REVIEW 3 major objections 4 minor 1 cited by
The paper argues that a fourth generation of quarks and leptons, with no extra free parameters, can supply both a strongly first-order electroweak phase transition and the CP-violating source needed to produce the observed baryon asymmetry
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
2026-08-03 06:58 UTC pith:XUG5KF5C
load-bearing objection Central η_B claim rests on replacing m_t'≈200 TeV with Λ_s≈22 TeV in Eq. (9); until that contradiction is resolved, the BAU estimate is not supported. the 3 major comments →
Lepton sourced baryon asymmetry in the fourth generation model
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 core discovery is that the dimension-six effective operators induced by fourth-generation quarks carry a definite, computable CP-odd phase from the 4×4 CKM matrix, and when the associated operators for the fourth-generation leptons τ′ and ν′ are fed into the established electroweak baryogenesis transport formalism, the predicted baryon-over-entropy ratio comes out at η_B ≈ 10^{-10}, matching the measured value (8.8±0.6)×10^{-11}. The coefficient is fixed by the three-loop heavy-quark penguin amplitude, the dispersive determination of V_ub′, V_cb′, V_tb′, and a two-stage RG estimate of the electroweak symmetry restoration scale. The paper states that no new free parameters are introduced:
What carries the argument
The central object is the effective operator -i(Φ†Φ)¯F_L Φ f_R (a Higgs doublet times left- and right-handed fermion fields), whose imaginary coefficient after symmetry breaking becomes -i s_f g_f v^2/(√2 Λ^2) ϕ ¯f γ5 f. The machinery that carries the argument is the three-loop matching calculation: a t′ quark loop with two charged scalars and a virtual pseudoscalar generates the sequence t′→b′→t→b→t′ and an imaginary product of 4×4 CKM elements — exactly one Jarlskog invariant — while the net vertex-plus-self-energy amplitude is proportional to q² and yields a local four-fermion operator. The scale Λ ≈ 16 TeV is obtained by setting m_t′ equal to the restoration scale Λ_s ≈ 22 TeV from a two
Load-bearing premise
The load-bearing premise is that the top-prime quark mass, despite being ~200 TeV as derived from dispersion relations, can be set equal to the electroweak symmetry restoration scale Λ_s ≈ 22 TeV when evaluating the three-loop operator coefficient; the resulting prediction for η_B is enormously sensitive to that substitution because the coefficient scales as the fourth power of the mass.
What would settle it
Recompute the three-loop CPV operator coefficient without replacing m_t′ by Λ_s — i.e., use m_t′ ≈ 200 TeV — and propagate the result through Eq. (33) and the scaling relation η_B ∝ g_f/Λ². The predicted η_B would fall to about 10^{-14}, far below observation, settling whether the quoted η_B ≈ 10^{-10} is an artifact of the mass substitution.
If this is right
- If the central claim is correct, the observed baryon asymmetry requires no new physics beyond a fourth fermion generation whose masses and mixings are fixed by dispersion relations — no additional CP phases, no tuning.
- The predicted 4×4 CKM elements V_ub′ ~ 2.5×10^{-4}, V_cb′ ~ 3.2×10^{-3}, V_tb′ ~ 5.2×10^{-2} provide concrete targets for B-meson and kaon-unitarity searches; the maximal third-row unitarity violation could resolve the Cabibbo-angle anomaly.
- The same heavy-quark condensates and bound states that make the phase transition first-order also set the effective scale Λ ≈ 16 TeV, tying the strength of the baryogenesis source to the phase-transition dynamics.
- The τ-sourced baryogenesis is predicted to be two orders of magnitude too weak in the SM4, so a future measurement that truly isolates a τ-only source would discriminate this framework from the minimal-flavor-violation scenario.
Where Pith is reading between the lines
- The paper's most delicate step is substituting m_t′ = Λ_s ≈ 22 TeV for the input m_t′ ≈ 200 TeV when evaluating the three-loop coefficient; since the coefficient grows like m_t′^4, keeping 200 TeV would raise Λ by roughly (m_t′/Λ_s)^2 ≈ 80 and drop η_B to ~10^{-14}, so a direct full-theory recomputation without that replacement is the cleanest check.
- If the framework survives that check, it suggests a broader principle: the baryogenesis scale and the electroweak restoration scale are set by the same Yukawa RG flow, meaning measurements of CKM unitarity and of the Higgs self-coupling could indirectly constrain the baryon asymmetry.
