REVIEW 3 major objections 4 minor 90 references
The bremsstrahlung-like production of the massive spin-2 dark matter mediator
T0 review · 3 major / 4 minor · reviewed 2026-08-11 · deepseek-v4-flash
Pith's one-line read The E137 beam-dump experiment rules out a massive spin-2 dark-matter mediator that couples to photons and electrons, for mediator masses between 100 MeV and 800 MeV and couplings in the range $8\times10^{-8}$ to $10^{-5}$ GeV$^{-1}$.
desk verdict Useful WW/ETL comparison for spin-2 mediators, but the E137 exclusion band is built on a photon width that looks 36x too small. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central object is the massive spin-2 mediator field $G_{\mu\nu}$ coupled to Standard Model fields through their energy-momentum tensors, with coupling constants $c_i^G$ of dimension GeV$^{-1}$. The calculation that carries the argument is the bremsstrahlung-like production process $lN\to lNG$, evaluated either by the exact tree-level matrix element or by the Weizsacker-Williams approximation that reduces it to a Compton-like $l\gamma^*\to lG$ subprocess with a virtual photon flux. The signal estimate then uses the decay lengths of the mediator in the lab frame, $l_G = (E_G/m_G)(1/\Gamma_{\rm tot}^G)$, together with the thick-target formula, to count how many produced mediators survive through the shielding and decay inside the E137 fiducial volume; the Tsai-Schiff nuclear form factor is used throughout for the target.
What would settle it
Recompute the E137 visible-decay signal by weighting every produced mediator with its actual energy fraction $x=E_G/E_e$ drawn from the exact tree-level differential cross section $d\sigma/dx$, and integrate the survival probability $e^{-L_{\rm sh}/l_G(E_G)}-e^{-L_{\rm tot}/l_G(E_G)}$ over $x$ from $0.1$ to $1$; if the resulting 90% confidence excluded band shifts noticeably from $8\times10^{-8}\,\mathrm{GeV}^{-1}\lesssim c_{ee}^G\lesssim10^{-5}\,\mathrm{GeV}^{-1}$, the central claim as stated would not hold at that precision.
Extended reading notes
Core claim
The paper establishes that the E137 null result excludes the simplified massive spin-2 mediator scenario with universal couplings to electrons and photons, $c_{ee}^G = c_{\gamma\gamma}^G$, over a specific coupling-mass band. The exclusion is derived by computing the number of visible decays $G\to\gamma\gamma$ and $G\to e^+e^-$ expected from bremsstrahlung-like production of the mediator, using both the exact tree-level cross section and the Weizsacker-Williams approximation, and comparing with the observed zero events under a 90% confidence level Poisson assumption. As a supporting technical claim, the paper shows that the Weizsacker-Williams and exact tree-level total cross sections agree at the $O(1)$ percent level for mediator masses $m_G\gtrsim200$ MeV across the fixed-target experiments considered, while discrepancies above 50% appear for light mediators below about 100 MeV because the exact amplitude contains terms that grow as $1/m_G^2$ and $1/m_G^4$.
Load-bearing premise
The signal estimate assumes that the produced mediator carries essentially all of the beam energy when computing its decay length, even though the production cross section is integrated over mediator energy fractions down to $x_{\rm cut}=0.1$; if a significant fraction of events have much lower mediator energy, the decay-length averaging changes and the excluded coupling band shifts.
Editorial extensions
If this is right
- The E137 experiment excludes spin-2 mediator couplings $8\times10^{-8}\lesssim c_{ee}^G\lesssim10^{-5}$ GeV$^{-1}$ for masses $100\,\mathrm{MeV}\lesssim m_G\lesssim800\,\mathrm{MeV}$, assuming universal couplings to electrons and photons and visible decays.
- The Weizsacker-Williams approximation is reliable at the percent level for mediator masses above roughly 200 MeV, so it can be used for future sensitivity projections in this mass range.
- For mediator masses below about 100 MeV the Weizsacker-Williams approximation disagrees with the exact tree-level result by more than 50% and should not be trusted there.
- The projected visible-mode sensitivity of LDMX with $10^{15}$ electrons on target is already covered by the BaBar mono-photon constraint for $m_G\lesssim7$ GeV and $c_{ee}^G\lesssim3\times10^{-5}$ GeV.
