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Causality Constraints on Corrections to the Graviton Three-Point Coupling (1407.5597v1)

Published 21 Jul 2014 in hep-th and gr-qc

Abstract: We consider higher derivative corrections to the graviton three-point coupling within a weakly coupled theory of gravity. Lorentz invariance allows further structures beyond the one present in the Einstein theory. We argue that these are constrained by causality. We devise a thought experiment involving a high energy scattering process which leads to causality violation if the graviton three-point vertex contains the additional structures. This violation cannot be fixed by adding conventional particles with spins $J \leq 2$. But, it can be fixed by adding an infinite tower of extra massive particles with higher spins, $J > 2$. In AdS theories this implies a constraint on the conformal anomaly coefficients $\left|{a - c \over c} \right| \lesssim {1 \over \Delta_{gap}2}$ in terms of $\Delta_{gap}$, the dimension of the lightest single particle operator with spin $J > 2$. For inflation, or de Sitter-like solutions, it indicates the existence of massive higher spin particles if the gravity wave non-gaussianity deviates significantly from the one computed in the Einstein theory.

Citations (563)

Summary

  • The paper shows that causality constraints limit extra higher derivative structures in graviton three-point interactions by necessitating higher-spin particles.
  • The study employs thought experiments and shock wave analyses in both flat and AdS spacetimes to reveal potential causality violations.
  • The paper connects these findings to quantum gravity frameworks, suggesting that string theory and AdS/CFT predictions mandate the emergence of higher-spin states.

An Analytical Exploration of Causality Constraints in Graviton Three-Point Couplings

The paper under review delivers a detailed exploration into higher derivative corrections to graviton three-point interactions within weakly coupled theories of gravity, remarkably advancing our understanding of its consistency through causality. Authored by Xi´an O. Camanho, Jos´e D. Edelstein, Juan Maldacena, and Alexander Zhiboedov, this paper examines the modifications allowed by Lorentz invariance to the graviton's three-point vertex and provides a thorough argument indicating how causality imposes significant constraints on these possible structures.

Key Findings and Approach

The theoretical framework focuses on the modifications to the graviton three-point interactions, which hold potential for causing violations of causality. The paper posits, through thought experiments involving high-energy scattering processes, that any additional structures in the graviton’s three-point vertex that result from higher derivative terms could lead to causality violations. These violations become apparent unless accounted for by new physical states — specifically, a tower of massive higher-spin particles with spins exceeding two (J > 2) — suggesting an intricate connection between the structure of gravitational three-point functions and the emergence of higher spin states.

The investigation of causality-induced constraints draws from both flat space and Anti-de Sitter (AdS) spacetime scenarios. The paper strategically leverages sophisticated techniques such as exploring the propagation of probe particles through shock wave backgrounds. The detailed calculations elucidate how perturbations at intermediate energy scales can be reconciled with weakly coupled string theory predictions, as seen by the presence of higher spin states.

Implications and Future Directions

One of the paper's pivotal outcomes is the identification of a necessary condition — the presence of higher-spin particles — for maintaining causality when non-Einstein structures appear in graviton interactions. In the context of AdS/CFT correspondence, this requirement aligns with expectations from dual gauge theories with large operator dimensions, linking the covered three-point functions to the operator spectra and offering predictions that impact the interpretation of conformal field theories (CFTs).

The research presented pushes the boundaries of our comprehension regarding the structure and constraints of gravitational interactions beyond the standard framework of Einstein's theory. It reinforces the idea that additional high-spin states are necessary to rectify any causality issues, a condition supported by findings within string theory. Notably, the examination dispels an often assumed sufficiency of Lorentz invariant local terms in ensuring consistency, redirecting focus on spectrum-rich theories to guarantee theoretical adherence.

Future research could further explore the ramifications of the identified constraints in alternative theories of gravity, aiming to substantiate predictions about CFT dimensions and the presence of non-standard particles during inflationary periods. Such investigations may enrich models of early universe cosmology, linking higher spin states to quantum gravity phenomena observable through gravitational wave detections.

Conclusion

This comprehensive exposition greatly contributes to the literature by clarifying causality constraints on gravitational interactions in weakly coupled theories. It conceptualizes a robust framework connecting the higher derivative corrections within such interactions to the necessity of additional higher-spin states. This paradigm elevates the interpretation of gravitation beyond conventional models, setting the stage for novel insights into the nature of gravitational interactions and their interplay with quantum gravity theories, including those supported by string theory frameworks. The paper constitutes a remarkable stride towards a more insightful understanding of causality within the fabric of quantum gravity, holding significant implications for both theoretical and applied physics.

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