REVIEW 3 major objections 4 minor 78 references
Gauge invariance can be relaxed by turning the longitudinal photon into a slow physical mode; the vacuum then absorbs momentum from charges, and xenon recoil searches already bound its speed below 10^-60.
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · deepseek-v4-flash
2026-08-01 00:40 UTC pith:P5H6N7IU
load-bearing objection A genuinely new mechanism with a likely-correct central rate, but the smooth c_L→0 limit and the flagship Xe bound each rest on an input the paper does not fully defend—worth refereeing with those two gaps named. the 3 major comments →
A Material Frame: Hard Recoils from Slow Force Carriers
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The central claim is that gauge invariance is not an exact structural requirement but the zero-speed limit of a stable, predictive theory of a slow longitudinal photon. Starting from the Hamiltonian with (c_L^2/2)(div A)^2, the longitudinal mode has dispersion omega = c_L k and is protected from acquiring a mass by a Galilean higher-form symmetry. Because its interactions are suppressed by c_L, the limit c_L -> 0 recovers QED observables; yet on-shell emission of the mode by a moving charge gives a rate Gamma = 4 alpha c_L (E_p - p^2/(3E_p)) with momentum transfer k of order p, so the recoil is nearly elastic in the preferred frame. Applied to bound states, the momentum transfer is capped by
What carries the argument
The central object is the longitudinal component of the photon, made physical via the Hamiltonian term (c_L^2/2)(div A)^2 in Weyl gauge (A_0 = 0). This single marginal deformation turns the would-be gauge mode into a gapless oscillator with dispersion omega = c_L k; residual Galilean higher-form symmetries protect it from acquiring a mass. A chain of identities carries the argument: integration by parts rewrites the coupling A_L . J as phi_dot J^0, so interactions carry an explicit c_L suppression; dressing charged fields as e^{-ie phi} psi makes that suppression manifest; and a Cherenkov-emission calculation gives the hard-recoil rate. The same machinery guarantees no strong coupling as c_L
Load-bearing premise
The flagship bound depends on the nuclear form factor F at roughly 30 MeV momentum transfer being order one, so that a xenon nucleus really deposits a few keV in a dark-matter detector; if that form factor suppresses the transferred momentum below threshold, the c_L <~ 10^-60 conclusion erodes without touching the point-particle kinematics.
What would settle it
Compute the Cherenkov matrix element for a xenon nucleus moving at beta ~ 10^-3 with a realistic nuclear form factor F(p ~ 30 MeV): if the form factor drives the emitted momentum below the few-keV detection threshold, the predicted recoil signal and therefore the 10^-60 bound disappear. Experimentally, a tonne-scale noble-liquid detector with low threshold and directional sensitivity would see or exclude the predicted few-keV nuclear recoils at the rate Gamma ~ (Z + Z^2 |F|^2) alpha c_L m_p.
If this is right
- If the paper is correct, every charged particle moving relative to the preferred frame is subject to rare, near-elastic momentum kicks, not gradual energy loss.
- Ordinary gauge theory is recovered as the transparent limit of a family of theories with a material preferred frame, so gauge redundancy corresponds to an infrared degeneracy of soft modes.
- The observational hierarchy runs from c_L ~ 10^-7 in precision tests and 10^-23 in cosmic-ray energy loss to 10^-60 in recoil searches, making momentum-sensitive systems the strongest probes.
- At c_L ~ 10^-60, the longitudinal modes are effectively immobile and the only observable role of c_L is as a recoil-rate parameter, so the theory is experimentally equivalent to the Standard Model plus a rigid momentum-absorbing frame.
- Future dark-matter exposures with lower thresholds and larger masses will improve the bound roughly linearly with exposure, continuing to test gauge invariance in this new regime.
Where Pith is reading between the lines
- Read as a template, the construction suggests that any would-be gauge mode could be made weakly physical by giving it a frozen speed, provided residual shift symmetries protect its mass; whether that template survives in non-abelian or gravitational settings, where ghosts may appear, is left open by the paper and is an editor's extension.
