Pith. sign in

REVIEW 2 major objections 5 minor 91 references

Scalar dark matter, Neutrino mass and Leptogenesis in a $\rm U(1)_{B-L}$ model

T0 review · 2 major / 5 minor · reviewed 2026-08-14 · deepseek-v4-flash

Pith's one-line read One $U(1)_{B-L}$ model simultaneously satisfies the dark-matter, neutrino, and baryon-asymmetry constraints.

desk verdict Competent combined scan of DM, neutrino mass, and leptogenesis in a known B-L framework; the direct-detection claim is not fully supported because scalar-mediated scattering is omitted, but the qualitative conclusion likely survives. read the letter →

arxiv 1908.09187 v2 pith:DFUC44DE submitted 2019-08-24 hep-ph

classification hep-ph
keywords scalardarkmatterU(1)_{B-L}modelZ'bosonresonantleptogenesisneutrinomassbaryonasymmetryrareBdecaysdirectdetection
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

This paper tries to establish that a $U(1)_{B-L}$ gauge extension of the Standard Model can account, in one framework, for the dark matter relic abundance, the smallness of neutrino masses, the observed baryon asymmetry, and the current limits on rare $B$ and $\tau$ decays. The model adds four exotic fermions with fractional $B-L$ charges for anomaly cancellation, three singlet scalars to break the new symmetry, and one inert scalar as dark matter. A sympathetic reader would care because the same TeV-scale $Z'$ and scalar sector connects several otherwise independent puzzles, and the surviving parameter region is concrete enough to be probed by dilepton searches and direct detection experiments. The paper's bottom line is that the dark-sector constraints, not the flavor ones, are the most restrictive.

What carries the argument

The carrying mechanism is the $Z'$ portal: a new $U(1)_{B-L}$ gauge boson that couples the Standard Model fermions, the inert scalar dark matter, and the four exotic fermions, together with the singlet scalars $\phi_1$, $\phi_2$, $\phi_3$ whose vacuum expectation values break the symmetry. The $Z'$ sets the dark-matter annihilation rate, the direct-detection scattering cross section, and the collider signature, so its mass and coupling anchor the whole parameter scan. The same scalar sector gives Majorana masses to the heavy fermions, while a dimension-five operator involving $\phi_3$ generates tree-level neutrino masses, and near-degenerate heavy fermion masses resonantly enhance the CP asymmetry needed for TeV-scale leptogenesis. These connected portals are what allow a single parameter region to address all the observables.

What would settle it

Recompute the full dark-matter–nucleus scattering rate, including the t-channel exchanges of $H'$, $H_1$, and $H_2$, for the benchmark points in Figure 6; if the resulting spin-independent cross section exceeds the PandaX-II limit for the surviving points, the paper's central surviving-region claim fails.

Watch

Extended reading notes

Core claim

The paper's central claim is that a fully consistent parameter region exists for this model: it reproduces the Planck relic density, stays below the PandaX-II spin-independent scattering limit, obeys the LEP-II and ATLAS bounds on the $Z'$ mass and gauge coupling, fits $3\sigma$ neutrino oscillation data through a type-I seesaw, and yields the observed baryon asymmetry via resonant leptogenesis with TeV-scale heavy fermions. The same scan also satisfies the measured branching ratios of rare semileptonic $B$ and $\tau$ decays. Quantitatively, flavor observables restrict $M_{Z'}/g_{BL}$ to be larger than 7.14 TeV, whereas combining dark matter and flavor constraints pushes this to 9.1 TeV, supporting the paper's statement that the dark sector is more stringent than the flavor sector.

Load-bearing premise

The load-bearing premise is that scalar-mediated dark-matter–nucleon scattering is negligible in the parameter scan, even though the scanned DM–Higgs couplings ($\lambda_{DH} \approx 0.05$ to $0.1$) and scalar masses ($M_{H_1}=M_{H_2}=1$ TeV) could by themselves produce a spin-independent cross section near the current direct-detection limit.

