REVIEW 2 major objections 5 minor 105 references
Minimal renormalon subtraction stabilizes pNRQCD spectroscopy of heavy multi-quark systems and yields baryon masses that undershoot lattice QCD by 125–175 MeV.
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 · grok-4.5
2026-07-13 06:28 UTC pith:G45OABBD
load-bearing objection First MRS-pNRQCD spectra for multi-heavy systems: scale stability is real, lattice offset is the expected size, non-singlet MRS is the only load-bearing caveat. the 2 major comments →
Renormalon subtracted nonrelativistic QCD for heavy hadron systems
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
When the leading renormalon is subtracted from the static two-body potentials of pNRQCD and the residual series is Borel-resummed, the resulting MRS Hamiltonian, solved by GFMC, produces triply-heavy baryon masses that undershoot lattice-QCD benchmarks by a systematic 125–175 MeV whose fractional size falls as ~1/mQ, while renormalization-scale bands shrink by factors of 3–10 relative to fixed-order results.
What carries the argument
Minimal renormalon subtraction (MRS) applied to the static potential: the factorial asymptotic series is split into a short-distance piece (fixed-order coefficients minus their asymptotic tails) plus a Borel-resummed tail, evaluated at a smooth dynamical scale μ'(r) = √(μ_cut^{2} + λ^{2}/r^{2}), then fed into a few-body Schrödinger equation solved by variational and Green’s-function Monte Carlo.
Load-bearing premise
The same Borel resummation that cancels the leading renormalon in the color-singlet channel is assumed to work without change for the non-singlet color channels that appear in baryons and tetraquarks.
What would settle it
Include the O(1/mQ) and O(1/mQ^{2}) spin-dependent and velocity-dependent potentials already present in lattice NRQCD and recompute the same baryon masses; if the 125–175 MeV gap closes while the MRS scale bands remain narrow, the central claim is confirmed.
If this is right
- Scale variation of bottomonium and Ωbbb binding energies drops from hundreds of MeV to ~10 MeV at NNLO, making residual theory error dominated by missing 1/mQ operators rather than renormalon instability.
- A single pair of MRS-tuned charm and bottom masses yields parameter-free predictions for all mixed-flavor mesons, triply-heavy baryons, and fully-heavy tetraquarks.
- Unequal-mass fully-heavy tetraquarks bind only for heavy-to-light mass ratios ≲ 0.085 (MRS NLO); equal-mass systems such as bb̄b̄b and cc̄c̄c remain unbound.
- The same MRS-pNRQCD-QMC pipeline supplies well-defined QCD benchmarks for top-containing systems and for composite dark-matter spectra without new lattice runs at every mass point.
Where Pith is reading between the lines
- If the non-singlet renormalon structure can be derived and shown to match the singlet case, MRS becomes a universal short-distance scheme for every color channel in multi-quark EFTs.
- The observed 1/mQ scaling of the lattice discrepancy already supplies a quantitative target for the size of the next-order 1/mQ potentials that must be matched.
- Because the method is coordinate-space and mass-continuous, it can scan dark-sector hadron spectra across continuous mass ratios far more cheaply than lattice QCD.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The paper implements minimal renormalon subtraction (MRS) for the static two-body potentials of pNRQCD through NNLO, combines them with fixed-order three-body forces, and solves the resulting few-body Schrödinger problems with VMC/GFMC. Charm and bottom masses are tuned to spin-averaged 1S quarkonium masses; the same masses are then used without retuning to predict triply-heavy baryon masses (Ωccc, Ωccb, Ωcbb, Ωbbb and top-containing analogues) and the binding landscape of fully-heavy tetraquarks QQ¯Q′¯Q′. MRS is shown to shrink renormalization-scale bands by factors of 3–10 relative to fixed-order results and to bring LO/NLO/NNLO bands into partial overlap. NNLO MRS baryon masses undershoot lattice QCD by 125–175 MeV, with fractional differences falling as ∼1/mQ, which the authors attribute to omitted O(1/mQ) operators. For tetraquarks a critical mass ratio mQ/mQ′≃0.085 is obtained at NLO MRS, below which bb¯t¯t, bc¯t¯t and cc¯t¯t are bound.