- A directional, low-threshold noble-liquid detector could in principle separate these preferred-frame recoils from a dark-matter wind, because the recoil axis would track Earth's motion relative to the cosmic frame rather than the galactic halo; the expected rate at c_L < 10^-60 is extraordinarily small, so this is a long-shot but logically clean test.
- The paper's classical Gauss-law violation produces charge tracks that, once the recoil bound is imposed, are unobservable; in a hypothetical world with larger c_L those tracks would mimic a millicharged background, offering a cross-check if anomalous low-energy events ever appear.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This paper proposes a deformation of QED in which the longitudinal component of the photon becomes a propagating, gapless degree of freedom with speed c_L, implemented by adding (c_L^2/2)(\nabla·A)^2 to the preferred-frame Hamiltonian (Eq. 5). The paper argues that the c_L→0 limit smoothly recovers ordinary gauge theory because all slow-mode interactions can be rewritten in terms of the speed-suppressed operator \dot\phi J^0 (Sec. 3). The main observable signature is Cherenkov emission of these slow modes: the rate is O(α c_L) (Eq. 38), but the momentum transfer remains of order the emitting particle's momentum, producing rare hard recoils. The author derives a hierarchy of constraints, with xenon nuclear-recoil searches giving c_L ≲ 10^{-60} (Eq. 63), and discusses classical Gauss-law violation, shadow charges, and extensions to Yang-Mills, gravity, and cosmology.
Significance. If correct, this is a significant contribution: it gives a controlled, technically natural Lorentz-violating deformation of gauge invariance with no new fields or mass scales, and it identifies a qualitatively new signature—rare hard recoils—that turns dark-matter detectors into probes of whether the vacuum can absorb momentum. The explicit computations of the Cherenkov rate, the ˙ϕ propagator, the tree-level exchange, and the one-loop self-energy are transparent and parameter-free in c_L, and the c_L-dependent power counting is clearly laid out. The 10^{-60} bound is a striking, falsifiable prediction. The main weaknesses are that the smooth decoupling limit is not yet demonstrated by a complete scattering observable, and the flagship bound depends on an unevaluated nuclear form factor.
major comments (3)
- [§3.1–§4.2, Eqs. (25) and (41)] The decoupling limit is not yet demonstrated by a complete scattering observable. The ˙ϕ propagator in Eq. (25) is verified by the direct mode-sum computation in App. B, but the only virtual-exchange amplitude shown, Eq. (41), has a zero-energy limit M ≃ −ie²/Δk² that is independent of c_L. For a system at rest in the preferred frame, the suppression that underpins the decoupling claim is therefore absent; Sec. 4.2 handles this only by a boost/energy estimate. I request one explicit O(e²) S-matrix element, e.g. electron-electron scattering, that includes transverse, longitudinal, and any contact/Coulomb contributions and is shown to reproduce standard QED in both the static and boosted regimes as c_L→0. Every bound in Sec. 5 presupposes this limit.
- [§5.3, Eqs. (62)–(63)] The flagship bound c_L ≲ 10^{-60} uses Γ_Xe ≈ (Z + Z²|F(p)|²) α c_L m_p with |F(p)|² taken to be O(1) at p ≈ 30 MeV, but the form factor is not computed or estimated. Since the rate is linear in this combination, a suppression of |F|² by, say, 10^{-2}–10^{-4} shifts the bound by the same factor, and a stronger suppression could push the recoil below the nuclear-recoil detection threshold, undermining the detection logic. The paper should either evaluate F(p) from a standard nuclear charge distribution or quote Eq. (63) with an explicit dependence on the unknown form factor and an order-of-magnitude error budget, including the coherence assumption pR_B ≈ 1.
- [§4.3, Eq. (46)] The claim that annihilation into slow modes has cross section σ₂ ∼ α²c_L^6 relies on a cancellation in the sum of the two diagrams, reducing the amplitude from αc_L^3 to αc_L^4. The paper states this cancellation without displaying the algebra. This is less central than the two issues above, but since the power-counting section presents Eq. (46) as a check of the general rules, the cancellation should be shown explicitly or relegated to an appendix with a clear statement of the assumptions.
minor comments (4)
- [Eq. (38)] The integration limits are printed as \int_{1}^{c_L E_p/p} d cosθ; as written the interval is empty. From Eq. (35) the range should be c_L E_p/p to 1. Please correct.
