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Linearized gravity as edge modes and manifest duality and Lorentz covariance
Phys. Rev. D 114, 086019 – Published 26 October, 2026
DOI: https://doi.org/10.1103/nt7c-cdpl
Abstract
We present the first formulation of linearized gravity in four dimensions which is manifestly Lorentz covariant and democratic, i.e., treats the two frames related by electric-magnetic duality on equal footing. It is well known that four-dimensional linearized gravity belongs to a class of singleton representations of the four-dimensional conformal algebra . Our key insight is viewing this algebra as the isometry of and realising the massless spin-2 field as edge modes of a five-dimensional topological field taking values in a specific finite-dimensional representation of . The desired four-dimensional action is then found by a covariant boundary reduction procedure.
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References (64)
- E. Schrödinger, Proc. R. Soc. A 150, 465 (1935).
- S. Deser and C. Teitelboim, Phys. Rev. D 13, 1592 (1976).
- M. K. Gaillard and B. Zumino, Nucl. Phys. B193, 221 (1981).
- S. Deser, J. Phys. A 15, 1053 (1982).
- E. S. Fradkin and A. A. Tseytlin, Ann. Phys. (N.Y.) 162, 31 (1985).
- A. Sen, Nucl. Phys. B404, 109 (1993).
- G. W. Gibbons and D. A. Rasheed, Nucl. Phys. B454, 185 (1995).
- M. Henneaux and C. Teitelboim, Phys. Rev. D 71, 024018 (2005).
- C. Bunster, M. Henneaux, and S. Hörtner, Phys. Rev. D 88, 064032 (2013).
- M. G. Calkin, Am. J. Phys. 33, 958 (1965).
- S. Deser and D. Seminara, Phys. Rev. D 71, 081502(R) (2005).
- M. Henneaux, B. Julia, V. Lekeu, and A. Ranjbar, Classical Quantum Gravity 35, 037001 (2018).
- R. Monteiro, J. High Energy Phys. 04 (2023) 093.
For instance, a prominent context in which linearised gravity describes the relevant dynamics at hand accurately is black hole perturbation theory. Here, electric-magnetic duality is related to Chandrasekhar duality and is responsible for isospectrality of the parity-even and -odd sectors [15, 16, 17]. This has significant consequence on physical observables such as the quasinormal mode spectrum and Love numbers, see, e.g., [18] for a review.
- T. Regge and J. A. Wheeler, Phys. Rev. 108, 1063 (1957).
- F. J. Zerilli, Phys. Rev. D 2, 2141 (1970).
- S. Chandrasekhar and S. L. Detweiler, Proc. R. Soc. A 344, 441 (1975).
- A. R. Solomon, Particles 6, 943 (2023).
- G. Barnich and C. Troessaert, J. High Energy Phys. 01 (2009) 030.
- M. Henneaux, V. Lekeu, and A. Leonard, Phys. Rev. D 95, 084040 (2017).
- V. Lekeu and A. Leonard, Classical Quantum Gravity 36, 045012 (2019).
- M. Henneaux, V. Lekeu, and A. Leonard, J. Phys. A 53, 014002 (2020).
- M. Henneaux and C. Teitelboim, Phys. Lett. B 206, 650 (1988).
- J. H. Schwarz and A. Sen, Nucl. Phys. B411, 35 (1994).
- S. Deser, A. Gomberoff, M. Henneaux, and C. Teitelboim, Nucl. Phys. B520, 179 (1998).
- M. Henneaux and C. Troessaert, J. High Energy Phys. 06 (2020) 081.
- R. Floreanini and R. Jackiw, Phys. Rev. Lett. 59, 1873 (1987).
- A. A. Tseytlin, Phys. Lett. B 242, 163 (1990).
- P. Pasti, D. P. Sorokin, and M. Tonin, Phys. Lett. B 352, 59 (1995).
- P. Pasti, D. P. Sorokin, and M. Tonin, Phys. Rev. D 52, R4277 (1995).
