Very Special Relativity (VSR) proposes that the space-time symmetry group of nature is a proper subgroup of the Poincare group - in its spurion-inaccessible avatars, HOM(2) or SIM(2) together with translations - rather than the full Lorentz group. Cohen and Glashow showed that such symmetries reproduce most consequences of special relativity while evading many Lorentz-violation searches, and explicitly acknowledged four open directions: no complete causal, unitary dynamical VSR theory was constructed; the allowed nonlocal operator structures were not classified; quantitative phenomenology was deferred; and no microscopic mechanism fixes the size of the VSR coefficients. Twenty years of follow-up literature has delivered effective nonlocal VSR gauge theories that are renormalizable and unitary (Alfaro, Rivelles and collaborators), a rigorous free-field construction (Lee), Finsler-geometric, noncommutative and background-field realizations, and an extensive phenomenology. However, causality and microcausality of the genuinely nonlocal operators are not established anywhere in the literature, no UV completion or microscopic origin exists, a Thomas-precession incompatibility claim remains contested, and the naturalness of the tiny VSR coefficients (e.g. the DISIMb(2)DISIM_b(2) deformation parameter bounded by ∣b∣<10−26|b| < 10^{-26}) is unexplained. The open problem is the construction of a single causal, unitary, microscopic VSR-invariant dynamical framework - or a proof of obstruction - together with a mechanism explaining the natural size of its coefficients.

Background

Special relativity (SR) identifies the space-time symmetry of nature with the Poincare group: space-time translations together with the full connected Lorentz group of rotations JiJ_i and boosts KiK_i. Cohen and Glashow (2006) asked whether the exact symmetry could instead be a proper subgroup of the Poincare group, which they called Very Special Relativity (VSR). Restricting to subgroups that contain translations and at least the two-parameter abelian group T(2)T(2) generated by T1=Kx+JyT_1 = K_x + J_y and T2=Ky−JxT_2 = K_y - J_x, there are four relevant avatars: T(2)T(2) itself; E(2)E(2) (adding JzJ_z; isomorphic to the Euclidean motions of a plane); HOM(2)HOM(2) (adding KzK_z; orientation-preserving similarities, or homotheties, of a plane); and SIM(2)SIM(2) (adding both JzJ_z and KzK_z; the four-parameter similitude group). Their defining property is that adjoining any one of the discrete transformations PP, TT, or CPCP enlarges the subgroup to the full Lorentz group. Consequently any theory conserving one of these discrete symmetries is automatically Lorentz invariant, and since CP-violating effects in nature are small, VSR departures from SR are expected to be small as well.

In perturbative approaches to Lorentz violation one inserts fixed background tensors, called spurions, into local operators. This works for T(2)T(2) and E(2)E(2), which admit invariant tensors (for E(2)E(2) the null four-vector n=(1,0,0,1)n = (1,0,0,1)). The avatars HOM(2)HOM(2) and SIM(2)SIM(2), however, admit no invariant local tensors at all - they are spurion-inaccessible. Lorentz-violating effects respecting HOM(2)HOM(2) or SIM(2)SIM(2) can therefore only be nonlocal: they are built from the non-invariant null vector nn, which is preserved by T1T_1, T2T_2 and rotations about the zz axis and merely rescales under boosts along zz, so that ratios such as (p1⋅n)/(p2⋅n)(p_1 \cdot n)/(p_2 \cdot n) are invariant. A key theorem of the source paper is that VSR implies SR in the context of local quantum field theory (or if CP is conserved); a VSR world therefore cannot be a precisely local quantum field theory, and its dynamics must be formulated with genuinely nonlocal operators.

Despite this, the kinematic content of SR survives almost intact in the SIM(2)SIM(2) and HOM(2)HOM(2) avatars: time dilation, the velocity-addition law, the existence of a center-of-mass frame, and a universal isotropic maximal attainable velocity all hold, and the little groups (the subgroups of the symmetry group that fix a standard momentum) of massive and massless particles have one-dimensional representations, unlike the Poincare case. VSR also offers an unusual origin for neutrino masses: lepton-number-conserving neutrino masses, while not Lorentz invariant, are VSR invariant and require no sterile states; an anisotropic charged-lepton electric dipole moment (EDM) of order dl∼(mν/2ml)2(e/2ml)d_l \sim (m_\nu/2m_l)^2(e/2m_l) is then tied to the neutrino-mass scale and lies near experimental sensitivity for mν2∼10−4 eV2m_\nu^2 \sim 10^{-4}\,\mathrm{eV}^2. With suitable analyticity assumptions, CPT invariance can even be derived from SIM(2)SIM(2) invariance.

