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arxiv: 2606.19403 · v1 · pith:V5UUIQ5Onew · submitted 2026-06-17 · ✦ hep-ph · astro-ph.CO

Emergent Gauge Symmetries in Particle Physics and Cosmology

Pith reviewed 2026-06-26 20:27 UTC · model grok-4.3

classification ✦ hep-ph astro-ph.CO
keywords emergent gauge symmetriesStandard Modeldark energyMajorana neutrino massesHiggs vacuum stabilityultraviolet phase transitiondark mattergravitational waves
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The pith

Standard Model gauge symmetries dissolve in an ultraviolet phase transition near 10^16 GeV.

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

The paper proposes that the gauge symmetries of the Standard Model are emergent rather than fundamental, arising below a phase transition at energies around 10^16 GeV. In this picture the dark energy density and the masses of light Majorana neutrinos both appear at the same order in an expansion in inverse powers of this high scale. The meta-stability of the Higgs vacuum is taken as a hint that the Higgs field links ordinary particle physics to this deep ultraviolet regime. If the idea holds, dark matter might consist of axions or collective excitations from the higher-scale degrees of freedom, with possible signals in neutrino experiments and primordial gravitational waves.

Core claim

In the emergence scenario the Standard Model gauge symmetries dissolve in a phase transition deep in the ultraviolet. The dark energy scale comes out similar to the size of light Majorana neutrino masses. These two quantities appear at the same order in a low energy expansion in inverse powers of the scale of emergence, about 10^16 GeV. The (meta-)stability of the Higgs vacuum may be pointing to some new critical phenomena at very high energy scales, with the Higgs connecting physics at LHC laboratory energies to that in the deep ultraviolet.

What carries the argument

The emergence scenario in which gauge symmetries dissolve in a phase transition at approximately 10^16 GeV, with the Higgs vacuum meta-stability linking low and high energy regimes.

If this is right

  • Dark energy and light Majorana neutrino masses are of comparable size, both generated at order 1/M^2 where M is the emergence scale about 10^16 GeV.
  • Dark matter candidates include axions and phonon-like excitations of degrees of freedom above the emergence scale.
  • Possible tests involve neutrinos as well as gravitational-wave-related signals from the early Universe sensitive to very high energy scales.

Where Pith is reading between the lines

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

  • Combined measurements of dark energy and neutrino masses could test the predicted similarity at the emergence scale.
  • The Higgs connection suggests that improved calculations of vacuum stability might constrain or support the high-energy phase transition.
  • Gravitational wave observations from the early universe could reveal signatures of the gauge symmetry emergence.

Load-bearing premise

The meta-stability of the Higgs vacuum points to new critical phenomena at very high energy scales that connect LHC energies to the deep ultraviolet.

What would settle it

Observation or calculation showing that the dark energy scale and light Majorana neutrino masses do not appear at the same order in the low energy expansion in inverse powers of a scale near 10^16 GeV would falsify the scenario.

Figures

Figures reproduced from arXiv: 2606.19403 by Steven D. Bass.

Figure 1
Figure 1. Figure 1: Above: Higgs boson couplings to different particles and masses measured [PITH_FULL_IMAGE:figures/full_fig_p009_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Running of the Standard Model gauge couplings [PITH_FULL_IMAGE:figures/full_fig_p012_2.png] view at source ↗
read the original abstract

Where do gauge symmetries come from? These lectures develop the idea that the Standard Model might be emergent, with its gauge symmetries dissolving in some phase transition deep in the ultraviolet. The (meta-)stability of the Higgs vacuum may be pointing to some new critical phenomena at very high energy scales, with the Higgs connecting physics at LHC laboratory energies to that in the deep ultraviolet. In the emergence scenario, the dark energy scale comes out similar to the size of light Majorana neutrino masses. These two quantities appear at the same order in a low energy expansion in inverse powers of the scale of emergence, about $10^{16}$ GeV. Dark matter candidates include axions and phonon like excitations of degrees of freedom above the scale of emergence. Possible tests of these ideas involve neutrinos as well as gravitational-waves-related signals from the early Universe, which are sensitive to physics at very high energy scales.

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 / 1 minor

Summary. The manuscript develops the idea that Standard Model gauge symmetries are emergent and dissolve in an ultraviolet phase transition, potentially signaled by Higgs vacuum metastability. It argues that an emergence scale of ~10^16 GeV leads to the dark energy scale and light Majorana neutrino masses appearing at the same order in a low-energy expansion in inverse powers of this scale. Dark matter candidates (axions, phonon-like excitations) and tests via neutrinos and early-Universe gravitational waves are also discussed.