- The transport-system scaling from τ to (τ′,ν′) assumes equal relaxation and Yukawa rates; a full SM4-specific solution of the transport equations, including the small mass splitting between τ′ and ν′, would be a natural next step and could either confirm or shift the quoted η_B.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript claims that the Standard Model with a sequential fourth generation (SM4) can accommodate the observed baryon asymmetry, η_B ≈ 10^-10, without adding free parameters. The central construction is a set of dimension-6 CPV operators of the form −i(Φ†Φ) \bar F_L Φ f_R, generated by three-loop diagrams with fourth-generation quarks. The CPV source is traced to a Jarlskog invariant of the 4×4 CKM matrix, whose elements are taken from the author's prior dispersive analyses. The effective operator coefficient is matched at a scale Λ_s ≈ 22 TeV, yielding a new-physics scale Λ ≈ 16 TeV. The η_B prediction is then obtained by scaling the τ-lepton EWBG result of Ref. [34] to fourth-generation leptons τ′, ν′, using the scaling η_B ∝ g_f/Λ².
Significance. If the result were correct, it would be significant: a single extension of the SM would provide both the strongly first-order electroweak phase transition (through bound-state scalars of fourth-generation quarks) and the CPV source needed for baryogenesis, with operator coefficients fixed unambiguously by prior dispersive analyses. The paper contains an explicit three-loop derivation of the effective operator and identifies a well-defined Jarlskog invariant, which are genuine strengths. However, the headline numerical result rests on an internally inconsistent replacement of the t′ mass by the restoration scale, and on a hand-picked RG matching scale. These issues affect the central claim by orders of magnitude and make the prediction unreliable in its present form.
major comments (3)
- [Sec. II, Eq. (9)] The central result Eq. (9) sets m_{t′} = Λ_s, replacing the input m_{t′} ≈ 200 TeV quoted in Sec. I and Sec. III. Sec. III explicitly states that m_{t′} is “much higher than the symmetry restoration scale Λ_s definitely.” The operator coefficient in Eq. (8) is proportional to m_{t′}^4 [1 + Li_2(−Λ_s²/m_{t′}²)]. With m_{t′} = 200 TeV and Λ_s = 22 TeV, the dilogarithm bracket is ≈ 0.988, not c = 1 − π²/12 ≈ 0.178, and (m_{t′}/Λ_s)^4 ≈ 6.8×10³. Thus Eq. (9) underestimates the full-theory coefficient by roughly four orders of magnitude. Repeating the matching with the actual m_{t′} changes Λ in Eq. (33) and η_B in Eq. (35) by orders of magnitude and would violate the EDM bounds quoted in Sec. IV. This is not a parameter uncertainty; it is an internal inconsistency that controls the headline claim.
- [Sec. IV, Fig. 4] The restoration scale Λ_s = m_Z exp(x_s) ≈ 22 TeV is determined by visually adjusting x_s to obtain a smooth RG matching. The choice x_s = 5.5 is called “reasonable,” while x_s = 8.0 is rejected because the curves are “jagged,” but no quantitative criterion is given. Since Λ in Eq. (33) scales as 1/Λ_s², an uncertainty in x_s translates directly into a large uncertainty in Λ and therefore in η_B ∝ Λ^(−2). This effectively introduces a free parameter, contradicting the abstract's claim that no free parameters are added.
- [Sec. IV, Eqs. (35)-(36)] The prediction η_B ≈ 10^(−10) is obtained by scaling the τ-lepton result of Ref. [34] via η_B ∝ g_f/Λ², assuming equal relaxation rates, Yukawa rates, diffusion lengths, and interaction lengths for τ′_L and ν′_L. No transport equations for the fourth-generation leptons are actually solved. Given that the manuscript itself acknowledges that source-term methods (VIA vs. WKB) can change η_B by orders of magnitude, this scaling assumption is a further unquantified source of uncertainty in the central numerical claim.
minor comments (4)
- [Sec. III, Eq. (19)] The unitarity relation is written as λ_d + λ_s + λ_s = −λ_b′; the second term should be λ_b, i.e., λ_d + λ_s + λ_b = −λ_b′.
- [Sec. II, Eq. (8)] The symbol g_t is used for the top-quark Yukawa coupling, but in Eq. (8) the factor g_t² multiplies m_{t′}^4. It should be clarified whether this is the t′ Yukawa coupling g_{t′} or the top Yukawa g_t, and the notation should be made consistent with Sec. IV.