Significance. If the MRS reorganization and its extension to multi-quark color channels hold, the work supplies a practical, computationally efficient route to renormalon-stable heavy-hadron spectroscopy that complements lattice QCD. The explicit isolation of the leading renormalon into a Borel-resummed tail (Appendix, Eqs. A.6–A.15), the systematic comparison of fixed-order versus MRS scale dependence (Figs. 1–4, Tables I–V), and the falsifiable 1/mQ scaling of the lattice discrepancy are genuine strengths. The tetraquark critical-ratio map and the top-containing benchmarks are new, parameter-free predictions once the quark masses are fixed. The framework is immediately reusable for dark-sector scans and for near-threshold tt¯ phenomenology.
major comments (2)
- Sec. II B (paragraph beginning “For multiquark systems…”) and Eq. (6): the MRS Borel resummation is derived for the color-singlet potential, yet is applied unchanged to the color-antisymmetric QQ channel that dominates the baryon Hamiltonian (Eq. 17, CB=2/3). The paper correctly labels this an unproven scheme choice. Because the absolute baryon masses in Table III (the central claim) rest on this channel, a quantitative estimate of the associated systematic—or an explicit statement that the quoted 125–175 MeV discrepancy already absorbs it—is needed before the numbers can be treated as controlled.
- Sec. IV B / Table III: the lattice discrepancy is interpreted as missing O(1/mQ) corrections because the fractional difference falls as ∼1/mQ. While the scaling is suggestive, no explicit O(1/mQ) operator is evaluated. A single controlled estimate (e.g., the leading Darwin or spin-orbit shift for Ωbbb) would convert the interpretation from plausible to quantitative and would strengthen the claim that MRS has removed the dominant perturbative uncertainty.
minor comments (5)
- Sec. II B and Appendix: the three regularization prescriptions (hard cutoff, frozen αs, µ′) are compared only for bottomonium (Figs. 6–8). A one-sentence statement that the same µcut=1 GeV choice was verified for the baryon and tetraquark systems would remove a minor reproducibility concern.
- Table I: the FO LO charmonium and bottomonium masses are listed without uncertainties while MRS LO entries carry them; a uniform convention would improve readability.
- Fig. 5 caption: the marker styles for the three scale choices are not fully legible in grayscale; adding a legend or distinct open/filled symbols would help.
- Sec. V: tetraquark results stop at NLO because multi-body potentials lack an MRS formula. A brief forward-looking sentence on how the three-body MRS problem might be approached would be useful for readers planning follow-up work.
- References: a few arXiv-only entries (e.g., [75], [100]–[102]) could be updated to journal versions if available at proof stage.
Circularity Check
No significant circularity: quark masses tuned to experimental 1S quarkonia are fixed inputs; baryon/tetraquark masses and critical ratios are independent GFMC outputs compared to external lattice benchmarks.
full rationale
The derivation chain is self-contained and non-circular. Quark masses m_c and m_b are tuned once to experimental spin-averaged 1S quarkonium masses (Eqs. 14-15, Table I) and then held fixed as inputs; all subsequent baryon masses (Table III), top-containing states (Table IV), mixed mesons (Table II), and tetraquark binding ratios/critical mass ratios (Fig. 5, Table V) are genuine GFMC solutions of the MRS-pNRQCD Hamiltonian and are compared to independent lattice-QCD and experimental benchmarks. The MRS reorganization (Eq. 6, Appendix) is applied order-by-order to the known static potentials; residual scale variation is reported as a diagnostic, not absorbed into the predictions. Self-citations to the authors' prior fixed-order QMC papers [23-25] and Kronfeld's MRS formalism serve only as methodological baselines or FO comparison columns; they do not force the NNLO MRS central values, the 125-175 MeV lattice undershoot, or the ~0.085 critical mass ratio. The openly flagged scheme choice of applying singlet MRS to non-singlet channels is an assumption, not a circular reduction. No equation equates a claimed prediction to a fitted input by construction.
Axiom & Free-Parameter Ledger
free parameters (5)
- m_c (MRS NNLO) =
1.55489 GeV
- m_b (MRS NNLO) =
4.80221 GeV
- µ_cut =
1 GeV
- r* =
0.35 GeV^{-1}
- λ (central) =
1
axioms (4)
- domain assumption pNRQCD static Hamiltonian at O(m_Q^0) plus fixed-order three-body potentials at NNLO is a controlled approximation for systems with m_Q ≫ Λ_QCD.
