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Quantization of Carrollian fermions

T0 review · 3 major / 3 minor · reviewed 2026-08-08 · deepseek-v4-flash

Pith's one-line read Taking the electric Carrollian limit of Yukawa theory yields quantized Dirac fermions whose interaction is a time-dependent Dirac-delta potential, and one-loop renormalization flow that is either unstable or Gaussian.

desk verdict The quantization half is solid and worth a referee; the one-loop fixed-point claim is withdrawn by the paper's own Appendix A and should not survive in current form. read the letter →

arxiv 2502.05645 v3 pith:B5TRSFXR submitted 2025-02-08 hep-th gr-qc

classification hep-thgr-qc
keywords CarrolliansymmetryultralocalfieldtheoryDiracfermionquantizationYukawaWilsonianrenormalizationgroupfixedpointsCPTtransformationsflat-bandsystems
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

Carrollian field theories are the $c \to 0$ contraction of relativistic theories: the light cone closes, particles cannot move through space, and only time evolution remains in the electric limit. This paper claims to provide the first quantized interacting example with Dirac fermions, obtained as the electric Carrollian limit of Yukawa theory. The fermions are canonically quantized, their charge-conjugation, parity, and time-reversal properties are worked out, and the tree-level Yukawa potential is exactly a spatial Dirac delta with a time-dependent factor, $V(t,x) = - i g^2 e^{-iM|t|}\delta^3(x)/(2M)$. The paper then applies one-loop Wilsonian renormalization to the same model and finds that the fixed-point structure is inverted relative to the relativistic theory: with a $\phi^4$ term the Carrollian theory has an unstable non-Gaussian fixed point, and without it only the Gaussian fixed point survives. The broader interest is that this connects Carrollian physics to well-studied point-like interactions in quantum optics and condensed matter and provides a field-theoretic origin for ultralocal interactions.

What carries the argument

The load-bearing object is the electric Carrollian limit, implemented by the rescalings $\tilde{\Psi} = \sqrt{c}\,\Psi$ and $\tilde{m} = m/c$, which sends the Dirac equation to $i\gamma^0\dot{\Psi} = m\Psi$ and the Klein-Gordon equation to $\ddot{\phi} + M^2\phi = 0$. Because no spatial derivatives survive, all propagators depend only on the frequency $w$, and the interaction vertex is local in space; this is what turns the Yukawa potential into a time-dependent Dirac delta. The Wilsonian machinery then scales only the frequency, $w' = bw$, leaving the spatial momenta untouched, which produces the unusual scaling dimensions $d_\phi = -1/2$ and $d_\psi = 0$ and the linear terms in the Carrollian $\beta$ functions. The divergent spatial momentum integral $K_3 = \int d^3k$ is regularized as $K_3 = a\Lambda$, so every loop correction carries this factor and the fixed-point values depend on it.

What would settle it

Compute the one-loop Carrollian $\beta$ functions keeping the field-strength renormalization terms and without imposing $M^2 \ll \Lambda^2$; if the non-Gaussian fixed point at $M_*^2 = -\Lambda^2/3$ shifts or disappears, the reported fixed-point structure is an artifact of the regulator. A complementary check is to repeat the Wilsonian analysis with a dimensionally regularized spatial integral instead of $K_3 = a\Lambda$; genuine regulator independence would keep the fixed points fixed, while scheme dependence would expose the assumption.

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Extended reading notes

Core claim

The core claim is that an interacting quantum field theory of Carrollian Dirac fermions exists and is described by the electric Carrollian limit of Yukawa theory. The authors start from the Carrollian Dirac Lagrangian $\mathcal{L}_{CD} = \bar{\Psi} i\gamma^0 \dot{\Psi} - m\bar{\Psi}\Psi$, obtain the Feynman propagator $S_F(w) = i(w\gamma^0 + m)/(w^2 - m^2 + i\epsilon)$, and couple the fermions to a Carrollian scalar through $g\phi\bar{\Psi}\Psi$ plus a $\lambda\phi^4$ self-interaction. Computing the tree-level scattering amplitude gives $V(t,x) = - i g^2 e^{-iM|t|}\delta^3(x)/(2M)$, an ultralocal, time-dependent point interaction. At one loop, Wilsonian renormalization with only the frequency rescaled gives $\beta$ functions whose fixed points are summarized by Table II: in the Carrollian theory with $\lambda \neq 0$ there is a non-Gaussian fixed point $(M^2_* = -\Lambda^2/3, m_* = 0, \lambda_* = 128\pi^4\Lambda^3/(9K_3), g_* = 0)$ with a relevant direction, while deleting $\lambda\phi^4$ leaves only Gaussian fixed points; the relativistic theory shows the opposite pattern. The paper also shows that the allowed CPT-invariant Lagrangian terms are only the kinetic and mass terms, because $\Psi^\dagger\Psi$ is odd under charge conjugation and $i\bar{\Psi}\gamma^5\Psi$ is odd under time reversal.

Load-bearing premise

The load-bearing premise is that the divergent spatial momentum integral $K_3 = \int d^3k$ can be treated as a finite constant times the cutoff, $K_3 = a\Lambda$, and that the resulting cutoff-dependent $\beta$ functions still describe the physics; this assumption is strained by the theory's own fixed point $M_*^2 = -\Lambda^2/3$, which violates the $M^2 \ll \Lambda^2$ condition used in the calculation.

