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Example text

From also. isation obtain of it. the product the result From of the the wave is no longer equivalent gravity. The sem~classical of eq. 23 we variation function equation particular of ¢ fields is that which of q u a n t u m to get (24> Schrodinger's The a theory ~ 0 a decomposition longer gives formulation form is defined. analagous but we of this For the to eq. get a non equation simplest 13, linear depends choice we no generalupon how ( ~(g,@))3, 49 It is well which resemble known that such the collapse when the~e exist solitonic solutions to the linearised equation cosmology, be possible without it may the i n t e r v e n t i o n Non-linear a many terms electron a single imation wave electron.

2 and universes a complicated can the wave a constraint the observer Next, class classical at this function ~(g,O,@i). their stage, and inter- is quant- functions introducing The replaces of F r a d k i n H 1 and theory of wave Q~ = O, w h i c h equat- we i n t r o d u c e the be fixed methods of H, whose finally, a suitable freedom Using the of the W h e e l e r - D e W i t t an a c t i o n equations. to fig. over Q in terms between to'involve quantisation constraint 01into imposes (7) and having terms function.

Phys. Lett. B69, 445 (1977). , Nilsson, Lett. 171B, 170. N. , Phys. , Nucl. Phys. B267, 266 (1986). 4568/86. , in Proceedings of the 1985 Les Houches Summer School (Eds. Ramond and Stora). 14) de Wit, B. 4359/86 (1986). 15) Chamseddine, A . , in preparation. , Ross, D. J. , Phys. Lett. 175B, 417 (1986). , Phys. Lett. B169, 41 (1986). , Diff. J. Geom. 17, 357 (1983). , The Mathematical Intelligencer ~, 39 (1985). , Dokl. Akad. Nauk SSR 84,221 (1952). , Bull. Amer. Math. Soc. 8, 81 (1985). , Vafa, C.

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