- The E137 exclusion also rules out a vector dark-matter benchmark with $m_V\simeq300$ MeV for couplings around $10^{-7}\lesssim c_{ee}^G\lesssim3\times10^{-6}$ GeV$^{-1}$.
Reading between the lines
- Because the decay-length averaging in the signal formula assumes the mediator carries essentially all of the beam energy ($E_e\simeq E_G$) while the production cross section is integrated down to $x_{\rm cut}=0.1$, the lower boundary of the excluded coupling band could shift once the actual energy distribution is folded in; a re-analysis with energy-weighted decay probabilities would sharpen the b
- The same exact tree-level machinery can be applied to the muon-beam experiments NA64$\mu$ and M3 in visible mode, which would produce analogous exclusions on a muonphilic spin-2 mediator coupling $c_{\mu\mu}^G$.
- The good Weizsacker-Williams and exact tree-level agreement for heavy mediators means future high-statistics fixed-target searches can use the cheaper Weizsacker-Williams cross section in Monte Carlo generators without introducing percent-level bias.
- Combining the E137 exclusion with relic-density curves for vector dark matter leaves a narrower surviving parameter window, and the paper's result removes one of the few remaining sub-GeV spin-2 thermal targets.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper studies bremsstrahlung-like production of a massive spin-2 mediator in lepton fixed-target experiments, comparing the Weizsäcker-Williams (WW) approximation with an exact tree-level (ETL) calculation, and then uses the E137 null result to derive a 90% C.L. exclusion band for the mediator coupling to electrons and photons. The central quantitative claim is that E137 excludes 8×10^-8 GeV^-1 ≲ c_ee^G ≲ 10^-5 GeV^-1 for mediator masses 100 MeV ≲ m_G ≲ 800 MeV under the assumption c_ee^G = c_γγ^G. The paper also gives a brief comparison with the LDMX reach and with BaBar constraints.
Significance. If the central calculation is correct, the paper provides a new and useful exclusion for a simplified massive spin-2 mediator scenario, and the WW/ETL comparison for masses above roughly 200 MeV is a valuable cross-check for future fixed-target proposals. The E137 bound is an external null-result recast rather than a fit, so the circularity burden is low. The paper is also notable for giving explicit analytic expressions for the ETL amplitude squared and for the spin-2 vertices. However, the numerical E137 exclusion range is not robust until the photon decay width and the energy-spectrum treatment are corrected and quantified.
major comments (3)
- [Eq. (32) and following paragraph] The decay width for G→γγ is given in Eq. (32) as Γ_{G→γγ} = (1/3) c² m_G³/(960π) = c² m_G³/(2880π). For the same Fierz-Pauli coupling to the photon energy-momentum tensor, the standard result is Γ_{G→γγ} = c² m_G³/(80π), a factor of 36 larger. This is not merely a convention issue: the numerical estimate for l_{G→γγ} stated in the text, 4.5×10^5 cm at E_G=10 GeV, m_G=100 MeV, and c=10^-6 GeV^-1, is consistent with the standard width and not with Eq. (32). Since l_G enters the decay-probability factor in Eq. (33) exponentially, the E137 exclusion band in Fig. 5 and the quoted range in the abstract must be re-evaluated; with c_ee=c_γγ the total width increases by a factor ≈54/19≈2.84, shifting the lower edge by about (54/19)^{1/4} and the upper edge by a comparable factor. The authors should correct Eq. (32) and recompute the limits.
- [Sec. V.B, Eq. (33)] The signal estimate in Eq. (33) assumes that the mediator carries essentially all of the beam energy, E_e ≈ E_G, when computing the decay probability, while the production cross section σ_tot is integrated over energy fractions x down to x_cut=0.1 for E137 (Table I). Because l_G is proportional to E_G, events with x≪1 have considerably shorter decay lengths, and the exponential factor in Eq. (33) is not correctly averaged over the production spectrum. The paper provides no quantification of the resulting shift in the exclusion band. The authors should either weight the decay probability over the ETL/WW differential cross section in x or justify explicitly that the spectrum is so sharply peaked near x≈1 that the approximation is accurate for the quoted bounds.
