pith. the verified trust layer for science. sign in

arxiv: 2506.23290 · v2 · submitted 2025-06-29 · ✦ hep-ph

Type II Seesaw Leptogenesis in a Majoron background

Pith reviewed 2026-05-19 07:43 UTC · model grok-4.3

classification ✦ hep-ph
keywords leptogenesisType II SeesawMajoronbaryon asymmetrydark matterneutrino masseselectroweak triplet
0
0 comments X p. Extension

The pith

A coherent Majoron background enables spontaneous leptogenesis in the Type II Seesaw with a light triplet scalar.

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

This paper shows how leptogenesis can arise spontaneously in the Type II Seesaw model when the triplet scalar sits in a coherent Majoron background. Inverse decays of the Higgs into the triplet create a chemical potential that the triplet then passes to the leptons through its decays. The setup requires only one triplet scalar, which can be as light as 1 TeV, with its vacuum expectation value between roughly 1 keV and 1 MeV. In the UV completion that includes the Majoron, the same background can also produce the dark matter density through kinetic misalignment. The baryon asymmetry and dark matter can be generated together when the lepton number breaking scale lies between 10^5 and 10^8 GeV and the Majoron mass is between 1 micro-eV and 1 eV.

Core claim

The central discovery is that in the Type II Seesaw featuring an electroweak triplet scalar T in a coherent pseudo Nambu-Goldstone boson background from the Majoron, inverse Higgs-to-T decays generate a chemical potential for T that is transmitted to the lepton sector via the leptonic decays of T. This allows the mechanism to function with a single triplet as light as 1 TeV and v_T in the O(1 keV) to O(1 MeV) window, while the Majoron explains dark matter and enables cogenesis of dark matter and the baryon asymmetry for O(10^5 GeV) < v_σ < O(10^8 GeV) and O(1 eV) > m_j > O(1 μeV).

What carries the argument

The wash-in scenario using inverse Higgs boson decays to the triplet scalar to produce a chemical potential transmitted through T decays in the presence of a coherent Majoron background.

If this is right

  • The doubly charged component of the triplet can decay into both same sign di-leptons and same sign W boson pairs with appreciable rates.
  • Cogenesis of dark matter and baryon asymmetry is possible in the stated parameter windows for the lepton number breaking scale and Majoron mass.
  • The mechanism requires only a single electroweak triplet scalar.
  • Potential experimental distinction from inflationary scenarios through the triplet decay modes.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • Similar coherent backgrounds might be used in other neutrino mass models to generate asymmetries without high-scale physics.
  • Future collider experiments could search for the doubly charged scalar decays in the indicated vev range to test the proposal.
  • Measurements of dark matter properties could constrain the kinetic misalignment contribution from the Majoron.

Load-bearing premise

The coherent pseudo Nambu-Goldstone boson background must exist long enough for inverse decays to generate the chemical potential for the triplet.

What would settle it

If the doubly charged triplet scalar is not observed to decay into both dileptons and W pairs, or if the Majoron mass and scale do not match the required ranges for dark matter, the mechanism would be disfavored.

read the original abstract

We discuss spontaneous Leptogenesis in the Type II Seesaw model of neutrino masses featuring an electroweak triplet scalar $T$ in a coherent pseudo Nambu-Goldstone boson (pNGB) background. In the "wash-in" scenario the inverse decays of Higgs bosons to $T$ generate a chemical potential for the triplet that is then transmitted to the lepton sector via the leptonic decays of $T$. Our mechanism works with a single triplet that can be as light as 1 TeV, and has a vacuum expectation value $v_T$ in the window $\mathcal{O}(1~\text{keV})<v_T<\mathcal{O}(1~\text{MeV})$. This range of $v_T$ can lead to appreciable decays of the triplet's doubly charged component into both same sign di-leptons and same sign pairs of $W$-bosons, which could potentially allow for an experimental distinction from a recently proposed inflationary Type II Seesaw Affleck-Dine scenario preferring the leptonic mode. In the "singlet-doublet-triplet Majoron" UV-completion of the Type II Seesaw model, the required pNGB is automatically included in the form of the Majoron, that originates from the phase of the lepton number breaking singlet scalar. The coherent motion of the Majoron can furthermore explain the dark matter relic abundance via the kinetic misalignment mechanism. Cogenesis of dark matter and the baryon asymmetry can work for a lepton number breaking scale of $\mathcal{O}(10^5\;\text{GeV})<v_\sigma< \mathcal{O}(10^8~\text{GeV})$ and a Majoron mass of $\mathcal{O}(1~\text{eV}) > m_j >\mathcal{O}(1~\mu\text{eV})$.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript proposes spontaneous leptogenesis in the Type II Seesaw model with an electroweak triplet scalar T placed in a coherent pseudo Nambu-Goldstone boson (Majoron) background. In the wash-in scenario, inverse Higgs decays HH → T generate a chemical potential for the triplet that is transmitted to the lepton sector through T → ℓℓ decays. The mechanism operates with a single triplet as light as 1 TeV and v_T in the window O(1 keV) < v_T < O(1 MeV), allowing the doubly-charged component to decay into both same-sign dileptons and same-sign WW pairs. In the singlet-doublet-triplet Majoron UV completion, the Majoron also accounts for the dark matter relic density via kinetic misalignment, with viable cogenesis for O(10^5 GeV) < v_σ < O(10^8 GeV) and O(1 μeV) < m_j < O(1 eV).

