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Pancosmic Relativity and Nature's Hierarchies

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arxiv 2202.08860 v3 pith:DG33OCZN submitted 2022-02-17 hep-th astro-ph.COgr-qchep-ph

classification hep-thastro-ph.COgr-qchep-ph
keywords lambdafieldformrelativitystrengthaxionchargescoupling
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abstract

We define `third derivative' General Relativity, by promoting the integration measure in Einstein-Hilbert action to be an arbitrary $4$-form field strength. We project out its local fluctuations by coupling it to another $4$-form field strength. This ensures that the gravitational sector contains only the usual massless helicity-2 propagating modes. Adding the charges to these $4$-forms allows for discrete variations of the coupling parameters of conventional General Relativity: $G_N, \Lambda, H_0$, and even $\langle {\tt Higgs }\rangle$ are all variables which can change by jumps. Hence de Sitter is unstable to membrane nucleation. Using this instability we explain how the cosmological constant problem can be solved. The scenario utilizes the idea behind the irrational axion, but instead of an axion it requires one more $4$-form field strength and corresponding charged membranes. When the membrane charges satisfy the constraint $\frac{2\kappa_{\tt eff}^2 \kappa^2 |{\cal Q}_i|}{3{\cal T}^2_i} < 1$, the theory which ensues exponentially favors a huge hierarchy $\Lambda/\mpl^4 \ll 1$ instead of $\Lambda/\mpl^4 \simeq 1$. The discharges produce the distribution of the values of $\Lambda$ described by the saddle point approximation of the Euclidean path integral.

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Forward citations

Cited by 3 Pith papers

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  1. Boiling After the Dust Settles: Constraining First-Order Phase Transitions During Dark Energy Domination

    hep-ph 2025-09 conditional novelty 7.0 of 10

    CMB anisotropies from stochastic bubble nucleation constrain late-time phase transitions to release less than ~1% of dark energy when β/H⋆≲25, much tighter than Hubble-budget limits.

  2. Discretely Evanescent Dark Energy

    hep-th 2025-06 conditional novelty 6.0 of 10

    Dark energy is proposed to be the vacuum energy of a hidden QCD-like sector, set by a topological phase, which decays in discrete membrane-nucleation steps and may vanish within roughly the current age of the universe.

  3. Electromagnetic Couplings of Dark Domain Walls

    hep-th 2026-02 reject novelty 4.0 of 10

    A Chern–Simons coupling between photons and a dark 3-form is claimed to rotate CMB polarization by ~10^-3 rad when light crosses dark domain walls, but the derivation has boundary-condition errors and the signal is fi...

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