- [Appendix B, Eq. (B1)] The ETL amplitude squared |A^G_{2→3}|² in Eq. (B1), with the coefficients in Eqs. (B3)–(B17), is central to both the WW/ETL comparison and the E137 limit, but it is presented without derivation and without an accompanying code or ancillary file. A reader cannot independently verify the expression, and the paper does not state which computer-algebra tool or method was used to obtain it. The authors should provide the derivation or a machine-readable ancillary file, and ideally a numerical cross-check against an independent evaluation at a representative phase-space point.
minor comments (4)
- [Abstract vs. Conclusion] The abstract states the lower edge of the excluded coupling range as 8×10^-8 GeV^-1, while the conclusion states 10^-7 GeV^-1. This numerical discrepancy should be resolved, especially after the width correction is applied.
- [Sec. IV A] The text refers to the small-mass regime as m_G ≲ 100 GeV; from context this should be 100 MeV.
- [Throughout] There are several typographical and grammatical errors, e.g., 'has been ruled out the the couplings' in the abstract and 'the E137 experiment has been ruled out the the parameter space' in Sec. V C. These should be corrected in a revision.
- [Eq. (29) and Sec. V B] The production estimate N^{brem}_G uses a single target radiation length for E137, but the shielding and detector geometry are described only in words; it would be clearer to state explicitly that L_T^{E137}=X_0 and to define all lengths in one place.
Circularity Check
No significant circularity: the E137 exclusion is an external null-result recast, and the central bound is computed from the paper's own ETL matrix element rather than from fitted inputs.
full rationale
The paper's central claim is the E137 exclusion range 8e-8 GeV^-1 <= c_ee <= 1e-5 GeV^-1 for 100 MeV <= mG <= 800 MeV. This is derived through Eq. (33), which combines the production yield Eq. (29) with the decay-probability factor (e^{-L_sh/l_G} - e^{-L_tot/l_G}). The inputs are the E137 null result (Ref. [83]), the fixed geometry parameters in Eq. (35), and the model decay widths in Eqs. (31)-(32). None of these quantities is fitted to make the claimed excluded range emerge; the range is the solution of N_vis^G >= 2.3 under Poisson statistics. The self-citations to Refs. [44,49,82] supply the WW amplitude and form-factor discussion, but the E137 reach shown in Fig. 5 is computed using the ETL cross section derived in this paper via Eq. (21) and Appendix B, so the central constraint does not reduce to a self-citation chain. The kinematic approximation Ee ~ EG stated in Eq. (33), while potentially shifting the bound numerically, is an assumption rather than a definitional identity with the output. Likewise, the possible factor-of-36 issue in Eq. (32) noted by a skeptic, if correct, would be an external consistency error in the width, not a circularity: the prediction is not equivalent to its input by construction. Overall, the derivation is a self-contained recast of an external experimental null result, with only minor, non-load-bearing self-citations.
Assumptions & free parameters
free parameters (1)
- theta_max =
0.1 rad
assumptions (6)
- domain assumption The spin-2 mediator is described by linearized Fierz-Pauli theory with polarization sum Eq. (A4) and propagator Eq. (A5).
- domain assumption The mediator couples universally to the SM energy-momentum tensor, Eq. (1), with c_ee = c_γγ for the visible decay scenario.
- domain assumption The nuclear current is approximated by a spin-0 form factor with Tsai-Schiff parametrization, Eqs. (13) and (14).
- domain assumption E137 is treated as a background-free experiment, so a null result gives a 90% C.L. upper limit of N = 2.3 signal events (Sec. V C).
- ad hoc to paper The mediator is produced within the first radiation length and carries the full beam energy when computing decay probabilities, Eqs. (29) and (33).
- domain assumption Secondary positron production and mediator absorption in the target are neglected.