- [Eq. (48)] The statement that the imaginary part of the self-energy 'can be verified numerically' to coincide with the Cherenkov rate should be supported by at least a plot or an analytic expression; this is a checkable claim and the paper would be stronger with the verification shown.
- [Table 1] Several bounds in Table 1 are order-of-magnitude estimates built on explicit assumptions (e.g., form factor, boost of the preferred frame, detection efficiency). A column listing the key assumption for each row would prevent the hierarchy from being over-interpreted.
- [General presentation] There are numerous LaTeX spacing artifacts (e.g., 'F ormal', 'c2 L' in places) and inconsistent notation for the scalar potential φ before its definition in Sec. 3.1. A careful proofreading pass is needed.
Circularity Check
No circular derivation; the central chain is self-contained, with one minor non-load-bearing self-citation.
full rationale
The paper's main derivation starts from the deformed Hamiltonian H = ∫[½E² + ½(∇∧A)² + (c_L²/2)(∇·A)²] (Eq. 5), obtains the longitudinal dispersion ω² = c_L²k² (Eq. 9), rewrites the interaction as eγ⁰φ̇ via the dressing Ψ = e^{-ieφ}ψ (Eqs. 27-28), computes the φ̇ propagator with a c_L² numerator (Eq. 25), and derives the Cherenkov rate Γ = 4αc_L(E_p − p²/3E_p) (Eq. 38). The experimental bounds in Sec. 5 then compare this rate to null or observed rates (e.g., Xe recoil null, Eqs. 62-63), with no parameter fitted to the target bound. Thus the signature calculation is not equivalent to its input by construction, and no 'prediction' is a renamed fit. The only author-overlap citation is [34] (Del Grosso, Kaplan, Serra), used for canonical quantization without Dirac brackets and for shadow-charge language (App. A, Sec. 7); this is a technical bookkeeping convenience, not a load-bearing uniqueness theorem nor the source of the c_L predictions. The paper itself flags unresolved items—form-factor evaluation at p ≈ 30 MeV in Sec. 5.3, precise matching of the low-energy EFT in Sec. 4.5, and 'further explor[ation of] the structural aspects of this limit' in Sec. 8. These are correctness/robustness limitations, not circularity. Accordingly the circularity score is low.
Axiom & Free-Parameter Ledger
free parameters (2)
- c_L (slow longitudinal photon speed) =
c_L ≲ 10^-60 (order-of-magnitude upper bound, not a positive fit)
- Nuclear form factor |F(p)|² at p ≈ 30 MeV =
≈ 1 (set to order one, with coherent Z² enhancement)
axioms (4)
- standard math Canonical/Hamiltonian formulation of QED in Weyl gauge with standard equal-time commutation relations (Apps. A, B).
- domain assumption The Galilean higher-form shift symmetries Π^i_1 and Π^{ij}_2 (Eqs. 13-14) are exact symmetries of the quantum theory and protect the photon mass.
- domain assumption Inclusive observables over slow modes have a smooth c_L→0 limit (KLN-type) and Ward identities suppress slow-mode couplings by c_L (Secs. 3.2-3.3, App. C).
- domain assumption The physical preferred frame is (close to) the CMB rest frame, so ground-based detectors move at β ~ 10^-3 relative to it.
invented entities (2)
-
Slow longitudinal photon (physical longitudinal mode, ω = c_L k)
independent evidence
-
Preferred (material) reference frame
independent evidence
read the original abstract
We modify the Standard Model by making the longitudinal component of the photon physical, propagating with small speed $c_L \ll 1$. This modification breaks gauge invariance and Lorentz symmetry, defining a preferred reference frame. No new fields or scales are introduced, and the photon mass is protected by a Galilean higher-form symmetry. The theory has a smooth $c_L\to0$ limit: the new modes decouple from standard matter and ordinary gauge theory predictions are recovered. Experimental constraints are severe. Charged particles Cherenkov-emit these slow modes, experiencing hard recoils against the preferred frame. The recoil rate decreases with $c_L$, but the momentum transfer remains of the order of the particle's momentum. Dark matter detectors, sensitive to keV-scale nuclear recoils, imply an order-of-magnitude bound $c_L \lesssim 10^{-60}$, tens of orders of magnitude stronger than speed-difference bounds. At such values, $c_L$ is better understood as a recoil-rate factor rather than a physically relevant speed. The slow modes, practically fixed in space, make the reference frame a material medium capable of absorbing momentum from charged particles.
