Abstract
By taking into account the relative energy between the diquark and the quark in nucleons, the gravitational singularity in a black hole created from a collapsing neutron star can be removed; compatibility with quantum mechanics is restored. This black hole becomes a “black” neutron star. The negative relative energy identified as dark matter in the previous paper can account for the galaxy rotation curve. The positive relative energy identified as dark energy in the previous paper can explain the accelerating expansion of the universe. A possible scenario for cosmic ray generation is given.
Highlights
By taking into account the relative energy between the diquark and the quark in nucleons, the gravitational singularity in a black hole created from a collapsing neutron star can be removed; compatibility with quantum mechanics is restored
The negative relative energy identified as dark matter in the previous paper can account for the galaxy rotation curve
A neutron star with mass greater that the Tolman-Oppenheimer-Volkoff (TOV) limit MTOV~3 solar mass MSUN becomes a black hole in which the star core collapses to a gravitational mass singularity in general relativity [[1] p172], [[2] black hole/§2.3]
Summary
A neutron star with mass greater that the Tolman-Oppenheimer-Volkoff (TOV) limit MTOV~3 solar mass MSUN becomes a black hole in which the star core collapses to a gravitational mass singularity in general relativity [[1] p172], [[2] black hole/§2.3]. G., the galaxy rotation curve, and the dark energy required to drive the rapidly expanding universe remain hypothetical as they cannot be observed It was shown [3] that the “hidden”, unobservable relative energy between the diquark and quark in nucleons can interact with their ambient gra-. The negative relative energy generated in an expanding galaxy can play the role of dark matter and account for the galaxy rotation curve. Lied together and the products of the quark spinors and those of the strong potentials are generalized to baryon wave functions and baryon potentials nonseparable in xI, xII and xIII according to [[4] [5] Sec. 9.2]. Χ 0b (2.3b) where χ0 and ψ0 the wave functions of the doublet baryons
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