invented entities (1)
-
Massive spin-2 mediator G
independent evidence
Cite this review
Pith. "Pith review of The bremsstrahlung-like production of the massive spin-2 dark matter mediator." pith.science (2026). https://pith.science/paper/2MSO6HHT
@misc{pith2026241210150,
author = {Pith},
title = {Pith review of: The bremsstrahlung-like production of the massive spin-2 dark matter mediator},
year = {2026},
howpublished = {\url{https://pith.science/paper/2MSO6HHT}},
note = {Machine review of arXiv:2412.10150}
}
abstract
The link between Standard Model (SM) particles and dark matter (DM) can be introduced via spin-2 massive mediator, G, that couples to photon and charged leptons. Moreover, in a mediator mass range from sub-MeV to sub-GeV, fixed-target facilities such as NA64e, LDMX, NA64$\mu$, M$^3$, and E137, can potentially probe such particle of the hidden sector via the signatures that are described by the bremsstrahlung-like process involving tensor mediator. We compare numerically the Weizsaker-Williams (WW) approximation and the exact tree-level (ETL) approach for the bremsstrahlung-like mediator production cross section by choosing various parameters of the fixed-target experiments. In addition, we derive novel constraints on spin-2 DM mediator parameter space from the data of the E137 fixed-target experiment. In particular, we demonstrate that the E137 experiment has been ruled out the the couplings of the spin-2 mediator at the level of $8\times10^{-8}~\mbox{GeV}^{-1}~\lesssim~c^{\rm G}_{ee}~\lesssim~10^{-5}~\mbox{GeV}^{-1}$ for the typical masses in the range $100~\mbox{MeV}~\lesssim~m_{\rm G}~\lesssim 800~\mbox{MeV}$, that corresponds to the statistics of $1.87\times 10^{20}$ electrons accumulated on target. The latter implies its universal coupling to photons and leptons, $c^{\rm G}_{ee} = c^{\rm G}_{\gamma \gamma}$.
Figures
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Reference graph
Works this paper leans on
-
[1]
L. Bergstrom, Annalen Phys. 524, 479 (2012), arXiv:1205.4882 [astro-ph.HE]
arXiv 2012
-
[2]
G. Bertone and D. Hooper, Rev. Mod. Phys.90, 045002 (2018), arXiv:1605.04909 [astro-ph.CO]
arXiv 2018
- [3]
-
[4]
G. Bertone, D. Hooper, and J. Silk, Phys. Rept.405, 279 (2005), arXiv:hep-ph/0404175
arXiv 2005
-
[5]
G. B. Gelmini, in Theoretical Advanced Study Institute in Elementary Particle Physics: Journeys Through the Precision Frontier: Amplitudes for Colliders (2015) pp. 559–616, arXiv:1502.01320 [hep-ph]
arXiv 2015
- [6]
-
[7]
Davis, G
M. Davis, G. Efstathiou, C. S. Frenk, and S. D. M. White, Astrophys. J.292, 371 (1985)
1985
-
[8]
P. A. R. Ade et al. (Planck), Astron. Astrophys. 594, A13 (2016), arXiv:1502.01589 [astro-ph.CO]
arXiv 2016
Show all 90 references
-
[9]
Aghanimet al
N. Aghanimet al. (Planck), Astron. Astrophys.641, A6 (2020), [Erratum: Astron.Astrophys. 652, C4 (2021)], arXiv:1807.06209 [astro-ph.CO]
2020 arXiv
-
