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Nonlinear Structure Formation with the Environmentally Dependent Dilaton

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arxiv 1102.3692 v1 pith:6TCC2IWI submitted 2011-02-17 astro-ph.CO gr-qchep-ph

classification astro-ph.COgr-qchep-ph
keywords dilatonmodeldependentenvironmentallyformationnonlinearstructureaccount
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abstract

We have studied the nonlinear structure formation of the environmentally dependent dilaton model using $N$-body simulations. We find that the mechanism of suppressing the scalar fifth force in high-density regions works very well. Within the parameter space allowed by the solar system tests, the dilaton model predicts small deviations of the matter power spectrum and the mass function from their $\Lambda$CDM counterparts. The importance of taking full account of the nonlinearity of the model is also emphasized.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. EFT-Ramses: a code to simulate the effective field theory of dark energy

    astro-ph.CO 2026-07 accept novelty 5.5 of 10

    A unified AMR N-body code embeds EFTofDE α-basis models into one master Vainshtein equation and matches legacy ECOSMOG and HiCOLA matter power spectra.

  2. Light scalars in light of UV/IR mixing: classicalization via synergy between Vainshtein and chameleon screenings

    hep-ph 2025-11 conditional novelty 5.0 of 10

    Classicalizing k-essence scalars need m << Λ* and, when potentials or fermion couplings are present, a chameleon-like screening layer to keep Vainshtein screening and classicalon stability intact.

  3. Weinberg's theorem, phantom crossing and screening

    astro-ph.CO 2025-07 conditional novelty 5.0 of 10

    Graviton-loop-induced screening forces single-field dilaton and chameleon dark energy models to keep their equation of state near -1, making observable phantom crossing impossible in this class.

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