Observer-dependent quantum vacua in curved space. II
An observer-dependent Hamiltonian is introduced in order to describe massless spin-1 particles in curved space-times. The vacuum state is defined by means of Hamiltonian diagonalization and minimization, which turns out to be equivalent criteria. This method works in an arbitrary geometry, although...
Guardado en:
| Autor principal: | |
|---|---|
| Otros Autores: | |
| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
1989
|
| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 04147caa a22005657a 4500 | ||
|---|---|---|---|
| 001 | PAPER-17954 | ||
| 003 | AR-BaUEN | ||
| 005 | 20241205091309.0 | ||
| 008 | 190411s1989 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-35949013038 | |
| 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. II |
| 260 | |c 1989 | ||
| 270 | 1 | 0 | |m Castagnino, M.A.; Instituto de Astronomía Y Física del Espacio, Casilla de Correo 67, Suc. 28 |
| 504 | |a Birrell, N.D., Davies, P.C., (1982) Quantum Fields in Curved Space, , Cambridge University Press, London, England | ||
| 504 | |a Unruh, W.G., (1976) Phys. Rev. D, 14, p. 870 | ||
| 504 | |a Castagnino, M.A., Ferraro, R., (1986) Phys. Rev. D, 34, p. 497 | ||
| 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 Castagnino, M.A., Sztrajman, J.B., (1986) J. Math. Phys., 27, p. 1037 | ||
| 504 | |a Padmanabhan, T., (1985) Class. Quantum Gravit., 2, p. 105 | ||
| 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 Creutz, M., (1979) Ann. Phys. (N.Y.), 117, p. 471 | ||
| 504 | |a Hawking, S.W., Ellis, G.F.R., (1973) The Large Scale Structure of Space-Time, , Cambridge University Press, London, England | ||
| 504 | |a 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 Candelas, P., Deutsch, D., (1977) Proc. R. Soc. London, 354 A, p. 79 | ||
| 504 | |a Bogolubov, N.N., (1958) Zh. Eksp. Teor. Fiz., 34, p. 58 | ||
| 504 | |a (1958) Sov. Phys. JETP, 7, p. 51 | ||
| 504 | |a Takagi, S., On the Response of a Rindler-Particle Detector (1984) Progress of Theoretical Physics, 72, p. 505 | ||
| 504 | |a Takagi, S., Vacuum Stress Induced by Uniform Acceletation (1985) Progress of Theoretical Physics, 74, p. 1219 | ||
| 504 | |a Sánchez, N., Analytic mappings: A new approach to quantum field theory in accelerated frames (1981) Physical Review D, 24, p. 2100 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a An observer-dependent Hamiltonian is introduced in order to describe massless spin-1 particles in curved space-times. The vacuum state is defined by means of Hamiltonian diagonalization and minimization, which turns out to be equivalent criteria. This method works in an arbitrary geometry, although a condition on the fluid of observers is required. Computations give the vacua commonly accepted in the literature. © 1989 The American Physical Society. |l eng | |
| 593 | |a Instituto de Astronomía Y Física del Espacio, Casilla de Correo 67, Suc. 28 | ||
| 593 | |a Ciudad Universitaria, 1428 Buenos Aires, Argentina | ||
| 593 | |a Instituto de Física de Rosario, Consejo Nacional de Investigaciones Científicas Y, Técnicas-Universidad Nacional de Rosario, Av. Pellegrini 250, 2000 Rosario, Argentina | ||
| 593 | |a Argentina and Area de Físico-Matemtica, Universidad de Buenos Aires, Ciudad Universitaria, Pabelln II, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Sztrajman, J.B. | |
| 773 | 0 | |d 1989 |g v. 40 |h pp. 1876-1885 |k n. 6 |x 05562821 |w (AR-BaUEN)CENRE-394 |t Physical Review D | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-35949013038&doi=10.1103%2fPhysRevD.40.1876&partnerID=40&md5=c0f60504a540bb4c85fb4c8ab68a69cb |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.40.1876 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_05562821_v40_n6_p1876_Castagnino |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v40_n6_p1876_Castagnino |y Registro en la Biblioteca Digital |
| 961 | |a paper_05562821_v40_n6_p1876_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 78907 | ||