- P. Pasti, D. P. Sorokin, and M. Tonin, Workshop on Gauge Theories, Applied Supersymmetry, and Quantum Gravity (1995), p. 167, arXiv:hep-th/9509052.
- P. Pasti, D. P. Sorokin, and M. Tonin, Phys. Rev. D 55, 6292 (1997).
- A. Maznytsia, C. R. Preitschopf, and D. P. Sorokin, Nucl. Phys. B539, 438 (1999).
- Y.-G. Miao, R. Manvelyan, and H. J. W. Mueller-Kirsten, Phys. Lett. B 482, 264 (2000).
- A. Sen, J. High Energy Phys. 07 (2015) 017.
- A. Sen, J. Phys. A 53, 084002 (2020).
- K. Mkrtchyan, J. High Energy Phys. 12 (2019) 076,
- Z. Avetisyan, O. Evnin, and K. Mkrtchyan, Phys. Rev. Lett. 127, 271601 (2021).
- O. Evnin and K. Mkrtchyan, Differential Geometry and its Applications 89, 102016 (2023).
- A. S. Arvanitakis, L. T. Cole, O. Hulik, A. Sevrin, and D. C. Thompson, Phys. Rev. D 107, 126024 (2023).
- O. Evnin, E. Joung, and K. Mkrtchyan, Phys. Rev. D 109, 066003 (2024).
- C. M. Hull, J. High Energy Phys. 04 (2023) 011.
- A. J. Bracken and B. Jessup, J. Math. Phys. (N.Y.) 23, 1925 (1982).
- W. Siegel, Int. J. Mod. Phys. A 04, 2015 (1989).
- O. V. Shaynkman, I. Y. Tipunin, and M. A. Vasiliev, Rev. Math. Phys. 18, 823 (2006).
- M. A. Vasiliev, Nucl. Phys. B793, 469 (2008).
- G. Barnich, X. Bekaert, and M. Grigoriev, J. Phys. A 48, 505402 (2015).
- H. Flores, arXiv:1702.04277.
- K. Farnsworth, K. Hinterbichler, and O. Hulik, Phys. Rev. D 105, 066026 (2022).
- K. Hinterbichler, D. M. Hofman, A. Joyce, and G. Mathys, J. High Energy Phys. 02 (2022) 151.
- C. Y.-R. Chen, E. Joung, K. Mkrtchyan, and J. Yoon, J. High Energy Phys. 05 (2025) 186,
- O. Coussaert, M. Henneaux, and P. van Driel, Classical Quantum Gravity 12, 2961 (1995).
- A. Campoleoni, S. Fredenhagen, S. Pfenninger, and S. Theisen, J. High Energy Phys. 11 (2010) 007.
- A. Campoleoni, S. Fredenhagen, and S. Pfenninger, J. High Energy Phys. 09 (2011) 113.
To show this, one can use arguments along the lines of [40] and Appendix C of [56].
- S. Bansal, O. Evnin, and K. Mkrtchyan, Eur. Phys. J. C 81, 257 (2021).
- P. Pasti, D. Sorokin, and M. Tonin, Phys. Rev. D 86, 045013 (2012).
- M. Henneaux, S. Hörtner, and A. Leonard, Phys. Rev. D 94, 105027 (2016); 97, 049901(E) (2018).
- C. M. Hull, Nucl. Phys. B583, 237 (2000).
- C. M. Hull, J. High Energy Phys. 09 (2001) 027.
- M. Henneaux, V. Lekeu, and A. Leonard, J. High Energy Phys. 01 (2018) 114; 05 (2018) 105(E).
- E. Joung and K. Mkrtchyan, J. High Energy Phys. 02 (2012) 134.
- E. S. Fradkin and A. A. Tseytlin, Phys. Rep. 119, 233 (1985).
- E. Joung and K. Mkrtchyan, J. High Energy Phys. 11 (2012) 153.