[10]
B. W. Lee and S. Weinberg, Phys. Rev. Lett.39, 165 (1977)
1977
-
[11]
E. W. Kolb and K. A. Olive, Phys. Rev. D 33, 1202 (1986)
1986
- [12]
-
[13]
McDonald, Phys
J. McDonald, Phys. Rev. D50, 3637 (1994), arXiv:hep- ph/0702143
1994
-
[14]
C. P. Burgess, M. Pospelov, and T. ter Veldhuis, Nucl. Phys. B619, 709 (2001), arXiv:hep-ph/0011335
2001 arXiv
-
[15]
J. D. Wells, , 283 (2008), arXiv:0803.1243 [hep-ph]
2008 arXiv
-
[16]
R. M. Schabinger and J. D. Wells, Phys. Rev. D 72, 093007 (2005), arXiv:hep-ph/0509209
2005 arXiv
-
[17]
Bickendorf and M
G. Bickendorf and M. Drees, Eur. Phys. J. C82, 1163 (2022), arXiv:2206.05038 [hep-ph]
2022 arXiv
-
[18]
E. E. Boos, V. E. Bunichev, and S. S. Trykov, Phys. Rev. D107, 075021 (2023), arXiv:2205.07364 [hep-ph]
2023 arXiv
-
[19]
Sieber, D
H. Sieber, D. V. Kirpichnikov, I. V. Voronchikhin, P. Crivelli, S. N. Gninenko, M. M. Kirsanov, N. V. Kras- nikov, L. Molina-Bueno, and S. K. Sekatskii, Phys. Rev. D 108, 056018 (2023), arXiv:2305.09015 [hep-ph]
2023 arXiv
- [20]
-
[21]
Holdom, Phys
B. Holdom, Phys. Lett. B166, 196 (1986)
1986
-
[22]
Izaguirre, G
E. Izaguirre, G. Krnjaic, P. Schuster, and N. Toro, Phys. Rev. Lett. 115, 251301 (2015), arXiv:1505.00011 [hep- ph]
2015 arXiv
-
[23]
Essig, P
R. Essig, P. Schuster, N. Toro, and B. Wojtsekhowski, JHEP 02, 009 (2011), arXiv:1001.2557 [hep-ph]
2011 arXiv
-
[24]
Y. Kahn, G. Krnjaic, J. Thaler, and M. Toups, Phys. Rev. D91, 055006 (2015), arXiv:1411.1055 [hep-ph]
2015 arXiv
-
[25]
Batell, R
B. Batell, R. Essig, and Z. Surujon, Phys. Rev. Lett. 113, 171802 (2014), arXiv:1406.2698 [hep-ph]
2014 arXiv
-
[26]
Izaguirre, G
E. Izaguirre, G. Krnjaic, P. Schuster, and N. Toro, Phys. Rev. D88, 114015 (2013), arXiv:1307.6554 [hep-ph]
2013 arXiv
-
[27]
Kachanovich, S
A. Kachanovich, S. Kovalenko, S. Kuleshov, V. E. Lyubovitskij, and A. S. Zhevlakov, Phys. Rev. D105, 075004 (2022), arXiv:2111.12522 [hep-ph]
2022 arXiv
-
[28]
V. E. Lyubovitskij, A. S. Zhevlakov, A. Kachanovich, and S. Kuleshov, Phys. Rev. D 107, 055006 (2023), arXiv:2210.05555 [hep-ph]
2023 arXiv
-
[29]
Gorbunov and D
D. Gorbunov and D. Kalashnikov, Phys. Rev. D107, 015014 (2023), arXiv:2211.06270 [hep-ph]
2023 arXiv
-
[30]
Claude, M
J. Claude, M. Dutra, and S. Godfrey, Phys. Rev. D107, 075006 (2023), arXiv:2208.09422 [hep-ph]
2023 arXiv
-
[31]
Wang, W.-L
W. Wang, W.-L. Xu, J. M. Yang, and R. Zhu, Nucl. Phys. B995, 116348 (2023), arXiv:2305.12668 [hep-ph]
2023 arXiv
-
[32]
H. M. Lee, M. Park, and V. Sanz, Eur. Phys. J. C74, 2715 (2014), arXiv:1306.4107 [hep-ph]
2014 arXiv
-
[33]
Y.-J.KangandH.M.Lee,Eur.Phys.J.C 80,602(2020), arXiv:2001.04868 [hep-ph]
2020 arXiv
-
[34]
Bernal, M
N. Bernal, M. Dutra, Y. Mambrini, K. Olive, M. Peloso, and M. Pierre, Phys. Rev. D 97, 115020 (2018), arXiv:1803.01866 [hep-ph]
2018 arXiv
-
[35]
M. G. Folgado, A. Donini, and N. Rius, JHEP04, 036 (2020), arXiv:1912.02689 [hep-ph]
2020 arXiv
-
[36]