Reference graph
Works this paper leans on
-
[1]
T. Jacobson and D. Mattingly,Gravity with a dynamical preferred frame,Phys. Rev. D64(2001) 024028 [gr-qc/0007031]
Pith/arXiv arXiv 2001
-
[2]
N. Arkani-Hamed, H.-C. Cheng, M.A. Luty and S. Mukohyama,Ghost condensation and a consistent infrared modification of gravity,JHEP05(2004) 074 [hep-th/0312099]
Pith/arXiv arXiv 2004
-
[3]
Weinberg,Photons and Gravitons inS-Matrix Theory: Derivation of Charge Conservation and Equality of Gravitational and Inertial Mass,Phys
S. Weinberg,Photons and Gravitons inS-Matrix Theory: Derivation of Charge Conservation and Equality of Gravitational and Inertial Mass,Phys. Rev.135(1964) B1049
1964
-
[4]
Gupta,Theory of longitudinal photons in quantum electrodynamics,Proc
S.N. Gupta,Theory of longitudinal photons in quantum electrodynamics,Proc. Phys. Soc. A63(1950) 681
1950
-
[5]
Bleuler,A New method of treatment of the longitudinal and scalar photons,Helv
K. Bleuler,A New method of treatment of the longitudinal and scalar photons,Helv. Phys. Acta23 (1950) 567
1950
-
[6]
Proca,Sur la theorie ondulatoire des electrons positifs et negatifs,J
A. Proca,Sur la theorie ondulatoire des electrons positifs et negatifs,J. Phys. Radium7(1936) 347
1936
-
[7]
Stueckelberg,Theory of the radiation of photons of small arbitrary mass,Helv
E.C.G. Stueckelberg,Theory of the radiation of photons of small arbitrary mass,Helv. Phys. Acta30 (1957) 209
1957
-
[8]
Llewellyn Smith,High-Energy Behavior and Gauge Symmetry,Phys
C.H. Llewellyn Smith,High-Energy Behavior and Gauge Symmetry,Phys. Lett. B46(1973) 233
1973
-
[9]
Cornwall, D.N
J.M. Cornwall, D.N. Levin and G. Tiktopoulos,Derivation of Gauge Invariance from High-Energy Unitarity Bounds on the s Matrix,Phys. Rev. D10(1974) 1145
1974
-
[10]
G. Gabadadze and L. Grisa,Lorentz-violating massive gauge and gravitational fields,Phys. Lett. B617 (2005) 124 [hep-th/0412332]
Pith/arXiv arXiv 2005
-
[11]
G. Dvali, M. Papucci and M.D. Schwartz,Infrared Lorentz violation and slowly instantaneous electricity,Phys. Rev. Lett.94(2005) 191602 [hep-th/0501157]. 32
Pith/arXiv arXiv 2005
-
[12]
S. Endlich, A. Nicolis, R. Rattazzi and J. Wang,The Quantum mechanics of perfect fluids,JHEP04 (2011) 102 [1011.6396]
Pith/arXiv arXiv 2011
-
[13]
R.C. Myers and M. Pospelov,Ultraviolet modifications of dispersion relations in effective field theory, Phys. Rev. Lett.90(2003) 211601 [hep-ph/0301124]
Pith/arXiv arXiv 2003
-
[14]
J. Collins, A. Perez, D. Sudarsky, L. Urrutia and H. Vucetich,Lorentz invariance and quantum gravity: an additional fine-tuning problem?,Phys. Rev. Lett.93(2004) 191301 [gr-qc/0403053]
Pith/arXiv arXiv 2004
-
[15]
Will and K
C.M. Will and K. Nordtvedt, Jr.,Conservation Laws and Preferred Frames in Relativistic Gravity. I. Preferred-Frame Theories and an Extended PPN Formalism,Astrophys. J.177(1972) 757
