Cosmological solutions of the semiclassical Einstein-Dirac equations
Exact solutions to the semiclassical backreaction equations with an unquantised Dirac field are found when the ratio of the renormalisation parameters beta and alpha is 9/4. For alpha (0 there is a one-parameter family of solutions which do not have particle horizons and a two-parameter family of so...
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1990
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003 | AR-BaUEN | ||
005 | 20230518202952.0 | ||
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024 | 7 | |2 scopus |a 2-s2.0-0038870440 | |
040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
100 | 1 | |a Chimento, L.P. | |
245 | 1 | 0 | |a Cosmological solutions of the semiclassical Einstein-Dirac equations |
260 | |c 1990 | ||
270 | 1 | 0 | |m Chimento, L.P.; Departamento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina |
506 | |2 openaire |e Política editorial | ||
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504 | |a Starobinsky, AA, Schmidt, HI, (1987) Class. Quantum Grav., 4 (3), p. 695 | ||
504 | |a Kofman, LA, Linde, AD, Starobinsky, AA, (1985) Phys. Lett., 157 (5-6), p. 361 | ||
504 | |a Suen, W, Anderson, P, (1987) Phys. Rev., 35 (10), p. 2940 | ||
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504 | |a Fischetti, MV, Hartle, JB, Hu, BL, (1979) Phys. Rev., 20 (8), p. 1757 | ||
504 | |a Starobinsky, AA, (1980) Phys. Lett., 91 (1), p. 99 | ||
504 | |a Anderson, P, (1983) Phys. Rev., 28 (2), p. 271 | ||
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504 | |a Anderson, P, (1985) Phys. Rev., 32 (6), p. 1302 | ||
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504 | |a Chimento, LP, (1988) Class. Quantum Grav., 5 (8), p. 1137 | ||
504 | |a Chimento, LP, (1989) Class. Quantum Grav., 6 (9), p. 1285 | ||
504 | |a Birrell, NB, Davies, PCW, (1982); Davies, PCW, Fulling, SA, Christensen, SM, Bunch, TS, (1977) Ann. Phys., NY, 109 (1), p. 108 | ||
504 | |a Bunch, TS, Davies, PCW, (1977) Proc. R. Soc., 356 (1687), p. 569 | ||
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504 | |a la Salle, J, Lefshetz, S, (1971) | ||
520 | 3 | |a Exact solutions to the semiclassical backreaction equations with an unquantised Dirac field are found when the ratio of the renormalisation parameters beta and alpha is 9/4. For alpha (0 there is a one-parameter family of solutions which do not have particle horizons and a two-parameter family of solutions which oscillate at about the Planck frequency and, on average, behave asymptotically as a matter-dominated Friedmann solution. There is a two-parameter family with an asymptotically de Sitter stage, which is stable for any alpha )0 and beta )0. |l eng | |
593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina | ||
593 | |a Consejo Nacional de Investigaciones Cientificas y Tecnicas | ||
700 | 1 | |a Jakubi, A.S. | |
700 | 1 | |a Pensa, F.G. | |
773 | 0 | |d 1990 |g v. 7 |h pp. 1561-1565 |k n. 9 |x 02649381 |w (AR-BaUEN)CENRE-326 |t Classical and Quantum Gravity | |
856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0038870440&doi=10.1088%2f0264-9381%2f7%2f9%2f008&partnerID=40&md5=4d777bb8b80aee9d1a544149e4d6c490 |y Registro en Scopus |
856 | 4 | 0 | |u https://doi.org/10.1088/0264-9381/7/9/008 |y DOI |
856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_02649381_v7_n9_p1561_Chimento |y Handle |
856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02649381_v7_n9_p1561_Chimento |y Registro en la Biblioteca Digital |
961 | |a paper_02649381_v7_n9_p1561_Chimento |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 61474 |