The source paper explicitly acknowledged what it did not do: (1) no complete causal, unitary dynamical theory invariant under SIM(2)SIM(2) or HOM(2)HOM(2) was constructed - the authors state they expect that such a theory can be formulated, but do not formulate it; (2) only prototype nonlocal amplitudes were exhibited, not a systematic classification of the allowed VSR-preserving nonlocal structures; (3) quantitative phenomenology for the proposed probes (CP-violating meson decays such as B0→J/ψKsB^0 \to J/\psi K_s, charged-lepton EDMs, and neutrino observables) was deferred to later work; (4) the origin and natural size of the VSR coefficients were not derived from any microscopic mechanism.

Subsequent literature built a substantial but incomplete structure. Gibbons, Gomis and Pope showed that general VSR is Finsler geometry (a geometry whose line element is homogeneous of degree one in displacements but anisotropic), that the inhomogeneous group ISIM(2)ISIM(2) (SIM(2)SIM(2) together with space-time translations) admits only a one-parameter physically acceptable deformation DISIMb(2)DISIM_b(2), and they emphasized the naturalness puzzle: the deformation parameter is bounded by ∣b∣<10−26|b| < 10^{-26}, raising the question of why such a dimensionless Lorentz-violating constant is so small. Alfaro, Rivelles and collaborators constructed nonlocal VSR-invariant gauge theories, Abelian and non-Abelian, that are renormalizable and unitary, including an electroweak model with the Standard Model particle content that generates neutrino masses; their loop calculations rely on Mandelstam-Leibbrandt-type regularization, a prescription for evaluating integrals containing light-like vectors that preserves gauge invariance and power counting, here requiring an auxiliary null vector whose removal must be taken as a careful limit to restore SIM(2)SIM(2). Lee gave a rigorous construction of quantum fields with a preferred direction from the irreducible unitary representations of ISIM(2)ISIM(2), finding that free massive spin-1/2 and spin-1 fields are local and satisfy the Dirac and Proca equations. Realizations of the VSR subgroups were found on spacetimes with light-like noncommutativity (Sheikh-Jabbari and Tureanu) and as effective theories emerging from ordinary QED in a rapidly oscillating plane-wave background (Ilderton). Two consistency questions remain. Das and Mohanty argued that VSR predicts the wrong Thomas precession - the SR kinematic rotation produced by successive non-collinear boosts, observable in atomic spin-orbit splittings and in the Thomas-BMT equation governing spin precession of particles in storage rings - claiming a factor-of-two excess in spin-orbit coupling and a 10310^3 excess in ring precession, which would rule VSR out; this is contested by Ganjitabar and Shojai, who find no observable departure. And Asorey, Falceto and Marmo generalized the classical no-interaction theorems (which forbid interactions between point particles under a full Poincare-symmetry implementation) to Poincare subgroups, showing that VSR-type subgroups weaken these constraints but still restrict the admissible interactions.

Problem Statement

The problem is to give the Very Special Relativity proposal a dynamical foundation: construct a complete, causal, unitary quantum dynamical theory - an action or Hamiltonian, together with its state space and quantization - whose exact space-time symmetry group is a spurion-inaccessible VSR subgroup, SIM(2) or HOM(2) (with space-time translations), or else prove rigorously that no such theory can exist.