- ad hoc to paper The MRS Borel resummation derived for the color-singlet static potential may be applied unchanged to every two-body color channel (octet, antisymmetric, symmetric).
- domain assumption The leading renormalon power correction Λ_R can be absorbed into the definition of the heavy-quark masses when those masses are tuned to experimental quarkonium masses.
- standard math GFMC imaginary-time projection with the given Trotter step and finite-τ extrapolation converges to the true ground-state energy of the static Hamiltonian.
read the original abstract
We present a renormalon-subtracted formulation of potential nonrelativistic QCD (pNRQCD) for precision spectroscopy of heavy hadron systems, combining variational and Green's function Monte Carlo (VMC/GFMC) methods with NNLO static two- and three-body potentials. Minimal renormalon subtraction (MRS) systematically sums leading factorially growing terms, thereby stabilizing perturbative convergence and reducing renormalization-scale dependence. We tune charm and bottom quark masses to spin-averaged $1S$ quarkonium states and predict $\Omega_{ccc}$, $\Omega_{ccb}$, $\Omega_{cbb}$, and $\Omega_{bbb}$ baryon masses, as well as QCD-stable baryons containing top quarks. NNLO MRS results undershoot lattice QCD by 125--175~MeV, with fractional differences decreasing as $\sim 1/m_Q$, consistent with neglected $\mathcal{O}(1/m_Q)$ corrections. Applying these methods to unequal-mass fully-heavy tetraquarks, we determine the critical heavy-to-light mass ratio for binding and compute binding energies across the mass-ratio landscape.
Figures
Reference graph
Works this paper leans on
-
[1]
renormalon subtraction
MRS formalism In pNRQCD, static potentials are matching coefficient taking the form VR(r) =V R(r) + ΛR, V R(r) =− CR r X l=0 vl(µr)αs(µ)l+1, (A.1) whereRlabels the irrep of the potential, Λ R is of order the QCD scale, andv l are perturbative coefficients. The beta function coefficients satisfy β(αs) =−α s ∞X k=0 βkαk+1 s , b≡ β1 2β2 0 .(A.2) The presence...
-
[2]
Implementation for pNRQCD potentials For the static potentialV(r, µ), the MRS procedure described above is applied at each quark-antiquark sep- arationrwith the identificationQ= 1/r. The short- distance coefficientsv l correspond to the perturbative expansion ofV(r, µ) in powers ofα s(µ), and the renor- malon sumR (p) B captures the leading infrared sensi...
-
[3]
D. J. Gross and F. Wilczek, Phys. Rev. Lett.30, 1343 (1973)
1973
-
[4]
H. D. Politzer, Phys. Rev. Lett.30, 1346 (1973)
1973
-
[5]
D. J. Gross and A. Neveu, Phys. Rev. D10, 3235 (1974)
1974
-
[6]
D. R. T. Jones, Nucl. Phys. B75, 531 (1974)
1974
-
[7]
W. E. Caswell, Phys. Rev. Lett.33, 244 (1974)
1974
-
[8]
O. V. Tarasov, A. A. Vladimirov, and A. Y. Zharkov, Phys. Lett. B93, 429 (1980)