- [Sec. IV, Fig. 4] The smoothness criterion for choosing x_s = 5.5 is described qualitatively. A quantitative measure (e.g., a tolerance on the discontinuity of g²_L and g²_t) would improve reproducibility.
- [Abstract] The phrase “no free parameters are added” is too strong given the choice of x_s (or Λ_s) and the assumption of equal rates for τ′ and ν′ in Sec. IV. This should be softened or explicitly qualified.
Circularity Check
No significant circularity; the numerical claim is conditional on an inconsistent matching-scale substitution, but that is a correctness defect, not a circular construction.
full rationale
Walking the derivation chain, I find no step where a 'prediction' is equivalent by construction to its input. The Jarlskog invariant in Eq. (32) is obtained from 4x4 CKM elements solved from dispersive constraints using external inputs (Wolfenstein parameters, m_b, m_s, m_W), and the results are checked against measured loose bounds; η_B plays no role in that derivation. The dimension-6 operator coefficient in Eqs. (4)-(9) is obtained by an explicit three-loop matching calculation; the BAU is then read off from the published tau-lepton computation of Ref. [34] via the scaling law in Eq. (35)/(36), not fitted to η_B. The heavy reliance on the author's prior dispersive analyses supplies m_t', m_b', m_tau', m_4 and the restoration scale; these are parameter-free prior results with stated assumptions that do not include the BAU and are externally falsifiable by collider searches, so under the review rules they count as independent support rather than circularity. The serious flaw is the ad hoc replacement 'Hence, we set m_t' = Lambda_s' (Sec. II, before Eq. (9)), which contradicts the paper's own input m_t' ≈ 200 TeV (Sec. I) and Sec. III's statement that m_t' is 'much higher than the symmetry restoration scale Lambda_s definitely.' Because Eq. (8) scales as m_t'^4 [1+Li_2(-Lambda_s^2/m_t'^2)], this substitution changes Lambda (Eq. (33)) and hence eta_B (Eq. (35)) by orders of magnitude. That is a serious internal-consistency and robustness problem, but it is not a circular reduction of the prediction to its input.
Axiom & Free-Parameter Ledger
free parameters (1)
- x_s (RG matching point / restoration scale Λ_s = m_Z exp(x_s)) =
x_s = 5.5 → Λ_s ≈ 22 TeV
axioms (5)
- domain assumption Electroweak symmetry is restored above a high scale Λ_s; mixing amplitudes vanish for m_Q > Λ_s.
- domain assumption The CPV source is dominated by the three-loop diagram with transition t'→b'→t→b→t' and the product V*_{t'b'} V_{tb'} V*_{tb} V_{t'b}; other quark-loop contributions are negligible.
- domain assumption For heavy fermions f = t, τ', ν', the effective operator coefficient is proportional to g_f; for light fermions the parametrization fails but their BAU contribution is negligible.
- domain assumption The transport equations and scaling law η_B ∝ y_f/Λ^2 from [34] apply to fourth-generation leptons with the same benchmark parameters and equal relaxation/Yukawa rates for τ'_L and ν'_L.
- ad hoc to paper Matching of the effective operator is performed at m_t' = Λ_s, replacing the actual t' mass (≈200 TeV) by the restoration scale (≈22 TeV).
invented entities (2)
-
Sequential fourth generation fermions t', b', τ', ν'
no independent evidence
-
Bound-state scalar η (and pseudoscalar) of t', b' quarks
no independent evidence
read the original abstract
We demonstrate that the observed baryon asymmetry in the Universe can be accommodated in the extended Standard Model with sequential fourth generation fermions (SM4). We first construct the dimension-6 effective operators of the type $-i(\Phi^\dagger\Phi)\bar F_L\Phi f_R$ induced by fourth generation quarks, which carry the $CP$ violation (CPV) source from the $4\times 4$ Cabibbo-Kobayashi-Maskawa (CKM) matrix, $\Phi$ ($F_L$, $f_R$) being a Higgs double (left-handed fermion doublet, right-handed fermion singlet). The required inputs of the fourth generation fermion masses were derived in our previous dispersive analyses on heavy quark decays and neutral meson mixing. The similar framework allows the determination of the $4\times 4$ CKM matrix elements $V_{ib'}$, $i=u$, $c$ and $t$, such that the strength of the CPV source can be evaluated unambiguously. The dimension-6 operators associated with fourth generation leptons, as implemented into the formalism for the electroweak baryogenesis in the literature, lead to the baryon-over-entropy ratio $\eta_B\approx 10^{-10}$.