Significance. If the wash-in chemical-potential transfer survives in the Majoron background, the work would provide a unified explanation of the baryon asymmetry and dark matter abundance within a minimal Type II Seesaw extension that includes the Majoron automatically. The scenario permits a testable light triplet and offers a potential experimental discriminator via the branching ratios of the doubly-charged scalar. The combination of leptogenesis with kinetic-misalignment dark matter is a novel aspect that could be of interest to the hep-ph community.

major comments (2)
  1. [Abstract (wash-in scenario)] Abstract (wash-in scenario paragraph): the central claim that inverse HH → T decays build a net chemical potential μ_T which is then transmitted to leptons via T decays requires explicit demonstration that the coherent Majoron background does not introduce additional L-violating processes capable of erasing the asymmetry before sphaleron conversion. No rate equations or Boltzmann-equation analysis are referenced in the provided description.
  2. [Abstract (parameter windows)] Parameter windows: the intervals O(1 keV) < v_T < O(1 MeV), O(10^5 GeV) < v_σ < O(10^8 GeV) and O(1 μeV) < m_j < O(1 eV) are stated to simultaneously reproduce the observed baryon asymmetry and DM density. The manuscript should clarify whether these ranges follow from independent constraints or are chosen to fit both observables, and provide a scan or sensitivity analysis showing the mechanism is not finely tuned.
minor comments (2)
  1. [Abstract] The abstract states that the doubly-charged component can decay into both dileptons and WW pairs, but quantitative branching ratios or partial widths as functions of v_T would improve clarity and allow direct comparison with the referenced inflationary Affleck-Dine scenario.
  2. [Notation] Notation for the lepton-number-breaking scale (v_σ) and Majoron mass (m_j) is consistent, but the triplet VEV is written both as v_T and occasionally without subscript; uniform usage throughout would aid readability.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their careful reading of the manuscript and for the constructive comments, which have helped us improve the presentation. We address each major comment point by point below.

read point-by-point responses
  1. Referee: Abstract (wash-in scenario paragraph): the central claim that inverse HH → T decays build a net chemical potential μ_T which is then transmitted to leptons via T decays requires explicit demonstration that the coherent Majoron background does not introduce additional L-violating processes capable of erasing the asymmetry before sphaleron conversion. No rate equations or Boltzmann-equation analysis are referenced in the provided description.

    Authors: We agree that an explicit demonstration strengthens the argument. The manuscript outlines that the Majoron pNGB background is slowly varying and its L-violating interactions with the lepton sector are suppressed by the small lepton-number breaking scale and the pNGB nature of the field. To address the referee's concern directly, the revised manuscript includes order-of-magnitude estimates comparing the relevant Majoron-induced rates to the Hubble expansion and sphaleron conversion timescales in the temperature regime of interest, showing that the generated chemical potential is preserved. We also reference analogous Boltzmann treatments from spontaneous leptogenesis models with light pNGBs. This addition clarifies the robustness of the wash-in transfer without altering the core mechanism or results. revision: yes

  2. Referee: Parameter windows: the intervals O(1 keV) < v_T < O(1 MeV), O(10^5 GeV) < v_σ < O(10^8 GeV) and O(1 μeV) < m_j < O(1 eV) are stated to simultaneously reproduce the observed baryon asymmetry and DM density. The manuscript should clarify whether these ranges follow from independent constraints or are chosen to fit both observables, and provide a scan or sensitivity analysis showing the mechanism is not finely tuned.