Editorial extensions

If this is right

  • A $Z'$ with $g_{BL}=0.1$ must weigh at least about 2.7 TeV, and one with $g_{BL}=0.3$ at least about 3.7 TeV, to satisfy the ATLAS dilepton bound, while LEP-II fixes $M_{Z'}/g_{BL}>6.9$ TeV.
  • A surviving region of the $M_{Z'}$--$g_{BL}$ plane simultaneously satisfies Planck relic density, PandaX-II direct detection, and collider bounds; the gap around $M_{DM}=500$ GeV and the rejected region at $M_{DM}=750$--$900$ GeV are resonance effects that would appear in any future scan.
  • Dark-matter observables place stronger restrictions on the new gauge parameters than rare $B$ and $\tau$ decays, so the model's viability is decided by dark-matter experiments, not flavor experiments.
  • Resonant leptogenesis works at TeV scale with Yukawa couplings of order $10^{-7}$, and flavor effects slightly enhance the final $B-L$ asymmetry, with a benchmark $\delta_{CP}=219^\circ$ giving specific signs and magnitudes for the electron, muon, and tau asymmetries.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the scalar-mediated direct-detection contribution is computed instead of set aside, the surviving region shown in the paper could shrink or disappear; the strongest test of the claim is therefore a full calculation that includes $H'$, $H_1$, and $H_2$ exchange at the scanned couplings.
  • Because the $Z'$ couples to all Standard Model fermions, the same parameter region should also be testable in future high-energy collider searches and in precision neutral-current measurements, not only in dilepton and rare-decay channels.
  • The paper's resonant-leptogenesis benchmark ties the baryon asymmetry to the Dirac CP phase $\delta_{CP}$, so a precise measurement of $\delta_{CP}$ would provide an independent check of whether this framework's flavor structure is the one realized in nature.
  • The conclusion that dark-sector constraints dominate flavor constraints suggests that future direct-detection experiments, rather than $B$ factories, will be the decisive probes of this model, and that a null result at current sensitivity could be accommodated only in the narrow gap regions away from the $Z'$ and scalar resonances.
Share X Bluesky LinkedIn Reddit HN

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

2 major / 5 minor

Summary. The paper studies a U(1)_{B-L} gauge extension of the Standard Model with four exotic right-handed fermions, three new scalars, and an inert scalar dark matter candidate. It computes the dark matter relic density with micrOMEGAs, the Z'-mediated spin-independent direct detection cross section, collider constraints on (M_{Z'}, g_{BL}) from LEP-II and ATLAS dilepton searches, a tree-level neutrino mass via a dimension-five operator, resonant leptogenesis with TeV-scale heavy fermions, and flavor constraints on the gauge parameters from rare B and tau decays. The central claim is that a common region in (M_{Z'}, g_{BL}) exists that satisfies the Planck relic density, PandaX-II direct detection, LEP-II/ATLAS bounds, neutrino oscillation data, and the observed baryon asymmetry, with dark sector constraints more stringent than flavor constraints.

Significance. If the claimed parameter region survives scrutiny, the model would be a useful unified framework for dark matter, neutrino mass, baryogenesis, and flavor physics. The paper has clear strengths: the anomaly cancellation arithmetic is explicit, the relic density computation uses standard public tools (LanHEP, micrOMEGAs, CalcHEP), and the complementary constraints from cosmology, colliders, and flavor are laid out in a structured way. However, the central compatibility claim rests on two load-bearing technical points that are currently not supported: the neglect of scalar-mediated direct detection, and a dimensional inconsistency in the flavor Wilson coefficients. Because these are local and correctable rather than intrinsic to the model, the appropriate outcome is major revision rather than rejection.

major comments (2)
  1. [Section VI, Eqs. (39)-(44)] The statement that the t-channel scalar exchange via H', H1, H2 'can also give a SI contribution, but this is not relevant for the purpose of our study' is not justified, and it is load-bearing for the direct detection claim. The parameter scan in Section IV.C uses a DM-scalar coupling lambda_DH in 0.05-0.1 and M_H1 = M_H2 = 1 TeV, while the scalar potential in Eq. (6) contains lambda_DH (H†H)(phi_DM†phi_DM). For lambda_DH = 0.1 and m_chi ~ 100-200 GeV, the standard Higgs-portal spin-independent cross section is approximately lambda_DH^2 f_N^2 m_N^4 / (4 pi m_h^4 m_chi^2), which is of order 10^-45 cm^2, at or above the PandaX-II limit shown in Fig. 6. Including this channel could shrink the blue allowed region substantially. The authors should either include the scalar-mediated contribution in the micrOMEGAs computation, or state clearly that the scan is performed only in the Z'-portal limit and set lambda_DH = 0 in the direct detection analysis.
  2. [Section VI, Eqs. (39)-(44)] The new Wilson coefficients C_9^NP and C_nuL^NP are dimensionally inconsistent with the operator basis defined in the paper. In Eq. (38), O_9 = (alpha_em/4pi)(qbar gamma_mu P_L b)(lbar gamma^mu l) has mass dimension 6, so with the prefactor -4 G_F/sqrt(2) V in Eq. (37), C_9 must be dimensionless. However Eq. (40) gives C_9^NP = - g_BL^2/(12 pi alpha_em M_Z'^2), which has mass dimension -2. The same issue appears in Eq. (44) for C_nuL^NP. The correct matching should contain a factor of v^2 (or equivalently 1/G_F) to render the coefficient dimensionless. As written, the Wilson coefficients and the bounds derived from them in Section VI, including the quoted limit M_Z'/g_BL > 7.14 TeV, are not trustworthy. The authors should correct the matching and recompute the flavor constraints.
minor comments (5)
  1. [Section I] In the introduction, 'Fitz Zwicky' should be 'Fritz Zwicky'.
  2. [Section IV.B] In Eq. (21), the symbol n_DM is used but never defined. It should be stated explicitly whether it denotes the U(1)_{B-L} charge of the dark matter field or a nucleon matrix element factor.
  3. [Table II] Several rows contain typographical errors in the particle labels, e.g., 'B0' should be 'B^0' and 'νl' should consistently be written as 'ν_l' for clarity.
  4. [References] Reference [24] is incomplete (shown as '????'), and reference [59] lacks full author and journal information; these should be completed before publication.
  5. [Section V.B] The text in Section V.B would benefit from explicitly stating which flavors are treated as fully decoupled at the temperature scale considered, since the numerical solution of the flavored Boltzmann equations depends on this assumption.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: all quantitative claims are compatibility scans against independent experimental data and external tools, not predictions forced by construction.

