Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields
Exact solutions to the Einstein Dirac Klein-Gordon equations are found in Bianchi type-I and type-V spacetimes. When the spinor field is massive, the Bianchi type-I universe has singularities of the Zel dovich type, and it may begin anisotropically at a singularity, leading to a dust-filled Friedman...
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1990
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| 008 | 190411s1990 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0040939061 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Chimento, L.P. | |
| 245 | 1 | 0 | |a Exact Bianchi type-(I,V) solutions of the Einstein equations with scalar and spinor fields |
| 260 | |c 1990 | ||
| 270 | 1 | 0 | |m Chimento, L.P.; Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Pabellan I, Ciudad Universitaria, 1428 Buenos Aires, Argentina |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a Exact solutions to the Einstein Dirac Klein-Gordon equations are found in Bianchi type-I and type-V spacetimes. When the spinor field is massive, the Bianchi type-I universe has singularities of the Zel dovich type, and it may begin anisotropically at a singularity, leading to a dust-filled Friedmann stage at late times. For ghost neutrinos we get an axisymmetric Zel dovich universe. These solutions have particle horizons. For the Bianchi type-V model there exist solutions which begin at a singularity, tending to flat spacetime at late times. In this case the neutrinos are not ghost ones. © 1990 The American Physical Society. |l eng | |
| 593 | |a Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Pabellan I, Ciudad Universitaria, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Pensa, F.G. | |
| 773 | 0 | |d 1990 |g v. 42 |h pp. 1098-1104 |k n. 4 |x 05562821 |w (AR-BaUEN)CENRE-394 |t Physical Review D | |
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| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_05562821_v42_n4_p1098_Chimento |y Handle |
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