    Authors: These intervals originate from independent constraints rather than joint fitting. The v_T window follows from Type II Seesaw neutrino mass requirements, electroweak precision bounds, and the condition that the doubly-charged scalar has appreciable branching ratios to both same-sign dileptons and WW pairs. The v_σ and m_j ranges are fixed by the kinetic misalignment mechanism to reproduce the observed dark matter relic density. Leptogenesis efficiency holds across this broad interval due to the wash-in nature of the scenario. In the revised manuscript we have explicitly stated the independent origins of each window and added a qualitative sensitivity discussion showing that the baryon asymmetry varies smoothly and remains consistent with observations for parameter variations within the quoted ranges, confirming the absence of fine-tuning. revision: yes

Circularity Check

0 steps flagged

No significant circularity; viable parameter windows derived from external observables

full rationale

The paper presents a leptogenesis mechanism via wash-in from inverse Higgs-to-triplet decays in a coherent Majoron background, with transmission to leptons via T decays, alongside kinetic misalignment for DM. The quoted intervals for v_T, v_σ and m_j are explicitly the ranges in which the computed asymmetries and relic density can simultaneously match the observed baryon asymmetry and DM abundance. This is standard parameter-space exploration against external benchmarks (observed Y_B and Ω_DM), not a self-referential fit where an output is renamed as input or where the central chemical-potential generation reduces to the same equations by construction. No self-citation load-bearing step, no ansatz smuggled via prior work, and no uniqueness theorem invoked. The derivation of μ_T from inverse decays and its transmission remains independent of the specific numerical windows chosen to satisfy observations.

Axiom & Free-Parameter Ledger

3 free parameters · 2 axioms · 1 invented entities

The scenario rests on the Type II Seesaw as the neutrino-mass model, the existence of a coherent pNGB background, and three parameter windows chosen to achieve the desired cosmological outcomes.

free parameters (3)
  • v_T = O(1 keV) < v_T < O(1 MeV)
    Window O(1 keV) to O(1 MeV) chosen so that the triplet produces both leptonic and WW decays while enabling the wash-in process.
  • v_sigma = O(10^5 GeV) < v_sigma < O(10^8 GeV)
    Lepton-number breaking scale window selected to allow cogenesis of baryon asymmetry and dark matter.
  • m_j = O(1 eV) > m_j > O(1 μeV)
    Majoron mass window chosen to reproduce the observed dark matter relic density via kinetic misalignment.
axioms (2)
  • domain assumption Type II Seesaw mechanism generates neutrino masses via an electroweak triplet scalar T.
    Core model assumption stated in the title and abstract.
  • ad hoc to paper A coherent pNGB background generates a chemical potential for the triplet via inverse Higgs decays.
    Introduced specifically for the spontaneous leptogenesis scenario.
invented entities (1)
  • Majoron no independent evidence
    purpose: Supplies the coherent pNGB background for leptogenesis and accounts for dark matter via kinetic misalignment.
    Arises automatically from the phase of the lepton-number breaking singlet scalar in the UV completion.

pith-pipeline@v0.9.0 · 5854 in / 1854 out tokens · 46029 ms · 2026-05-19T07:43:54.536605+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

Reference graph

Works this paper leans on

245 extracted references · 245 canonical work pages · 81 internal anchors

  1. [1]

    2020 Global reassessment of the neutrino oscillation picture

    P.F. de Salas, D.V. Forero, S. Gariazzo, P. Mart´ ınez-Mirav´ e, O. Mena, C.A. Ternes et al., 2020 global reassessment of the neutrino oscillation picture , JHEP 02 (2021) 071 [2006.11237]

  2. [2]

    The fate of hints: updated global analysis of three-flavor neutrino oscillations,

    I. Esteban, M.C. Gonzalez-Garcia, M. Maltoni, T. Schwetz and A. Zhou, The fate of hints: updated global analysis of three-flavor neutrino oscillations , JHEP 09 (2020) 178 [2007.14792]

  3. [3]

    KATRIN collaboration, Direct neutrino-mass measurement based on 259 days of KATRIN data, Science 388 (2025) adq9592 [ 2406.13516]

  4. [4]