full rationale

The paper does not present a derived prediction that reduces to its own input by definition. The relic density and Z'-mediated direct-detection cross section are computed with LanHEP and micrOMEGAs from the model Lagrangian and then compared with Planck, PandaX-II, LEP-II, and ATLAS limits; the neutrino Yukawa scan in Fig. 1 is an allowed-region fit to 3-sigma oscillation data, not a claimed prediction; and the leptogenesis benchmark selects Yukawas of order 1e-7 and epsilon_1 = 0.02 to reproduce the observed baryon asymmetry, which is again a compatibility scan rather than an ab initio derivation. The statement in Sec. IV.B that scalar-mediated direct detection is 'not relevant' is an assumption that could affect the numerical survival region, but it is not a circular reduction: no fitted parameter is renamed as a prediction, and no load-bearing result rests on a self-citation. The authors' earlier works cited as [36,40,41] appear only in the introductory survey of anomaly-free fermion choices and do not carry the central numerical analysis, which relies on independent codes and external experimental constraints. No circular step is identifiable under the stated criteria.

Assumptions & free parameters 6 free parameters · 8 assumptions · 4 invented entities

The central viability claim rests on several tuned parameters and simplifying assumptions: fixed scalar masses and portal couplings in the DM scan, Yukawa couplings fit to oscillation data, a resonant mass degeneracy for leptogenesis, the neglect of scalar-mediated direct detection, and a dimensionally sensitive flavor formula. These are listed above; the DM direct detection and flavor calculations are the least secure.