Figures
Forward citations
Cited by 1 Pith paper
-
LHC di-dijet excesses as signals of fourth-generation tetraquarks
LHC di-dijet excesses are attributed to resonant and non-resonant production of b'b'b'b' tetraquarks from fourth-generation quarks of mass ~2 TeV, with dijet resonances from color-octet bound states in a Yukawa potential.
Reference graph
Works this paper leans on
-
[1]
H. n. Li, Phys. Rev. D107, no.9, 094007 (2023)
2023
-
[2]
Progress of Theoretical Bootstrap
+ r3m3 m4(m2 W −m 2 3) .(B15) Our alternative strategy to solve the coupled Eqs. (B9)-(B11) and (B13) is detailed as follows. We first solve for u3 andv 3 in terms ofu 1 andv 1 from the real part of Eq. (B9) u1 m2 4 −m 2 1 m2 W −m 2 1 + m2 4 −m 2 2 m2 W −m 2 2 +u 3 m2 4 −m 2 3 m2 W −m 2 3 =v 1 m2 4 −m 2 1 m2 W −m 2 1 +v 3 m2 4 −m 2 3 m2 W −m 2 3 ,(B16) an...
-
[3]
H. n. Li, [arXiv:2306.03463 [hep-ph]]
-
[4]
H. n. Li, Phys. Rev. D108, no.5, 054020 (2023)
2023
-
[5]
G. F. Chew, Rev. Mod. Phys.34, no.3, 394-401 (1962)
1962
-
[6]
H. n. Li, Chin. J. Phys.92, 1043-1054 (2024)
2024
-
[7]
van Leeuwen, Stud
R. van Leeuwen, Stud. Hist. Phil. Sci.104(2024), 130-149
2024
-
[8]
J. T. Cushing, Stud. Hist. Phil. Sci. A16, 31-48 (1985)
1985
-
[9]
H. n. Li, Phys. Rev. D109, no.11, 115024 (2024)
2024
-
[10]
G. F. Chew and J. Finkelstein, Phys. Rev. Lett.50, 795 (1983)
1983
-
[11]
H. n. Li, JHEP09(2025), 037
2025
-
[12]
H. n. Li, J. Phys. G52(2025) 025001
2025
-
[13]
P. Q. Hung and C. Xiong, Nucl. Phys. B847, 160-178 (2011)
2011
-
[14]
W. A. Bardeen, C. T. Hill and M. Lindner, Phys. Rev. D41(1990) 1647
1990
-
[15]
Chen and H
N. Chen and H. J. He, JHEP04, 062 (2012); O. Eberhardt, G. Herbert, H. Lacker, A. Lenz, A. Menzel, U. Nierste and M. Wiebusch, Phys. Rev. Lett.109, 241802 (2012); A. Djouadi and A. Lenz, Phys. Lett. B715, 310-314 (2012); E. Kuflik, Y. Nir and T. Volansky, Phys. Rev. Lett.110, no.9, 091801 (2013)
2012
-
[16]
Enkhbat, W
T. Enkhbat, W. S. Hou and H. Yokoya, Phys. Rev. D84, 094013 (2011)
2011
- [17]
-
[18]
H. J. He, N. Polonsky and S. f. Su, Phys. Rev. D64, 053004 (2001)
2001
-
[19]
A. D. Sakharov, Pisma Zh. Eksp. Teor. Fiz.5, 32-35 (1967)
1967
- [20]
-
[21]
G. R. Farrar and M. E. Shaposhnikov, Phys. Rev. D50, 774 (1994)
1994
-
[22]
G. R. Farrar and M. E. Shaposhnikov, Phys. Rev. Lett.70, 2833-2836 (1993) [erratum: Phys. Rev. Lett.71, 210 (1993)]
1993
-
[23]
M. B. Gavela, M. Lozano, J. Orloff and O. Pene, Nucl. Phys. B430, 345-381 (1994)
1994
-
[24]
M. B. Gavela, P. Hernandez, J. Orloff and O. Pene, Mod. Phys. Lett. A9, 795-810 (1994)
1994
-
[25]
Kajantie, M
K. Kajantie, M. Laine, K. Rummukainen and M. E. Shaposhnikov, Phys. Rev. Lett.77, 2887-2890 (1996)
1996
-
[26]
