Spontaneous symmetry breaking for long-wave gravitons in the early Universe
A. A. Grib, V. Yu. Dorofeev

TL;DR
The paper demonstrates that nonlinear effects in gravitons within an expanding universe can resolve issues with negative effective mass squared, leading to spontaneous symmetry breaking and a modified graviton spectrum.
Contribution
It introduces a mechanism of spontaneous symmetry breaking for gravitons in the early universe, altering their spectrum through nonlinear effects and vacuum expectation values.
Findings
Nonlinear terms resolve negative mass squared problem for gravitons.
Two graviton fields emerge with different masses due to symmetry breaking.
Numerical results provided for dust universe case.
Abstract
It is shown that nonlinear terms in equations of gravitons on the background of curved space-time of the expanding Universe can solve the problem of the negative square of the effective mass formally arising in linear approximation for gravitons. Similar to well known spontaneous breaking of symmetry in Goldstone model one must take another vacuum so that nonzero vacuum expectation value of the quantized graviton field leads to change of spectrum for gravitons. There appears two graviton fields, one with the positive mass, another with the zero mass. Energy density and the density of particles created by gravitation of the expanding Universe are calculated for some special cases of the scale factor. Numerical results are obtained for the dust universe case.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
