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Gravity Beyond a Single Metric: Ghost-free interactions of spin-2 fields
Stockholm University, Faculty of Science, Department of Physics.ORCID iD: 0009-0004-4545-3123
2026 (English)Doctoral thesis, comprehensive summary (Other academic)
Abstract [en]

The mathematical formulations of the fundamental interactions in nature are all expressed in terms of fields classified by their mass and spin. The structure of two of the most successful theories in physics, General Relativity and the Standard Model of particle physics, can both be derived more or less uniquely from fields with fixed mass and spin, guided by theoretical consistency conditions. The Standard Model contains well-understood interactions of particles with spins less than two, while theories involving spins higher than two are generally problematic. Theories of spin-2 fields are much less explored, and in particular, any consistent multiplet structure, crucial for the Standard Model, is practically unknown.

Even without considering multiplet structures, classical theories with interacting spin-2 fields generically propagate additional pathological fields, so-called Boulware–Deser ghosts, rendering such theories physically unacceptable. Until recently, only a non-derivative interaction between two spin-2 fields, called bimetric theory, had been proven consistent. While the bimetric interaction can to some extent be trivially extended to more than two fields, genuine ghost-free multi-field interactions have remained elusive.

In this thesis, we derive necessary conditions on ghost-free non-derivative interactions between multiple spin-2 fields. With a suitable parametrisation of the fields, the ghost mode can be isolated, allowing one to derive necessary conditions for it to be non-propagating. These conditions essentially determine the form of the interaction potential uniquely, up to a set of free constant parameters. The admissible class contains all previously known ghost-free theories, but is not itself ghost-free in general. Imposing an additional necessary condition for ghost-freedom on these parameters further restricts the interaction to the Hassan–Schmidt–May theory and trivial extensions thereof. Thus, much as for the lower-spin theories in the Standard Model, the requirement of theoretical consistency, here the absence of ghosts, essentially singles out the admissible theory. We then show that this theory possesses the full set of constraints needed to eliminate all ghost modes, establishing it as the most general known ghost-free multi-gravity interaction. Finally, we derive the mass spectrum, finding one massless and multiple massive spin-2 fields with a non-tachyonic spectrum.

Place, publisher, year, edition, pages
Stockholm: Department of Physics, Stockholms University , 2026. , p. 80
Keywords [en]
multi-gravity, modified gravity, bimetric theory, spin-2 fields, classical field theory
National Category
Other Physics Topics
Research subject
Theoretical Physics
Identifiers
URN: urn:nbn:se:su:diva-253727ISBN: 978-91-8107-576-2 (print)ISBN: 978-91-8107-577-9 (electronic)OAI: oai:DiVA.org:su-253727DiVA, id: diva2:2049670
Public defence
2026-05-15, sal FB42, AlbaNova universitetscentrum, Roslagstullsbacken 21, Stockholm, 13:00 (English)
Opponent
Supervisors
Available from: 2026-04-22 Created: 2026-03-30 Last updated: 2026-04-22Bibliographically approved
List of papers
1. On the Uniqueness of Ghost-Free Multi-Gravity - II: Constraining antisymmetrised multi spin-2 interactions
Open this publication in new window or tab >>On the Uniqueness of Ghost-Free Multi-Gravity - II: Constraining antisymmetrised multi spin-2 interactions
(English)Manuscript (preprint) (Other academic)
National Category
Other Physics Topics
Research subject
Theoretical Physics
Identifiers
urn:nbn:se:su:diva-253816 (URN)
Available from: 2026-03-30 Created: 2026-03-30 Last updated: 2026-03-30
2. Canonical Vielbeins for General Relativity: D + 1 Decomposition and Constraint Analysis
Open this publication in new window or tab >>Canonical Vielbeins for General Relativity: D + 1 Decomposition and Constraint Analysis
(English)Manuscript (preprint) (Other academic)
Abstract [en]

We provide a self-contained derivation of the Hamiltonian formulation of General Relativity in vielbein variables in d=D+1 dimensions. Starting from the Einstein--Hilbert action in a standard metric D+1 decomposition, we derive Lorentz- and SO(D)-covariant phase-space actions, identify the primary Lorentz constraints, and obtain the Hamiltonian and momentum constraints. We compute the resulting first-class constraint algebra, relate the vielbein and metric phase-space formulations, and discuss the rotation/boost decomposition. In particular, we construct the boost generator in the SO(D)-covariant formulation, thereby recovering full local Lorentz symmetry.

National Category
Other Physics Topics
Research subject
Theoretical Physics
Identifiers
urn:nbn:se:su:diva-253732 (URN)
Available from: 2026-03-26 Created: 2026-03-26 Last updated: 2026-03-30
3. Existence of ghost-eliminating constraints in multivielbein theory
Open this publication in new window or tab >>Existence of ghost-eliminating constraints in multivielbein theory
(English)Manuscript (preprint) (Other academic)
Abstract [en]

We perform a Hamiltonian constraint analysis of the multivielbein theory proposed in arXiv:1804.09723. The analysis shows that the secondary constraints have the correct form to constrain the dynamical variables, thereby eliminating the problematic ghost modes that generally plague theories of interacting spin-2 fields. Under mild restrictions on the solution space, we also identify the tertiary constraints and show that these eliminate the canonical momenta associated with the ghost modes. Our analysis confirms that the theory with N interacting vielbeins propagates 2+5(N−1) modes, corresponding to a nonlinear theory of one massless and N−1 massive spin-2 fields free of the Boulware-Deser ghost instabilities.

National Category
Other Physics Topics
Research subject
Theoretical Physics
Identifiers
urn:nbn:se:su:diva-253731 (URN)
Available from: 2026-03-26 Created: 2026-03-26 Last updated: 2026-03-30
4. Mass spectrum & linear perturbations of ghost-free multi-spin-2 theory
Open this publication in new window or tab >>Mass spectrum & linear perturbations of ghost-free multi-spin-2 theory
2025 (English)In: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, no 2, article id 176Article in journal (Refereed) Published
Abstract [en]

Motivated by the spin-2 nature of gravity, we consider a theory of N interacting spin-2 fields, formulated in terms of vielbeins, which has been argued to be free of Boulware-Deser ghost instabilities. This is the only known such theory with non-trivial multi-field interactions. We develop an all-order expansion of the vielbein in terms of the metric and Lorentz field perturbations, enabling an expansion of the action in arbitrary backgrounds to any order. The mass matrix is then analysed around proportional vielbein solutions corresponding to vacuum Einstein spacetimes. It is shown that the theory exhibits a non-tachyonic spectrum with one massless and N − 1 massive spin-2 modes, regardless of the sign of the cosmological constant. While the massless mode is universal, the non-zero masses cannot generally be determined analytically, but we obtain the lower and upper bounds on each mass eigenvalue in terms of the parameters of the theory.

Keywords
Classical Theories of Gravity, Cosmological models
National Category
Subatomic Physics
Identifiers
urn:nbn:se:su:diva-242118 (URN)10.1007/JHEP02(2025)176 (DOI)001435016100004 ()2-s2.0-85219542721 (Scopus ID)
Available from: 2025-04-15 Created: 2025-04-15 Last updated: 2026-03-30Bibliographically approved

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Flinckman, Joakim

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