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A 2D Stress Tensor for 4D Gravity (1609.00282v2)

Published 1 Sep 2016 in hep-th and gr-qc

Abstract: We use the subleading soft-graviton theorem to construct an operator $T_{zz}$ whose insertion in the four-dimensional tree-level quantum gravity $\mathcal{S}$-matrix obeys the Virasoro-Ward identities of the energy momentum tensor of a two-dimensional conformal field theory (CFT$_2$). The celestial sphere at Minkowskian null infinity plays the role of the Euclidean sphere of the CFT$_2$, with the Lorentz group acting as the unbroken $SL(2,\mathbb{C})$ subgroup.

Citations (235)

Summary

  • The paper establishes that 4D quantum gravity amplitudes can be reformulated as celestial sphere 2D CFT correlators using subleading soft-graviton insertions.
  • It introduces the operator Tzz within the 4D S-matrix, showing that it satisfies Virasoro-Ward identities analogous to a 2D stress tensor.
  • The results extend gauge theory insights by linking soft gravitational excitations to Virasoro representations, paving the way for advanced quantum gravity models.

Overview of "A 2D Stress Tensor for 4D Gravity"

The paper by Daniel Kapec, Prahar Mitra, Ana-Maria Raclariu, and Andrew Strominger provides a detailed analysis of how four-dimensional (4D) tree-level quantum gravity scattering amplitudes can be reformulated as two-dimensional (2D) conformal field theory (CFT) correlators on the celestial sphere. The authors utilize subleading soft-graviton insertions to construct an operator, denoted as TzzT_{zz}, within the 4D S-matrix that satisfies the Virasoro-Ward identities akin to those for the energy momentum tensor in a 2D CFT. This work builds on and extends earlier research demonstrating that 4D gauge theories can manifest as algebraic structures known as Kac-Moody algebras when considering soft-theorem identities.

Core Contributions and Methodology

The paper primarily hinges on the concept that any scattering amplitude involving massless particles in a 4D asymptotically Minkowskian spacetime can be expressed as a correlation function on the celestial sphere at null infinity. The celestial sphere is treated as the Euclidean sphere of the CFT, with the Lorentz group SL(2,C) embodying the unbroken subgroup. The paper shows that specific soft-graviton excitations (TzzT_{zz}) can be incorporated into the tree-level S-matrix and that these excitations comply with the Virasoro-Ward identities standard to stress tensor insertions in a CFT.

The authors utilize the subleading soft-graviton theorem to establish a rigorous mathematical framework for this reformulation. Their approach is rooted in examining how energy and other quantum numbers label distinct operator insertions, which can be represented as SL(2,C) conformal representations on the celestial sphere.

Results and Implications

One of the key results is the identification of Virasoro representations in quantum gravity scattering amplitudes, showing an extension from gauge theory, where soft-photon and soft-gluon insertions have been linked to Kac-Moody algebras. This interpretation aligns with earlier conjectures and addresses specific quantum gravity scenarios with the Virasoro group, commonly associated with 2D conformal symmetries.

The paper posits several limitations, notably its restriction to massless particles and tree-level scatterings. While extensions to massive particles are conceivable, as suggested by previous works, they present unique conceptual challenges, such as integrating potential central terms when considering multiple soft insertions.

Theoretical and Practical Implications

This research carries several theoretical implications. First, it confirms that certain aspects of quantum gravity can be reinterpreted through the lens of 2D CFT structures. This reframing provides a deeper understanding of the correspondence between spacetime symmetries and gauge symmetries. Practically, understanding such correspondences may aid in the development of more sophisticated quantum gravity theories and enhance our comprehension of related symmetries' algebraic properties.

The findings suggest future directions, including exploring one-loop corrections and implications of the soft-graviton theorem at higher orders. Additionally, investigating the nature of the representation associated with these Virasoro structures could further delineate distinctions or commonalities with traditional 2D CFTs.

In conclusion, this paper offers a significant advancement in our understanding of how 2D symmetries manifest in quantum gravity, providing a bridge between gravitational and conformal symmetries that warrants further exploration.