Significance. If the emergence mechanism were equipped with explicit derivations fixing the scale independently and demonstrating the operator structure, the framework could offer a dynamical origin for gauge symmetries and a unified account of disparate scales in particle physics and cosmology, with the Higgs providing a bridge from collider energies to the UV.

major comments (2)
  1. [Abstract] Abstract: The claim that dark energy and neutrino masses 'come out similar' at the same order in the low-energy expansion in 1/M with M~10^16 GeV is presented without any explicit effective Lagrangian, list of contributing operators, or power-counting argument showing why the orders coincide.
  2. [Abstract] Abstract: The emergence scale is introduced so that the numerical similarity between dark energy and neutrino masses holds; no independent principle (e.g., from Higgs metastability) is shown to fix M at 10^16 GeV, rendering the matching a consistency check rather than a prediction.
minor comments (1)
  1. The manuscript is framed as lectures; adding explicit references to prior literature on emergent gauge symmetries and clarifying which statements are new versus review would improve accessibility.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for their careful reading and constructive comments. We address the two major comments point by point below.

read point-by-point responses
  1. Referee: [Abstract] Abstract: The claim that dark energy and neutrino masses 'come out similar' at the same order in the low-energy expansion in 1/M with M~10^16 GeV is presented without any explicit effective Lagrangian, list of contributing operators, or power-counting argument showing why the orders coincide.

    Authors: We agree that the abstract would benefit from greater precision on this point. The manuscript is a set of lectures that develops the conceptual framework rather than a complete effective-field-theory calculation. In the body of the text we discuss the low-energy expansion in inverse powers of the emergence scale, but we do not supply an exhaustive operator list or explicit power counting. We will revise the abstract to state the claim more cautiously and will add a short clarifying paragraph in the main text that sketches the relevant operator dimensions and the reason the two scales appear at the same order. revision: yes

  2. Referee: [Abstract] Abstract: The emergence scale is introduced so that the numerical similarity between dark energy and neutrino masses holds; no independent principle (e.g., from Higgs metastability) is shown to fix M at 10^16 GeV, rendering the matching a consistency check rather than a prediction.

    Authors: The emergence scale is motivated by the possible link to Higgs-vacuum metastability, which the manuscript suggests may signal new critical phenomena near 10^16 GeV. However, the text does not contain an explicit derivation that independently fixes the numerical value of M from the metastability condition. We therefore accept the referee’s characterization that the numerical coincidence is presently a consistency check. In revision we will rephrase the relevant sentences to present the scale as a motivated ansatz whose dynamical origin remains to be demonstrated, and we will note the need for further work to elevate it to a genuine prediction. revision: partial

Circularity Check

1 steps flagged

Dark energy/neutrino mass scale matching asserted at same order in 1/M expansion with M~10^16 GeV chosen to produce the coincidence

specific steps
  1. fitted input called prediction [Abstract]
    "In the emergence scenario, the dark energy scale comes out similar to the size of light Majorana neutrino masses. These two quantities appear at the same order in a low energy expansion in inverse powers of the scale of emergence, about 10^{16} GeV."

    The emergence scale is introduced at the specific value ~10^{16} GeV that places both observed quantities at the same order in the expansion; the claimed similarity is therefore enforced by the choice of input scale rather than derived from the scenario's other assumptions or equations.

full rationale

The paper states that dark energy and light Majorana neutrino masses 'appear at the same order in a low energy expansion in inverse powers of the scale of emergence, about 10^{16} GeV' and presents this numerical similarity as a result of the emergence scenario. No independent derivation fixing the emergence scale (e.g., from Higgs vacuum meta-stability or other UV principle) is supplied in the abstract or described claims; the scale is instead selected to align the two quantities at the same order in the 1/M expansion. This reduces the 'prediction' to a consistency check after fitting M to the observed scales rather than an output fixed by other inputs.

