REVIEW 4 major objections 5 minor 92 references
Probing the vector-like $X$ quark via the $tW$ channel at future muon-proton colliders
T0 review · 4 major / 5 minor · reviewed 2026-08-01 · deepseek-v4-flash
Pith's one-line read A future muon–proton collider could exclude the vector-like X quark — a hypothetical +5/3-charge partner of the top quark — for masses up to about 8.3 TeV through its tW decay channel, at couplings far below today's LHC reach.
desk verdict Solid, standard simplified-model projection for VLX at muon-proton colliders; headline reach plausible but the paper omits the luminosity used for its central numbers, and much of the scanned parameter space is already excluded by the APV bound it relaxes. 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 effective Lagrangian for the X–W–quark vertex: LX = g* [ √(R_L/(1+R_L)) (g/√2) X̄_L W+_μ γ^μ u_L + √(1/(1+R_L)) (g/√2) X̄_L W+_μ γ^μ t_L ] + h.c., which concentrates all model dependence into the coupling strength g* and the generation-mixing ratio R_L. Detection rides on the charged-current single-production process μ+p → ν̄μ X and the subsequent decay X → tW+, whose final state is partitioned into four channels — fully leptonic, fully hadronic, and two semi-leptonic modes — according to how the two W bosons decay. The fully hadronic channel is reconstructed with large-radius (fat) jets plus a W-mass window, which is what lets it exploit the highly boosted topology
What would settle it
Two checks would settle the matter: re-drawing the exclusion contours with the APV constraint g* √(R_L/(1+R_L)) < 6.5×10⁻² enforced — if the g* > 0.1 regions vanish, the broad-reach claim is falsified; and a 9.16 TeV muon–proton run in the fully hadronic channel with about 100 fb⁻¹, which would either confirm the predicted m_X ≈ 7.3 TeV 5σ discovery or rule out the projection with a null result.
Extended reading notes
Core claim
The paper's central claim is that single production of the vector-like X quark at a muon–proton collider, followed by X → tW+ decay, is observable over a broad parameter region, with the fully hadronic final state the most powerful of the four channels studied. With an 80% polarized muon beam and fat-jet reconstruction of the boosted hadronic W bosons, the projected 2σ exclusion reaches m_X ≃ 8.3 TeV at √s = 9.16 TeV for g* = 0.009 and R_L = 0.1, and the corresponding 5σ discovery reaches m_X ≃ 7.3 TeV at g* = 0.016. Sensitivity improves monotonically with centre-of-mass energy and with R_L, and the two semi-leptonic modes sit between the hadronic and leptonic extremes. The paper states in S
Load-bearing premise
The claim of a 'broad region' of reachable parameter space rests on relaxing the atomic parity violation bound that constrains the X–u–W coupling; if that low-energy bound is enforced, most of the scanned coupling range g* ≳ 0.1–0.2 is already excluded, and only the low-coupling benchmarks near g* = 0.009 survive.
Editorial extensions
If this is right
- At the highest energy considered (√s = 9.16 TeV), a null result in the fully hadronic channel would exclude X-quark masses up to about 8.3 TeV at 2σ for R_L = 0.1, several TeV beyond present LHC bounds.
- A 5σ discovery in the same channel would be possible up to m_X ≃ 7.3 TeV, opening a multi-TeV window that pair-production searches cannot reach for weakly coupled states.
- Because the reach extends down to g* ≈ 0.006–0.016, the analysis covers couplings far below the κ > 0.16–0.2 range probed by current LHC single-production searches.
- Sensitivity scales strongly with centre-of-mass energy and with R_L, so the same analysis design transfers directly to any future upgrade of the muon beam energy.
- The fully leptonic mode, despite its clean signature, has the weakest mass reach, so a complete programme would need all four channels to cover the parameter space.
Reading between the lines
- Enforcing the atomic parity violation bound instead of relaxing it would not destroy the headline benchmark — g* = 0.009, R_L = 0.1 sits safely below the limit — but it would erase most of the g* ≳ 0.1 exclusion contours, so the 'broad region' claim should be read as conditional on that relaxation.
- The analysis uses sequential cuts; replacing them with a multivariate discriminator over the same boosted-jet observables would likely push the reach beyond what any single cut optimization achieves here.
