The Approach of

Collaborators and some publications Introduction Action of the Approach Yukawa couplings and scalar fields The spinor represent
In the S ab sector appear massless gauge fields of
Y = τ 4 + τ 23 , and τ 1i ,
˜τ 1 = ( 1 2 (S 58 − S 67 ), 1 2 (S 57 + S 68 ), 1 2 (S 56 − S 78 ))
and massive of τ 2i ,
˜τ 2 = ( 1 2 (S 58 + S 67 ), 1 2 (S 57 − S 68 ), 1 2 (S 56 + S 78 ))
Similar breaks occur in the ˜S ab sector.
The properties of the upper massive four families are under
consideration, treating loop corrections.
The lowest one of the upper four families (all with no
Yukawa couplings to the lowest four families) is
predicted to constitute the dark matter.
N.S. Mankoč Borštnik, Cape Town 2010, 01-06 February University of Ljubljana
The Approach Unifying spins and charges