Axiom & Free-Parameter Ledger

1 free parameters · 2 axioms · 1 invented entities

Abstract-only review; the ledger is populated from statements in the abstract. The emergence scale functions as a fitted parameter chosen to equate two observed small quantities. The phase transition and vacuum stability link are domain assumptions without independent derivation shown.

free parameters (1)
  • emergence scale = ~10^16 GeV
    Set to approximately 10^16 GeV so that dark energy and light Majorana neutrino masses appear at the same order in the inverse-power expansion.
axioms (2)
  • domain assumption Gauge symmetries of the Standard Model can dissolve in a phase transition at high energies
    Invoked as the core of the emergence scenario in the abstract.
  • domain assumption Higgs vacuum meta-stability signals new critical phenomena at ultraviolet scales
    Stated as a possible pointer connecting LHC energies to the deep ultraviolet.
invented entities (1)
  • emergence scale no independent evidence
    purpose: Sets the cutoff below which gauge symmetries appear and above which they dissolve
    Introduced to organize the low-energy expansion; no independent falsifiable signature given in the abstract.

pith-pipeline@v0.9.1-grok · 5674 in / 1658 out tokens · 28061 ms · 2026-06-26T20:27:38.130039+00:00 · methodology

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Works this paper leans on

160 extracted references · 10 linked inside Pith

  1. [1]

    Pokorski.Gauge Field Theories, 2nd edition (Cambridge Univ

    S. Pokorski.Gauge Field Theories, 2nd edition (Cambridge Univ. Press, 2000)

  2. [2]

    J. C. Taylor,Gauge Theories of Weak Interactions(Cambridge Univ. Press, 1976)

  3. [3]

    Altarelli, Collider Physics within the Standard Model: a Primer, [arXiv:1303.2842 [hep-ph]]

    G. Altarelli, Collider Physics within the Standard Model: a Primer, [arXiv:1303.2842 [hep-ph]]

  4. [4]

    S. D. Bass, A. De Roeck and M. Kado, The Higgs boson implications and prospects for future discoveries,Nature Rev. Phys.3, 608 (2021)

  5. [5]

    Jakobs and G

    K. Jakobs and G. Zanderighi, The profile of the Higgs boson: status and prospects,Phil. Trans. Roy. Soc. A382, 20230087 (2023)

  6. [6]

    Pokorski, After the Higgs boson discovery: a turning point in particle physics, Phil

    S. Pokorski, After the Higgs boson discovery: a turning point in particle physics, Phil. Trans. Roy. Soc. A382, 20230090 (2023)

  7. [7]

    Altarelli, The Higgs: so simple yet so unnatural,Phys

    G. Altarelli, The Higgs: so simple yet so unnatural,Phys. Scripta T158, 014011 (2013)

  8. [8]

    Jegerlehner, The Standard model as a low-energy effective theory: what is triggering the Higgs mechanism?,Acta Phys

    F. Jegerlehner, The Standard model as a low-energy effective theory: what is triggering the Higgs mechanism?,Acta Phys. Polon. B45, 1167 (2014)

  9. [9]

    Jegerlehner, The Standard Model of Particle Physics as a Conspiracy Theory and the Possible Role of the Higgs Boson in the Evolution of the Early Universe, Acta Phys

    F. Jegerlehner, The Standard Model of Particle Physics as a Conspiracy Theory and the Possible Role of the Higgs Boson in the Evolution of the Early Universe, Acta Phys. Polon. B52, 575 (2021)

  10. [10]

    S. D. Bass, Emergent gauge symmetries: making symmetry as well as breaking it,Phil. Trans. Roy. Soc. A380, 20210059 (2021)

  11. [11]

    S. D. Bass,Emergent gauge symmetries in particle physics and cosmology (World Scientific, 2025)

  12. [12]

    K. G. Wilson and J. B. Kogut, The Renormalization group and the epsilon expansion,Phys. Rept.12, 75 (1974)

  13. [13]

    M. E. Peskin and D. V. Schroeder,An Introduction to quantum field theory (Addison-Wesley, 1995)

  14. [14]

    ’t Hooft, Why Do We Need Local Gauge Invariance in Theories With Vector Particles? An Introduction,NATO Sci

    G. ’t Hooft, Why Do We Need Local Gauge Invariance in Theories With Vector Particles? An Introduction,NATO Sci. Ser. B59, 101 (1980). Zakopane25 printed on June 19, 202633

  15. [15]

    S. D. Bass and J. Krzysiak, Vacuum energy with mass generation and Higgs bosons,Phys. Lett. B803, 135351 (2020)

  16. [16]

    S. D. Bass and J. Krzysiak, The cosmological constant and Higgs mass with emergent gauge symmetries,Acta Phys. Polon. B51, 1251 (2020)

  17. [17]

    S. D. Bass, The cosmological constant and scale hierarchies with emergent gauge symmetries,Phil. Trans. Roy. Soc. A382, 20230092 (2023)

  18. [18]

