13/15. The weakness of string theory revisited
Standard arguments for supersymmetry (super = fermionic):
-
Nature has fermions.
Polchinski (1995)
taught us that fermions can live on D-branes.
-
Evades Coleman-Mandula (1967) no-go theorem.
Spin(11,1) obeys theorem: Dirac and internal algebras always commute.
-
Gets 3 coupling parameters of standard model to meet at grand unification.
Spin(11,1): 3 couplings meet in 2 separate steps.
-
The ground state of bosonic strings is tachyonic, therefore unstable.
In cosmology, high energy vacua are unstable by the Higgs mechanism.
Are these the tachyons?
-
Fermion-boson infinities cancel each other in scalar boson masses.
Can standard particle qft be applied to the electroweak Higgs boson?
-
Magically cancels gauge anomalies in string theory.
Spin(11,1): gauge anomalies vanish because the theory is chirally balanced.
Problems with supersymmetry:
-
Predicts symmetries that are not observed.
Spin(11,1) is not supersymmetric.
-
Preempts symmetries that are observed.
Spin(11,1) possesses the symmetries that are observed.
Supersymmetry algebra posits that anticommutators of
\(R,L\)-handed spinor generators \(Q\) generate translations \(P\):
\[
\{ Q_R , Q_L \} = P
\ , \quad
[ P , P ] = 0
\ .
\]
But Brauer-Weyl (1935) theorem shows
\[
\bigl[ \{ Q_R , Q_L \} , \{ Q_R , Q_L \} \bigr]
=
\{ Q_R , Q_R \} + \{ Q_L , Q_L \}
\ ,
\]
which are the observed symmetries of the standard model.
14/15. The multiverse just got a whole lot bigger