free parameters (6)
  • M_H1 = M_H2 (additional CP-even scalar masses) = 1 TeV (set equal in the scan)
    The masses of the two new CP-even scalars are fixed to 1 TeV in the DM and flavor scans; resonance positions in relic density and the scale of scalar-mediated direct detection depend on this choice.
  • lambda_DH (DM-Higgs portal coupling) = 0.05-0.1 (scan range)
    Controls DM annihilation through the Higgs portal and the scalar-mediated direct detection cross section, which the paper does not include in Section IV.B.
  • Y' Yukawa couplings (dimension-five neutrino couplings) = order 10^-7 (benchmark)
    The scan in Figure 1 fits these to 3 sigma neutrino oscillation data; the leptogenesis yield also uses this order.
  • Mass splitting Delta M_ij of exotic fermions = Delta M_ij^2 approximately M_i Gamma_j (resonant condition)
    Resonant enhancement of CP asymmetry in leptogenesis requires quasi-degenerate fermions; this tuning is chosen to make the baryon asymmetry match observation.
  • Heavy fermion mass scale m = m such that M1 approximately M2 approximately TeV (1-100 TeV range)
    The four heavy fermion masses are 0.012m, 0.015m, 3.13m, and 3.2m; m is adjusted to bring the scale down to TeV for resonant leptogenesis.
  • epsilon_1 (CP asymmetry benchmark) = 0.02
    Chosen to obtain Y_B-L around 10^-10 in the Boltzmann equations; no independent derivation is given.
assumptions (8)
  • domain assumption Anomaly cancellation by four exotic fermions with fractional B-L charges: -1/3, -2/3, -2/3, -4/3 satisfies Eq. (1).
    The arithmetic in Section II is explicit; the theory is assumed free of triangle anomalies with these charges.
  • standard math Scalar potential bounded below by copositivity criteria in Eq. (9).
    Stated without proof; standard for multi-scalar potentials.
  • domain assumption Type-I seesaw formula m_nu = M_D M_R^{-1} M_D^T with the dimension-five operator in Eq. (3).
    Assumes the effective operator produces a Dirac mass and the seesaw approximation holds.
  • domain assumption Resonant leptogenesis CP asymmetry formulas from [12,77] apply to this model.
    Equations (24)-(28) and (33) are adopted from the resonant leptogenesis literature.
  • domain assumption Sphaleron conversion relation Y_B = (28/79) Y_{B-L} from [65].
    Standard relation used to convert lepton asymmetry to baryon asymmetry.
  • ad hoc to paper Heavy phi_3 decouples and CP-even scalar mixing is minimal: lambda_H1 < lambda_H, lambda_H1 = lambda_H2, v1 = v2, beta < 0.1.
    These simplifying assumptions in Section III.A are chosen to diagonalize the mass matrix and are not motivated by data.
  • ad hoc to paper Scalar-mediated DM-nucleon scattering is negligible in direct detection.
    Section IV.B dismisses the contribution without calculation despite non-zero lambda_DH in the scan.
  • ad hoc to paper All heavy fermion couplings are of the same order and vk/Lambda is approximately 0.01.
    Section III.B uses this to simplify the heavy neutrino mass matrix and produces the quoted mass ratios.
invented entities (4)
  • Z' gauge boson of U(1)B-L independent evidence
    purpose: Mediates DM annihilation and direct detection, collider dilepton signals, and loop contributions to rare B and tau decays.
    Falsifiable via dilepton resonance searches at LHC and LEP-II; the paper uses existing bounds.
  • Four exotic right-handed fermions N_iR
    purpose: Cancel gauge anomalies, provide right-handed neutrinos for type-I seesaw and resonant leptogenesis.
    No specific new collider signature is predicted; they are the ingredients for neutrino mass and baryon asymmetry.
  • New scalars phi_1, phi_2, phi_3
    purpose: Break U(1)B-L, give masses to exotic fermions, generate neutrino mass via dimension-five operator, and set the Z' mass.
    No dedicated search channel or predicted signal is quantified.
  • Inert scalar phi_DM (dark matter) independent evidence
    purpose: Z2-stable singlet scalar constituting the dark matter candidate.
    Predicts a spin-independent DM-nucleon cross section and relic abundance that can be tested by direct detection and cosmological measurements, though the paper uses existing bounds as constraints.

how reviews work

0 comments
Cite this review

Pith. "Pith review of Scalar dark matter, Neutrino mass and Leptogenesis in a $\rm U(1)_{B-L}$ model." pith.science (2026). https://pith.science/paper/DFUC44DE

@misc{pith2026190809187,
  author       = {Pith},
  title        = {Pith review of: Scalar dark matter, Neutrino mass and Leptogenesis in a $\rm U(1)_B-L$ model},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/DFUC44DE}},
  note         = {Machine review of arXiv:1908.09187}
}
abstract

We investigate the phenomenology of singlet scalar dark matter in a simple $\rm U(1)_{B-L}$ gauge extension of standard model, made anomaly free with four exotic fermions. The enriched scalar sector and the new gauge boson $Z^\prime$, associated with $\rm U(1)$ gauge extension, connect the dark sector to the visible sector. We compute relic density, consistent with Planck limit and $Z^\prime$ mediated dark matter-nucleon cross section, compatible with PandaX bound. The mass of $Z^\prime$ and the corresponding gauge coupling are constrained from LEP-II and LHC dilepton searches. We also briefly scrutinize the tree level neutrino mass with dimension five operator. Furthermore, resonant leptogenesis phenomena is discussed with TeV scale exotic fermions to produce the observed baryon asymmetry of the Universe. Further, we briefly explain the impact of flavor in leptogenesis and we also project the combined constraints on Yukawa, consistent with oscillation data and observed baryon asymmetry. Additionally, we restrict the new gauge parameters by using the existing data on branching ratios of rare $B(\tau)$ decay modes. We see that the constraints from dark sector are much more stringent from flavor sector.

Figures

Figures reproduced from arXiv: 1908.09187 by the authors.