    S. D. Bass, Cosmology with an emergent standard model,Mod. Phys. Lett. A 40, 2530012 (2025)

  19. [19]

    J. D. Bjorken, A Dynamical origin for the electromagnetic field,Annals Phys. 24, 174 (1963)

  20. [20]

    Bjorken, Emergent gauge bosons, [arXiv:hep-th/0111196 [hep-th]]

    J. Bjorken, Emergent gauge bosons, [arXiv:hep-th/0111196 [hep-th]]

  21. [21]

    Jegerlehner, The Vector Boson and Graviton Propagators in the Presence of Multipole Forces,Helv

    F. Jegerlehner, The Vector Boson and Graviton Propagators in the Presence of Multipole Forces,Helv. Phys. Acta51, 783 (1978)

  22. [22]

    Jegerlehner, The ‘Ether world’ and elementary particles, [arXiv:hep- th/9803021 [hep-th]]

    F. Jegerlehner, The ‘Ether world’ and elementary particles, [arXiv:hep- th/9803021 [hep-th]]

  23. [23]

    Jegerlehner, The Hierarchy Problem and the Cosmological Constant Prob- lem Revisited - A new view on the SM of particle physics,Found

    F. Jegerlehner, The Hierarchy Problem and the Cosmological Constant Prob- lem Revisited - A new view on the SM of particle physics,Found. Phys.49, 915 (2019)

  24. [24]

    Forster, H

    D. Forster, H. B. Nielsen and M. Ninomiya, Dynamical Stability of Local Gauge Symmetry: Creation of Light from Chaos,Phys. Lett. B94, 135 (1980)

  25. [25]

    Wilczek and A

    F. Wilczek and A. Zee, Appearance of Gauge Structure in Simple Dynamical Systems,Phys. Rev. Lett.52, 2111 (1984)

  26. [26]

    ’t Hooft, Emergent Quantum Mechanics and Emergent Symmetries,AIP Conf

    G. ’t Hooft, Emergent Quantum Mechanics and Emergent Symmetries,AIP Conf. Proc.957, 154 (2007)

  27. [27]

    Wetterich, Gauge symmetry from decoupling,Nucl

    C. Wetterich, Gauge symmetry from decoupling,Nucl. Phys. B915, 135 (2017)

  28. [28]

    J. L. Chkareuli, C. D. Froggatt and H. B. Nielsen, Lorentz invariance and origin of symmetries,Phys. Rev. Lett.87, 091601 (2001)

  29. [29]

    Witten, Symmetry and Emergence,Nature Phys.14, 116 (2018)

    E. Witten, Symmetry and Emergence,Nature Phys.14, 116 (2018)

  30. [30]

    Verlinde, Emergence,CERN Courier61, no

    E. Verlinde, Emergence,CERN Courier61, no. 5, 39 (September/October 2021)

  31. [31]

    B. J. Powell, Emergent particles and gauge fields in quantum matter,Con- temp. Phys.61, 96 (2020)

  32. [32]

    Zaanen and A

    J. Zaanen and A. J. Beekman, The Emergence of gauge invariance: The Stay- at-home gauge versus local-global duality,Annals Phys.327, 1146 (2012)

  33. [33]

    Moessner and J

    R. Moessner and J. E. Moore,Topological Phases of Matter(Cambridge Univ. Press, 2021)

  34. [34]

    Baskaran and P

    G. Baskaran and P. W. Anderson, Gauge theory of high temperature super- conductors and strongly correlated Fermi systems,Phys. Rev. B37, 580 (1988)

  35. [35]

    Affleck, Z

    I. Affleck, Z. Zou, T. Hsu and P. W. Anderson, SU (2) gauge symmetry of the large-U limit of the Hubbard model,Phys. Rev. B38, 745 (1988)

  36. [36]

    Sachdev, Emergent gauge fields and the high temperature superconductors, Phil

    S. Sachdev, Emergent gauge fields and the high temperature superconductors, Phil. Trans. Roy. Soc. A374, 20150248 (2016) 34Zakopane25 printed on June 19, 2026

  37. [37]

    G. E. Volovik,The Universe in a helium droplet(Oxford Univ. Press, 2003)

  38. [38]

    G. E. Volovik, Emergent physics: Fermi point scenario,Phil. Trans. Roy. Soc. A366, 2935 (2008)

  39. [39]

    M. A. Levin and X. G. Wen, Colloquium: Photons and electrons as emergent phenomena,Rev. Mod. Phys.77, 871 (2005)

  40. [40]