1972
-
[16]
C. Csaki, J. Erlich and C. Grojean,Gravitational Lorentz violations and adjustment of the cosmological constant in asymmetrically warped space-times,Nucl. Phys. B604(2001) 312 [hep-th/0012143]
Pith/arXiv arXiv 2001
-
[17]
Gripaios,Modified gravity via spontaneous symmetry breaking,JHEP10(2004) 069 [hep-th/0408127]
B.M. Gripaios,Modified gravity via spontaneous symmetry breaking,JHEP10(2004) 069 [hep-th/0408127]
Pith/arXiv arXiv 2004
-
[18]
T. Jacobson and D. Mattingly,Einstein-Aether waves,Phys. Rev. D70(2004) 024003 [gr-qc/0402005]
Pith/arXiv arXiv 2004
-
[19]
N. Arkani-Hamed, H.-C. Cheng, M. Luty and J. Thaler,Universal dynamics of spontaneous Lorentz violation and a new spin-dependent inverse-square law force,JHEP07(2005) 029 [hep-ph/0407034]
Pith/arXiv arXiv 2005
-
[20]
N. Arkani-Hamed, H.-C. Cheng, M.A. Luty, S. Mukohyama and T. Wiseman,Dynamics of gravity in a Higgs phase,JHEP01(2007) 036 [hep-ph/0507120]
Pith/arXiv arXiv 2007
-
[21]
H.-C. Cheng, M.A. Luty, S. Mukohyama and J. Thaler,Spontaneous Lorentz breaking at high energies, JHEP05(2006) 076 [hep-th/0603010]
Pith/arXiv arXiv 2006
-
[22]
Jacobson,Einstein-aether gravity: A Status report,PoSQG-PH(2007) 020 [0801.1547]
T. Jacobson,Einstein-aether gravity: A Status report,PoSQG-PH(2007) 020 [0801.1547]
Pith/arXiv arXiv 2007
-
[23]
Horava,Quantum Gravity at a Lifshitz Point,Phys
P. Horava,Quantum Gravity at a Lifshitz Point,Phys. Rev. D79(2009) 084008 [0901.3775]
Pith/arXiv arXiv 2009
-
[24]
D. Blas, O. Pujolas and S. Sibiryakov,Consistent Extension of Horava Gravity,Phys. Rev. Lett.104 (2010) 181302 [0909.3525]
Pith/arXiv arXiv 2010
-
[25]
D. Blas, O. Pujolas and S. Sibiryakov,On the Extra Mode and Inconsistency of Horava Gravity,JHEP 10(2009) 029 [0906.3046]
Pith/arXiv arXiv 2009
-
[26]
D. Blas, O. Pujolas and S. Sibiryakov,Models of non-relativistic quantum gravity: The Good, the bad and the healthy,JHEP04(2011) 018 [1007.3503]
Pith/arXiv arXiv 2011
-
[27]
Jacobson,Extended Horava gravity and Einstein-aether theory,Phys
T. Jacobson,Extended Horava gravity and Einstein-aether theory,Phys. Rev. D81(2010) 101502 [1001.4823]
Pith/arXiv arXiv 2010
-
[28]
D. Colladay and V.A. Kostelecky,CPT violation and the standard model,Phys. Rev. D55(1997) 6760 [hep-ph/9703464]
Pith/arXiv arXiv 1997
-
[29]
D. Colladay and V.A. Kostelecky,Lorentz violating extension of the standard model,Phys. Rev. D58 (1998) 116002 [hep-ph/9809521]
Pith/arXiv arXiv 1998
-
[30]
V.A. Kostelecky and M. Mewes,Signals for Lorentz violation in electrodynamics,Phys. Rev. D66 (2002) 056005 [hep-ph/0205211]
Pith/arXiv arXiv 2002
-
[31]
Kostelecky,Gravity, Lorentz violation, and the standard model,Phys
V.A. Kostelecky,Gravity, Lorentz violation, and the standard model,Phys. Rev. D69(2004) 105009 [hep-th/0312310]. 33