1980
-
[9]
S. A. Larin and J. A. M. Vermaseren, Phys. Lett. B303, 334 (1993), arXiv:hep-ph/9302208
Pith/arXiv arXiv 1993
-
[10]
T. van Ritbergen, J. A. M. Vermaseren, and S. A. Larin, Phys. Lett. B400, 379 (1997), arXiv:hep-ph/9701390
Pith/arXiv arXiv 1997
-
[11]
M. F. Zoller, JHEP , 118 (2016), arXiv:1608.08982 [hep- ph]
Pith/arXiv arXiv 2016
-
[12]
P. A. Baikov, K. G. Chetyrkin, and J. H. K¨ uhn, Phys. Rev. Lett.118, 082002 (2017), arXiv:1606.08659 [hep- ph]
Pith/arXiv arXiv 2017
-
[13]
F. Herzog, B. Ruijl, T. Ueda, J. A. M. Vermaseren, and A. Vogt, JHEP , 090 (2017), arXiv:1701.01404 [hep-ph]
Pith/arXiv arXiv 2017
-
[14]
T. Luthe, A. Maier, P. Marquard, and Y. Schr¨ oder, JHEP , 020 (2017), arXiv:1701.07068 [hep-ph]
Pith/arXiv arXiv 2017
-
[15]
Appelquist, M
T. Appelquist, M. Dine, and I. J. Muzinich, Phys. Rev. D17, 2074 (1978)
2074
-
[16]
W. E. Caswell and G. P. Lepage, Phys. Lett. B167, 437 (1986)
1986
-
[17]
G. P. Lepage, L. Magnea, C. Nakhleh, U. Magnea, and K. Hornbostel, Phys. Rev. D46, 4052 (1992), arXiv:hep-lat/9205007
Pith/arXiv arXiv 1992
-
[18]
N. Brambilla, A. Pineda, J. Soto, and A. Vairo, Phys. Rev. D60, 091502 (1999), arXiv:hep-ph/9903355
Pith/arXiv arXiv 1999
-
[19]
A. Pineda and J. Soto, Nucl. Phys. B Proc. Suppl.64, 428 (1998), arXiv:hep-ph/9707481
Pith/arXiv arXiv 1998
-
[20]
A. Pineda and J. Soto, Phys. Lett. B495, 323 (2000), arXiv:hep-ph/0007197
Pith/arXiv arXiv 2000
-
[21]
N. Brambilla, A. Pineda, J. Soto, and A. Vairo, Rev. Mod. Phys.77, 1423 (2005), arXiv:hep-ph/0410047
Pith/arXiv arXiv 2005
-
[22]
N. Brambilla, X. Garcia i Tormo, J. Soto, and A. Vairo, Phys. Lett. B647, 185 (2007), arXiv:hep-ph/0610143
Pith/arXiv arXiv 2007
-
[23]
N. Brambilla, A. Vairo, X. Garcia i Tormo, and J. Soto, Phys. Rev. D80, 034016 (2009), arXiv:0906.1390 [hep- ph]
Pith/arXiv arXiv 2009
-
[24]
A. Pineda, Prog. Part. Nucl. Phys.67, 735 (2012), arXiv:1111.0165 [hep-ph]
Pith/arXiv arXiv 2012
-
[25]
B. Assi and M. L. Wagman, Phys. Rev. D108, 096004 (2023), arXiv:2305.01685 [hep-ph]
Pith/arXiv arXiv 2023
-
[26]
B. Assi and M. L. Wagman, Phys. Rev. D110, 094001 (2024), arXiv:2311.01498 [hep-ph]
Pith/arXiv arXiv 2024
-
[27]
B. Assi, A. V. Grebe, and M. L. Wagman, Phys. Rev. D113, 016013 (2026), arXiv:2508.10090 [hep-ph]
arXiv 2026
-
[28]
S. Meinel, Phys. Rev. D82, 114514 (2010), arXiv:1008.3154 [hep-lat]
Pith/arXiv arXiv 2010
-
[29]
Z. S. Brown, W. Detmold, S. Meinel, and K. Orginos, Phys. Rev. D90, 094507 (2014), arXiv:1409.0497 [hep- lat]
Pith/arXiv arXiv 2014
-
[30]
N. Mathur, M. Padmanath, and S. Mondal, Phys. Rev. Lett.121, 202002 (2018), arXiv:1806.04151 [hep-lat]
Pith/arXiv arXiv 2018
-
[31]
A. Bazavov, N. Brambilla, X. Garcia i Tormo, P. Petreczky, J. Soto, A. Vairo, and J. H. We- ber (TUMQCD), Phys. Rev. D100, 114511 (2019), arXiv:1907.11747 [hep-lat]