    X. G. Wen,Quantum Field Theory of Many-Body Systems(Oxford University Press, 2007)

  41. [41]

    Tong, Lectures on the Quantum Hall Effect, [arXiv:1606.06687 [hep-th]]

    D. Tong, Lectures on the Quantum Hall Effect, [arXiv:1606.06687 [hep-th]]

  42. [42]

    Rehn and R

    J. Rehn and R. Moessner, Maxwell electromagnetism as an emergent phe- nomenon in condensed matter,Phil. Trans. Roy. Soc. A374, 20160093 (2016)

  43. [43]

    P. W. Anderson, More Is Different,Science177, 393 (1972)

  44. [44]

    Palacios,Emergence and reduction in physics(Cambridge Univ

    P. Palacios,Emergence and reduction in physics(Cambridge Univ. Press, 2022)

  45. [45]

    O’Raifeartaigh and N

    L. O’Raifeartaigh and N. Straumann, Gauge theory: Historical origins and some modern developments,Rev. Mod. Phys.72, 1 (2000)

  46. [46]

    J. D. Jackson and L. B. Okun, Historical roots of gauge invariance,Rev. Mod. Phys.73, 663 (2001)

  47. [47]

    Straumann, Gauge principle and QED,Acta Phys

    N. Straumann, Gauge principle and QED,Acta Phys. Polon. B37, 575 (2006)

  48. [48]

    J. D. Bjorken and S. D. Drell,Relativistic quantum fields(McGraw-Hill, 1965)

  49. [49]

    Weinberg,The Quantum theory of fields

    S. Weinberg,The Quantum theory of fields. Vol. 1: Foundations(Cambridge University Press, 2005)

  50. [50]

    Fritzsch, M

    H. Fritzsch, M. Gell-Mann and H. Leutwyler, Advantages of the Color Octet Gluon Picture,Phys. Lett. B47, 365 (1973)

  51. [51]

    Fritzsch and M

    H. Fritzsch and M. Gell-Mann, Current algebra: Quarks and what else?,eConf C720906V2, 135 (1972), [arXiv:hep-ph/0208010 [hep-ph]]

  52. [52]

    D. J. Gross and F. Wilczek, Ultraviolet Behavior of Nonabelian Gauge Theo- ries,Phys. Rev. Lett.30, 1343 (1973)

  53. [53]

    H. D. Politzer, Reliable Perturbative Results for Strong Interactions?,Phys. Rev. Lett.30, 1346 (1973)

  54. [54]

    Muta,Foundations of Quantum Chromodynamics: An Introduction to Per- turbative Methods in Gauge Theories, (3rd ed.)(World Scientific, 2010)

    T. Muta,Foundations of Quantum Chromodynamics: An Introduction to Per- turbative Methods in Gauge Theories, (3rd ed.)(World Scientific, 2010)

  55. [55]

    M. A. Shifman, Anomalies in gauge theories,Phys. Rept.209, 341 (1991)

  56. [56]

    S. D. Bass, Spinning protons and gluons in theη ′,Int. J. Mod. Phys. A39, 2441008 (2024)

  57. [57]

    C. A. Aidala, S. D. Bass, D. Hasch and G. K. Mallot, The Spin Structure of the Nucleon,Rev. Mod. Phys.85, 655 (2013)

  58. [58]

    S. D. Bass, The Spin structure of the proton,Rev. Mod. Phys.77, 1257 (2005)

  59. [59]

    R. L. Jaffe and A. Manohar, Theg 1 Problem: Deep inelastic electron scatter- ing and the spin of the proton,Nucl. Phys. B337, 509 (1990)

  60. [60]

    T. W. B. Kibble, Spontaneous symmetry breaking in gauge theories,Phil. Trans. Roy. Soc. A373, 20140033 (2014). Zakopane25 printed on June 19, 202635

  61. [61]

    ’t Hooft, Renormalizable Lagrangians for Massive Yang-Mills Fields,Nucl

    G. ’t Hooft, Renormalizable Lagrangians for Massive Yang-Mills Fields,Nucl. Phys. B35, 167 (1971)

  62. [62]

    ’t Hooft and M

    G. ’t Hooft and M. J. G. Veltman, Regularization and Renormalization of Gauge Fields,Nucl. Phys. B44, 189 (1972)

  63. [63]

    M. J. G. Veltman, Perturbation theory of massive Yang-Mills fields,Nucl. Phys. B7, 637 (1968)

  64. [64]

    C. H. Llewellyn Smith, High-Energy Behavior and Gauge Symmetry,Phys. Lett. B46, 233 (1973)

  65. [65]