Y.-J.KangandH.M.Lee,Eur.Phys.J.C 81,868(2021), arXiv:2002.12779 [hep-ph]
2021 arXiv
-
[37]
Dutra, PoS LeptonPhoton2019, 076 (2019), arXiv:1911.11844 [hep-ph]
M. Dutra, PoS LeptonPhoton2019, 076 (2019), arXiv:1911.11844 [hep-ph]
2019 arXiv
-
[38]
Clery, Y
S. Clery, Y. Mambrini, K. A. Olive, A. Shkerin, and S. Verner, Phys. Rev. D 105, 095042 (2022), arXiv:2203.02004 [hep-ph]
2022 arXiv
-
[39]
J. A. Gill, D. Sengupta, and A. G. Williams, Phys. Rev. D 108, L051702 (2023), arXiv:2303.04329 [hep-ph]
2023 arXiv
-
[40]
W. Wang, L. Wu, J. M. Yang, H. Zhou, and B. Zhu, JHEP 12, 072 (2020), [Erratum: JHEP 02, 052 (2021)], arXiv:1912.09904 [hep-ph]
2020 arXiv
- [41]
- [42]
-
[43]
Jod lowski, Phys
K. Jod lowski, Phys. Rev. D 108, 115017 (2023), arXiv:2305.05710 [hep-ph]
2023 arXiv
-
[44]
I. V. Voronchikhin and D. V. Kirpichnikov, Phys. Rev. D 106, 115041 (2022), arXiv:2210.00751 [hep-ph]
2022 arXiv
-
[45]
S. N. Gninenko, D. V. Kirpichnikov, M. M. Kirsanov, and N. V. Krasnikov, Phys. Lett. B 782, 406 (2018), arXiv:1712.05706 [hep-ph]
2018 arXiv
-
[46]
Y.-S. Liu, D. McKeen, and G. A. Miller, Phys. Rev. D 95, 036010 (2017), arXiv:1609.06781 [hep-ph]
2017 arXiv
-
[47]
Liu and G
Y.-S. Liu and G. A. Miller, Phys. Rev. D96, 016004 (2017), arXiv:1705.01633 [hep-ph]
2017 arXiv
-
[48]
D. V. Kirpichnikov, H. Sieber, L. M. Bueno, P. Crivelli, and M. M. Kirsanov, Phys. Rev. D104, 076012 (2021), arXiv:2107.13297 [hep-ph]
2021 arXiv
-
[49]
I. V. Voronchikhin and D. V. Kirpichnikov, (2024), arXiv:2409.12748 [hep-ph]
2024 arXiv
-
[50]
Fermi, Nuovo Cim
E. Fermi, Nuovo Cim. 2, 143 (1925), arXiv:hep- th/0205086
1925
-
[51]
C. F. von Weizsacker, Z. Phys.88, 612 (1934)
1934
-
[52]
E. J. Williams, Kong. Dan. Vid. Sel. Mat. Fys. Med. 13N4, 1 (1935)
1935
-
[53]
V. M. Budnev, I. F. Ginzburg, G. V. Meledin, and V. G. Serbo, Phys. Rept.15, 181 (1975)
1975
-
[54]
Bl¨ umlein and J
J. Bl¨ umlein and J. Brunner, Phys. Lett. B731, 320 (2014), arXiv:1311.3870 [hep-ph]
2014 arXiv
-
[55]
Foroughi-Abari and A
S. Foroughi-Abari and A. Ritz, Phys. Rev. D105, 095045 (2022), arXiv:2108.05900 [hep-ph]
2022 arXiv
-
[56]
Foroughi-Abari, P
S. Foroughi-Abari, P. Reimitz, and A. Ritz, (2024), arXiv:2409.09123 [hep-ph]. 12
2024 arXiv
-
[57]
Gorbunov and E
D. Gorbunov and E. Kriukova, JHEP01, 058 (2024), arXiv:2306.15800 [hep-ph]
2024 arXiv
-
[58]
Harland-Lang, J
L. Harland-Lang, J. Jaeckel, and M. Spannowsky, Phys. Lett. B793, 281 (2019), arXiv:1902.04878 [hep-ph]
2019 arXiv
- [59]
- [60]
-
[61]
d’Enterria, M
D. d’Enterria, M. A. Tamlihat, L. Schoeffel, H.-S. Shao, and Y. Tayalati, Phys. Lett. B 846, 138237 (2023), arXiv:2306.15558 [hep-ph]
2023 arXiv
-
[62]
H. M. Lee, M. Park, and V. Sanz, (2024), arXiv:2412.07850 [hep-ph]
2024 arXiv
-
[63]
M. G. Folgado, A. Donini, and N. Rius, (2019), 10.1007/JHEP01(2020)161, arXiv:1907.04340 [hep-ph]
2019 arXiv
-
[64]
Banerjee et al
D. Banerjee et al. (NA64), Phys. Rev. D 97, 072002 (2018), arXiv:1710.00971 [hep-ex]
