2017
DOI: 10.4236/jhepgc.2017.31008
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Does GW Generation Have Semi-Classical Features?

Abstract: We argue in this document that initial vacuum state values possibly responsible for GW generation in relic conditions in the initial onset of inflation may have a temporary un squeezed, possibly even coherent initial value, which would permit in certain models classical coherent initial gravitational wave states. Furthermore, several arguments pro and con as to if or not initial relic GW should be high frequency will be presented. The existence of higher dimensions, in itself if the additional dimensions are s… Show more

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Cited by 1 publication
(3 citation statements)
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“…We submit here, that should we fully examine what is written up in Equation (G4) will under the influence of [45] be a measure of a deformation from usual space-time, but that the existence of a magnetic field, which would allow us to take our route to Quantum gravity would require an initially non infinite deformation parameter k which is in its own way similar to what was done by the author in his analysis of gravity as possibly having semi classical features, as given in [46].…”
Section: Appendix H Inhomogeneity Of Pre Plankian To Planckian Spacementioning
confidence: 93%
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“…We submit here, that should we fully examine what is written up in Equation (G4) will under the influence of [45] be a measure of a deformation from usual space-time, but that the existence of a magnetic field, which would allow us to take our route to Quantum gravity would require an initially non infinite deformation parameter k which is in its own way similar to what was done by the author in his analysis of gravity as possibly having semi classical features, as given in [46].…”
Section: Appendix H Inhomogeneity Of Pre Plankian To Planckian Spacementioning
confidence: 93%
“…We submit that what we would be doing, is a physical motivation, i.e. a necessary condition for the formation of a Gravi-Magnetic field, and that [46] delineates the role of the deformation parameter as necessary and sufficient for the "evolution" of our initial conditions to quantum mechanics.…”
Section: Appendix H Inhomogeneity Of Pre Plankian To Planckian Spacementioning
confidence: 99%
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