Pith/arXiv arXiv 2019
-
[32]
N. Brambilla, V. Leino, O. Philipsen, C. Reisinger, A. Vairo, and M. Wagner, Phys. Rev. D105, 054514 (2022), arXiv:2106.01794 [hep-lat]
Pith/arXiv arXiv 2022
-
[33]
N. Mathur, M. Padmanath, and D. Chakraborty, Phys. Rev. Lett.130, 111901 (2023), arXiv:2205.02862 [hep- lat]
Pith/arXiv arXiv 2023
-
[34]
N. Brambilla, R. L. Delgado, A. S. Kronfeld, V. Leino, P. Petreczky, S. Steinbeißer, A. Vairo, and J. H. We- ber (TUMQCD), Phys. Rev. D107, 074503 (2023), arXiv:2206.03156 [hep-lat]. 16
Pith/arXiv arXiv 2023
-
[35]
M. Beneke and V. M. Braun, Nucl. Phys. B426, 301 (1994), arXiv:hep-ph/9402364
Pith/arXiv arXiv 1994
-
[36]
I. I. Y. Bigi, M. A. Shifman, N. G. Uraltsev, and A. I. Vainshtein, Phys. Rev. D50, 2234 (1994), arXiv:hep- ph/9402360
arXiv 1994
- [37]
-
[38]
M. E. Luke, A. V. Manohar, and M. J. Savage, Phys. Rev. D51, 4924 (1995), arXiv:hep-ph/9407407
Pith/arXiv arXiv 1995
-
[39]
A. S. Kronfeld, Phys. Rev. D58, 051501 (1998), arXiv:hep-ph/9805215
Pith/arXiv arXiv 1998
- [40]
- [41]
-
[42]
Komijani, JHEP08, 062 (2017), arXiv:1701.00347 [hep-ph]
J. Komijani, JHEP08, 062 (2017), arXiv:1701.00347 [hep-ph]
Pith/arXiv arXiv 2017
-
[43]
Y. Sumino and H. Takaura, JHEP , 116 (2020), arXiv:2001.00770 [hep-ph]
Pith/arXiv arXiv 2020
-
[44]
C. M. Bender and T. T. Wu, Phys. Rev. Lett.27, 461 (1971)
1971
-
[45]
C. M. Bender and T. T. Wu, Phys. Rev. D7, 1620 (1973)
1973
-
[46]
B. E. Lautrup, Phys. Lett. B69, 109 (1977)
1977
-
[47]
’t Hooft, inThe Whys of Subnuclear Physics, edited by A
G. ’t Hooft, inThe Whys of Subnuclear Physics, edited by A. Zichichi (Plenum, New York, 1979) pp. 943–982
1979
-
[48]
L. S. Brown, L. G. Yaffe, and C.-X. Zhai, Phys. Rev. D46, 4712 (1992), arXiv:hep-ph/9205213
Pith/arXiv arXiv 1992
- [49]
-
[50]
Billoire, Phys
A. Billoire, Phys. Lett. B92, 343 (1980)
1980
-
[51]
Fischler, Nucl
W. Fischler, Nucl. Phys. B129, 157 (1977)
1977
- [52]
- [53]
-
[54]
C. Anzai, Y. Kiyo, and Y. Sumino, Phys. Rev. Lett. 104, 112003 (2010), arXiv:0911.4335 [hep-ph]
Pith/arXiv arXiv 2010
-
[55]
A. V. Smirnov, V. A. Smirnov, and M. Steinhauser, Phys. Lett. B668, 293 (2008), arXiv:0809.1927 [hep- ph]
Pith/arXiv arXiv 2008
-
[56]
A. V. Smirnov, V. A. Smirnov, and M. Steinhauser, Phys. Rev. Lett.104, 112002 (2010), arXiv:0911.4742 [hep-ph]
Pith/arXiv arXiv 2010
-
[57]
N. Brambilla, J. Komijani, A. S. Kronfeld, and A. Vairo (TUMQCD), Phys. Rev. D97, 034503 (2018), arXiv:1712.04983 [hep-ph]
Pith/arXiv arXiv 2018
-
[58]
A. S. Kronfeld, JHEP12, 108 (2023), arXiv:2310.15137 [hep-ph]
Pith/arXiv arXiv 2023
-
[59]
A. S. Kronfeld, PoSLATTICE2023, 341 (2024), arXiv:2401.07380 [hep-ph]
Pith/arXiv arXiv 2024
-
[60]
A. S. Kronfeld, PoSQCHSC24, 020 (2025), arXiv:2505.20531 [hep-ph]
Pith/arXiv arXiv 2025
-
[61]
