Search arXiv⌕ Search

arXiv · 0707.1373

Polarized Parton Densities and Higher Twist in the Light of the Recent CLAS and COMPASS data

Abstract

The impact of the recent very precise CLAS and COMPASS g_1/F_1 data on polarized parton densities and higher twist effects is discussed. We demonstrate that the low Q^2 CLAS data improve essentially our knowledge of higher twist corrections to the spin structure function g1, while the large Q^2 COMPASS data influence mainly the strange quark and gluon polarizations which slightly decrease. We find also that the present inclusive DIS data cannot rule out a negative polarized and changing in sign gluon densities.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Elliot Leader, Aleksander V. Sidorov, Dimiter B. Stamenov. 2007-07-12. Polarized Parton Densities and Higher Twist in the Light of the Recent CLAS and COMPASS data. https://arxiv.org/abs/0707.1373

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↗