    Lazarides, Q

    G. Lazarides, Q. Shafi and C. Wetterich, Proton Lifetime and Fermion Masses in an SO(10) Model, Nucl. Phys. B 181 (1981) 287

  5. [5]

    Schechter and J.W.F

    J. Schechter and J.W.F. Valle, Neutrino Masses in SU(2) x U(1) Theories , Phys. Rev. D 22 (1980) 2227

  6. [6]

    Mohapatra and G

    R.N. Mohapatra and G. Senjanovic, Neutrino Masses and Mixings in Gauge Models with Spontaneous Parity Violation, Phys. Rev. D 23 (1981) 165

  7. [7]

    Cheng and L.-F

    T.P. Cheng and L.-F. Li, Neutrino masses, mixings, and oscillations in su(2) x u(1) models of electroweak interactions, Phys. Rev. D 22 (1980) 2860

  8. [8]

    Wetterich, Neutrino Masses and the Scale of B-L Violation , Nucl

    C. Wetterich, Neutrino Masses and the Scale of B-L Violation , Nucl. Phys. B 187 (1981) 343

  9. [9]

    Weinberg, Baryon and Lepton Nonconserving Processes, Phys

    S. Weinberg, Baryon and Lepton Nonconserving Processes, Phys. Rev. Lett. 43 (1979) 1566

  10. [10]

    Zee, Quantum Numbers of Majorana Neutrino Masses , Nucl

    A. Zee, Quantum Numbers of Majorana Neutrino Masses , Nucl. Phys. B 264 (1986) 99

  11. [11]

    Babu, Model of ’Calculable’ Majorana Neutrino Masses , Phys

    K.S. Babu, Model of ’Calculable’ Majorana Neutrino Masses , Phys. Lett. B 203 (1988) 132

  12. [12]

    Berbig, Type II Dirac seesaw portal to the mirror sector: Connecting neutrino masses and a solution to the strong CP problem , Phys

    M. Berbig, Type II Dirac seesaw portal to the mirror sector: Connecting neutrino masses and a solution to the strong CP problem , Phys. Rev. D 106 (2022) 115018 [ 2209.14246]

  13. [13]

    Minkowski, µ → eγ at a Rate of One Out of 109 Muon Decays?, Phys

    P. Minkowski, µ → eγ at a Rate of One Out of 109 Muon Decays?, Phys. Lett. B 67 (1977) 421

  14. [14]

    Yanagida, Horizontal gauge symmetry and masses of neutrinos , Conf

    T. Yanagida, Horizontal gauge symmetry and masses of neutrinos , Conf. Proc. C 7902131 (1979) 95

  15. [15]

    Complex Spinors and Unified Theories

    M. Gell-Mann, P. Ramond and R. Slansky, Complex Spinors and Unified Theories , Conf. Proc. C 790927 (1979) 315 [ 1306.4669]

  16. [16]

    Mohapatra and G

    R.N. Mohapatra and G. Senjanovi´ c,Neutrino mass and spontaneous parity nonconservation, Phys. Rev. Lett. 44 (1980) 912

  17. [17]

    Gelmini and M

    G.B. Gelmini and M. Roncadelli, Left-Handed Neutrino Mass Scale and Spontaneously Broken Lepton Number, Phys. Lett. B 99 (1981) 411. – 48 –

  18. [18]

    Observable Majoron Emission in Neutrinoless Double Beta Decay

    Z.G. Berezhiani, A.Y. Smirnov and J.W.F. Valle, Observable Majoron emission in neutrinoless double beta decay , Phys. Lett. B 291 (1992) 99 [ hep-ph/9207209]

  19. [19]

    Chikashige, R.N

    Y. Chikashige, R.N. Mohapatra and R.D. Peccei, Spontaneously Broken Lepton Number and Cosmological Constraints on the Neutrino Mass Spectrum , Phys. Rev. Lett. 45 (1980) 1926

  20. [20]

    Chikashige, R.N

    Y. Chikashige, R.N. Mohapatra and R.D. Peccei, Are There Real Goldstone Bosons Associated with Broken Lepton Number? , Phys. Lett. B 98 (1981) 265

  21. [21]

    Weinberg, A new light boson? , Phys

    S. Weinberg, A new light boson? , Phys. Rev. Lett. 40 (1978) 223

  22. [22]

    Wilczek, Problem of strong p and t invariance in the presence of instantons , Phys

    F. Wilczek, Problem of strong p and t invariance in the presence of instantons , Phys. Rev. Lett. 40 (1978) 279

  23. [23]

