Pith. sign in

REVIEW 4 cited by

Why should we care about the top quark Yukawa coupling?

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1411.1923 v2 pith:UDEDESSD submitted 2014-11-07 hep-ph astro-ph.COhep-th

classification hep-phastro-ph.COhep-th
keywords scalecouplingquarkyukawacritexperimentalmeasurementsphysics
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

In the cosmological context, for the Standard Model to be valid up to the scale of inflation, the top quark Yukawa coupling $y_t$ should not exceed the critical value $y_t^{crit}$, coinciding with good precision (about 0.02%) with the requirement of the stability of the electroweak vacuum. So, the exact measurements of $y_t$ may give an insight on the possible existence and the energy scale of new physics above 100 GeV, which is extremely sensitive to $y_t$. We overview the most recent theoretical computations of $y_t^{crit}$ and the experimental measurements of $y_t$. Within the theoretical and experimental uncertainties in $y_t$ the required scale of new physics varies from $10^7$ GeV to the Planck scale, urging for precise determination of the top quark Yukawa coupling.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 139 citations worldwide. Full citation record

  1. Fixed points of the renormalisation group running of quark and fermion mixing matrices in the Standard Model and beyond

    hep-ph 2026-01 unverdicted novelty 6.0 of 10

    Six fixed points exist for the massless one-loop RG running of three-generation fermion mixing matrices, remaining fixed points to all orders via geometric properties of vector fields on the space of mixing matrices.

  2. Probing Solar Heavy Neutrinos with Heliospheric Electrons

    astro-ph.HE 2024-12 conditional novelty 6.0 of 10

    Using Ulysses and SOHO MeV electron data, the authors set the strongest direct upper bound U_e^2 ~ 10^-6 on solar-produced heavy neutral leptons, reaching that value at a mass near 10 MeV.

  3. Ultraviolet boundary condition and the Higgs mass

    hep-ph 2026-07 conditional novelty 3.0 of 10

    Two-loop SM evolution with λ(M_P)=0 and experimental inputs predicts m_h=121.99±2.5 GeV, 3.21 GeV below the measured 125.20 GeV.

  4. Dark Horse, Dark Matter: Revisiting the SO(16)x SO(16)' Nonsupersymmetric Model in the LHC and Dark Energy Era

    hep-th 2019-07 unverdicted novelty 2.0 of 10

    Reexamination of the SO(16)xSO(16)' nonsupersymmetric model for implications on dark energy, vacuum stabilization, dark matter candidates, and gauge-Higgs unification in light of LHC and dark energy data.

Pith tools