Preprint Article Version 2 Preserved in Portico This version is not peer-reviewed

Gravitational Field and Mass

Version 1 : Received: 16 September 2021 / Approved: 17 September 2021 / Online: 17 September 2021 (10:07:22 CEST)
Version 2 : Received: 30 November 2021 / Approved: 1 December 2021 / Online: 1 December 2021 (12:49:09 CET)

How to cite: Zhu, Y. Gravitational Field and Mass. Preprints 2021, 2021090302. https://doi.org/10.20944/preprints202109.0302.v2 Zhu, Y. Gravitational Field and Mass. Preprints 2021, 2021090302. https://doi.org/10.20944/preprints202109.0302.v2

Abstract

It is extremely fascinating and astonishing that the gravitational field on the surface of a neutron star is with a relativistic mass density of 2.65*1016~5.87*1018kgm-3 which can be larger than the mass density of the neutron star (~1017kgm-3).Therefore, it is the author’s first intuitional imagining that this field could directly convert into mass. In so strong a gravitational field, electron and proton could be produced directly from graviton–photon collision. The gravitational field exists in everywhere in our universe. No vacuum that the region of a space is “empty” does exist. A particle is clearly always being acted on by the gravitational field. The quantum vacuum fluctuation and vacuum polarization need be re-understood with the interaction between photon and gravitational field. Therefore, the gravitational field is naturally one of the foundations of modern physics.

Keywords

Super strong gravitational field; Mass-Gravitational field conversion; Graviton-photon conversion; Graviton-photon to electron-proton conversion; Vacuum fluctuation; Vacuum polarization

Subject

Physical Sciences, Particle and Field Physics

Comments (1)

Comment 1
Received: 1 December 2021
Commenter: yin zhu
Commenter's Conflict of Interests: Author
Comment: In the first version, the calculation about the relativistic mass density of the gravitational field is wrong. In the new version, it is corrected to be 2.65*1016~5.87*1018kgm-3 which can be larger than the mass density of the neutron star (~1017kgm-3)
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