2018 arXiv
-
[65]
Y. M. Andreev et al. (NA64), Phys. Rev. Lett. 132, 211803 (2024), arXiv:2401.01708 [hep-ex]
2024 arXiv
-
[66]
Mans (LDMX), EPJ Web Conf.142, 01020 (2017)
J. Mans (LDMX), EPJ Web Conf.142, 01020 (2017)
2017
- [67]
- [68]
-
[69]
M. D. Schwartz,Quantum Field Theory and the Standard Model (Cambridge University Press, 2014)
2014
-
[70]
S. D. Drell and J. D. Walecka, Annals Phys. 28, 18 (1964)
1964
-
[71]
V. B. Berestetskii, E. M. Lifshitz, and L. P. Pitaevskii, QUANTUM ELECTRODYNAMICS, Course of Theoret- ical Physics, Vol. 4 (Pergamon Press, Oxford, 1982)
1982
-
[72]
Beranek, H
T. Beranek, H. Merkel, and M. Vanderhaeghen, Phys. Rev. D88, 015032 (2013), arXiv:1303.2540 [hep-ph]
2013 arXiv
-
[73]
C. F. Perdrisat, V. Punjabi, and M. Vanderhaeghen, Prog. Part. Nucl. Phys. 59, 694 (2007), arXiv:hep- ph/0612014
2007
-
[74]
J. D. Bjorken, R. Essig, P. Schuster, and N. Toro, Phys. Rev. D80, 075018 (2009), arXiv:0906.0580
2009 arXiv
-
[75]
Tsai, Rev
Y.-S. Tsai, Rev. Mod. Phys.46, 815 (1974)
1974
-
[76]
L. I. Schiff, Phys. Rev. 92, 988 (1953), [Erratum: Phys.Rev. 93, 1434–1434 (1954)]
1953
-
[77]
K. J. Kim and Y.-S. Tsai, Phys. Rev. D8, 3109 (1973)
1973
-
[78]
C.-Y. Chen, M. Pospelov, and Y.-M. Zhong, Phys. Rev. D 95, 115005 (2017), arXiv:1701.07437 [hep-ph]
2017 arXiv
-
[79]
Y. Kahn, G. Krnjaic, N. Tran, and A. Whitbeck, JHEP 09, 153 (2018), arXiv:1804.03144 [hep-ph]
2018 arXiv
-
[80]
Bondi, A
M. Bondi, A. Celentano, R. R. Dusaev, D. V. Kirpich- nikov, M. M. Kirsanov, N. V. Krasnikov, L. Marsicano, and D. Shchukin, Comput. Phys. Commun.269, 108129 (2021), arXiv:2101.12192 [hep-ph]
2021 arXiv
-
[81]
B. B. Oberhauseret al., Comput. Phys. Commun.300, 109199 (2024), arXiv:2401.12573 [hep-ph]
2024 arXiv
-
[82]
I. V. Voronchikhin and D. V. Kirpichnikov, Phys. Rev. D 107, 115034 (2023), arXiv:2304.14052 [hep-ph]
2023 arXiv
-
[83]
J. D. Bjorken, S. Ecklund, W. R. Nelson, A. Abashian, C. Church, B. Lu, L. W. Mo, T. A. Nunamaker, and P. Rassmann, Phys. Rev. D38, 3375 (1988)
1988
-
[84]
Y. M. Andreevet al. (NA64), Phys. Rev. D106, 032015 (2022), arXiv:2206.03101 [hep-ex]
2022 arXiv
-
[85]
Berlin, N
A. Berlin, N. Blinov, G. Krnjaic, P. Schuster, and N. Toro, Phys. Rev. D 99, 075001 (2019), arXiv:1807.01730 [hep-ph]
2019 arXiv
-
[86]
Marsicano, M
L. Marsicano, M. Battaglieri, M. Bondi’, C. D. R. Car- vajal, A. Celentano, M. De Napoli, R. De Vita, E. Nardi, M. Raggi, and P. Valente, Phys. Rev. D 98, 015031 (2018), arXiv:1802.03794 [hep-ex]
2018 arXiv
-
[87]
Andreas, C
S. Andreas, C. Niebuhr, and A. Ringwald, Phys. Rev. D 86, 095019 (2012), arXiv:1209.6083 [hep-ph]
2012 arXiv
-
[88]
Hinterbichler, Rev
K. Hinterbichler, Rev. Mod. Phys. 84, 671 (2012), arXiv:1105.3735 [hep-th]
2012 arXiv
- [89]
-
[90]
Fierz and W
M. Fierz and W. Pauli, Proc. Roy. Soc. Lond. A173, 211 (1939)
1939
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