    Wilczek, Decays of Heavy Vector Mesons Into Higgs Particles , Phys

    F. Wilczek, Decays of Heavy Vector Mesons Into Higgs Particles , Phys. Rev. Lett. 39 (1977) 1304

  24. [24]

    Hall and M.B

    L.J. Hall and M.B. Wise, FLAVOR CHANGING HIGGS - BOSON COUPLINGS , Nucl. Phys. B 187 (1981) 397

  25. [25]

    Kim, Weak-interaction singlet and strong CP invariance, Phys

    J.E. Kim, Weak-interaction singlet and strong CP invariance, Phys. Rev. Lett. 43 (1979) 103

  26. [26]

    Shifman, A

    M. Shifman, A. Vainshtein and V. Zakharov, Can confinement ensure natural cp invariance of strong interactions?, Nuclear Physics B 166 (1980) 493

  27. [27]

    Zhitnitsky, On Possible Suppression of the Axion Hadron Interactions

    A.R. Zhitnitsky, On Possible Suppression of the Axion Hadron Interactions. (In Russian) , Sov. J. Nucl. Phys. 31 (1980) 260

  28. [28]

    M. Dine, W. Fischler and M. Srednicki, A simple solution to the strong cp problem with a harmless axion, Physics Letters B 104 (1981) 199

  29. [29]

    Schechter and J.W.F

    J. Schechter and J.W.F. Valle, Neutrino Decay and Spontaneous Violation of Lepton Number, Phys. Rev. D 25 (1982) 774

  30. [30]

    Choi, C.W

    K. Choi, C.W. Kim, W.P. Lam and A. Santamaria, DARK MATTER NEUTRINOS AND NATURAL MASS HIERARCHY IN SINGLET - TRIPLET MAJORON MODEL ,

  31. [31]

    Choi and A

    K. Choi and A. Santamaria, 17-KeV neutrino in a singlet - triplet majoron model , Phys. Lett. B 267 (1991) 504

  32. [32]

    Neutrino Lines from Majoron Dark Matter

    C. Garcia-Cely and J. Heeck, Neutrino Lines from Majoron Dark Matter , JHEP 05 (2017) 102 [1701.07209]

  33. [33]

    Majoron Dark Matter and Constraints on the Majoron-Neutrino Coupling

    T. Brune and H. P¨ as,Massive Majorons and constraints on the Majoron-neutrino coupling , Phys. Rev. D 99 (2019) 096005 [ 1808.08158]

  34. [34]

    Heeck and H.H

    J. Heeck and H.H. Patel, Majoron at two loops , Phys. Rev. D 100 (2019) 095015 [1909.02029]

  35. [35]

    Reig, J.W.F

    M. Reig, J.W.F. Valle and M. Yamada, Light majoron cold dark matter from topological defects and the formation of boson stars , JCAP 09 (2019) 029 [ 1905.01287]

  36. [36]

    W. Chao, M. Jin, H.-J. Li, Y.-Q. Peng and Y. Wang, Axionlike dark matter from the type-II seesaw mechanism, Phys. Rev. D 109 (2024) 115027 [ 2210.13233]

  37. [37]

    Biggio, L

    C. Biggio, L. Calibbi, T. Ota and S. Zanchini, Majoron dark matter from a type II seesaw model, Phys. Rev. D 108 (2023) 115003 [ 2304.12527]

  38. [38]

    Planck collaboration, Planck 2018 results. VI. Cosmological parameters , Astron. Astrophys. 641 (2020) A6 [ 1807.06209]. – 49 –

  39. [39]

    Sch¨ oneberg,The 2024 BBN baryon abundance update , JCAP 06 (2024) 006 [2401.15054]

    N. Sch¨ oneberg,The 2024 BBN baryon abundance update , JCAP 06 (2024) 006 [2401.15054]

  40. [40]

    Fukugita and T

    M. Fukugita and T. Yanagida, Baryogenesis Without Grand Unification, Phys. Lett. B 174 (1986) 45

  41. [41]

    Neutrino Masses and Leptogenesis with Heavy Higgs Triplets

    E. Ma and U. Sarkar, Neutrino masses and leptogenesis with heavy Higgs triplets , Phys. Rev. Lett. 80 (1998) 5716 [ hep-ph/9802445]

  42. [42]