Editorial extensions

If this is right

  • The tree-level potential $V(t,x) = -i g^2 e^{-iM|t|}\delta^3(x)/(2M)$ gives Carrollian Yukawa theory as a field-theoretic origin for the time-dependent Dirac-delta potentials used in quantum tunnelling, quantum defects, and quantum optics.
  • Because the Carrollian beta functions contain linear terms in $g$ and $\lambda$, the deformed ($\lambda=0$) Carrollian theory has only irrelevant couplings and flows to the Gaussian fixed point, so it remains perturbatively trivial at all scales.
  • With $\lambda\phi^4$ included, the non-Gaussian Carrollian fixed point has stability eigenvalues $-3/2$, $-1$, $1-\sqrt{10}$, and $1+\sqrt{10}$, so exactly one direction is relevant and the fixed point is unstable.
  • In the relativistic theory the roles are reversed: the $\lambda \neq 0$ theory has only Gaussian fixed points, while the deformed theory has non-Gaussian points $m_* = \pm\Lambda$, $g_* = \pm4\pi$ with oscillatory unstable flow, as collected in Table II.
  • The Carrollian limit systematically converts marginal relativistic couplings into irrelevant couplings, which suggests that interacting Carrollian theories do not generate new universality classes at one loop.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • Editorial inference: if the spatial-momentum integral $K_3$ factorizes at all loop orders, the ultralocal interaction may be exact rather than a tree-level accident, and a lattice regularization of the spatial directions would provide a direct numerical test.
  • Editorial inference: the negative scalar mass-squared at the non-Gaussian fixed point hints at a Carrollian analogue of spontaneous symmetry breaking; adding a symmetry-breaking term could lift the instability and turn the fixed point into a physical critical point.
  • Editorial inference: because the free Carrollian Dirac propagator carries no spatial momentum, the model may be exactly solvable in the ultralocal sector, and the same Wilsonian treatment applied to magnetic Carrollian fermions (which keep spatial derivatives) could restore a richer fixed-point structure.
  • Editorial inference: since $\Psi^\dagger\Psi$ is odd under charge conjugation, a Carrollian theory coupled to an electromagnetic-like field through this bilinear would break C and could produce distinct transport signatures in flat-band systems.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 3 minor

Summary. The paper studies the electric Carrollian limit of Dirac fermions in 3+1 dimensions. It constructs the free Carrollian Dirac action, canonically quantizes the field, computes the Feynman propagator, and analyzes charge conjugation, parity, and time reversal for the relevant bilinears. It then couples the fermions to a Carrollian scalar through a Yukawa interaction and obtains the tree-level scattering amplitude, which yields an ultralocal, time-dependent delta-function potential, Eq. (66). The rest of the paper applies Wilsonian renormalization at one loop: the authors derive beta functions (101), identify a non-Gaussian fixed point (102), analyze its stability via the matrix (104), and summarize the fixed-point structure in Table II. An appendix presents a more complete one-loop calculation and reaches a different conclusion about the Carrollian fixed points.

Significance. The free-field quantization of the electric Carrollian Dirac fermion and the derivation of the tree-level ultralocal Yukawa potential are clean, self-contained, and potentially useful: they provide an explicit fermionic example in Carrollian field theory, connect the Carrollian limit to time-dependent point-like interactions relevant in condensed matter and quantum mechanics, and the discrete symmetry analysis is systematic. The paper is also honest in presenting limitations in Appendix A. However, the renormalization-group analysis, which is advertised in the abstract and Section V, is not supported as written: the non-Gaussian fixed point in the main text is contradicted by the paper's own Appendix A, and the one-loop beta functions depend on an ad hoc regularization of the divergent spatial momentum integral K3. The fixed-point claim should therefore be corrected or substantially qualified before the paper can be accepted.

major comments (3)
  1. [Section V.A.2, Eq. (102) and Table II] The non-Gaussian fixed point M*^2 = -Λ^2/3, λ* = 128π^4Λ^3/(9K3) presented in the main text is internally contradicted by Appendix A. The beta functions (101) were derived assuming M^2 << Λ^2, but the fixed point violates this condition. Appendix A explicitly states that the non-Gaussian fixed points for M^2 are O(Λ^2), that this 'invalidates the condition M^2 << Λ^2', and that 'Consequently, we are left with only Gaussian fixed points.' Table II and the discussion around Eq. (102) therefore do not represent a consistent result of the paper as a whole; this contradiction must be resolved before the renormalization claim can be accepted.
  2. [Section V.A.2, Eqs. (96)-(101) and Appendix A] The one-loop results depend on the divergent spatial volume K3 = ∫d^3k, which is treated as a finite constant. Since the Carrollian propagators depend only on frequency, K3 factors out of every loop integral and is not a Wilsonian momentum-shell contribution. The replacement K3 = aΛ used in Appendix A is an ad hoc regularization, and the fixed point value λ* in Eq. (102) changes with the choice of K3 (for example K3 ~ (4π/3)Λ^3 versus K3 = aΛ); the appendix's own conclusion is that only Gaussian fixed points survive in the regime of validity. The beta functions (101) and the stability analysis (104) are therefore regulator-dependent as stated, and a physical justification for K3, or a regulator-independent statement of the results, is required.
  3. [Section V.A.2 and Appendix A] The main text derives the beta functions (101) after setting external momenta to zero and neglecting field-strength renormalization, referring to Appendix A for details. The full one-loop beta functions in Appendix A contain additional contributions from field-strength renormalization, and the appendix finds that the non-Gaussian Carrollian fixed points lie outside the M^2 << Λ^2 regime used in the derivation. The relationship between the truncated beta functions (101) and the more complete expressions (A9)-(A11) is not explained, and it is not shown that the fixed point (102) is robust under the inclusion of the omitted terms. The authors should either justify the truncation or present the fixed-point structure only in the regime where the approximations are controlled.
minor comments (3)
  1. [Eq. (66)] The tree-level potential V(t,x) = -i g^2 e^{-iM|t|} δ^3(x)/(2M) is complex, while the interaction term -g φ Ψbar Ψ in the Lagrangian (62) is Hermitian. The authors should clarify whether this is an effective or non-Hermitian potential and how the imaginary coefficient is to be interpreted physically.
  2. [Eq. (34)] The operator ordering in the expression for the Carroll boost charge C^i is not normal ordered; using the anticommutation relation (29) may introduce a divergent c-number term. The authors should specify the normal-ordering prescription or verify the commutator [P^i, C^j] = iδ^{ij}H with the ordering as written.
  3. [References] Reference [7] appears to contain an incomplete author name ('J., E. Have' should presumably be 'J. Hartong, E. Have'), and a few equation numbers are missing or inconsistently referenced; a final proofreading pass would be helpful.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: the Carrollian fermion quantization, tree-level ultralocal potential, and one-loop beta functions are derived self-containedly from the stated Lagrangian.