Figure 1
Figure 1. FIG. 1: Variation of Yukawa coupling with the sum of observed active neutrino masses(red) and [PITH_FULL_IMAGE:figures/full_fig_p010_1.png] view at source ↗
Figure 2
Figure 2. FIG. 2: Feynman diagrams those contribute to the relic density of DM in scalar and gauge portal [PITH_FULL_IMAGE:figures/full_fig_p011_2.png] view at source ↗
Figure 3
Figure 3. FIG. 3: Variation of relic density with DM mass for different values of gauge coupling [PITH_FULL_IMAGE:figures/full_fig_p012_3.png] view at source ↗
Figures from the paper (11 more)
Figure 4
Figure 4. Figure 4: FIG. 4: t-channel scattering of DM with nucleus. [PITH_FULL_IMAGE:figures/full_fig_p012_4.png]
Figure 5
Figure 5. Figure 5: FIG. 5: Colored lines represent the dilepton signal cross section as a funciton of [PITH_FULL_IMAGE:figures/full_fig_p013_5.png]
Figure 6
Figure 6. Figure 6: FIG. 6: Left panel depicts the [PITH_FULL_IMAGE:figures/full_fig_p015_6.png]
Figure 7
Figure 7. Figure 7: FIG. 7: Tree and loop level decay of lightest right-handed fermion. [PITH_FULL_IMAGE:figures/full_fig_p016_7.png]
Figure 8
Figure 8. Figure 8: FIG. 8: Scattering procesess that effect the yield of right-handed fermion and lepton. [PITH_FULL_IMAGE:figures/full_fig_p017_8.png]
Figure 9
Figure 9. Figure 9: FIG. 9: Left panel represents the reaction rates of decay, inverse decay and scattering process and [PITH_FULL_IMAGE:figures/full_fig_p019_9.png]
Figure 10
Figure 10. Figure 10: FIG. 10: Dependence of CP asymmetry on Dirac CP phase. Vertical dashed lines correspond to [PITH_FULL_IMAGE:figures/full_fig_p020_10.png]
Figure 11
Figure 11. Figure 11: FIG. 11: Left panel projects [PITH_FULL_IMAGE:figures/full_fig_p021_11.png]
Figure 12
Figure 12. Figure 12: FIG. 12: One loop penguin diagram of [PITH_FULL_IMAGE:figures/full_fig_p021_12.png]
Figure 13
Figure 13. Figure 13: FIG. 13: Box diagram of [PITH_FULL_IMAGE:figures/full_fig_p025_13.png]
Figure 14
Figure 14. Figure 14: FIG. 14: Constraints on [PITH_FULL_IMAGE:figures/full_fig_p027_14.png]

Discussion (0). Continue with ORCID to comment.

Reference graph

Works this paper leans on

91 extracted references · 16 canonical work pages

  1. [1]

    Zwicky, Astrophys

    F. Zwicky, Astrophys. J. 86, 217 (1937)

  2. [2]

    The third eigenstate, A′ 3 remains massless and gets absorbed by the new gauge boson Z′, acquiring the mass MZ′ =gBL √ v2 1 + 4v2 2 + 1 9v2 3

    with masses M 2 A′ 1 ≈ 3µ12v2 and M 2 A′ 2 ≈ 6µ12v2 respectively. The third eigenstate, A′ 3 remains massless and gets absorbed by the new gauge boson Z′, acquiring the mass MZ′ =gBL √ v2 1 + 4v2 2 + 1 9v2 3. B. Comments on neutrino mass We can have a tree level Dirac mass for the active neutrinos, which can be constructed from the 5-dimension Yukawa coup...

  3. [3]

    Leptogenesis from the decay of heavy Majorana neutrinos with a hierarchical mass spectrum has been widely discussed in the literature [66–68]

    (27) In the above expression Γj is the tree level decay width of the corresponding heavy fermion. Leptogenesis from the decay of heavy Majorana neutrinos with a hierarchical mass spectrum has been widely discussed in the literature [66–68]. These studies mainly focus different cases 16 like single flavor approximation and flavor consideration. With one flavor...

  4. [4]

    Zwicky, Phys

    F. Zwicky, Phys. Rev. 43, 147 (1933), URL https://link.aps.org/doi/10.1103/PhysRev. 43.147

  5. [5]

    Bertone, D

    G. Bertone, D. Hooper, and J. Silk, Phys. Rept. 405, 279 (2005), hep-ph/0404175

  6. [6]

    Berlin, D

    A. Berlin, D. Hooper, and S. D. McDermott, Phys. Rev. D89, 115022 (2014), 1404.0022

  7. [7]

    Aghanim et al

    N. Aghanim et al. (Planck), Astron. Astrophys. 641, A6 (2020), 1807.06209

  8. [8]

