Particle creation amplification in curved space due to thermal effects
A physical system composed by a scalar field minimally coupled to gravity and a thermal reservoir, as in thermo field dynamics, all of them in curved space-time, is considered. When the formalism of thermo field dynamics is generalized to the above case, an amplification in the number of created par...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
1997
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| Acceso en línea: | Registro en Scopus Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 02494caa a22003617a 4500 | ||
|---|---|---|---|
| 001 | PAPER-20072 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205128.0 | ||
| 008 | 190411s1997 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0039377951 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Laciana, C.E. | |
| 245 | 1 | 0 | |a Particle creation amplification in curved space due to thermal effects |
| 260 | |c 1997 | ||
| 270 | 1 | 0 | |m Laciana, C.E.; Instituto de Astronomia, Física del Espacio, Casilla de Correo 67, Sucursal 28, 1428 Buenos Aires, Argentina; email: laciana@iafe.uba.ar |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Takahashi, Y., Umezawa, H., (1975) Collective Phenomena, 2, p. 55 | ||
| 504 | |a Chu, H., Umezawa, H., (1994) Int. J. Mod. Phys. A, 9, p. 2363 | ||
| 504 | |a Umezawa, H., Matsumoto, H., Tachiki, M., (1982) Thermo Field Dynamics and Condensed States, , North-Holland, Amsterdam | ||
| 504 | |a Parker, L., (1969) Phys. Rev., 183, p. 1057 | ||
| 504 | |a Hardman, I., Umezawa, H., Yamanaka, Y., (1987) J. Math, Phys., 28, p. 2925 | ||
| 504 | |a Arimitsu, T., Guida, M., Umezawa, H., (1988) Physica A, 148, p. 1 | ||
| 504 | |a Lagiana, C.E., (1994) Gen. Relativ. Gravit., 26, p. 363 | ||
| 504 | |a Laciana, C.E., (1995) Physica A, 216, p. 511 | ||
| 520 | 3 | |a A physical system composed by a scalar field minimally coupled to gravity and a thermal reservoir, as in thermo field dynamics, all of them in curved space-time, is considered. When the formalism of thermo field dynamics is generalized to the above case, an amplification in the number of created particles is predicted. |l eng | |
| 593 | |a Instituto de Astronomia, Física del Espacio, Casilla de Correo 67, Sucursal 28, 1428 Buenos Aires, Argentina | ||
| 773 | 0 | |d 1997 |g v. 112 |h pp. 805-810 |k n. 5 |p Nuovo Cimento Soc. Ital. Fis. B |x 03693554 |w (AR-BaUEN)CENRE-2204 |t Nuovo Cimento della Societa Italiana di Fisica B | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0039377951&partnerID=40&md5=0edff3c144ece59e961268b952077ee6 |y Registro en Scopus |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_03693554_v112_n5_p805_Laciana |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_03693554_v112_n5_p805_Laciana |y Registro en la Biblioteca Digital |
| 961 | |a paper_03693554_v112_n5_p805_Laciana |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 999 | |c 81025 | ||