Chiral Bargmann-Wigner Equations for Spin-1 Massive Fields
T.B. Watson, Z.E. Musielak

TL;DR
This paper extends the Bargmann-Wigner equations to include chiral symmetry for spin-1 massive fields, revealing a new coupling phenomenon with potential implications for Higgs and dark matter physics.
Contribution
It introduces chiral Bargmann-Wigner equations for spin-1 fields and uncovers a novel chirality coupling to a spin-0 field, linking to Higgs and dark matter.
Findings
Derived chiral Bargmann-Wigner equations for spin-1 fields
Reduced equations to Proca-like form in chiral basis
Identified a new chirality coupling with potential physical implications
Abstract
The Bargman-Wigner equations are generalized to include chiral symmetry based on the irreps of the Poincar\'{e} group, and the chirial Bargmann-Wigner equations are derived for spin-1 massive fields. By specifying the chiral basis, the chiral Bargmann-Wigner equations are reduced to the Proca-like equation, which is coupled by chirality to an auxiliary equation for spin-0 massive field. The coupling is a new phenomenon whose physical implications for the Higgs field and dark matter are discussed.
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