. Front. Research. A 18, 4 v.1, p. 25 (2018) (open access)

H.P. Morsch, Unique structure of free particle bound states, Brit. J. Math. and Comp. Sc. 17(6): 1-11 (2016)

(open access)

H.P. Morsch and S. Ghosh, Chiral structure of particle bound states, J. Adv. Math. and Comp. Sc. 24(4): 1-11

(2017) (open access)

H.P. Morsch, Acceleration in a fundamental bound state theory and the fate of gravitational systems, J. Adv.

Math. and Comp. Sc. 28(3): 1-13 (2018) (open access)

A.G. Ries et al., New Hubble Space Telescope discoveries of Type Ia supernovae at z 1: Narrowing constraints

on the early behavior of dark energy, Astrophys. J. 659, 98 (2007)

Published
2019-04-30
How to Cite
Morsch, H.-P. (2019). Decay (Expansion) of the Universe and Stabilized Solar System in a Fundamental Quantum Description. To Physics Journal, 2, 40-45. Retrieved from http://purkh.com/index.php/tophy/article/view/278
Section
Research Articles