Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration (1001.4525v3)

Abstract: We present a screening mechanism that allows a scalar field to mediate a long range (~Mpc) force of gravitational strength in the cosmos while satisfying local tests of gravity. The mechanism hinges on local symmetry restoration in the presence of matter. In regions of sufficiently high matter density, the field is drawn towards \phi = 0 where its coupling to matter vanishes and the \phi-> -\phi symmetry is restored. In regions of low density, however, the symmetry is spontaneously broken, and the field couples to matter with gravitational strength. We predict deviations from general relativity in the solar system that are within reach of next-generation experiments, as well as astrophysically observable violations of the equivalence principle. The model can be distinguished experimentally from Brans-Dicke gravity, chameleon theories and brane-world modifications of gravity.

• The paper presents a mechanism where the scalar field’s vacuum expectation value varies with local density to screen gravitational interactions.
• It employs spontaneous symmetry breaking and restoration to mediate long-range forces without conflicting with solar system tests.
• The study predicts observable effects such as equivalence principle violations and measurable deviations in cosmic structures in low-density regions.

Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration

The paper "Symmetron Fields: Screening Long-Range Forces Through Local Symmetry Restoration" by Kurt Hinterbichler and Justin Khoury presents a novel mechanism designed to enable a scalar field to mediate long-range forces of gravitational strength in cosmic environments while remaining compliant with local gravity tests. This mechanism is predicated on local symmetry restoration in the presence of matter, creating an innovative way to obscure the effects of scalar fields in high-density regions without modifying their behavior in low-density areas.

Mechanism Overview and Theoretical Framework

The symmetron mechanism relies fundamentally on a scalar field whose vacuum expectation value (VEV) depends on the local matter density. This field, underpinned by a symmetry-breaking potential $$V(\phi) = -\frac{1}{2}\mu^2\phi^2 + \frac{1}{4}\lambda\phi^4$$, exhibits distinct behavior based on ambient density. In regions with high matter density, such as near the Earth or within galaxies, the field gravitates towards $\phi = 0$, restoring the symmetry and decoupling its gravitational interaction. Conversely, in low-density cosmic environments, the symmetry breaks, and the field acquires a non-zero VEV, allowing it to couple with matter at gravitational strength.

Symmetron fields are differentiated from other screening mechanisms such as chameleon fields and Vainshtein mechanisms. The symmetron approach does not require strong coupling to enlarge kinetic terms or rely on derivative self-couplings. Instead, it introduces universal coupling with matter through local VEV variation, relying on spontaneous symmetry breaking and restoration, which allows it to mediate long-range forces effectively while complying with Earth-bound gravitational experiments.

Astrophysical and Experimental Implications

The paper outlines several astrophysical and experimental predictions that the symmetron model makes, which should be testable by upcoming experiments. Challenges to General Relativity within the solar system are particularly noteworthy; next-generation experiments should be able to detect the predicted deviations. Specifically, the paper anticipates measurable violations of the equivalence principle, a haLLMark prediction that distinguishes symmetron fields from standard gravitational theories.

Moreover, the symmetron mechanism promises a long-range force on the order of megaparsecs, potentially leaving an observable imprint on the motion of large-scale cosmic structures. In contrast to Brans-Dicke, conventional chameleon theories, or alternative gravity models, symmetron fields can predict unique observational signatures by allowing gravitational variations over astronomical distances without conflicting with established solar system measurements.

Constraints and Future Prospects

While demonstrating that current solar system and binary pulsar constraints do not eliminate the possibility of symmetron fields, the paper highlights the nuanced dependence of the coupling on local environments. Estimations indicate that the Milky Way's screening should not exempt solar system objects from symmetron interactions, providing compelling alignment with data from solar-system scale experiments.

The paper concludes by recognizing that the symmetron field formulation sustains quantum corrections when regarded as an effective field theory, noting the need for fine-tuning similar to other scalar field theories devoid of a shift symmetry. Additionally, the authors acknowledge the role of renormalization from the Standard Model interactions, leaving room for further exploration into the theory's foundational aspects.

Conclusion

Hinterbichler and Khoury's work on symmetron fields offers a rigorously defined framework for integrating scalar fields of gravitational strength across cosmic expanses while remaining concealed on planetary scales. Though it proposes new theoretical constructs, it underlines unexplored experimental landscapes, poised for validation with advancing observational techniques. Assessing the symmetron fields' experimental viability might offer profound insights into long-standing questions about cosmic-scale forces and the architecture of gravity itself, which promises an engaging avenue for future research in physics and cosmology.