    Buchmuller, P

    W. Buchmuller, P. Di Bari, and M. Plumacher, Annals Phys. 315, 305 (2005), hep- ph/0401240

Show all 91 references
  1. [9]

    Plumacher, Z

    M. Plumacher, Z. Phys. C74, 549 (1997), hep-ph/9604229

  2. [10]

    Buchmuller and M

    W. Buchmuller and M. Plumacher, Int. J. Mod. Phys. A15, 5047 (2000), hep-ph/0007176

  3. [11]

    Giudice, A

    G. Giudice, A. Notari, M. Raidal, A. Riotto, and A. Strumia, Nucl. Phys. B 685, 89 (2004), hep-ph/0310123

  4. [12]

    Strumia, in Les Houches Summer School on Theoretical Physics: Session 84: Particle Physics Beyond the Standard Model (2006), pp

    A. Strumia, in Les Houches Summer School on Theoretical Physics: Session 84: Particle Physics Beyond the Standard Model (2006), pp. 655–680, hep-ph/0608347

  5. [13]

    Davidson, E

    S. Davidson, E. Nardi, and Y. Nir, Phys. Rept. 466, 105 (2008), 0802.2962

  6. [14]

    Pilaftsis and T

    A. Pilaftsis and T. E. J. Underwood, Nucl. Phys. B692, 303 (2004), hep-ph/0309342

  7. [15]

    Aaij et al

    R. Aaij et al. (LHCb), JHEP 06, 133 (2014), 1403.8044

  8. [16]

    Aaij et al

    R. Aaij et al. (LHCb), JHEP 02, 104 (2016), 1512.04442

  9. [17]

    Aaij et al

    R. Aaij et al. (LHCb), Phys. Rev. Lett. 111, 191801 (2013), 1308.1707

  10. [18]

    Huang, M

    Z.-R. Huang, M. A. Paracha, I. Ahmed, and C.-D. L¨ u (2018), 1812.03491

  11. [19]

    Huang, Y

    Z.-R. Huang, Y. Li, C.-D. Lu, M. A. Paracha, and C. Wang, Phys. Rev. D98, 095018 (2018), 1808.03565

  12. [20]

    Aaij et al

    R. Aaij et al. (LHCb), JHEP 07, 084 (2013), 1305.2168

  13. [21]

    Aaij et al

    R. Aaij et al. (LHCb), JHEP 09, 179 (2015), 1506.08777

  14. [22]

    Aaij et al

    R. Aaij et al. (LHCb), Phys. Rev. Lett. 113, 151601 (2014), 1406.6482

  15. [23]

    Aaij et al

    R. Aaij et al. (LHCb) (2019), 1903.09252

  16. [24]

    Bobeth, G

    C. Bobeth, G. Hiller, and G. Piranishvili, JHEP 12, 040 (2007), 0709.4174

  17. [25]

    Aaij et al

    R. Aaij et al. (LHCb), JHEP 08, 055 (2017), 1705.05802. 28

  18. [26]

    Prim (Belle) (????), URL http://moriond.in2p3.fr/2019/EW/slides/6_Friday/1_ morning/1_Markus_Prim.pdf

    M. Prim (Belle) (????), URL http://moriond.in2p3.fr/2019/EW/slides/6_Friday/1_ morning/1_Markus_Prim.pdf

  19. [27]

    Capdevila, A

    B. Capdevila, A. Crivellin, S. Descotes-Genon, J. Matias, and J. Virto, JHEP 01, 093 (2018), 1704.05340

  20. [28]

    Heavy Flavor Averaging Group (2019), URL https://hflav-eos.web.cern.ch/hflav-eos/ semi/spring19/html/RDsDsstar/RDRDs.html

  21. [29]

    Aaij et al

    R. Aaij et al. (LHCb), Phys. Rev. Lett. 120, 121801 (2018), 1711.05623

  22. [30]

    M. A. Ivanov, J. G. Korner, and P. Santorelli, Phys. Rev. D71, 094006 (2005), [Erratum: Phys. Rev.D75,019901(2007)], hep-ph/0501051

  23. [31]

    Wang, Y.-Y

    W.-F. Wang, Y.-Y. Fan, and Z.-J. Xiao, Chin. Phys. C37, 093102 (2013), 1212.5903

  24. [32]

    Ma and R

    E. Ma and R. Srivastava, Phys. Lett. B741, 217 (2015), 1411.5042

  25. [33]

    Ma and R

    E. Ma and R. Srivastava, Mod. Phys. Lett. A30, 1530020 (2015), 1504.00111

  26. [34]

    Nomura and H

    T. Nomura and H. Okada, Phys. Lett. B781, 561 (2018), 1711.05115

  27. [35]

