Twistors and Spin 3/2 Potentials in Quantum Gravity

dc.creatorEsposito, Giampiero
dc.creatorPollifrone, Giuseppe
dc.date1995-06-27
dc.date.accessioned2026-07-07T03:30:43Z
dc.date.available2026-07-07T03:30:43Z
dc.descriptionLocal boundary conditions involving field strengths and the normal to the boundary, originally studied in anti-de Sitter space-time, have been recently considered in one-loop quantum cosmology. This paper derives the conditions under which spin-lowering and spin-raising operators preserve these local boundary conditions on a 3-sphere for fields of spin 0,1/2,1,3/2 and 2. Moreover, the two-component spinor analysis of the four potentials of the totally symmetric and independent field strengths for spin 3/2 is applied to the case of a 3-sphere boundary. It is shown that such boundary conditions can only be imposed in a flat Euclidean background, for which the gauge freedom in the choice of the potentials remains. Alternative boundary conditions for supergravity involving the spinor-valued 1-forms for gravitinos and the normal to the boundary are also studied.
dc.description20 pages, plain-tex, recently appearing in: Twistor Theory, edited by Stephen Huggett (Marcel Dekker, New York, 1994). The authors apologize for the delay in circulating the paper, which was due to technical problems now fixed
dc.identifierhttps://arxiv.org/abs/gr-qc/9506058
dc.identifierhttp://arxiv.org/abs/gr-qc/9506058
dc.identifierLect.Notes Pure Appl.Math. 169 (1995) 35-54
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35617
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleTwistors and Spin 3/2 Potentials in Quantum Gravity
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