full rationale

The paper's central derivations are self-contained. The Carrollian Dirac action (20) is obtained by the stated electric limit and quantization conditions, and the Feynman rules (63) follow from that action. The tree-level Yukawa potential (66) is a direct Fourier transform of the amplitude (64), with no input equivalent to the output. The one-loop beta functions (101) are computed from the standard Wilsonian procedure applied to the diagrams of Figure 2; they contain no fitted parameter and no quantity defined in terms of the target fixed points. The spatial-momentum integral K3 is a regulator-dependent constant, and treating it as a*Lambda in Appendix A is a regularization assumption, not a circular definition or a fit. The fixed points (102) are then solved from beta=0 rather than assumed. Self-citations (e.g., [34,49,50]) appear only as background or as extensions, not as load-bearing justification for the present results; the key comparison [30] is independent prior work by different authors. The Appendix A limitation, which notes that the non-Gaussian fixed point has M*^2 = -Lambda^2/3 and thereby invalidates the M^2 << Lambda^2 approximation, is an internal consistency and physical-interpretation concern, not a circularity: the derivation chain does not reduce to its own inputs. All model-specific predictions (ultralocal interaction, beta functions, fixed-point structure) are consequences of the explicitly written Lagrangian and standard perturbative rules.

Assumptions & free parameters 1 free parameters · 3 assumptions · 0 invented entities

The central claims rest on the standard Carrollian limiting procedure and on an anisotropic Wilsonian RG. The only ad hoc element is the regularization of the spatial volume factor K3, which directly controls the beta functions and fixed points. No new particles or forces are introduced.

free parameters (1)
  • K3 (spatial momentum volume) = K3 = a Lambda
    The loop integrals over spatial momenta are independent of k and produce the divergent volume K3 = integral d^3k. The paper regularizes it as K3 = a Lambda with an arbitrary constant a. All beta functions (101) and the fixed point (102) depend on this constant.
assumptions (3)
  • domain assumption The electric Carrollian limit is obtained by the rescalings phi = c phi_tilde, M = M_tilde/c, Psi = sqrt(c) Psi_tilde, m = m_tilde/c, g = g_tilde/c^2, lambda = lambda_tilde/c^4 followed by c to 0.
    This is the standard Carrollian limiting procedure used throughout the paper (Sections III and V), and it defines the theory under study.
  • domain assumption The Wilsonian renormalization group can be applied to Carrollian theories by scaling only the energy component w' = b w, leaving spatial momenta k unchanged.
    Used in Section V.A.2; the validity of this anisotropic RG procedure for Carrollian field theories is assumed from reference [30].
  • ad hoc to paper The spatial momentum integral K3 = integral d^3k can be treated as a finite constant a Lambda.
    Introduced in Appendix A to regularize the divergent spatial volume in loop integrals; the beta functions depend on this ad hoc regulator.

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Cite this review

Pith. "Pith review of Quantization of Carrollian fermions." pith.science (2026). https://pith.science/paper/B5TRSFXR

@misc{pith2026250205645,
  author       = {Pith},
  title        = {Pith review of: Quantization of Carrollian fermions},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/B5TRSFXR}},
  note         = {Machine review of arXiv:2502.05645}
}
read the original abstract

We provide the first example of interacting quantized Carrollian Dirac fermions and investigate their discrete symmetries, including charge conjugation (C), parity (P), and time reversal (T) transformations. As a toy model, we couple these fermions to a Carrollian scalar field using Carrollian Yukawa theory and compute the tree-level diagram, revealing an ultralocal interaction between the Carrollian fermions and the scalar field. This interaction, widely known as a Dirac delta interaction with time-dependent factor, frequently appears in quantum physics. We then address the renormalization of the theory by employing the Wilsonian procedure at one-loop order. Furthermore, we analyze the fixed points and stability properties of Carrollian Yukawa theory, comparing them with their relativistic counterparts. Beyond the specific Yukawa model studied here, we expect that our framework will have broader applications in Carrollian physics, particularly in understanding ultralocal interactions and their role in condensed matter systems, where similar phenomena arise in strongly correlated and non-relativistic regimes.

Figures

Figures reproduced from arXiv: 2502.05645 by the authors.

Figure 1
Figure 1. FIG. 1. Yukawa vertex [PITH_FULL_IMAGE:figures/full_fig_p010_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2. Here diagrams (a) and (b) illustrate the scalar’s self-energy diagrams resulting from the couplings [PITH_FULL_IMAGE:figures/full_fig_p013_2.png] view at source ↗

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Interacting Galilean and Finite-Energy Carroll Fermions

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    A c-dependent similarity transformation generates new Galilean and Carrollian fermion actions, including a Carrollian model with non-removable finite energy and a Galilean model with an accidental fermionic gauge symmetry.

  2. Carroll fermions of arbitrary spin

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    Free massless fermions of arbitrary spin admit two inequivalent Carrollian (c→0) limits, electric and magnetic, derived from the Fang–Fronsdal actions, with the magnetic theory reducible to the projected relativistic ...

  3. A finite Carrollian critical point

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Reference graph

Works this paper leans on

102 extracted references · 10 canonical work pages · cited by 3 Pith papers

  1. [1]

    Charge conjugation defines the symmetry between particles and antiparticles and is implemented by a unitary operator C

    Charge conjugation We begin our discussion with the charge conjugation transformation. Charge conjugation defines the symmetry between particles and antiparticles and is implemented by a unitary operator C. This operator transforms a fermion 4 Note that CPT transformations in two and three dimensions are discussed in [86, 87] in different context. 8 into ...