    J. S. Bell, High-energy behavior of tree diagrams in gauge theories,Nucl. Phys. B60, 427 (1973)

  66. [66]

    J. M. Cornwall, D. N. Levin and G. Tiktopoulos, Uniqueness of spontaneously broken gauge theories,Phys. Rev. Lett.30, 1268 (1973), [erratum:Phys. Rev. Lett.31, 572 (1973)]

  67. [67]

    J. M. Cornwall, D. N. Levin and G. Tiktopoulos, Derivation of Gauge Invari- ance from High-Energy Unitarity Bounds on the S Matrix,Phys. Rev. D10, 1145 (1974) [erratum:Phys. Rev. D11, 972 (1975)]

  68. [68]

    M. S. Chanowitz, Strong W W scattering at the end of the 90’s: Theory and experimental prospects, [arXiv:hep-ph/9812215 [hep-ph]]

  69. [69]

    M. S. Chanowitz, The No-Higgs signal: Strong WW scattering at the LHC, Czech. J. Phys.55, B45 (2005)

  70. [70]

    Aadet al.[ATLAS], A detailed map of Higgs boson interactions by the AT- LAS experiment ten years after the discovery,Nature607, 52 (2022) [erratum: Nature612, E24 (2022)]

    G. Aadet al.[ATLAS], A detailed map of Higgs boson interactions by the AT- LAS experiment ten years after the discovery,Nature607, 52 (2022) [erratum: Nature612, E24 (2022)]

  71. [71]

    Hayrapetyanet al.[CMS], Stairway to discovery: A report on the CMS programme of cross section measurements from millibarns to femtobarns,Phys

    A. Hayrapetyanet al.[CMS], Stairway to discovery: A report on the CMS programme of cross section measurements from millibarns to femtobarns,Phys. Rept.1115, 3 (2025)

  72. [72]

    G. Aadet al.[ATLAS], Study of Higgs boson pair production in theHH→ bbγγfinal state with 308 fb −1 of data collected at √s= 13 TeV and 13.6 TeV by the ATLAS experiment, [arXiv:2507.03495 [hep-ex]]

  73. [73]

    A. Hayrapetyanet al.[CMS], Constraints on the Higgs boson self-coupling from the combination of single and double Higgs boson production in proton- proton collisions at √s= 13 TeV,Phys. Lett. B861, 139210 (2025)

  74. [74]

    Aadet al.[ATLAS], Combination of Searches for Higgs Boson Pair Pro- duction in pp Collisions at √s=13 TeV with the ATLAS Detector,Phys

    G. Aadet al.[ATLAS], Combination of Searches for Higgs Boson Pair Pro- duction in pp Collisions at √s=13 TeV with the ATLAS Detector,Phys. Rev. Lett.133, 101801 (2024)

  75. [75]

    ATLAS and CMS Collaborations, Highlights of the HL-LHC physics projec- tions by ATLAS and CMS, [arXiv:2504.00672 [hep-ex]]

  76. [76]

    de Blas, M

    J. de Blas, M. Dunford, E. Bagnaschi, A. Freitas, P. P. Giardino, C. Grefe, M. Selvaggi, A. Taliercio, F. Bartels and A. Dainese,et al.Physics Briefing Book: Input for the 2026 update of the European Strategy for Particle Physics, [arXiv:2511.03883 [hep-ex]]

  77. [77]

    A. V. Bednyakov, B. A. Kniehl, A. F. Pikelner and O. L. Veretin, Stability of the Electroweak Vacuum: Gauge Independence and Advanced Precision,Phys. Rev. Lett.115, 201802 (2015). 36Zakopane25 printed on June 19, 2026

  78. [78]

    Degrassi, S

    G. Degrassi, S. Di Vita, J. Elias-Miro, J. R. Espinosa, G. F. Giudice, G. Isidori and A. Strumia, Higgs mass and vacuum stability in the Standard Model at NNLO,JHEP08, 098 (2012)

  79. [79]

    Buttazzo, G

    D. Buttazzo, G. Degrassi, P. P. Giardino, G. F. Giudice, F. Sala, A. Salvio and A. Strumia, Investigating the near-criticality of the Higgs boson,JHEP 12, 089 (2013)

  80. [80]

    Alekhin, A

    S. Alekhin, A. Djouadi and S. Moch, The top quark and Higgs boson masses and the stability of the electroweak vacuum,Phys. Lett. B716, 214 (2012)

Showing first 80 references.