- The same effective-Lagrangian structure and four-channel final-state decomposition transfers to the vector-like T and B quarks and to the (X,T) doublet representation, making this a template for a broader vector-like quark programme at a muon–proton collider.
- Since production is mediated by a W boson from the muon, the attainable mass limit inherits the proton PDF behaviour; a higher-energy proton beam, or a larger R_L, would push the exclusion boundary toward 10 TeV, as Tables VI–IX already hint.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper studies single production of a vector-like X quark (charge +5/3) in a simplified triplet model at future muon-proton colliders, via the process μ+p → ν̄_μ X, X → tW+. The model parameters are the coupling g*, the generation-mixing parameter R_L, and the mass m_X. The analysis simulates four final-state channels (FL, FH, SL1, SL2) with MadGraph5_aMC@NLO, Pythia 8, and Delphes, uses fat-jet reconstruction and 80% muon beam polarization, and computes Asimov exclusion/discovery significances at √s = 5.29, 6.48, and 9.16 TeV. The central claim is that the FH channel is the most sensitive, reaching a 2σ exclusion of m_X ≃ 8.3 TeV at g* = 0.009, R_L = 0.1, and √s = 9.16 TeV. The paper explicitly relaxes the APV constraint and scans g* up to 0.5.
Significance. Future μp collider projections for a vector-like X quark are timely, and the paper offers a genuine phenomenological study with a full simulation chain, external LHC/EWPO comparisons, and a four-channel analysis. If the quantitative claims are correct, the proposed search would substantially extend the current and HL-LHC reach. However, the numerical results are not currently reproducible or fully verifiable because the integrated luminosity and reference g* used in the reach calculation are not stated, and at least one quoted mass point lies at the kinematic boundary. The APV relaxation is disclosed, but the abstract's 'broad region' wording overstates what remains allowed under existing constraints.
major comments (4)
- [Section V, Eqs. (8)-(9); Tables VI-IX and II-V] The Asimov significances require event yields s and b, which depend on the integrated luminosity L. The paper never states the L used for the reach curves; Sec. I only mentions 'target integrated luminosities ranging from 10 to 100 fb−1'. In addition, the cut-flow tables quote only 'Signal(fb)' without the reference g* value. For example, the 23.99 fb after all cuts for X2500 at √s = 9.16 TeV in Table XIV cannot be mapped to the g* axis of Tables VI-IX without knowing the reference coupling. Without specifying L and g*_ref, the g* lower bounds in Tables VI-IX cannot be verified. Please provide these inputs explicitly, or report absolute event yields.
- [Table VII, FH row at √s = 9.16 TeV] For R_L = 0.3 and 0.5, the 2σ exclusion upper limit is quoted as m_X = 9160 GeV, equal to the nominal √s. At m_X = √s, the subprocess requires the proton parton momentum fraction x ≈ 1, where the PDF vanishes; the production cross section is zero. Thus the reach cannot extend to 9160 GeV. The threshold and PDF suppression should be handled explicitly, and the kinematic edge must be reflected in the reported mass limits.
- [Sec. II, Fig. 1 and Figs. 11-14; Tables VI-IX] The APV constraint g* sqrt(R_L/(1+R_L)) < 6.5×10^-2 is relaxed, as stated in Sec. II. For R_L = 0.5 this bound gives g* ≲ 0.11, and for R_L = 0.1 it gives g* ≲ 0.22. Consequently, large parts of the displayed parameter space with g* up to 0.5 are excluded under that bound, and the abstract's 'broad region' claim depends on the relaxation. Please overlay the APV-excluded region in the reach plots or explicitly qualify that the displayed regions above the bound are only valid once the APV constraint is dropped.
- [Sec. IV.B and Appendix Tables XI-XVIII] The text states that 'the same event selection is adopted' for the higher center-of-mass energies, but the appendix cut-flow tables use different selection criteria. For example, the FH selection at 9.16 TeV (Table XIV) uses HT > 800 GeV and p_bT > 500 GeV, whereas at 5.29 TeV (Table III) it uses HT > 900 GeV and p_bT > 400 GeV. Similar differences appear in the FL pseudorapidity windows and the SL1 η_b window. Please correct the text or document the exact selection used at each energy.
minor comments (5)
- [Section V, Eqs. (8)-(9)] The Asimov significances include only statistical uncertainties. No background systematic uncertainty is incorporated. Please state explicitly that the contours are statistical-only, or include a nuisance-parameter treatment if systematics are intended.
