Quantum Gravity and String Theory

    

The E- and B-Modes in the CMB

Authors: Sylwester Kornowski

Here, on base of the lacking part of ultimate theory, i.e. the Scale-Symmetric Theory, we described the production of the E- and B-modes in the CMB. The obtained result 0.22 for the ratio of amplitudes of the B-modes to E-modes (i.e. the tensor-to-scalar ratio) for the beginning of expansion of the very early Universe, for multipole moment equal to 384, is close to the central value in the BICEP2 data. The tensor-to-scalar ratio depends on density of the Einstein-spacetime and is higher for higher densities. The calculated energies carried by the Einstein-spacetime components the spreading condensates were built of (such condensates produced the B-modes in the CMB), were in approximation the sixteen powers of ten of GeV.

Comments: 5 Pages.

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Submission history

[v1] 2014-03-21 11:48:15
[v2] 2015-12-29 04:10:36

Unique-IP document downloads: 436 times

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