  2. [2]

    The parity operator transforms the state as† ⃗k |0⟩ into as† −⃗k |0⟩ as we know from the Lorentzian case

    Parity Now, we proceed by investigating the parity transformation of the Carrollian Dirac field. The parity operator transforms the state as† ⃗k |0⟩ into as† −⃗k |0⟩ as we know from the Lorentzian case. Consequently, we may interpret the operator as follows: P as ⃗kP = ηaas −⃗k & P bs ⃗kP = ηbbs −⃗k , (53) 9 where ηa and ηb represents possible phase facto...

  3. [3]

    Essentially, electric Carrollian field theory can be considered as a one-dimensional quantum mechanics [34]

    Time reversal As a final exploration of discrete symmetry transformations, we shall investigate the time reversal transformation and its consequences. Essentially, electric Carrollian field theory can be considered as a one-dimensional quantum mechanics [34]. Consequently, the time reversal operator remains an antiunitary operator in Carrollian field theo...

  4. [4]

    In Wilsonian renormalization, the RG flow describes how parameters of the theory scale as the high energy degrees of freedom are integrated out

    Warming up: Relativistic theory The Wilsonian renormalization is a powerful conceptual and technical framework in theoretical physics, particularly in quantum field theory and statistical mechanics, for understanding how physical theories behave at different energy scales. In Wilsonian renormalization, the RG flow describes how parameters of the theory sc...

  5. [5]

    − 1 M 2 (Λ2 + M 2) + log 1 + M 2/Λ2 M 4 # βg = g3 8π2 Λ2 Λ2 + M 2 + g3 8π2 + g3Λ4 8π2

    Carrollian theory A similar analysis can be carried out for the Carrollian regime. However, it is crucial to note that in the Carrollian regime, as seen from propagators and other quantities, fields strictly depend on the energy component but not on the spatial momentum component. Since the fields do not explicitly depend on spatial momentum, any rescalin...

  6. [6]

    Carroll stories,

    J. de Boer, J. Hartong, N. A. Obers, W. Sybesma, and S. Vandoren, “Carroll stories,” JHEP 09 (2023) 148, arXiv:2307.06827 [hep-th]

  7. [7]

    A non-lorentzian primer,

    E. Bergshoeff, J. Figueroa-O’Farrill, and J. Gomis, “A non-lorentzian primer,” SciPost Phys. Lect. Notes 69 (2023) 1, arXiv:2206.12177 [hep-th]

  8. [8]

    Aspects of Nonrelativistic Strings,

    G. Oling and Z. Yan, “Aspects of Nonrelativistic Strings,” Front. in Phys. 10 (2022) 832271, arXiv:2202.12698 [hep-th]

Show all 102 references
  1. [9]

    On the Contraction of groups and their represenations,

    E. Inonu and E. P. Wigner, “On the Contraction of groups and their represenations,” Proc. Nat. Acad. Sci. 39 (1953) 510–524

  2. [10]

    Une nouvelle limite non-relativiste du groupe de poincar´ es,

    J.-M. L´ evy-Leblond, “Une nouvelle limite non-relativiste du groupe de poincar´ es,”JAnn. l’I. H. P. Phys. Th´ eor.3 no. 1, (1965)

  3. [11]

    On an analogue of the galilei group,

    N. D. S. Gupta, “On an analogue of the galilei group,” Il Nuovo Cimento A (1965-1970) 44, 512(1966)

  4. [12]

    Ultralocal scalar field models,

    J. R. Klauder, “Ultralocal scalar field models,” Commun. Math. Phys. 18 (1970) 307–318. 22

  5. [13]

    Fractons, dipole symmetries and curved spacetime,

    L. Bidussi, J. , E. Have, J. Musaeus, and S. Prohazka, “Fractons, dipole symmetries and curved spacetime,” SciPost Phys. 12 no. 6, (2022) 205, arXiv:2111.03668 [hep-th]

  6. [14]

    Space-Dependent Symmetries and Fractons,

    K. T. Grosvenor, C. Hoyos, F. Pe˜ na Benitez, and P. Sur´ owka, “Space-Dependent Symmetries and Fractons,”Front. in Phys. 9 (2022) 792621, arXiv:2112.00531 [hep-th]

  7. [15]

    Carroll/fracton particles and their correspondence,

    J. Figueroa-O’Farrill, A. P´ erez, and S. Prohazka, “Carroll/fracton particles and their correspondence,” Journal of High Energy Physics 2023 no. 6, (June, 2023) . http://dx.doi.org/10.1007/JHEP06(2023)207

  8. [16]

    Quantum Carroll/fracton particles,

    J. Figueroa-O’Farrill, A. P´ erez, and S. Prohazka, “Quantum Carroll/fracton particles,”JHEP 10 (2023) 041, arXiv:2307.05674 [hep-th]

  9. [17]

    Magic fermions: Carroll and flat bands,

    A. Bagchi, A. Banerjee, R. Basu, M. Islam, and S. Mondal, “Magic fermions: Carroll and flat bands,” JHEP 03 (2023) 227, arXiv:2211.11640 [hep-th]

  10. [18]

    Hall effects in Carroll dynamics,

    L. Marsot, P. M. Zhang, M. Chernodub, and P. A. Horvathy, “Hall effects in Carroll dynamics,” Phys. Rept. 1028 (2023) 1–60, arXiv:2212.02360 [hep-th]

  11. [19]

    Perfect Fluids,

    J. de Boer, J. Hartong, N. A. Obers, W. Sybesma, and S. Vandoren, “Perfect Fluids,” SciPost Phys. 5 no. 1, (2018) 003, arXiv:1710.04708 [hep-th]

  12. [20]