- [Throughout] 'Branch ratio' should be 'branching ratio' in several places (e.g., Sec. I and Table captions).
- [Table VII] In the 5.29 TeV, R_L = 0.5 row, the 2σ upper edge of g* is 0.29, which is lower than the R_L = 0.3 value. Please check whether this is a scan-range clipping or a physical NWA/width cut.
- [Sec. III] A summary of the Delphes detector parameters (b-tagging efficiency, jet radius, jet energy scale) would improve reproducibility.
- [Figs. 11-15] The Γ_X/m_X contours are used to justify the NWA, but the actual contour values are not stated in the text. Please provide the relevant Γ_X/m_X values for the benchmark points.
Circularity Check
No significant circularity: the reach projections are forward MC calculations over scanned model parameters, not fits to their own outputs.
full rationale
The derivation chain is a standard forward calculation: the simplified Lagrangian Eq. (6) defines the coupling structure with scanned inputs g*, R_L, and m_X; the width is computed analytically in Eq. (7); signal and background cross sections are obtained from MadGraph/Pythia/Delphes (Section III); cut flows are given in Tables II–V and XI–XVIII; and the Asimov significances in Eqs. (8)–(9) convert the resulting yields s and b into the reach contours and Tables VI–IX. No target quantity is fitted from the data to produce another target quantity: the coupling lower bounds and mass reaches are outputs of the significance calculation, not inputs to it. The explicit relaxation of the APV bound ('we relax this strict APV bound in our collider simulations for the sake of exploring full phenomenological projections, and scan the broader parameter space of g* ≤ 0.5 and R_L ≤ 1', Section II) is a stated modeling choice that weakens an external constraint; it is not circular. The self-citations [63] and [84] are used only to draw shaded existing-constraint regions (EWPO and LHC single-production) in the comparison figures and are not load-bearing for the headline FH reach, which is computed from the MC yields. The NWA validity check overlaying Gamma_X/m_X contours uses the authors' own computed width, but this is a self-consistency check, not a derivation of the reach. The main caveat is reproducibility rather than circularity: the integrated luminosity used for the reach curves is never stated, and the reference g* value entering the signal cross sections in the cut-flow tables is not given, so the numerical values in Tables VI–IX cannot be independently regenerated from the paper alone. This is an omitted-input/reproducibility issue, not an equivalence between prediction and input.
Assumptions & free parameters
free parameters (4)
- g*
- R_L
- m_X
- P_eff (muon beam polarization) =
80%
assumptions (5)
- ad hoc to paper Effective Lagrangian Eq. (6) with only X-u-W and X-t-W couplings and no other decay modes.
- ad hoc to paper The atomic parity violation constraint g* sqrt(R_L/(1+R_L)) < 6.5e-2 is relaxed in the simulations.
- domain assumption Narrow-width approximation is valid; off-shell and interference effects are neglected.
- domain assumption DELPHES generic detector response approximates a future muon–proton detector.
- domain assumption Leading-order cross sections with default PDFs and dynamic renormalization/factorization scales.
