English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Spinor description for the curvatures of $D=5$ Yang-Mills, Rarita-Schwingerand gravitational fields is elaborated. Restrictions imposed on the curvaturespinors by the dynamical equations and Bianchi identities are analyzed. In theabsence of sources symmetric curvature spinors with $2s$ indices obeyfirst-order equations that in the linearized limit reduce to Dirac-typeequations for massless free fields. These equations allow for a higher-spingeneralization similarly to $4d$ case. Their solution in the form of theintegral over Lorentz-harmonic variables parametrizing coset manifold$SO(1,4)/(SO(1,1)\times ISO(3))$ isomorphic to the three-sphere is considered.Superparticle model that contains such Lorentz harmonics as dynamicalvariables, as well as harmonics parametrizing the two-sphere $SU(2)/U(1)$ isproposed. The states in its spectrum are given by the functions on $S^3$ thatupon integrating over the Lorentz harmonics reproduce on-shell symmetriccurvature spinors for various massless supermultiplets of $D=5$ space-timesupersymmetry.

Spinor description of $D=5$ massless low-spin gauge fields