    Covariant Galilean versus Carrollian hydrodynamics from relativistic fluids,

    L. Ciambelli, C. Marteau, A. C. Petkou, P. M. Petropoulos, and K. Siampos, “Covariant Galilean versus Carrollian hydrodynamics from relativistic fluids,” Class. Quant. Grav. 35 no. 16, (2018) 165001, arXiv:1802.05286 [hep-th]

  13. [21]

    Two-dimensional fluids and their holographic duals,

    A. Campoleoni, L. Ciambelli, C. Marteau, P. M. Petropoulos, and K. Siampos, “Two-dimensional fluids and their holographic duals,” Nucl. Phys. B 946 (2019) 114692, arXiv:1812.04019 [hep-th]

  14. [22]

    Relativistic fluids, hydrodynamic frames and their Galilean versus Carrollian avatars,

    A. C. Petkou, P. M. Petropoulos, D. R. Betancour, and K. Siampos, “Relativistic fluids, hydrodynamic frames and their Galilean versus Carrollian avatars,” JHEP 09 (2022) 162, arXiv:2205.09142 [hep-th]

  15. [23]

    Carrollian hydrodynamics from symmetries,

    L. Freidel and P. Jai-akson, “Carrollian hydrodynamics from symmetries,” Class. Quant. Grav. 40 no. 5, (2023) 055009, arXiv:2209.03328 [hep-th]

  16. [24]

    Carrollian Origins of Bjorken Flow,

    A. Bagchi, K. S. Kolekar, and A. Shukla, “Carrollian Origins of Bjorken Flow,” Phys. Rev. Lett. 130 no. 24, (2023) 241601, arXiv:2302.03053 [hep-th]

  17. [25]

    Carroll Symmetry, Dark Energy and Inflation,

    J. de Boer, J. Hartong, N. A. Obers, W. Sybesma, and S. Vandoren, “Carroll Symmetry, Dark Energy and Inflation,” Front. in Phys. 10 (2022) 810405, arXiv:2110.02319 [hep-th]

  18. [26]

    Quintessence and the Higgs portal in the Carroll limit,

    B. Avila, J. Gamboa, R. B. MacKenzie, F. Mendez, and M. B. Paranjape, “Quintessence and the Higgs portal in the Carroll limit,” Phys. Lett. B 855 (2024) 138819, arXiv:2312.17393 [hep-th]

  19. [27]

    Tensionless Strings from Worldsheet Symmetries,

    A. Bagchi, S. Chakrabortty, and P. Parekh, “Tensionless Strings from Worldsheet Symmetries,” JHEP 01 (2016) 158, arXiv:1507.04361 [hep-th]

  20. [28]

    Strings near black holes are Carrollian,

    A. Bagchi, A. Banerjee, J. Hartong, E. Have, K. S. Kolekar, and M. Mandlik, “Strings near black holes are Carrollian,” Phys. Rev. D 110 no. 8, (2024) 086009, arXiv:2312.14240 [hep-th]

  21. [29]

    Strings near black holes are Carrollian. Part II,

    A. Bagchi, A. Banerjee, J. Hartong, E. Have, and K. S. Kolekar, “Strings near black holes are Carrollian. Part II,” JHEP 11 (2024) 024, arXiv:2407.12911 [hep-th]

  22. [30]

    Path-integral quantization of tensionless (super) string,

    B. Chen, Z. Hu, Z.-f. Yu, and Y.-f. Zheng, “Path-integral quantization of tensionless (super) string,” JHEP 08 (2023) 133, arXiv:2302.05975 [hep-th]

  23. [31]

    Unification of Decoupling Limits in String and M Theory,

    C. D. A. Blair, J. Lahnsteiner, N. A. Obers, and Z. Yan, “Unification of Decoupling Limits in String and M Theory,” Phys. Rev. Lett. 132 no. 16, (2024) 161603, arXiv:2311.10564 [hep-th]

  24. [32]

    Field Theories with Conformal Carrollian Symmetry,

    A. Bagchi, A. Mehra, and P. Nandi, “Field Theories with Conformal Carrollian Symmetry,” JHEP 05 (2019) 108, arXiv:1901.10147 [hep-th]

  25. [33]

    Carroll contractions of Lorentz-invariant theories,

    M. Henneaux and P. Salgado-Rebolledo, “Carroll contractions of Lorentz-invariant theories,” JHEP 11 (2021) 180, arXiv:2109.06708 [hep-th]

  26. [34]

    BMS 3 (Carrollian) field theories from a bound in the coupling of current-current deformations of CFT 2,

    P. Parekh, D. Tempo, and R. Troncoso, “BMS 3 (Carrollian) field theories from a bound in the coupling of current-current deformations of CFT 2,” JHEP 09 (2023) 083, arXiv:2307.06367 [hep-th]

  27. [35]

    One-loop quantum effects in Carroll scalars,

    K. Banerjee, R. Basu, B. Krishnan, S. Maulik, A. Mehra, and A. Ray, “One-loop quantum effects in Carroll scalars,” Phys. Rev. D 108 no. 8, (2023) 085022, arXiv:2307.03901 [hep-th]

  28. [36]

    Super-Carrollian and Super-Galilean Field Theories,

    K. Koutrolikos and M. Najafizadeh, “Super-Carrollian and Super-Galilean Field Theories,” Phys. Rev. D 108 no. 12, (2023) 125014, arXiv:2309.16786 [hep-th]

  29. [37]

    Toward Carrollian quantization: Renormalization of Carrollian electrodynamics,

    A. Mehra and A. Sharma, “Toward Carrollian quantization: Renormalization of Carrollian electrodynamics,” Phys. Rev. D 108 no. 4, (2023) 046019, arXiv:2302.13257 [hep-th]

  30. [38]

    Carrollian origin of spacetime subsystem symmetry,

    O. Kasikci, M. Ozkan, and Y. Pang, “Carrollian origin of spacetime subsystem symmetry,” Phys. Rev. D 108 no. 4, (2023) 045020, arXiv:2304.11331 [hep-th]

  31. [39]