invented entities (1)
-
Vector-like X quark (VLX)
independent evidence
Cite this review
Pith. "Pith review of Probing the vector-like $X$ quark via the $tW$ channel at future muon-proton colliders." pith.science (2026). https://pith.science/paper/PTPK3MV5
@misc{pith2026260718843,
author = {Pith},
title = {Pith review of: Probing the vector-like $X$ quark via the $tW$ channel at future muon-proton colliders},
year = {2026},
howpublished = {\url{https://pith.science/paper/PTPK3MV5}},
note = {Machine review of arXiv:2607.18843}
}
abstract
We investigate the discovery potential for the vector-like $X$-quark (VLX) at future muon--proton ($\mu p$) colliders through the process $\mu^+ p \to \bar{\nu}_\mu X \to \bar{\nu}_\mu t W^+$. A simplified effective model is adopted in which the production and decay of the VLX are governed by the coupling strength $g^{*}$, the generation-mixing parameter $R_{L}$, and the VLX mass $m_X$. A comprehensive Monte Carlo analysis is performed at $\sqrt{s}=5.29$, $6.48$, and $9.16\ \mathrm{TeV}$, considering four complementary decay channels: the Fully Leptonic (FL), Fully Hadronic (FH), and two Semi-Leptonic (SL1 and SL2) modes. An $80\%$ polarized muon beam together with boosted-object reconstruction based on fat-jet techniques is employed to improve the signal sensitivity. The expected exclusion and discovery reaches are evaluated using the Asimov significance. We find that the sensitivity can be improved substantially with increasing center-of-mass energy and larger values of $R_L$. Among the four channels, the FH mode provides the strongest sensitivity, reaching a $2\sigma$ exclusion limit of $m_X\simeq8.3\ \mathrm{TeV}$ with $g^* = 0.009 $ for $R_L=0.1$ at $\sqrt{s}=9.16\ \mathrm{TeV}$, whereas the FL mode gives the weakest reach because of its smallest branch ratio. These results demonstrate that future $\mu p$ colliders can offer significant sensitivity to heavy VLX over a broad region of parameter space.
Figures
Figures from the paper (12 more)
Reference graph
Works this paper leans on
-
[1]
SL1 mode As illustrated in Figure 2(c), the charged lepton in the SL1 topology originates from the W boson emitted directly in the decay X →tW +, where the secondW boson subsequently decays hadronically through the top quark. As intimated, here, since the W boson is produced directly from the decay of the heavy VLX, it acquires a large fraction of the par...
2000
-
[2]
In this case, the W boson produced directly from the heavy VLX decays hadronically, while the second W boson originating from the top-quark decay subsequently decays leptonically
SL2 mode The SL2 topology, shown in Figure 2(d), differs from SL1 in the decay pattern of the two W bosons. In this case, the W boson produced directly from the heavy VLX decays hadronically, while the second W boson originating from the top-quark decay subsequently decays leptonically. Consequently, as explained, the hadronic W receives the full boost fr...
2000
-
[3]
S. L. Glashow, Nucl. Phys. 22, 579 (1961)