Pith/arXiv arXiv 2004
-
[32]
V.A. Kostelecky and N. Russell,Data Tables for Lorentz and CPT Violation,Rev. Mod. Phys.83 (2011) 11 [0801.0287]
arXiv 2011
-
[33]
B. Altschul, Q.G. Bailey and V.A. Kostelecky,Lorentz violation with an antisymmetric tensor,Phys. Rev. D81(2010) 065028 [0912.4852]
Pith/arXiv arXiv 2010
-
[34]
L. Del Grosso, D.E. Kaplan and F. Serra,Shadow sectors of gauge theories,2510.14079
-
[35]
Henneaux and C
M. Henneaux and C. Teitelboim,Quantization of gauge systems(1992)
1992
-
[36]
A. Nicolis, R. Rattazzi and E. Trincherini,The Galileon as a local modification of gravity,Phys. Rev. D 79(2009) 064036 [0811.2197]
Pith/arXiv arXiv 2009
-
[37]
C. Deffayet, S. Deser and G. Esposito-Farese,Arbitraryp-form Galileons,Phys. Rev. D82(2010) 061501 [1007.5278]
Pith/arXiv arXiv 2010
-
[38]
Tasinato,Cosmic Acceleration from Abelian Symmetry Breaking,JHEP04(2014) 067 [1402.6450]
G. Tasinato,Cosmic Acceleration from Abelian Symmetry Breaking,JHEP04(2014) 067 [1402.6450]
Pith/arXiv arXiv 2014
-
[39]
D. Gaiotto, A. Kapustin, N. Seiberg and B. Willett,Generalized Global Symmetries,JHEP02(2015) 172 [1412.5148]
Pith/arXiv arXiv 2015
-
[40]
W.D. Goldberger and P. Tadi´ c,Quantum dynamics of perfect fluids,2512.23793
-
[41]
Lee and M
T.D. Lee and M. Nauenberg,Degenerate Systems and Mass Singularities,Phys. Rev.133(1964) B1549
1964
-
[42]
Kinoshita,Mass singularities of Feynman amplitudes,J
T. Kinoshita,Mass singularities of Feynman amplitudes,J. Math. Phys.3(1962) 650
1962
-
[43]
Kamefuchi, L
S. Kamefuchi, L. O’Raifeartaigh and A. Salam,Change of variables and equivalence theorems in quantum field theories,Nucl. Phys.28(1961) 529
1961
-
[44]
Coleman, J
S.R. Coleman, J. Wess and B. Zumino,Structure of phenomenological Lagrangians. 1.,Phys. Rev.177 (1969) 2239
1969
-
[45]
Callan, Jr., S.R
C.G. Callan, Jr., S.R. Coleman, J. Wess and B. Zumino,Structure of phenomenological Lagrangians. 2., Phys. Rev.177(1969) 2247
1969
-
[46]
Caswell and G.P
W.E. Caswell and G.P. Lepage,Effective Lagrangians for Bound State Problems in QED, QCD, and Other Field Theories,Phys. Lett. B167(1986) 437
1986
-
[47]
A. Pineda and J. Soto,Effective field theory for ultrasoft momenta in NRQCD and NRQED,Nucl. Phys. B Proc. Suppl.64(1998) 428 [hep-ph/9707481]
Pith/arXiv arXiv 1998
-
[48]
Chadha and H.B
S. Chadha and H.B. Nielsen,LORENTZ INV ARIANCE AS A LOW-ENERGY PHENOMENON,Nucl. Phys. B217(1983) 125
1983
-
[49]
G.F. Giudice, M. Raidal and A. Strumia,Lorentz Violation from the Higgs Portal,Phys. Lett. B690 (2010) 272 [1003.2364]. [50]XENONcollaboration,Dark Matter Search Results from a One Ton-Year Exposure of XENON1T, Phys. Rev. Lett.121(2018) 111302 [1805.12562]. [51]XENONcollaboration,Excess electronic recoil events in XENON1T,Phys. Rev. D102(2020) 072004 [200...