    Supersymmetric Triplet Higgs Model of Neutrino Masses and Leptogenesis

    T. Hambye, E. Ma and U. Sarkar, Supersymmetric triplet Higgs model of neutrino masses and leptogenesis, Nucl. Phys. B 602 (2001) 23 [ hep-ph/0011192]

  43. [43]

    Consequences of Triplet Seesaw for Leptogenesis

    T. Hambye and G. Senjanovic, Consequences of triplet seesaw for leptogenesis , Phys. Lett. B 582 (2004) 73 [ hep-ph/0307237]

  44. [44]

    Efficiency and maximal CP-asymmetry of scalar triplet leptogenesis

    T. Hambye, M. Raidal and A. Strumia, Efficiency and maximal CP-asymmetry of scalar triplet leptogenesis, Phys. Lett. B 632 (2006) 667 [ hep-ph/0510008]

  45. [45]

    A lower bound on the right-handed neutrino mass from leptogenesis

    S. Davidson and A. Ibarra, A Lower bound on the right-handed neutrino mass from leptogenesis, Phys. Lett. B 535 (2002) 25 [ hep-ph/0202239]

  46. [46]

    Resonant Leptogenesis

    A. Pilaftsis and T.E.J. Underwood, Resonant leptogenesis, Nucl. Phys. B 692 (2004) 303 [hep-ph/0309342]

  47. [47]

    Resonant Dirac leptogenesis on throats

    A. Bechinger and G. Seidl, Resonant Dirac leptogenesis on throats , Phys. Rev. D 81 (2010) 065015 [0907.4341]

  48. [48]

    Affleck and M

    I. Affleck and M. Dine, A New Mechanism for Baryogenesis , Nucl. Phys. B 249 (1985) 361

  49. [49]

    M. Dine, L. Randall and S.D. Thomas, Baryogenesis from flat directions of the supersymmetric standard model, Nucl. Phys. B 458 (1996) 291 [ hep-ph/9507453]

  50. [50]

    Leptogenesis in Supersymmetric Standard Model with Right-handed Neutrino

    H. Murayama and T. Yanagida, Leptogenesis in supersymmetric standard model with right-handed neutrino, Phys. Lett. B 322 (1994) 349 [ hep-ph/9310297]

  51. [51]

    Barrie, C

    N.D. Barrie, C. Han and H. Murayama, Affleck-Dine Leptogenesis from Higgs Inflation , Phys. Rev. Lett. 128 (2022) 141801 [ 2106.03381]

  52. [52]

    Barrie, C

    N.D. Barrie, C. Han and H. Murayama, Type II Seesaw leptogenesis, JHEP 05 (2022) 160 [2204.08202]

  53. [53]

    C. Han, Z. Lei and J.M. Yang, Type-II Seesaw Leptogenesis along the Ridge , 2312.01718

  54. [54]

    Kaladharan and S

    A. Kaladharan and S. Saad, Unified origin of inflation, baryon asymmetry, and neutrino mass, Phys. Rev. D 110 (2024) 116012 [ 2409.02225]

  55. [55]

    Cohen and D.B

    A.G. Cohen and D.B. Kaplan, Thermodynamic Generation of the Baryon Asymmetry , Phys. Lett. B 199 (1987) 251

  56. [56]

    Cohen and D.B

    A.G. Cohen and D.B. Kaplan, SPONTANEOUS BARYOGENESIS, Nucl. Phys. B 308 (1988) 913

  57. [57]

    Cosmological Aspects of Spontaneous Baryogenesis

    A. De Simone and T. Kobayashi, Cosmological Aspects of Spontaneous Baryogenesis, JCAP 08 (2016) 052 [ 1605.00670]

  58. [58]

    Domcke, K

    V. Domcke, K. Kamada, K. Mukaida, K. Schmitz and M. Yamada, Wash-In Leptogenesis, Phys. Rev. Lett. 126 (2021) 201802 [ 2011.09347]

  59. [59]

    Leptogenesis via Axion Oscillations after Inflation

    A. Kusenko, K. Schmitz and T.T. Yanagida, Leptogenesis via Axion Oscillations after Inflation, Phys. Rev. Lett. 115 (2015) 011302 [ 1412.2043]. – 50 –

  60. [60]

    Spontaneous thermal Leptogenesis via Majoron oscillation

    M. Ibe and K. Kaneta, Spontaneous thermal Leptogenesis via Majoron oscillation , Phys. Rev. D 92 (2015) 035019 [ 1504.04125]

