344 P. <strong>van</strong> Nieuwenhuizen, Supergravitycannot be coupled consistently to either gravity or to simple matter systems, it seems as if nature stopsat spin 2, and supergravity at N = 8 (see subsection 1.14).The simplest extended supergravity is the N = 2 model (Ferrara and <strong>van</strong> Nieuwenhuizen [203]). Itwas obtained by coupling the (2, 3/2) gauge action to the (3/2, 1) matter multiplet by means of theNoether method. It was only afterwards found that the model had a larger symmetry, namely (to beginwith) a manifest 0(2) invariance which rotates the two gravitinos into each other. This model unifieselectromagnetism with gravity. The action reads= — ~ R(e, co)— ~ ti,~F”D~(o4cui, — + 4V2 [e(F”‘~+ E””) + ~y 5(P~+ ft~a)]~b1~E11 (1)and is invariant under general coordinate, local Lorentz and Maxwell transformations (SA,. = 3,.A) aswell as under the following two local supersymmetriesse tm,, =!~L~iym~,i 5A,. (2)~Ii — I \ ‘~_..!L..4I~ A11 ~ A \ I(J(J1,. — ~~~(O~?E-‘ ‘. ,~AY ~ 2e~,.A7 751E.Indeed, each gravitino gauges one local supersymmetry as one sees from Si/i,,’ = a,.e’ + more. Thesymbol .F,,,. equals ~ and .F,,,. is the supercovariant photon curl= (a~A~— 2\/2 i/I~ifr~~Eu’)— (j ~-* v). (3)One may always take the spin connection co in the Hilbert action as that function of tetrads andgravitinos which solves SI/Sw = 0 (1.5 order formalism). If one would have started in the Hilbert actionwith (0+ T where r is arbitrary, then one finds only r 2 = terms upon expanding about co. These i/i4~p4terms are absorbed into the F,,,. tensors, and it is easy to argue why this must be possible (as of coursehas been checked explicitly). Since fermionic field equations rotate into bosonic field equations and theformer have only one derivative while the latter have two derivatives, no derivative can act on e. (Sinceotherwise there would no longer be two derivatives available for the bosonic field equations. Thisargument breaks down when there are nonpropagating (auxiliary) fields.) The gravitino field equation isobtained by varying all t,li fields, and since the terms with P have four i/i’s which appear symmetrically,one must take one half of the former in order that the field equation only contains the supercovariantF~,,,but not, for example, bare F,,,,’s. Note that this argument also tells one that the spin connection inthe gravitino field equation must be supercovariant. As it happens, w is itself supercovariant, henceboth in Hilbert and gravitino action one finds a. (In other cases, for example in d = 11 or d = 5dimensions, one finds in the gravitino action ~(w+ ó~)instead of w, but, based on our argument givenbefore, one always chooses co in the Hilbert action.)The same kind of argument shows that if auxiliary fields are absent the gauge algebra must close onbosonic fields, and this is also a helpful criterion in constructing theories. (It is difficult to credit oneparticular person, but certainly J. <strong>Scherk</strong> gave an important contribution.)This model was the model where finite quantum corrections were found for the first time (see ref.
P. <strong>van</strong> Nieuwenhuizen~Supergravity 345[2821). Some chiral—dual symmetries were first found in another model which was not finite butdisplayed miraculous cancellations [510]. For a complete treatment of dual—chiral symmetries, see ref.[3821.An explanation of this finiteness was given by using these symmetries in this model which wenow discuss.According to the analysis of Haag, Lopuszanski and Sohnius (subsection 3.3), the maximal symmetrygroup of the S-matrix of supersymmetry algebras containing the Poincaré algebra is U(2). In fact, thefield theory has this global symmetry only on-shell (i.e., only the field equations have an U(2) globalsymmetry). Off-shell, only an SU(2) remains. These symmetries read [382]547,.L = iw $,.‘- — ~ = ~(1+ y~)i/i,.= ~ ~ ~I’~— kg)’ ~,.R = ~(1— y 5)çb,.U(1): Si/i,. = —iy5~’,, and SE,.,, = ie ,.,.~F”. (4)Thus the SU(2) part rotates ~,L as (2) and i/,’~as (~),while the U(1) part is a combined chirality-dualitytransformation. <strong>To</strong> prove the U(2) invariance, note that in the gravitino action i/’L couples to çIITRC sothat these terms are SU(2) and of course chirally (U(1)) invariant. The torsion is separately U(2)invariant, and, finally, the remaining terms can be analyzed by eliminating the F~,.kinetic terms throughthe equation of motion for F,.,.. This cancels half of the Noether coupling with bareF,.,, and the result isthat the action is the sum of the tetrad and gravitino actions plus the following term4V2 çi’,.[eP”~ + ~y5F”~]çb,,’E”. (5)Clearly, also this last term is U(2) invariant. The SU(2) invariance holds off-shell, but for N >2 only the0(N) invariance holds off-shell.An interesting connection between the coupling of photons and the cosmological constant was foundby Das and Freedman [108]and Fradkin and Vasiliev [225]. When one couples the photons minimallyto the fermions one needs at the same time a cosmological constant and a mass like term in the action.Thus it would seem that electromagnetism is due to the curvature of a de-Sitter universe. Actually, thiscosmological constant is much too large, and can be eliminated altogether by spontaneous symmetrybreaking, as we shall discuss in subsection 5.For the N = 2 model one can find this extension of the action by adding a cosmological constant tothe action and finding the further modifications by the Noether method. The complete set of extra termsis given by.~‘(cosm.)= 6eg 2 + 2eifr,.’o-”~47,.’— ~ 1F””°(D~i/i,,.’+ ge”A,,i/i,~,”) (6)8./i,.’ = D,.(a(e,i/J))E’ + gy,. ’+ gE”A,.E”where we added the terms with D,. for comparison. Clearly, g is a dimensionless gauge coupling, but itis remarkable that also a mass-like term is needed (as well as a cosmological term) when one couples thephoton to the gravitinos in an electromagnetic manner. Note that the theory still has the same numberof local invariances. The mass term is actually needed in order that i/i,.’ still be massless in de-Sitter
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In memoriam Joel ScherkJoel Scherk
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