Pith/arXiv arXiv 2010
-
[53]
Aoyama et al.,The anomalous magnetic moment of the muon in the Standard Model,Phys
T. Aoyama et al.,The anomalous magnetic moment of the muon in the Standard Model,Phys. Rept. 887(2020) 1 [2006.04822]. 34 [54]Muon g-2collaboration,Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm,Phys. Rev. Lett.126(2021) 141801 [2104.03281]. [55]Muon g-2collaboration,Measurement of the Positive Muon Anomalous Magnetic Moment to 127...
Pith/arXiv arXiv 2020
-
[56]
Parker, C
R.H. Parker, C. Yu, W. Zhong, B. Estey and H. M¨ uller,Measurement of the fine-structure constant as a test of the standard model,Science360(2018) 191
2018
-
[57]
L. Morel, Z. Yao, P. Clad´ e and S. Guellati-Kh´ elifa,Determination of the fine-structure constant with an accuracy of 81 parts per trillion,Nature588(2020) 61. [58]Pierre Augercollaboration,Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above8×10 18 eV,Science357(2017) 1266 [1709.07321]
Pith/arXiv arXiv 2020
-
[59]
Anchordoqui,Ultra-High-Energy Cosmic Rays,Phys
L.A. Anchordoqui,Ultra-High-Energy Cosmic Rays,Phys. Rept.801(2019) 1 [1807.09645]
Pith/arXiv arXiv 2019
-
[60]
Greisen,End to the cosmic ray spectrum?,Phys
K. Greisen,End to the cosmic ray spectrum?,Phys. Rev. Lett.16(1966) 748
1966
-
[61]
Zatsepin and V.A
G.T. Zatsepin and V.A. Kuzmin,Upper limit of the spectrum of cosmic rays,JETP Lett.4(1966) 78
1966
-
[62]
S.R. Coleman and S.L. Glashow,High-energy tests of Lorentz invariance,Phys. Rev. D59(1999) 116008 [hep-ph/9812418]
Pith/arXiv arXiv 1999
-
[63]
S.R. Coleman and S.L. Glashow,Cosmic ray and neutrino tests of special relativity,Phys. Lett. B405 (1997) 249 [hep-ph/9703240]. [64]LHC Design Report Vol.1: The LHC Main Ring, Tech. Rep. (6, 2004), DOI
Pith/arXiv arXiv 1997
-
[65]
Holzer et al.,Beam loss monitoring system for the LHC, in2005 IEEE Nuclear Science Symposium and Medical Imaging Conference, no
E.B. Holzer et al.,Beam loss monitoring system for the LHC, in2005 IEEE Nuclear Science Symposium and Medical Imaging Conference, no. 2, pp. 1052–1056, 2005, DOI. [66]Particle Data Groupcollaboration,Review of particle physics,Phys. Rev. D110(2024) 030001. [67]ATLAScollaboration,Technical Design Report for the ATLAS Inner Tracker Pixel Detector, Tech. Rep...
2005
-
[68]
Lorimer,Binary and Millisecond Pulsars,Living Rev
D.R. Lorimer,Binary and Millisecond Pulsars,Living Rev. Rel.11(2008) 8 [0811.0762]
Pith/arXiv arXiv 2008
-
[69]
G.D. Mack, J.F. Beacom and G. Bertone,Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth’s Heat Flow,Phys. Rev. D76(2007) 043523 [0705.4298]
Pith/arXiv arXiv 2007
-
[70]
Beardsmore and J.P
G.R. Beardsmore and J.P. Cull,Crustal Heat Flow. A Guide to Measurement and Modelling., Cambridge University Press, New York(2001)
2001
-
[71]
I.P. Lopes, G. Bertone and J. Silk,Solar seismic model as a new constraint on supersymmetric dark matter,Mon. Not. Roy. Astron. Soc.337(2002) 1179 [astro-ph/0205066]
Pith/arXiv arXiv 2002
-
[72]
G. Bertone and M. Fairbairn,Compact Stars as Dark Matter Probes,Phys. Rev. D77(2008) 043515 [0709.1485]
Pith/arXiv arXiv 2008
-
[73]
A. Prˇ sa, P. Harmanec, G. Torres, E. Mamajek, M. Asplund, N. Capitaine et al.,Nominal values for selected solar and planetary quantities: Iau 2015 resolution b3,The Astronomical Journal152(2016) 41. [74]DarkSide-20kcollaboration,DarkSide-20k: A 20 tonne two-phase LAr TPC for direct dark matter detection at LNGS,Eur. Phys. J. Plus133(2018) 131 [1707.08145...