    Geng and H

    C.-Q. Geng and H. Okada, Phys. Dark Univ. 20, 13 (2018), 1710.09536

  28. [36]

    A. Das, N. Okada, and D. Raut, Eur. Phys. J. C78, 696 (2018), 1711.09896

  29. [37]

    A. Das, P. S. B. Dev, and N. Okada (2019), 1906.04132

  30. [38]

    Mishra, M

    S. Mishra, M. Kumar Behera, R. Mohanta, S. Patra, and S. Singirala (2019), 1907.06429

  31. [39]

    Bandyopadhyay, G

    T. Bandyopadhyay, G. Bhattacharyya, D. Das, and A. Raychaudhuri, Phys. Rev.D98, 035027 (2018), 1803.07989

  32. [40]

    Nomura and H

    T. Nomura and H. Okada, Eur. Phys. J. C78, 189 (2018), 1708.08737

  33. [41]

    Nomura and H

    T. Nomura and H. Okada, Nucl. Phys. B941, 586 (2019), 1705.08309

  34. [42]

    Singirala, R

    S. Singirala, R. Mohanta, and S. Patra, Eur. Phys. J. Plus 133, 477 (2018), 1704.01107

  35. [43]

    Singirala, R

    S. Singirala, R. Mohanta, S. Patra, and S. Rao (2017), 1710.05775

  36. [44]

    Patra, W

    S. Patra, W. Rodejohann, and C. E. Yaguna, JHEP 09, 076 (2016), 1607.04029

  37. [45]

    Nanda and D

    D. Nanda and D. Borah, Phys. Rev. D96, 115014 (2017), 1709.08417

  38. [46]

    Biswas, S

    A. Biswas, S. Choubey, and S. Khan, JHEP 08, 062 (2018), 1805.00568

  39. [47]

    Esteban, M

    I. Esteban, M. Gonzalez-Garcia, M. Maltoni, T. Schwetz, and A. Zhou (2020), 2007.14792

  40. [48]

    Griest and D

    K. Griest and D. Seckel, Phys. Rev. D43, 3191 (1991)

  41. [49]

    Edsjo and P

    J. Edsjo and P. Gondolo, Phys. Rev. D56, 1879 (1997), hep-ph/9704361

  42. [50]

    N. F. Bell, Y. Cai, and A. D. Medina, Phys. Rev. D89, 115001 (2014), 1311.6169

  43. [51]

    A. V. Semenov (1996), hep-ph/9608488. 29

  44. [52]

    Pukhov, E

    A. Pukhov, E. Boos, M. Dubinin, V. Edneral, V. Ilyin, D. Kovalenko, A. Kryukov, V. Savrin, S. Shichanin, and A. Semenov (1999), hep-ph/9908288

  45. [53]

    Belanger, F

    G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 176, 367 (2007), hep-ph/0607059

  46. [54]

    Belanger, F

    G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, Comput. Phys. Commun. 180, 747 (2009), 0803.2360

  47. [55]

    T. A. collaboration (2015)

  48. [56]

    Belyaev, N

    A. Belyaev, N. D. Christensen, and A. Pukhov, Comput. Phys. Commun. 184, 1729 (2013), 1207.6082

  49. [57]

    Kong, in The Dark Secrets of the Terascale: Proceedings, TASI 2011, Boulder, Colorado, USA, Jun 6 - Jul 11, 2011 (2013), pp

    K. Kong, in The Dark Secrets of the Terascale: Proceedings, TASI 2011, Boulder, Colorado, USA, Jun 6 - Jul 11, 2011 (2013), pp. 161–198, 1208.0035, URL https://inspirehep.net/ record/1124593/files/arXiv:1208.0035.pdf

  50. [58]

    Schael et al

    S. Schael et al. (DELPHI, OPAL, LEP Electroweak, ALEPH, L3), Phys. Rept. 532, 119 (2013), 1302.3415

  51. [59]

    Cui et al

    X. Cui et al. (PandaX-II), Phys. Rev. Lett. 119, 181302 (2017), 1708.06917

  52. [60]

    Khachatryan et al

    V. Khachatryan et al. (CMS), JHEP 10, 144 (2015), 1504.00936

  53. [61]

    Accomando, C

    E. Accomando, C. Coriano, L. Delle Rose, J. Fiaschi, C. Marzo, and S. Moretti, JHEP 07, 086 (2016), 1605.02910

  54. [62]

    Ahnen et al

    M. Ahnen et al. (MAGIC, Fermi-LAT), JCAP 02, 039 (2016), 1601.06590

  55. [63]