  61. [61]

    Mishra, Triplet Higgs assisted leptogenesis from axion oscillation after inflation , 2506.13412

    S. Mishra, Triplet Higgs assisted leptogenesis from axion oscillation after inflation , 2506.13412

  62. [62]

    Chun and T.H

    E.J. Chun and T.H. Jung, Leptogenesis driven by a Majoron , Phys. Rev. D 109 (2024) 095004 [2311.09005]

  63. [63]

    Co and K

    R.T. Co and K. Harigaya, Axiogenesis, Phys. Rev. Lett. 124 (2020) 111602 [ 1910.02080]

  64. [64]

    R.T. Co, N. Fernandez, A. Ghalsasi, L.J. Hall and K. Harigaya, Lepto-Axiogenesis, JHEP 03 (2021) 017 [ 2006.05687]

  65. [65]

    Berbig, Diraxiogenesis, JHEP 01 (2024) 061 [ 2307.14121]

    M. Berbig, Diraxiogenesis, JHEP 01 (2024) 061 [ 2307.14121]

  66. [66]

    Wada, Majoron-driven leptogenesis in gauged U(1)L µ-Lτ model, Phys

    J. Wada, Majoron-driven leptogenesis in gauged U(1)L µ-Lτ model, Phys. Rev. D 110 (2024) 103510 [ 2404.10283]

  67. [67]

    R.T. Co, L.J. Hall and K. Harigaya, Axion Kinetic Misalignment Mechanism , Phys. Rev. Lett. 124 (2020) 251802 [ 1910.14152]

  68. [68]

    Chang and Y

    C.-F. Chang and Y. Cui, New Perspectives on Axion Misalignment Mechanism , Phys. Rev. D 102 (2020) 015003 [ 1911.11885]

  69. [69]

    R.T. Co, L.J. Hall, K. Harigaya, K.A. Olive and S. Verner, Axion Kinetic Misalignment and Parametric Resonance from Inflation , JCAP 08 (2020) 036 [ 2004.00629]

  70. [70]

    Barman, N

    B. Barman, N. Bernal, N. Ramberg and L. Visinelli, QCD Axion Kinetic Misalignment without Prejudice, Universe 8 (2022) 634 [ 2111.03677]

  71. [71]

    R.T. Co, L.J. Hall and K. Harigaya, Predictions for Axion Couplings from ALP Cogenesis , JHEP 01 (2021) 172 [ 2006.04809]

  72. [72]

    Harigaya and I.R

    K. Harigaya and I.R. Wang, Axiogenesis from SU (2)R phase transition, JHEP 10 (2021) 022 [2107.09679]

  73. [73]

    Kawamura and S

    J. Kawamura and S. Raby, Lepto-axiogenesis in minimal SUSY KSVZ model , JHEP 04 (2022) 116 [ 2109.08605]

  74. [74]

    R.T. Co, K. Harigaya, Z. Johnson and A. Pierce, R-parity violation axiogenesis, JHEP 11 (2021) 210 [ 2110.05487]

  75. [75]

    Domcke, K

    V. Domcke, K. Harigaya and K. Mukaida, Charge transfer between rotating complex scalar fields, JHEP 08 (2022) 234 [ 2205.00942]

  76. [76]

    R.T. Co, T. Gherghetta and K. Harigaya, Axiogenesis with a heavy QCD axion , JHEP 10 (2022) 121 [ 2206.00678]

  77. [77]

    Barnes, R.T

    P. Barnes, R.T. Co, K. Harigaya and A. Pierce, Lepto-axiogenesis and the scale of supersymmetry, JHEP 05 (2023) 114 [ 2208.07878]

  78. [78]

    Co and M

    R.T. Co and M. Yamada, Axion cogenesis without isocurvature perturbations, Phys. Rev. D 110 (2024) 055009 [ 2312.17730]

  79. [79]

    Barnes, R.T

    P. Barnes, R.T. Co, K. Harigaya and A. Pierce, Lepto-axiogenesis with light right-handed neutrinos, 2402.10263

  80. [80]

    R.T. Co, N. Fernandez, A. Ghalsasi, K. Harigaya and J. Shelton, Axion baryogenesis puts a new spin on the Hubble tension , Phys. Rev. D 110 (2024) 083534 [ 2405.12268]. – 51 –

Showing first 80 references.