Pith/arXiv arXiv 2015
-
[78]
R. Essig, J. Mardon and T. Volansky,Direct Detection of Sub-GeV Dark Matter,Phys. Rev. D85 (2012) 076007 [1108.5383]
Pith/arXiv arXiv 2012
-
[79]
D.C. Moore, A.D. Rider and G. Gratta,Search for Millicharged Particles Using Optically Levitated Microspheres,Phys. Rev. Lett.113(2014) 251801 [1408.4396]
Pith/arXiv arXiv 2014
-
[80]
G. Magill, R. Plestid, M. Pospelov and Y.-D. Tsai,Millicharged particles in neutrino experiments, Phys. Rev. Lett.122(2019) 071801 [1806.03310]. [81]ArgoNeuTcollaboration,Improved Limits on Millicharged Particles Using the ArgoNeuT Experiment at Fermilab,Phys. Rev. Lett.124(2020) 131801 [1911.07996]
Pith/arXiv arXiv 2019
-
[82]
M. Pospelov and H. Ramani,Earth-bound millicharge relics,Phys. Rev. D103(2021) 115031 [2012.03957]
Pith/arXiv arXiv 2021
-
[83]
D. Budker, P.W. Graham, H. Ramani, F. Schmidt-Kaler, C. Smorra and S. Ulmer,Millicharged Dark Matter Detection with Ion Traps,PRX Quantum3(2022) 010330 [2108.05283]
Pith/arXiv arXiv 2022
-
[84]
C.A. Arg¨ uelles Delgado, K.J. Kelly and V. Mu˜ noz Albornoz,Millicharged particles from the heavens: single- and multiple-scattering signatures,JHEP11(2021) 099 [2104.13924]
Pith/arXiv arXiv 2021
-
[85]
D. Carney, H. H¨ affner, D.C. Moore and J.M. Taylor,Trapped Electrons and Ions as Particle Detectors, Phys. Rev. Lett.127(2021) 061804 [2104.05737]
Pith/arXiv arXiv 2021
-
[86]
E. Iles, S. Heeba and K. Schutz,Dark Matter Direct Detection Experiments Are Sensitive to the Millicharged Background,Phys. Rev. Lett.134(2025) 121002 [2407.21096]
Pith/arXiv arXiv 2025
- [87]
-
[88]
D.E. Kaplan, T. Melia and S. Rajendran,The Classical Equations of Motion of Quantized Gauge Theories, Part 2: Electromagnetism,2307.09475
-
[89]
Isham,Canonical quantum gravity and the problem of time,NATO Sci
C.J. Isham,Canonical quantum gravity and the problem of time,NATO Sci. Ser. C409(1993) 157 [gr-qc/9210011]
Pith/arXiv arXiv 1993
-
[90]
D.E. Kaplan, T. Melia and S. Rajendran,The Classical Equations of Motion of Quantized Gauge Theories, Part I: General Relativity,2305.01798
-
[91]
L. Del Grosso, D.E. Kaplan, T. Melia, V. Poulin, S. Rajendran and T.L. Smith,Cosmological Consequences of Unconstrained Gravity and Electromagnetism,2405.06374
-
[92]
Kulish and L.D
P.P. Kulish and L.D. Faddeev,Asymptotic conditions and infrared divergences in quantum electrodynamics,Theor. Math. Phys.4(1970) 745. 36
1970
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.