    Carrollian supersymmetry and SYK-like models,

    O. Kasikci, M. Ozkan, Y. Pang, and U. Zorba, “Carrollian supersymmetry and SYK-like models,” Phys. Rev. D 110 no. 2, (2024) L021702, arXiv:2311.00039 [hep-th]

  32. [40]

    Carroll-invariant propagating fields,

    F. Ecker, D. Grumiller, M. Henneaux, and P. Salgado-Rebolledo, “Carroll-invariant propagating fields,” Phys. Rev. D 110 no. 4, (2024) L041901

  33. [41]

    Quantizing Carrollian field theories,

    J. Cotler, K. Jensen, S. Prohazka, A. Raz, M. Riegler, and J. Salzer, “Quantizing Carrollian field theories,” JHEP 10 (2024) 049, arXiv:2407.11971 [hep-th]

  34. [42]

    Quantization of Carrollian conformal scalar theories,

    B. Chen, H. Sun, and Y.-f. Zheng, “Quantization of Carrollian conformal scalar theories,” Phys. Rev. D 110 no. 12, (2024) 125010, arXiv:2406.17451 [hep-th]

  35. [43]

    Supersymmetric Carroll Galileons in Three Dimensions,

    U. Zorba, I. Bulunur, O. Kasikci, M. Ozkan, Y. Pang, and M. S. Zog, “Supersymmetric Carroll Galileons in Three Dimensions,” arXiv:2409.15428 [hep-th]

  36. [44]

    Carroll in Shallow Water,

    A. Bagchi, A. Banerjee, S. Mondal, and S. Sarkar, “Carroll in Shallow Water,” arXiv:2411.04190 [hep-th]

  37. [45]

    Studies on Carrollian Quantum Field Theories,

    A. Sharma, “Studies on Carrollian Quantum Field Theories,” arXiv:2502.00487 [hep-th]. 23

  38. [46]

    Gauging the Carroll Algebra and Ultra-Relativistic Gravity,

    J. Hartong, “Gauging the Carroll Algebra and Ultra-Relativistic Gravity,” JHEP 08 (2015) 069, arXiv:1505.05011 [hep-th]

  39. [47]

    Carroll versus Galilei Gravity,

    E. Bergshoeff, J. Gomis, B. Rollier, J. Rosseel, and T. ter Veldhuis, “Carroll versus Galilei Gravity,” JHEP 03 (2017) 165, arXiv:1701.06156 [hep-th]

  40. [48]

    AdS Carroll Chern-Simons supergravity in 2 + 1 dimensions and its flat limit,

    L. Ravera, “AdS Carroll Chern-Simons supergravity in 2 + 1 dimensions and its flat limit,” Phys. Lett. B 795 (2019) 331–338, arXiv:1905.00766 [hep-th]

  41. [49]

    N -extended Chern-Simons Carrollian supergravities in 2 + 1 spacetime dimensions,

    F. Ali and L. Ravera, “ N -extended Chern-Simons Carrollian supergravities in 2 + 1 spacetime dimensions,” JHEP 02 (2020) 128, arXiv:1912.04172 [hep-th]

  42. [50]

    Limits of JT gravity,

    D. Grumiller, J. Hartong, S. Prohazka, and J. Salzer, “Limits of JT gravity,” JHEP 02 (2021) 134, arXiv:2011.13870 [hep-th]

  43. [51]

    Non-relativistic and Carrollian limits of Jackiw-Teitelboim gravity,

    J. Gomis, D. Hidalgo, and P. Salgado-Rebolledo, “Non-relativistic and Carrollian limits of Jackiw-Teitelboim gravity,” JHEP 05 (2021) 162, arXiv:2011.15053 [hep-th]

  44. [52]

    Carroll Expansion of General Relativity,

    D. Hansen, N. A. Obers, G. Oling, and B. T. Sogaard, “Carroll Expansion of General Relativity,” SciPost Phys. 13 no. 3, (2022) 055, arXiv:2112.12684 [hep-th]

  45. [53]

    Three-dimensional Maxwellian Carroll gravity theory and the cosmological constant,

    P. Concha, D. Pe˜ nafiel, L. Ravera, and E. Rodr ´ ıguez, “Three-dimensional Maxwellian Carroll gravity theory and the cosmological constant,” Phys. Lett. B 823 (2021) 136735, arXiv:2107.05716 [hep-th]

  46. [54]

    Carrollian and non-relativistic Jackiw–Teitelboim supergravity,

    L. Ravera and U. Zorba, “Carrollian and non-relativistic Jackiw–Teitelboim supergravity,” Eur. Phys. J. C 83 no. 2, (2023) 107, arXiv:2204.09643 [hep-th]

  47. [55]

    Non-relativistic and ultra-relativistic scaling limits of multimetric gravity,

    E. Ekiz, O. Kasikci, M. Ozkan, C. B. Senisik, and U. Zorba, “Non-relativistic and ultra-relativistic scaling limits of multimetric gravity,” JHEP 10 (2022) 151, arXiv:2207.07882 [hep-th]

  48. [56]

    Extended kinematical 3D gravity theories,

    P. Concha, D. Pino, L. Ravera, and E. Rodr ´ ıguez, “Extended kinematical 3D gravity theories,”JHEP 01 (2024) 040, arXiv:2310.01335 [hep-th]

  49. [57]

    Non-Lorentzian Supergravity and Kinematical Superalgebras,

    P. Concha and L. Ravera, “Non-Lorentzian Supergravity and Kinematical Superalgebras,” arXiv:2412.07665 [hep-th]

  50. [58]

    Carroll black holes,

    F. Ecker, D. Grumiller, J. Hartong, A. P´ erez, S. Prohazka, and R. Troncoso, “Carroll black holes,” SciPost Phys. 15 no. 6, (2023) 245, arXiv:2308.10947 [hep-th]

  51. [59]

