Deparametrization and quantization of the Taub universe

Previous analysis about the deparametrization and path integral quantization of cosmological models are extended to models which do not admit an intrinsic time. The formal expression for the transition amplitude is written down for the Taub anisotropic universe with a clear notion of time. The relat...

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Detalles Bibliográficos
Autor principal: Giribet, G.
Otros Autores: Simeone, C.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2002
Acceso en línea:Registro en Scopus
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Registro en la Biblioteca Digital
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100 1 |a Giribet, G. 
245 1 0 |a Deparametrization and quantization of the Taub universe 
260 |c 2002 
270 1 0 |m Giribet, G.; Inst. de Astron./Fisica del Espacio, C.C. 67, Sucursal 28, 1428 Buenos Aires, Argentina; email: gaston@iafe.uba.ar 
506 |2 openaire  |e Política editorial 
504 |a Ferraro, R., Simeone, C., (1997) J. Math. Phys., 38, p. 599 
504 |a De Cicco, H., Simeone, C., (1999) Int. J. Mod. Phys., A14, p. 5105 
504 |a Simeone, C., (1999) J. Math. Phys., 40, p. 4527 
504 |a Catren, G., Ferraro, R., (2001) Phys. Rev., D63, p. 023502 
504 |a Salopek, D.S., Bond, J.R., (1990) Phys. Rev., D42, p. 3936 
504 |a Giribet, G., Simeone, C., (2001) Mod. Phys. Lett., A16, p. 19 
504 |a Simeone, C., (2002) Deparametrization and Path Integral Quantization of Cosmological Models, 69. , World Scientific Lecture Notes in Physics 
504 |a Castagnino, M., Catren, G., Ferraro, R., in preparation; Giribet, G., Leston, M., Simeone, C., in preparation; Moncrief, V., Ryan, M.P., (1991) Phys. Rev., D44, p. 2375 
504 |a Hartle, J., Hawking, S., (1983) Phys. Rev., D28, p. 2960 
504 |a Barvinsky, A.O., (1993) Phys. Rep., 230, p. 237 
520 3 |a Previous analysis about the deparametrization and path integral quantization of cosmological models are extended to models which do not admit an intrinsic time. The formal expression for the transition amplitude is written down for the Taub anisotropic universe with a clear notion of time. The relation existing between the deparametrization associated to gauge fixation required in the path integral approach and the procedure of reduction of the Wheeler-DeWitt equation is also studied.  |l eng 
536 |a Detalles de la financiación: Comisión Nacional de Energía Atómica, Gobierno de Argentina, CNEA 
536 |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas 
536 |a Detalles de la financiación: The authors are grateful to Esteban Calzetta for useful conversations. This work was supported by CNEA and CONICET. 
593 |a Instituto de Astronomía y Física del Espacio, C.C. 67, Sucursal 28, 1428 Buenos Aires, Argentina 
593 |a Departamento de Física, Comisión Nacional de Energía Atómica, Av. del Libertador 8250, 1429 Buenos Aires, Argentina 
593 |a Departamento de Física, Ciudad Universitaria, Pabellón I, 1428, Buenos Aires, Argentina 
690 1 0 |a CONSTRAINED HAMILTONIAN SYSTEM 
690 1 0 |a GLOBAL PHASE TIME 
690 1 0 |a MINISUPERSPACE 
690 1 0 |a QUANTUM COSMOLOGY 
690 1 0 |a ANISOTROPY 
690 1 0 |a ARTICLE 
690 1 0 |a MATHEMATICAL ANALYSIS 
690 1 0 |a PHASE TRANSITION 
690 1 0 |a QUANTUM MECHANICS 
700 1 |a Simeone, C. 
773 0 |d 2002  |g v. 17  |h pp. 2885-2896  |k n. 21  |p Int. J. Mod. Phys. A  |x 0217751X  |w (AR-BaUEN)CENRE-596  |t International Journal of Modern Physics A 
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