Observer-dependent quantum vacua in curved space

An observer-dependent Hamiltonian is introduced. The vacuum state is defined by means of Hamiltonian diagonalization and minimization, which result to be equivalent criteria. This method encompasses a great number of known vacuum definitions, and works in an arbitrary geometry if the observers field...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Castagnino, Mario Alberto
Otros Autores: Ferraro, R.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 1986
Acceso en línea:Registro en Scopus
DOI
Handle
Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
LEADER 04223caa a22005417a 4500
001 PAPER-944
003 AR-BaUEN
005 20241205091845.0
008 190411s1986 xx ||||fo|||| 00| 0 eng|d
024 7 |2 scopus  |a 2-s2.0-0000027498 
040 |a Scopus  |b spa  |c AR-BaUEN  |d AR-BaUEN 
100 1 |a Castagnino, Mario Alberto 
245 1 0 |a Observer-dependent quantum vacua in curved space 
260 |c 1986 
270 1 0 |m Castagnino, M.; Instituto de Física de Rosario (CONICET-UNR), Facultad de Ingeniería, Av. Pellegrini 250, 2000 Rosario, Argentina 
504 |a Fulling, S.A., (1979) Gen. Relativ. Gravit., 10, p. 807 
504 |a Grib, A.A., Mamayev, S.G., Mostepanenko, V.M., (1980) J. Phys. A, 13, p. 2057 
504 |a Birrel, N.D., Davies, P.C.W., (1982) Quantum Fields in Curved Space, , Cambridge University Press, Cambridge 
504 |a Unruh, W.G., (1976) Phys. Rev. D, 14, p. 870 
504 |a Sánchez, N., Analytic mappings: A new approach to quantum field theory in accelerated frames (1981) Physical Review D, 24, p. 2100 
504 |a Brown, M.R., Ottewill, A.C., Siklos, T.C., (1982) Phys. Rev. D, 26, p. 1881. , and S 
504 |a Castagnino, M., Mazzittelli, F.D., (1985) Phys. Rev. D, 31, p. 742 
504 |a M. Castagnino, in Quantum Gravity, proceedings of Third Seminar, Moscow, 1984, edited by M. A. Markov et al. (World Scientific, Singapore, 1985), p. 496; Cattaneo, C., (1958) Nuovo Cimento, 10, p. 318 
504 |a Moller, C., (1952) The Theory of Relativity, , Oxford University Press, London 
504 |a Ashtekar, A., Magnon, A., Quantum Fields in Curved Space-Times (1975) Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, 346 A, p. 375 
504 |a Misner, C.W., Thorne, K.S., Wheeler, J.A., (1973) Gravitation, , Freeman, San Francisco 
504 |a Hawking, S.W., Ellis, G.F.R., (1973) The Large Scale Structure of Space-Time, , Cambridge University Press, Cambridge, England 
504 |a It may be proved that different choices for Ek do not modify the vacuum because they only involve Bogoliubov's transformations (Ref. 3) with vanishing beta coefficients; Boulware, D., (1975) Phys. Rev. D, 11, p. 1404 
504 |a Ford, L.H., (1975) Phys. Rev. D, 11, p. 3370 
504 |a Ford, L.H., (1976) Phys. Rev. D, 14, p. 3304 
504 |a Castagnino, M., Nuñez, C.A., (1985) Rev. Mex. Astron. Astrofis., 10, p. 43 
504 |a Castagnino, M., Ferraro, R., (1985) Ann. Phys. (N.Y.), 161, p. 1 
504 |a Born, M., (1909) Ann. Phys. (Leipzig), 30, p. 1 
506 |2 openaire  |e Política editorial 
520 3 |a An observer-dependent Hamiltonian is introduced. The vacuum state is defined by means of Hamiltonian diagonalization and minimization, which result to be equivalent criteria. This method encompasses a great number of known vacuum definitions, and works in an arbitrary geometry if the observers field satisfies certain properties. © 1986 The American Physical Society.  |l eng 
593 |a Instituto de Física de Rosario (CONICET-UNR), Facultad de Ingeniería, Av. Pellegrini 250, 2000 Rosario, Argentina 
593 |a Instituto de Astronomía y Física Del Espacio, Casilla de Correo 67, Sucursal 28, 1428 Buenos Aires, Argentina 
593 |a Mathematics Department, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, 1428 Buenos Aires, Argentina 
700 1 |a Ferraro, R. 
773 0 |d 1986  |g v. 34  |h pp. 497-503  |k n. 2  |x 05562821  |w (AR-BaUEN)CENRE-394  |t Physical Review D 
856 4 1 |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0000027498&doi=10.1103%2fPhysRevD.34.497&partnerID=40&md5=0f07ed6e7e7f01e6c9d88c8958e2b221  |y Registro en Scopus 
856 4 0 |u https://doi.org/10.1103/PhysRevD.34.497  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_05562821_v34_n2_p497_Castagnino  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v34_n2_p497_Castagnino  |y Registro en la Biblioteca Digital 
961 |a paper_05562821_v34_n2_p497_Castagnino  |b paper  |c PE 
962 |a info:eu-repo/semantics/article  |a info:ar-repo/semantics/artículo  |b info:eu-repo/semantics/publishedVersion 
963 |a VARI 
999 |c 61897