A. F. Falk, M. Neubert, and M. E. Luke, Nucl. Phys. B388, 363 (1992), arXiv:hep-ph/9204229
Pith/arXiv arXiv 1992
-
[62]
A. F. Falk and M. Neubert, Phys. Rev. D47, 2965 (1993), arXiv:hep-ph/9209268
Pith/arXiv arXiv 1993
-
[63]
I. I. Y. Bigi and N. G. Uraltsev, Phys. Lett. B321, 412 (1994), arXiv:hep-ph/9311337
Pith/arXiv arXiv 1994
-
[64]
Bottom quark mass from Υ mesons: Charm mass effects,
A. H. Hoang, “Bottom quark mass from Υ mesons: Charm mass effects,” (2000), arXiv:hep-ph/0008102
Pith/arXiv arXiv 2000
-
[65]
Pineda, JHEP , 022 (2001), arXiv:hep-ph/0105008
A. Pineda, JHEP , 022 (2001), arXiv:hep-ph/0105008
Pith/arXiv arXiv 2001
-
[66]
C. Ayala, G. Cvetiˇ c, and A. Pineda, JHEP , 045 (2014), arXiv:1407.2128 [hep-ph]
Pith/arXiv arXiv 2014
-
[67]
A. H. Hoang, A. Jain, I. Scimemi, and I. W. Stewart, Phys. Rev. Lett.101, 151602 (2008), arXiv:0803.4214 [hep-ph]
Pith/arXiv arXiv 2008
-
[68]
X. Garcia i Tormo, Mod. Phys. Lett. A28, 1330028 (2013), arXiv:1307.2238 [hep-ph]
Pith/arXiv arXiv 2013
-
[69]
C. Ayala, X. Lobregat, and A. Pineda, JHEP , 016 (2020), arXiv:2005.12301 [hep-ph]
Pith/arXiv arXiv 2020
-
[70]
H. Takaura, T. Kaneko, Y. Kiyo, and Y. Sumino, JHEP , 155 (2019), arXiv:1808.01643 [hep-ph]
Pith/arXiv arXiv 2019
-
[71]
Bazavovet al.(Fermilab Lattice, MILC, TUMQCD), Phys
A. Bazavovet al.(Fermilab Lattice, MILC, TUMQCD), Phys. Rev. D98, 054517 (2018), arXiv:1802.04248 [hep- lat]
Pith/arXiv arXiv 2018
-
[72]
V. Leino, A. Bazavov, N. Brambilla, A. S. Kronfeld, J. Mayer-Steudte, P. Petreczky, S. Steinbeißer, A. Vairo, and J. H. Weber (TUMQCD), PoSLATTICE2024, 298 (2025), arXiv:2502.01453 [hep-lat]
Pith/arXiv arXiv 2025
-
[73]
N. Brambilla, J. Ghiglieri, and A. Vairo, Phys. Rev. D 81, 054031 (2010), arXiv:0911.3541 [hep-ph]
Pith/arXiv arXiv 2010
-
[75]
B. Fuks, K. Hagiwara, K. Ma, and Y.-J. Zheng, Phys. Rev. D104, 034023 (2021), arXiv:2102.11281 [hep-ph]
Pith/arXiv arXiv 2021
-
[77]
F. Maltoni, C. Severi, S. Tentori, and E. Vryonidou, (2024), arXiv:2401.08751 [hep-ph]
Pith/arXiv arXiv 2024
-
[78]
A. Hayrapetyanet al.(CMS), Rept. Prog. Phys.88, 087801 (2025), arXiv:2503.22382 [hep-ex]
Pith/arXiv arXiv 2025
-
[79]
Aadet al.(ATLAS), (2026), arXiv:2601.11780 [hep- ex]
G. Aadet al.(ATLAS), (2026), arXiv:2601.11780 [hep- ex]
Pith/arXiv arXiv 2026
-
[80]
P. Asadi, E. D. Kramer, E. Kuflik, G. W. Ridgway, T. R. Slatyer, and J. Smirnov, Phys. Rev. Lett.127, 211101 (2021), arXiv:2103.09822 [hep-ph]
Pith/arXiv arXiv 2021
-
[81]
P. Asadi, E. D. Kramer, E. Kuflik, G. W. Ridgway, T. R. Slatyer, and J. Smirnov, Phys. Rev. D104, 095013 (2021), arXiv:2103.09827 [hep-ph]
Pith/arXiv arXiv 2021
-
[82]
G. D. Kribs, T. S. Roy, J. Terning, and K. M. Zurek, Phys. Rev. D81, 095001 (2010), arXiv:0909.2034 [hep- ph]
Pith/arXiv arXiv 2010
discussion (0)
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