A dynamical foundation of VSR is a single framework that establishes: (1) Consistency: exact invariance under the full VSR group (not enlarged to the Lorentz group by quantization or radiative corrections), unitarity (a unitary S-matrix or probability-conserving evolution), and causal behavior - a suitable microcausality or analyticity condition holding despite the necessarily nonlocal n-dependent operators such as (p⋅n)/(q⋅n)(p \cdot n)/(q \cdot n) - together with a resolution of, or escape from, the disputed incompatibility with observed spin-precession (Thomas-precession) data. (2) Structure: the systematic determination of the VSR-preserving nonlocal operator content of the theory - which interactions are allowed, their gauge invariance, and their relation to the one-dimensional little-group representations. (3) Origin and size: a microscopic mechanism (a UV completion, emergent-symmetry dynamics, or comparable) from which the theory derives and which fixes the size of its VSR coefficients, explaining why they are small enough to have evaded precision Lorentz-invariance tests (for instance the bound ∣b∣<10−26|b| < 10^{-26} on the DISIMb(2)DISIM_b(2) deformation parameter) while being plausibly connected to the observed neutrino-mass scale; the framework must reproduce the established VSR phenomenology (neutrino-mass phenomenology, charged-lepton EDM and g-2 bounds, meson-decay and clock-comparison constraints) as its low-energy limits.

Alternatively, a rigorous proof that no such theory can exist resolves the problem. The completion boundary is a single framework that establishes all three components above - consistency, structure, and origin and size - or a proof that this is impossible; effective models with unproven causality, an unclassified VSR-preserving operator content, or unexplained coefficients do not by themselves complete it.