    Carroll-Hawking effect,

    A. Aggarwal, F. Ecker, D. Grumiller, and D. Vassilevich, “Carroll-Hawking effect,” Phys. Rev. D 110 no. 4, (2024) L041506, arXiv:2403.00073 [hep-th]

  52. [60]

    Carrollian Physics at the Black Hole Horizon,

    L. Donnay and C. Marteau, “Carrollian Physics at the Black Hole Horizon,” Class. Quant. Grav. 36 no. 16, (2019) 165002, arXiv:1903.09654 [hep-th]

  53. [61]

    Non-linear black hole dynamics and carrollian fluids,

    J. Redondo-Yuste and L. Lehner, “Non-linear black hole dynamics and carrollian fluids,” Journal of High Energy Physics 2023 no. 2, (Feb., 2023) . http://dx.doi.org/10.1007/JHEP02(2023)240

  54. [62]

    Gravitational waves in general relativity. vii. waves from axi-symmetric isolated systems,

    H. Bondi, M. G. J. van der Burg, and A. W. K. Metzner, “Gravitational waves in general relativity. vii. waves from axi-symmetric isolated systems,” Proceedings of the Royal Society. A. Mathematical, Physical and Engineering Sciences 269 no. 1336, (8, 1962) . https://www.osti.g...

  55. [63]

    Asymptotic symmetries in gravitational theory,

    R. Sachs, “Asymptotic symmetries in gravitational theory,” Phys. Rev. 128 (1962) 2851–2864

  56. [64]

    Carroll versus Newton and Galilei: two dual non-Einsteinian concepts of time,

    C. Duval, G. W. Gibbons, P. A. Horvathy, and P. M. Zhang, “Carroll versus Newton and Galilei: two dual non-Einsteinian concepts of time,” Class. Quant. Grav. 31 (2014) 085016, arXiv:1402.0657 [gr-qc]

  57. [65]

    Conformal Carroll groups and BMS symmetry,

    C. Duval, G. W. Gibbons, and P. A. Horvathy, “Conformal Carroll groups and BMS symmetry,” Class. Quant. Grav. 31 (2014) 092001, arXiv:1402.5894 [gr-qc]

  58. [66]

    Conformal Carroll groups,

    C. Duval, G. W. Gibbons, and P. A. Horvathy, “Conformal Carroll groups,” J. Phys. A 47 no. 33, (2014) 335204, arXiv:1403.4213 [hep-th]

  59. [67]

    Flat holography and Carrollian fluids,

    L. Ciambelli, C. Marteau, A. C. Petkou, P. M. Petropoulos, and K. Siampos, “Flat holography and Carrollian fluids,” JHEP 07 (2018) 165, arXiv:1802.06809 [hep-th]

  60. [68]

    Carrollian and celestial spaces at infinity,

    J. Figueroa-O’Farrill, E. Have, S. Prohazka, and J. Salzer, “Carrollian and celestial spaces at infinity,” JHEP 09 (2022) 007, arXiv:2112.03319 [hep-th]

  61. [69]

    Carrollian manifolds and null infinity: a view from Cartan geometry,

    Y. Herfray, “Carrollian manifolds and null infinity: a view from Cartan geometry,” Class. Quant. Grav. 39 no. 21, (2022) 215005, arXiv:2112.09048 [gr-qc]

  62. [70]

    Ehlers, Carroll, charges and dual charges,

    N. Mittal, P. M. Petropoulos, D. Rivera-Betancour, and M. Vilatte, “Ehlers, Carroll, charges and dual charges,” JHEP 07 (2023) 065, arXiv:2212.14062 [hep-th]

  63. [71]

    Flat from anti de Sitter,

    A. Campoleoni, A. Delfante, S. Pekar, P. M. Petropoulos, D. Rivera-Betancour, and M. Vilatte, “Flat from anti de Sitter,” JHEP 12 (2023) 078, arXiv:2309.15182 [hep-th]

  64. [72]

    Flat Space Amplitudes and Conformal Symmetry of the Celestial Sphere,

    S. Pasterski, S.-H. Shao, and A. Strominger, “Flat Space Amplitudes and Conformal Symmetry of the Celestial Sphere,” Phys. Rev. D 96 no. 6, (2017) 065026, arXiv:1701.00049 [hep-th]

  65. [73]

    Carrollian Perspective on Celestial Holography,

    L. Donnay, A. Fiorucci, Y. Herfray, and R. Ruzziconi, “Carrollian Perspective on Celestial Holography,” Phys. Rev. Lett. 129 no. 7, (2022) 071602, arXiv:2202.04702 [hep-th]

  66. [74]

    Scattering Amplitudes: Celestial and Carrollian,

    A. Bagchi, S. Banerjee, R. Basu, and S. Dutta, “Scattering Amplitudes: Celestial and Carrollian,” Phys. Rev. Lett. 128 no. 24, (2022) 241601, arXiv:2202.08438 [hep-th]

  67. [75]

    Bridging Carrollian and celestial holography,

    L. Donnay, A. Fiorucci, Y. Herfray, and R. Ruzziconi, “Bridging Carrollian and celestial holography,” Phys. Rev. D 107 no. 12, (2023) 126027, arXiv:2212.12553 [hep-th]

  68. [76]

    Lectures on Celestial Holography,

    A.-M. Raclariu, “Lectures on Celestial Holography,” arXiv:2107.02075 [hep-th]

  69. [77]

    Lectures on celestial amplitudes,

    S. Pasterski, “Lectures on celestial amplitudes,” Eur. Phys. J. C 81 no. 12, (2021) 1062, arXiv:2108.04801 [hep-th]

  70. [78]

    Carrollian Conformal Fields and Flat Holography,

    K. Nguyen and P. West, “Carrollian Conformal Fields and Flat Holography,” Universe 9 no. 9, (2023) 385, arXiv:2305.02884 [hep-th]

  71. [79]

    Carrollian conformal correlators and massless scattering amplitudes,

    K. Nguyen, “Carrollian conformal correlators and massless scattering amplitudes,” JHEP 01 (2024) 076, 24 arXiv:2311.09869 [hep-th]

