A rainbow-deformed McVittie spacetime with one energy history reduces exactly to standard McVittie dynamics, and a linear late-time rainbow closure fitted to 32 cosmic chronometers and 1580 Pantheon+ supernovae is consistent with the general-relativistic limit.
Gravity's rainbow: a bridge between LQC and DSR
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abstract
The doubly special relativity (DSR) theories are investigated in order to take into account an observer-independent length scale in special relativity framework. It is widely believed that any quantum theory of gravity would reduce to a DSR model at the flat limit when purely gravitational and quantum mechanical effects are negligible. Gravity's rainbow is a simple generalization of DSR theories to incorporate gravity. In this paper, we show that the effective Friedmann equations that are suggested by loop quantum cosmology (LQC) can be exactly reobtained in rainbow cosmology setup. The deformed geometry of LQC then completely fixes the modified dispersion relation and results in unique DSR model. In comparison with standard LQC scenario where only the geometry is modified, both of the geometry and matter parts get modifications in our setup. In this respect, we find that the total number of microstates for the universe is finite which suggests the statistical origin for the energy and entropy density bounds. These results explicitly show that the DSR theories are appropriate candidates for the flat limit of loop quantum gravity.
fields
gr-qc 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
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Rainbow McVittie Horizons in an Expanding Universe
A rainbow-deformed McVittie spacetime with one energy history reduces exactly to standard McVittie dynamics, and a linear late-time rainbow closure fitted to 32 cosmic chronometers and 1580 Pantheon+ supernovae is consistent with the general-relativistic limit.