References

  1. Andrew G. Cohen and Sheldon L. Glashow, 'Very Special Relativity', Physical Review Letters 97, 021601 (2006), arXiv:hep-ph/0601236, DOI: 10.1103/PhysRevLett.97.021601, https://doi.org/10.1103/PhysRevLett.97.021601
  2. Andrew G. Cohen and Sheldon L. Glashow, 'A Lorentz-Violating Origin of Neutrino Mass?', arXiv:hep-ph/0605036 (2006), https://arxiv.org/abs/hep-ph/0605036 (unpublished preprint)
  3. Andrew G. Cohen and Daniel Z. Freedman, 'SIM(2) and SUSY', Journal of High Energy Physics JHEP07(2007)039, arXiv:hep-th/0605172, DOI: 10.1088/1126-6708/2007/07/039, https://arxiv.org/abs/hep-th/0605172
  4. G. W. Gibbons, Joaquim Gomis and C. N. Pope, 'General very special relativity is Finsler geometry', Physical Review D 76, 081701 (2007), arXiv:0707.2174, DOI: 10.1103/PhysRevD.76.081701, https://arxiv.org/abs/0707.2174
  5. M. M. Sheikh-Jabbari and A. Tureanu, 'Realization of Cohen-Glashow Very Special Relativity on Noncommutative Space-Time', Physical Review Letters 101, 261601 (2008), arXiv:0806.3699, DOI: 10.1103/PhysRevLett.101.261601, https://arxiv.org/abs/0806.3699
  6. Sangmo Cheon, Choonkyu Lee and Seung Jae Lee, 'SIM(2)-invariant Modifications of Electrodynamic Theory', Physics Letters B 679, 73-76 (2009), arXiv:0904.2065, DOI: 10.1016/j.physletb.2009.07.007, https://arxiv.org/abs/0904.2065
  7. Suratna Das and Subhendra Mohanty, 'Very Special Relativity is Incompatible with Thomas Precession', Modern Physics Letters A 26, 139-150 (2011), arXiv:0902.4549, DOI: 10.1142/S0217732311034037, https://arxiv.org/abs/0902.4549
  8. Jorge Alfaro and Victor O. Rivelles, 'Non Abelian Fields in Very Special Relativity', Physical Review D 88, 085023 (2013), arXiv:1305.1577, DOI: 10.1103/PhysRevD.88.085023, https://arxiv.org/abs/1305.1577
  9. Jorge Alfaro and Victor O. Rivelles, 'Very Special Relativity and Lorentz Violating Theories', Physics Letters B 734, 239-244 (2014), arXiv:1306.1941, DOI: 10.1016/j.physletb.2014.05.068, https://arxiv.org/abs/1306.1941
  10. R. V. Maluf, J. E. G. Silva, W. T. Cruz and C. A. S. Almeida, 'Dirac equation in very special relativity for hydrogen atom', Physics Letters B 738, 341-345 (2014), arXiv:1407.4757, DOI: 10.1016/j.physletb.2014.09.059, https://arxiv.org/abs/1407.4757
  11. Hassan Ganjitabar and Ali Shojai, 'Thomas precession and spin interaction energy in very special relativity', Modern Physics Letters A 29, 1450140 (2014), DOI: 10.1142/S0217732314501405, https://doi.org/10.1142/S0217732314501405
  12. Jorge Alfaro, Pablo González and Ricardo Ávila, 'Electroweak standard model with very special relativity', Physical Review D 91, 105007 (2015), arXiv:1504.04222, DOI: 10.1103/PhysRevD.91.105007, https://arxiv.org/abs/1504.04222
  13. Cheng-Yang Lee, 'Quantum field theory with a preferred direction: The very special relativity framework', Physical Review D 93, 045011 (2016), arXiv:1512.09175, DOI: 10.1103/PhysRevD.93.045011, https://arxiv.org/abs/1512.09175
  14. Anton Ilderton, 'Very Special Relativity as a background field theory', Physical Review D 94, 045019 (2016), arXiv:1605.04967, DOI: 10.1103/PhysRevD.94.045019, https://arxiv.org/abs/1605.04967
  15. Alekha C. Nayak and Pankaj Jain, 'Phenomenological Implications of Very Special Relativity', Physical Review D 96, 075020 (2017), arXiv:1610.01826, DOI: 10.1103/PhysRevD.96.075020, https://arxiv.org/abs/1610.01826
  16. Tripurari Srivastava and Alekha C. Nayak, 'Prospects of charged lepton flavor violation in very special relativity', The European Physical Journal Plus 135, 679 (2020), DOI: 10.1140/epjp/s13360-020-00676-2, https://doi.org/10.1140/epjp/s13360-020-00676-2
  17. Jorge Alfaro and Alessandro Santoni, 'Very special linear gravity: A gauge-invariant graviton mass', Physics Letters B 829, 137080 (2022), arXiv:2204.05485, DOI: 10.1016/j.physletb.2022.137080, https://arxiv.org/abs/2204.05485
  18. Benjamin Koch, Enrique Muñoz and Alessandro Santoni, 'Corrections to the gyromagnetic factor in very special relativity', Physical Review D 106, 096009 (2022), arXiv:2208.09824, DOI: 10.1103/PhysRevD.106.096009, https://arxiv.org/abs/2208.09824
  19. Jorge Alfaro, 'Renormalization of Very Special Relativity gauge theories', Journal of High Energy Physics JHEP06(2023)003, arXiv:2304.12933, DOI: 10.1007/JHEP06(2023)003, https://arxiv.org/abs/2304.12933
  20. Alessandro Santoni, Jorge Alfaro and Alex Soto, 'Graviton mass bounds in very special relativity from binary pulsar gravitational waves', Physical Review D 108, 044072 (2023), arXiv:2306.02464, DOI: 10.1103/PhysRevD.108.044072, https://arxiv.org/abs/2306.02464
  21. Jorge Alfaro, 'Light-Light scattering in Very Special Relativity Quantum Electrodynamics and Cosmic Anisotropies', Physics Letters B 858, 139021 (2024), arXiv:2406.04381, DOI: 10.1016/j.physletb.2024.139021, https://arxiv.org/abs/2406.04381
  22. Manuel Asorey, Fernando Falceto and Giuseppe Marmo, 'Interaction anomalies and one-particle dynamics in very special relativity theories', arXiv:2505.08329 (2025), https://arxiv.org/abs/2505.08329 (published version under the title 'Interaction anomalies and one-particle dynamics for maximal relativity subgroups', Geometric Mechanics 02, 433-444 (2025), DOI: 10.1142/S2972458925400106)
  23. I. H. Brevik, M. M. Chaichian, B. A. Couto e Silva and B. L. Sánchez-Vega, 'Very special relativity: Cherenkov effect and an analogy with Minkowski's electrodynamics of continuous media', The European Physical Journal C 85, 440 (2025), arXiv:2501.14409, DOI: 10.1140/epjc/s10052-025-14140-x, https://doi.org/10.1140/epjc/s10052-025-14140-x