  72. [80]

    Massive carrollian fields at timelike infinity,

    E. Have, K. Nguyen, S. Prohazka, and J. Salzer, “Massive carrollian fields at timelike infinity,” JHEP 07 (2024) 054, arXiv:2402.05190 [hep-th]

  73. [81]

    On the definition of Carrollian amplitudes in general dimensions,

    W.-B. Liu, J. Long, H.-Y. Xiao, and J.-L. Yang, “On the definition of Carrollian amplitudes in general dimensions,” JHEP 11 (2024) 027, arXiv:2407.20816 [hep-th]

  74. [82]

    Holographic Carrollian currents for massless scattering,

    R. Ruzziconi and A. Saha, “Holographic Carrollian currents for massless scattering,” JHEP 01 (2025) 169, arXiv:2411.04902 [hep-th]

  75. [83]

    w 1∞ and Carrollian holography,

    A. Saha, “w 1∞ and Carrollian holography,” JHEP 05 (2024) 145, arXiv:2308.03673 [hep-th]

  76. [84]

    Carrollian approach to 1 + 3D flat holography,

    A. Saha, “Carrollian approach to 1 + 3D flat holography,” JHEP 06 (2023) 051, arXiv:2304.02696 [hep-th]

  77. [85]

    BMS-invariant free scalar model,

    P.-x. Hao, W. Song, X. Xie, and Y. Zhong, “BMS-invariant free scalar model,” Phys. Rev. D 105 no. 12, (2022) 125005, arXiv:2111.04701 [hep-th]

  78. [86]

    Quantization of interacting Galilean field theories,

    K. Banerjee and A. Sharma, “Quantization of interacting Galilean field theories,” JHEP 08 (2022) 066, arXiv:2205.01918 [hep-th]

  79. [87]

    Galilean fermions: Classical and quantum aspects,

    A. Sharma, “Galilean fermions: Classical and quantum aspects,” Phys. Rev. D 107 no. 12, (2023) 125009, arXiv:2301.04538 [hep-th]

  80. [88]

    Carroll fermions,

    E. A. Bergshoeff, A. Campoleoni, A. Fontanella, L. Mele, and J. Rosseel, “Carroll fermions,” SciPost Phys. 16 no. 6, (2024) 153, arXiv:2312.00745 [hep-th]

  81. [89]

    M. E. Peskin and D. V. Schroeder, An Introduction to quantum field theory . Addison-Wesley, Reading, USA, 1995

  82. [90]

    Free field realization of the BMS Ising model,

    Z.-f. Yu and B. Chen, “Free field realization of the BMS Ising model,” JHEP 08 (2023) 116, arXiv:2211.06926 [hep-th]

  83. [91]

    BMS-invariant free fermion models,

    P.-X. Hao, W. Song, Z. Xiao, and X. Xie, “BMS-invariant free fermion models,” Phys. Rev. D 109 no. 2, (2024) 025002, arXiv:2211.06927 [hep-th]

  84. [92]

    Carroll fermions in two dimensions,

    A. Banerjee, S. Dutta, and S. Mondal, “Carroll fermions in two dimensions,” Phys. Rev. D 107 no. 12, (2023) 125020, arXiv:2211.11639 [hep-th]

  85. [93]

    M. D. Schwartz, Quantum Field Theory and the Standard Model . Cambridge University Press, 3, 2014

  86. [94]

    Transmission properties of the oscillating δ-function potential,

    D. Martinez and L. Reichl, “Transmission properties of the oscillating δ-function potential,” Physical Review B 64 no. 24, (2001) 245315

  87. [95]

    The Propagators for δ and δ ’ Potentials with Time-Dependent Strengths,

    F. Erman, M. Gadella, and H. Uncu, “The Propagators for δ and δ ’ Potentials with Time-Dependent Strengths,” Frontiers in Physics 8 (Apr., 2020) 65

  88. [96]

    Propagator calculations for time dependent Dirac delta potentials and corresponding two state models,

    S. Mudra and A. Chakraborty, “Propagator calculations for time dependent Dirac delta potentials and corresponding two state models,” Phys. Lett. A 418 (2021) 127725

  89. [97]

    Renormalization group and critical phenomena. 1. Renormalization group and the Kadanoff scaling picture,

    K. G. Wilson, “Renormalization group and critical phenomena. 1. Renormalization group and the Kadanoff scaling picture,” Phys. Rev. B 4 (1971) 3174–3183

  90. [98]

    Renormalization group and critical phenomena. 2. Phase space cell analysis of critical behavior,

    K. G. Wilson, “Renormalization group and critical phenomena. 2. Phase space cell analysis of critical behavior,” Phys. Rev. B 4 (1971) 3184–3205

  91. [99]

    Wilson renormalization group analysis of theories with scalars and fermions,

    T. E. Clark, B. Haeri, and S. T. Love, “Wilson renormalization group analysis of theories with scalars and fermions,” Nucl. Phys. B 402 (1993) 628–656, arXiv:hep-ph/9211261

  92. [100]

    Asymptotic safety of simple Yukawa systems,

    H. Gies and M. M. Scherer, “Asymptotic safety of simple Yukawa systems,” Eur. Phys. J. C 66 (2010) 387–402, arXiv:0901.2459 [hep-th]

  93. [101]

    Fine-tuning and vacuum stability in the Wilsonian effective action,

    T. Krajewski and Z. Lalak, “Fine-tuning and vacuum stability in the Wilsonian effective action,” Phys. Rev. D 92 no. 7, (2015) 075009, arXiv:1411.6435 [hep-ph]

  94. [102]

    Flat Bands and Compact Localised States: A Carrollian roadmap,

    N. Ara, A. Banerjee, R. Basu, and B. Krishnan, “Flat Bands and Compact Localised States: A Carrollian roadmap,” arXiv:2412.18965 [hep-th]

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