Authors: Andrew Beckwith
The author asks if octonion quantum gravity is relevant near the Planck scale. Furthermore, the question is raised if gravitational waves would be generated during the initial phase, , of the universe when an increase in degrees of freedom have in setting , so that the result can be observed by a gravitational detector.. The well appreciated .quantum gravity problem that the notion of a quantum state, representing the structure of spacetime at some instant, and the notion of the evolution of the state, does not get traction, since there are no real “instants”, is avoided by having the initial octonion geometry embedded in a larger, non linear “pilot model” (semi classical) embedding structure. The Penrose suggestion of re cycled space time avoiding a ‘big crunch’ is picked as the embedding structure, so as to avoid the ‘instants’ of time issue. In addition the favored idea is to avoid the well known string theory trap known as the dimensionality problem of an equation of motion (consistency condition) which is the reason why string theory dimensionality is either (10 or 26) depending upon if super symmetry is imposed. Getting octonion gravity as embedded in a larger, Pilot theory embedding structure may restore Quantum Gravity to its rightful place in early cosmology without the lunacy of then afterwards ‘Schrodinger equation ‘ states of the universe, forevermore afterwards. Setting , in a GW detector due to appropriate measurement procedures may allow the opportunity to find experimental clues as to this embedding structure in which octonion gravity may emerge in the Planckian regime.of evolutionary cosmology
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[v1] 2013-05-19 07:58:57
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