Search arXiv⌕ Search

arXiv · hep-ph/9706518

The asymptotics of the transition form factor γγ* -> pi^o and QCD sum rules

Abstract

In this paper we present the result of a direct QCD sum rule calculation of the transition form factor γγ* -> pi^o in the region of moderately large invariant momentum Q^2 > 1GeV^2 of the virtual photon. In contrast to pQCD, we make no assumptions about the shape of the pion distribution amplitude ϕ_π(x). Our results agree with the Brodsky-Lepage proposal that the Q^2-dependence of this form factor is given by an interpolation between its Q^2=0 value fixed by the axial anomaly and 1/Q^2 pQCD behaviour for large Q^2, with normalization corresponding to the asymptotic form ϕ_π^as (x)=6 f_πx (1-x) of the pion distribution amplitude. Our prediction for the from factor $F_{γ^*γ^*π^\circ}(q_1^2 = 0,q_2^2 = -Q^2)$ is in good agreement with new CLEO data.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

A. V. Radyushkin, R. Ruskov. 1997-06-26. The asymptotics of the transition form factor γγ* -> pi^o and QCD sum rules. https://arxiv.org/abs/hep-ph/9706518

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Particle Correlations in Jets

We study particle correlations in high energy jets by comparing the measured energy-energy correlator (EEC) with that constructed from two individual energy flows with respect to the jet axis. This comparison demonstrates that the genuine correlations are stronger at moderate/large angle across all jet energies, indicating that they are coming from correlated splitting. Meanwhile, at small angle, they increase with jet energy, exhibiting a peculiar pattern that can be used to explore jet energy loss in heavy ion collisions. This method will provide a unique tool to disentangle different physics, by comparing the genuine correlations in jet EEC between heavy-ion collisions and proton-proton collisions.

hep-ph↗

Reality-constrained Minimal Yukawa Structure in SO(10) GUT

We investigate the minimal Yukawa sector of $\mathrm{SO}(10)$ grand unified theories with Higgs representations $\mathbf{10}_{\mathbb{R}}\oplus\mathbf{120}_{\mathbb{R}}\oplus\mathbf{126}$. Taking $\mathbf{10}_{\mathbb{R}}$ and $\mathbf{120}_{\mathbb{R}}$ to be real scalars, we derive the corresponding reality conditions for their weak-doublet components and revisit previously reported fermion mass relations. We find a relative sign difference between the reality constraints on the two weak doublets in $\mathbf{120}_{\mathbb{R}}$, introducing a new magnitude parameter in the mass relations. We establish this result through four complementary approaches: an explicit $\mathrm{SO}(10)$ tensorial calculation of invariants, a Pati-Salam embedding map, an algorithm transporting reality structures from parent to daughter irreps, and an $\mathrm{SU}(5)$ calculation using the $\mathrm{SO}(10)$ oscillator method, all yielding consistent results. The methods for determining reality conditions can be applied to any parent-daughter representation pair of $\mathrm{SO}(10)$ and its Pati-Salam subgroup, while the transport algorithm generalizes to arbitrary groups $H\subset G$. Incorporating the correct mass relations, we perform an extensive numerical scan and find that the model successfully reproduces SM fermion masses and mixings, including recent precision measurements of solar oscillation parameters by JUNO. It accommodates both octants of $θ_{23}$ while mildly disfavoring $δ_\mathrm{PMNS} \sim (140^\circ - 220^\circ)$. The model predicts a strongly hierarchical right-handed neutrino spectrum $(10^{5},10^{12},10^{15})$ GeV and a neutrinoless double beta decay parameter $m_{ββ}\sim 3$-$4$ meV, just below future experimental sensitivity. Proton decay is dominated by $p\toπ^+\overlineν$ and $p\toπ^0 e^+$, making these channels testable in upcoming experiments.

hep-ph↗

Weak Triplet Models of Neutrino Magnetic Moments

Experimental limits on neutrino magnetic moments remain several orders of magnitude above the predictions of the Standard Model; therefore, any future detection would provide unambiguous evidence for new physics. In models with Dirac neutrinos, however, mechanisms that enhance the magnetic moment typically generate excessively large neutrino masses. Recently, it has been argued that in frameworks where neutrinos mix with weak-triplet Dirac fermions, the magnetic moment can be decoupled from the neutrino mass. In this work, we revisit this possibility and show that sizable enhancements remain highly nontrivial to realize naturally. We demonstrate that, although the minimal realization allows the magnetic moment to be decoupled from the neutrino mass, obtaining an observable enhancement requires a delicate adjustment of the model parameters. Moreover, in extended scenarios, the decoupling no longer persists: the magnetic moment and neutrino mass become intrinsically linked, such that attempts to enhance the former inevitably induce large contributions to the latter.

hep-ph↗