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Lorentz Violation in Emergent Gravity and Its Cosmological Consequences

Raymond Isichei, Joao Magueijo

Abstract

We show that General Relativity and other geometrical theories can be viewed as a degenerate Otto cycle with only heat-exchange legs in emergent gravity. Including work-producing legs yields controlled violations of local Lorentz invariance and energy-momentum conservation, which produce late-time cosmological acceleration. Implications for the cosmological constant problem, structure formation and local observations are discussed.

Lorentz Violation in Emergent Gravity and Its Cosmological Consequences

Abstract

We show that General Relativity and other geometrical theories can be viewed as a degenerate Otto cycle with only heat-exchange legs in emergent gravity. Including work-producing legs yields controlled violations of local Lorentz invariance and energy-momentum conservation, which produce late-time cosmological acceleration. Implications for the cosmological constant problem, structure formation and local observations are discussed.

Paper Structure

This paper contains 4 sections, 33 equations, 2 figures.

Figures (2)

  • Figure 1: Sketch of an infinitesimal Otto cycle in the $(N,\mu)$ and $(S,T)$ planes. GR and its geometric relatives arise from a degenerate cycle, obtained by collapsing the red legs to a point and retaining the blue legs (corresponding to the fluxes through $\mathscr{I}^{\mp}$). Adding the isentropic red legs leads to the proposed new theories, for which the heat in an out are not the same, and "chemical" work is done.
  • Figure 2: Sketch of an infinitesimal Otto cycle in the $(N,\mu)$ and $(S,T)$ planes generating $W>0$ but assuming $\tfrac{\partial T}{\partial N}=\tfrac{\partial \mu}{\partial S}<0$, in contrast with Fig. \ref{['FigOtto']}. To obtain the corresponding cycles with $W<0$ one should reverse all arrows and swap labels 1 and 3 in this figure and in Fig. \ref{['FigOtto']}.