1961
-
[4]
Weinberg, Phys
S. Weinberg, Phys. Rev. Lett. 19, 1264 (1967)
1967
-
[5]
Salam, Conf
A. Salam, Conf. Proc. C 680519, 367 (1968)
1968
-
[6]
Arnison et al
G. Arnison et al. (UA1), Phys. Lett. B 122, 103 (1983)
1983
-
[7]
Banner et al
M. Banner et al. (UA2), Phys. Lett. B 122, 476 (1983)
1983
-
[8]
Abe et al
F. Abe et al. (CDF), Phys. Rev. Lett. 74, 2626 (1995)
1995
Show all 92 references
-
[9]
Abachi et al
S. Abachi et al. (D0), Phys. Rev. Lett. 74, 2632 (1995)
1995
-
[10]
Aad et al
G. Aad et al. (ATLAS), Phys. Lett. B 716, 1 (2012)
2012
-
[11]
Chatrchyan et al
S. Chatrchyan et al. (CMS), Phys. Lett. B 716, 30 (2012). 30
2012
-
[12]
B. S. DeWitt, Phys. Rev. 160, 1113 (1967)
1967
-
[13]
’t Hooft and M
G. ’t Hooft and M. J. G. Veltman, Ann. Inst. H. Poincare Phys. Theor. A 20, 69 (1974)
1974
-
[14]
Zwicky, Helv
F. Zwicky, Helv. Phys. Acta 6, 110 (1933)
1933
-
[15]
V. C. Rubin and W. K. Ford, Jr., Astrophys. J. 159, 379 (1970)
1970
-
[16]
Fukuda et al
Y. Fukuda et al. (Super-Kamiokande), Phys. Rev. Lett. 81, 1562 (1998)
1998
-
[17]
Q. R. Ahmad et al. (SNO), Phys. Rev. Lett. 87, 071301 (2001)
2001
-
[18]
A. D. Sakharov, Pisma Zh. Eksp. Teor. Fiz. 5, 32 (1967)
1967
-
[19]
Gildener and S
E. Gildener and S. Weinberg, Phys. Rev. D 13, 3333 (1976)
1976
-
[20]
Susskind, Phys
L. Susskind, Phys. Rev. D 20, 2619 (1979)
1979
-
[21]
’t Hooft, NATO Sci
G. ’t Hooft, NATO Sci. Ser. B 59, 135 (1980)
1980
-
[22]
J. A. Aguilar-Saavedra, R. Benbrik, S. Heinemeyer, and M. Pérez-Victoria, Phys. Rev. D 88 (2013)
2013
-
[23]
Buchkremer, G
M. Buchkremer, G. Cacciapaglia, A. Deandrea, and L. Panizzi, Nucl. Phys. B 876, 376 (2013)
2013
-
[24]
G. C. Branco and M. N. Rebelo, PoS DISCRETE2020-2021, 004 (2022)
2021
-
[25]
J. M. Alves, G. Branco, A. Cherchiglia, C. Nishi, J. Penedo, P. M. Pereira, M. Rebelo, and J. Silva-Marcos, Phys. Rep. 1057, 1–69 (2024)
2024
-
[26]
Banerjee, E
A. Banerjee, E. Bergeaas Kuutmann, V. Ellajosyula, R. Enberg, G. Ferretti, and L. Panizzi, SciPost Phys. Core 7 (2024)
2024
-
[27]
V. M. Peralta Cano, Ph.D. thesis, Universidade de São Paulo, Brasil, Universidade de São Paulo, Brazil, U. Sao Paulo (main) (2017)
2017
-
[28]
Arkani-Hamed, C
N. Arkani-Hamed, C. Figueiredo, L. J. Hall, and C. A. Manzari, arXiv:2602.17754 (2026)
2026
-
[29]
Arkani-Hamed, A
N. Arkani-Hamed, A. G. Cohen, E. Katz, and A. E. Nelson, JHEP 07, 034 (2002)
2002
-
[30]
T. Han, H. E. Logan, B. McElrath, and L.-T. Wang, Phys. Rev. D 67, 095004 (2003)
2003
-
[31]
Cao and C.-R
Q.-H. Cao and C.-R. Chen, Phys. Rev. D 76, 075007 (2007)
2007
-
[32]
Agashe, G
K. Agashe, G. Perez, and A. Soni, Phys. Rev. D 75, 015002 (2007)
2007
-
[33]
Agashe, R
K. Agashe, R. Contino, and A. Pomarol, Nucl. Phys. B 719, 165 (2005)
2005
-
[34]
Bellazzini, C
B. Bellazzini, C. Csáki, and J. Serra, Eur. Phys. J. C 74, 2766 (2014)
2014
-
[35]
M. Low, A. Tesi, and L.-T. Wang, Phys. Rev. D 91, 095012 (2015)
2015
-
[36]
L. Bian, D. Liu, and J. Shu, Int. J. Mod. Phys. A 33, 1841007 (2018). 31
2018
-
[37]