M. B. Gavela, P. Hernandez, J. Orloff, O. Pene and C. Quimbay, Nucl. Phys. B430, 382-426 (1994)
1994
-
[27]
Csikor, Z
F. Csikor, Z. Fodor and J. Heitger, Phys. Rev. Lett.82, 21-24 (1999)
1999
-
[28]
Rummukainen, M
K. Rummukainen, M. Tsypin, K. Kajantie, M. Laine and M. E. Shaposhnikov, Nucl. Phys. B532, 283-314 (1998)
1998
-
[29]
S. R. Coleman and E. J. Weinberg, Phys. Rev. D7(1973) 1888-1910
1973
-
[30]
Y. Aoki, F. Csikor, Z. Fodor and A. Ukawa, Phys. Rev. D60, 013001 (1999)
1999
-
[31]
J. van de Vis, J. de Vries and M. Postma, [arXiv:2508.09989 [hep-ph]]
-
[32]
Dolan and R
L. Dolan and R. Jackiw, Phys. Rev. D9(1974) 3320-3341
1974
-
[33]
Balazs, G
C. Balazs, G. White and J. Yue, JHEP03(2017), 030
2017
-
[34]
For light fermions, the parametrization does not hold in the SM4, because contributions from other types of diagrams may be comparable to that from Fig
applies to heavy fermionsf=t, τ ′, ν′, and theCP-odd phase identified above is maximal. For light fermions, the parametrization does not hold in the SM4, because contributions from other types of diagrams may be comparable to that from Fig. 2(b). For instance, changing the virtual pseudoscalar to a virtualZboson causes a suppression factorg/g b′ from the ...
- [35]
-
[36]
De Vries, M
J. De Vries, M. Postma and J. van de Vis, JHEP04(2019), 024
2019
-
[37]
Zhang, S
X. Zhang, S. K. Lee, K. Whisnant and B. L. Young, Phys. Rev. D50(1994), 7042-7047
1994
-
[38]
Joyce, T
M. Joyce, T. Prokopec and N. Turok, Phys. Lett. B338, 269-275 (1994)
1994
-
[39]
D. J. H. Chung, B. Garbrecht, M. J. Ramsey-Musolf and S. Tulin, Phys. Rev. D81(2010), 063506
2010
-
[40]
D. J. H. Chung, B. Garbrecht, M. J. Ramsey-Musolf and S. Tulin, Phys. Rev. Lett.102, 061301 (2009)
2009
-
[41]
Fuchs, M
E. Fuchs, M. Losada, Y. Nir and Y. Viernik, JHEP05, 056 (2020)
2020
-
[42]
Alonso-Gonz´ alez, L
J. Alonso-Gonz´ alez, L. Merlo and S. Pokorski, JHEP06, 166 (2021)
2021
-
[43]
Y. Z. Li, M. J. Ramsey-Musolf and J. H. Yu, [arXiv:2404.19197 [hep-ph]]
- [44]
-
[45]
Bodeker, L
D. Bodeker, L. Fromme, S. J. Huber and M. Seniuch, JHEP02(2005), 026
2005
-
[46]
Fromme and S
L. Fromme and S. J. Huber, JHEP03(2007), 049
2007
-
[47]
A. B. Beneito, I, A. Palavri´ c and A. Sainaghi, [arXiv:2512.14813 [hep-ph]]
-
[48]
Koˇ snik, A
N. Koˇ snik, A. Palavri´ c and A. Smolkoviˇ c, Phys. Rev. D112(2025) no.9, 095046
2025
-
[49]
C. Lee, V. Cirigliano and M. J. Ramsey-Musolf, Phys. Rev. D71(2005), 075010
2005
-
[50]
F. P. Huang, P. H. Gu, P. F. Yin, Z. H. Yu and X. Zhang, Phys. Rev. D93(2016) no.10, 103515
2016
-
[51]
de Vries, M
J. de Vries, M. Postma, J. van de Vis and G. White, JHEP01(2018), 089. 18
2018
-
[52]
Jarlskog, Phys
C. Jarlskog, Phys. Rev. Lett.55(1985) 1039
1985
-
[53]
Jarlskog, Z