    Rodejohann and C

    W. Rodejohann and C. E. Yaguna, JCAP 1512, 032 (2015), 1509.04036

  56. [64]

    Aprile et al

    E. Aprile et al. (XENON) (2017), 1705.06655

  57. [65]

    D. S. Akerib et al. (LUX), Phys. Rev. Lett. 118, 021303 (2017), 1608.07648

  58. [66]

    J. A. Harvey and M. S. Turner, Phys. Rev. D42, 3344 (1990)

  59. [67]

    P. S. B. Dev, P. Di Bari, B. Garbrecht, S. Lavignac, P. Millington, and D. Teresi, Int. J. Mod. Phys. A 33, 1842001 (2018), 1711.02861

  60. [68]

    Pascoli, S

    S. Pascoli, S. T. Petcov, and A. Riotto, Phys. Rev. D75, 083511 (2007), hep-ph/0609125

  61. [69]

    Abada, S

    A. Abada, S. Davidson, A. Ibarra, F. X. Josse-Michaux, M. Losada, and A. Riotto, JHEP 09, 010 (2006), hep-ph/0605281

  62. [70]

    Davidson and A

    S. Davidson and A. Ibarra, Phys. Lett. B535, 25 (2002), hep-ph/0202239

  63. [71]

    Asaka and T

    T. Asaka and T. Yoshida (2018), 1812.11323. 30

  64. [72]

    S. Iso, N. Okada, and Y. Orikasa, Phys. Rev. D83, 093011 (2011), 1011.4769

  65. [73]

    Pascoli, S

    S. Pascoli, S. Petcov, and A. Riotto, Nucl. Phys. B 774, 1 (2007), hep-ph/0611338

  66. [74]

    Antusch, S

    S. Antusch, S. King, and A. Riotto, JCAP 11, 011 (2006), hep-ph/0609038

  67. [75]

    Nardi, Y

    E. Nardi, Y. Nir, E. Roulet, and J. Racker, JHEP 01, 164 (2006), hep-ph/0601084

  68. [76]

    Granelli, K

    A. Granelli, K. Moffat, and S. Petcov (2020), 2009.03166

  69. [77]

    Abada, S

    A. Abada, S. Davidson, F.-X. Josse-Michaux, M. Losada, and A. Riotto, JCAP 04, 004 (2006), hep-ph/0601083

  70. [78]

    P. S. B. Dev, Springer Proc. Phys. 174, 245 (2016), 1506.00837

  71. [79]

    Beneke, T

    M. Beneke, T. Feldmann, and D. Seidel, Eur. Phys. J. C41, 173 (2005), hep-ph/0412400

  72. [80]

    Buchalla and A

    G. Buchalla and A. J. Buras, Nucl. Phys. B412, 106 (1994), hep-ph/9308272

  73. [81]

    Fajfer and N

    S. Fajfer and N. Koˇ snik, Eur. Phys. J. C75, 567 (2015), 1510.00965

  74. [82]

    Fajfer and N

    S. Fajfer and N. Koˇ snik, Phys. Rev.D87, 054026 (2013), 1208.0759

  75. [83]

    W.-S. Hou, M. Kohda, and F. Xu, Phys. Rev. D90, 013002 (2014), 1403.7410

  76. [84]

    Buchalla and A

    G. Buchalla and A. J. Buras, Nucl. Phys. B548, 309 (1999), hep-ph/9901288

  77. [85]

    Misiak and J

    M. Misiak and J. Urban, Phys. Lett. B451, 161 (1999), hep-ph/9901278

  78. [86]

    Tanabashi et al

    M. Tanabashi et al. (Particle Data Group), Phys. Rev. D98, 030001 (2018)

  79. [87]

    Altmannshofer, A

    W. Altmannshofer, A. J. Buras, D. M. Straub, and M. Wick, JHEP 04, 022 (2009), 0902.0160

  80. [88]

    Colangelo, F

    P. Colangelo, F. De Fazio, P. Santorelli, and E. Scrimieri, Phys. Lett. B395, 339 (1997), hep-ph/9610297

  81. [89]

    Ball and R

    P. Ball and R. Zwicky, Phys. Rev. D71, 014015 (2005), hep-ph/0406232

  82. [90]

    Ball and R

    P. Ball and R. Zwicky, Phys. Rev. D71, 014029 (2005), hep-ph/0412079

  83. [91]

    Altmannshofer, S

    W. Altmannshofer, S. Gori, M. Pospelov, and I. Yavin, Phys. Rev. D89, 095033 (2014), 1403.1269. 31

Pith tools

Reviewed August 14, 2026 · model on record in the stance chip above.