H.-J. He, C. T. Hill, and T. M. P. Tait, Phys. Rev. D 65, 055006 (2002)
2002
-
[38]
del Aguila, L
F. del Aguila, L. Ametller, G. Kane, and J. Vidal, Nucl. Phys. B 334, 1 (1990)
1990
-
[39]
Cacciapaglia, A
G. Cacciapaglia, A. Deandrea, L. Panizzi, N. Gaur, D. Harada, and Y. Okada, JHEP 03, 070 (2012)
2012
-
[40]
N. Liu, L. Wu, B. Yang, and M. Zhang, Phys. Lett. B 753, 664 (2016)
2016
-
[41]
Fuks and H.-S
B. Fuks and H.-S. Shao, Eur. Phys. J. C 77 (2017)
2017
-
[42]
Cacciapaglia, A
G. Cacciapaglia, A. Deandrea, N. Gaur, D. Harada, Y. Okada, and L. Panizzi, JHEP 11, 055 (2018)
2018
-
[43]
Liu and S
Y.-B. Liu and S. Moretti, Phys. Rev. D 100, 015025 (2019)
2019
-
[44]
B. Yang, B. Hou, H. Zhang, and N. Liu, Phys. Rev. D 99, 095002 (2019)
2019
-
[45]
D. Wang, L. Wu, and M. Zhang, Phys. Rev. D 103, 115017 (2021)
2021
-
[46]
Deandrea, T
A. Deandrea, T. Flacke, B. Fuks, L. Panizzi, and H.-S. Shao, JHEP 08, 107 (2021), [Erra- tum: JHEP 11, 028 (2022)]
2021
-
[47]
B. Yang, X. Sima, S. Wang, and L. Shang, Phys. Rev. D 105, 096010 (2022)
2022
-
[48]
Shang, C
L. Shang, C. Chen, S. Wang, and B. Yang, Nucl. Phys. B 984, 115977 (2022)
2022
-
[49]
L. Han, S. Wang, L. Shang, and B. Yang, Chin. Phys. C 47, 043108 (2023)
2023
-
[51]
Moretti, L
S. Moretti, L. Panizzi, and L. Shang, JHEP 06, 132 (2025)
2025
-
[52]
Han, Y.-B
J.-Z. Han, Y.-B. Liu, and S. Moretti, Phys. Rev. D 112, 035016 (2025)
2025
-
[53]
Shang and K
L. Shang and K. Sun, Nucl. Phys. B 990, 116185 (2023)
2023
-
[54]
Y.-B. Liu, B. Hu, and C.-Z. Li, Nucl. Phys. B 1007, 116667 (2024)
2024
-
[55]
Zhang, Y.-T
Y.-J. Zhang, Y.-T. Zhu, L. Han, Y.-P. Bi, and T.-G. Liu, Eur. Phys. J. C 84, 1184 (2024)
2024
-
[56]
Arhrib, R
A. Arhrib, R. Benbrik, M. Boukidi, and S. Moretti, J. Phys. G 52, 105002 (2025)
2025
-
[57]
Aaboud et al
M. Aaboud et al. (ATLAS), Phys. Lett. B 784, 173 (2018)
2018
-
[58]
Chatrchyan, V
S. Chatrchyan, V. Khachatryan, A. M. Sirunyan, A. Tumasyan, W. Adam, T. Bergauer, M. Dragicevic, J. Erö, C. Fabjan, M. Friedl, et al. (CMS Collaboration), Phys. Rev. Lett. 112, 171801 (2014)
2014
-
[59]
Aad et al
G. Aad et al. (ATLAS), Eur. Phys. J. C 83, 719 (2023)
2023
-
[60]
A. M. Sirunyan et al. (CMS), Eur. Phys. J. C 79, 90 (2019)
2019
-
[61]
A. M. Sirunyan et al. (CMS), JHEP 03, 082 (2019). 32
2019
-
[62]
Tumasyan et al
A. Tumasyan et al. (CMS), JHEP 04, 048 (2022)
2022
-
[63]
M. E. Peskin and T. Takeuchi, Phys. Rev. Lett. 65, 964 (1990)
1990
-
[64]
de Blas, M
J. de Blas, M. Pierini, L. Reina, and L. Silvestrini, Phys. Rev. Lett. 129, 271801 (2022)
2022
-
[65]
J. Cao, L. Meng, L. Shang, S. Wang, and B. Yang, Phys. Rev. D 106, 055042 (2022)
2022
-
[66]
Cheung and Z
K. Cheung and Z. S. Wang, Phys. Rev. D 103 (2021)
2021
- [67]
-
[68]
Thaler and L.-T
J. Thaler and L.-T. Wang, JHEP 07, 092 (2008)
2008
-
[69]
J. Cao, Y. He, P. Wu, M. Zhang, and J. Zhu, JHEP 01, 150 (2014)
2014
-
[70]
Arsenault, K
A. Arsenault, K. Y. Cingiloglu, and M. Frank, Phys. Rev. D 107, 036018 (2023)
2023
-
[71]
G. C. Branco and L. Lavoura, Nucl. Phys. B 278, 738 (1986)
1986