C. Jarlskog, Z. Phys. C29(1985) 491-497
1985
-
[54]
M. E. Shaposhnikov, JETP Lett.44(1986) 465-468
1986
-
[55]
Silvestrini, [arXiv:1905.00798 [hep-ph]]
L. Silvestrini, [arXiv:1905.00798 [hep-ph]]
Pith/arXiv arXiv 1905
-
[56]
H. n. Li, H. Umeeda, F. Xu and F. S. Yu, Phys. Lett. B810, 135802 (2020)
2020
-
[57]
H. n. Li, Phys. Rev. D107, no.5, 054023 (2023)
2023
-
[58]
Y. T. Chien and H. n. Li, Phys. Rev. D97, no.5, 053006 (2018)
2018
-
[59]
A. K. Alok, A. Dighe and D. London, Phys. Rev. D83, 073008 (2011)
2011
-
[60]
Y. H. Ahn, H. Y. Cheng and S. Oh, Phys. Lett. B703, 571-575 (2011)
2011
-
[61]
Navas et al
S. Navas et al. (Particle Data Group), Phys. Rev. D110, 030001 (2024)
2024
-
[62]
G. Kaur, G. Ahuja, D. Shukla and M. Gupta, Int. J. Mod. Phys. A39(2024) no.25, 2450102
2024
-
[63]
Kitahara, Int
T. Kitahara, Int. J. Mod. Phys. A39(2024) no.26n27, 2442011
2024
-
[64]
Gorchtein, V
M. Gorchtein, V. Katyal, B. Ohayon, B. K. Sahoo and C. Y. Seng, Phys. Rev. Res.7(2025) no.4, 4
2025
-
[65]
C. Y. Seng, Mod. Phys. Lett. A37, no.02, 2230002 (2022)
2022
-
[66]
S. J. Huber, M. Pospelov and A. Ritz, Phys. Rev. D75, 036006 (2007)
2007
-
[67]
J. M. Cline and B. Laurent, Phys. Rev. D104(2021) no.8, 083507
2021
-
[68]
Joyce, T
M. Joyce, T. Prokopec and N. Turok, Phys. Rev. Lett.75(1995), 1695-1698 [erratum: Phys. Rev. Lett.75(1995), 3375]
1995
-
[69]
J. M. Cline, M. Joyce and K. Kainulainen, JHEP07(2000), 018
2000
-
[70]
J. M. Cline, Phil. Trans. Roy. Soc. Lond. A376, 20170116 (2018), [arXiv:1704.08911 [hep-ph]]
Pith/arXiv arXiv 2018
-
[71]
R. N. Mohapatra and X. m. Zhang, Phys. Rev. D45(1992), 2699-2705
1992
-
[72]
G. F. Giudice and M. E. Shaposhnikov, Phys. Lett. B326(1994), 118-124
1994
-
[73]
Fuchs, M
E. Fuchs, M. Losada, Y. Nir and Y. Viernik, JHEP07(2021), 060
2021
-
[74]
Joyce, T
M. Joyce, T. Prokopec and N. Turok, Phys. Rev. D53(1996), 2930-2957
1996
-
[75]
J. van de Vis, P. Schicho, L. Niemi, B. Laurent, J. Hirvonen and O. Gould, [arXiv:2510.27691 [hep-ph]]
-
[76]
C. L. Bennettet al.[WMAP], Astrophys. J.583(2003), 1-23
2003
-
[77]
Aghanimet al.[Planck], Astron
N. Aghanimet al.[Planck], Astron. Astrophys.641(2020), A6 [erratum: Astron. Astrophys.652(2021), C4]
2020
-
[78]
B. D. Fields, K. A. Olive, T. H. Yeh and C. Young, JCAP03(2020), 010 [erratum: JCAP11(2020), E02]
2020
-
[79]
Holdom, Phys
B. Holdom, Phys. Rev. Lett.57, 2496 (1986), [Erratum-ibid. 58, 177 (1987)]; W. A. Bardeen, C. T. Hill and M. Lindner, Phys. Rev. D41, 1647 (1990); C. T. Hill, M. A. Luty and E. A. Paschos, Phys. Rev. D43, 3011 (1991); T. Elliott and S. F. King, Phys. Lett. B283, 371 (1992)
1986
-
[80]
P. Q. Hung and C. Xiong, Nucl. Phys. B848(2011) 288-302
2011
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.