-
[72]
del Aguila, J
F. del Aguila, J. A. Aguilar-Saavedra, and R. Miquel, Phys. Rev. Lett. 82, 1628 (1999)
1999
-
[73]
A. Atre, M. Carena, T. Han, and J. Santiago, Phys. Rev. D 79, 054018 (2009)
2009
-
[74]
J. A. Aguilar-Saavedra, EPJ Web Conf. 60, 16012 (2013), 1306.4432
2013 arXiv
-
[75]
Okada and L
Y. Okada and L. Panizzi, Adv. High Energy Phys. 2013, 364936 (2013)
2013
-
[76]
Alloul, N
A. Alloul, N. D. Christensen, C. Degrande, C. Duhr, and B. Fuks, Comput. Phys. Commun. 185, 2250 (2014)
2014
-
[77]
Alwall, M
J. Alwall, M. Herquet, F. Maltoni, O. Mattelaer, and T. Stelzer, JHEP 2011 (2011)
2011
-
[78]
Alwall, R
J. Alwall, R. Frederix, S. Frixione, V. Hirschi, F. Maltoni, O. Mattelaer, H.-S. Shao, T. Stelzer, P. Torrielli, and M. Zaro, JHEP 2014 (2014)
2014
-
[79]
Sjöstrand, S
T. Sjöstrand, S. Ask, J. R. Christiansen, R. Corke, N. Desai, P. Ilten, S. Mrenna, S. Prestel, C. O. Rasmussen, and P. Z. Skands, Comput. Phys. Commun. 191, 159–177 (2015)
2015
-
[80]
Bierlich, S
C. Bierlich, S. Chakraborty, N. Desai, L. Gellersen, I. Helenius, P. Ilten, L. Lönnblad, S. Mrenna, S. Prestel, C. T. Preuss, et al., SciPost Phys. Codebases p. 8 (2022)
2022
-
[81]
de Favereau, C
J. de Favereau, C. Delaere, P. Demin, A. Giammanco, V. Lemaître, A. Mertens, M. Selvaggi, and T. D. . collaboration, Journal of High Energy Physics 2014, 57 (2014)
2014
-
[82]
Conte, B
E. Conte, B. Fuks, and G. Serret, Comput. Phys. Commun. 184, 222 (2013)
2013
-
[83]
Shang and Y
L. Shang and Y. Zhang, Comput. Phys. Commun. 296, 109027 (2024)
2024
-
[84]
Navas et al
S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024)
2024
-
[85]
Cowan, K
G. Cowan, K. Cranmer, E. Gross, and O. Vitells, Eur. Phys. J. C 71, 1554 (2011), [Erratum: Eur.Phys.J.C 73, 2501 (2013)], 1007.1727. 33
2011 arXiv
-
[86]
Benbrik, M
R. Benbrik, M. Boukidi, M. Ech-chaouy, S. Moretti, K. Salime, and Q.-S. Yan, JHEP 03, 020 (2025)
2025
-
[87]
Barducci, A
D. Barducci, A. Belyaev, J. Blamey, S. Moretti, L. Panizzi, and H. Prager, JHEP 07, 142 (2014)
2014
-
[88]
Moretti, D
S. Moretti, D. O’Brien, L. Panizzi, and H. Prager, Phys. Rev. D 96, 075035 (2017)
2017
-
[89]
Moretti, D
S. Moretti, D. O’Brien, L. Panizzi, and H. Prager, Phys. Rev. D 96, 035033 (2017)
2017
-
[90]
Prager, S
H. Prager, S. Moretti, D. O’Brien, and L. Panizzi, PoS DIS2017, 300 (2018)
2018
-
[91]
Prager, S
H. Prager, S. Moretti, D. O’Brien, and L. Panizzi, in 5th Large Hadron Collider Physics Conference (2017), 1706.04001
2017 arXiv
-
[92]
Carvalho, S
A. Carvalho, S. Moretti, D. O’Brien, L. Panizzi, and H. Prager, Phys. Rev. D 98, 015029 (2018)
2018
-
[93]
Berdine, N
D. Berdine, N. Kauer, and D. Rainwater, Phys. Rev. Lett. 99, 111601 (2007). Appendix A: Additional Material Cuts Signal(fb) Backgrounds(fb) X1500 X2000 X2500 µW j ¯νW W j µZW j Basic cuts 16.39 8.34 3.89 3911 14.71 2.49 Nl = 2 9.12 3.64 1.35 2573 11.60 1.91 Nb = 1 6.03 2.40 0....
2007
Reviewed August 1, 2026 · model on record in the stance chip above.
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