Spherically symmetric nonlinear structures
We present an analytical method to extract observational predictions about the nonlinear evolution of perturbations in a Tolman universe. We assume no a priori profile for them. We solve perturbatively a Hamilton-Jacobi equation for a timelike geodesic and obtain the null one as a limiting case in t...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
1997
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| LEADER | 05381caa a22006497a 4500 | ||
|---|---|---|---|
| 001 | PAPER-20128 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205131.0 | ||
| 008 | 190411s1997 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0009244656 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Calzetta, E.A. | |
| 245 | 1 | 0 | |a Spherically symmetric nonlinear structures |
| 260 | |c 1997 | ||
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a (1970) Astron. Astrophys., 5, p. 84 | ||
| 504 | |a Scoccimarro, R., Frieman, J., (1996) Astrophys. J. Suppl. Ser., 105, p. 37. , APJSA2 | ||
| 504 | |a Shandarin, S.F., Ya Zeldovich, B., (1989) Rev. Mod. Phys., 61, p. 185 | ||
| 504 | |a Hobill, D., Burd, A., Coley, A., (1994) Deterministic Chaos in General Relativity, NATO Advanced Study Institute, , Plenum Press, New York | ||
| 504 | |a Kramer, D., Stephani, H., Herlt, E., MacCallum, M.A.H., (1980) Exact Solutions of Einstein Field Equations, , Cambridge University Press, Cambridge, England | ||
| 504 | |a Krasinski, A., ; Blumenthal, G.R., Nicolaci Da Costa, L., Goldwirth, D.S., Lecar, M., Piran, T., (1992) Astrophys. J., 388, p. 234 | ||
| 504 | |a Piran, T., (1990) Astrophys. J., 364, p. 341 | ||
| 504 | |a Panek, M., (1992) Astrophys. J., 388, p. 225 | ||
| 504 | |a Ribeiro, M.B., (1992) Astrophys. J., 388, p. 1 | ||
| 504 | |a Moffat, J.W., Tatarski, D.C., (1992) Phys. Rev. D, 45, p. 3512 | ||
| 504 | |a Fullana, M.J., Arnau, J.V., Sáez, D., (1996) Mon. Not. R. Astron. Soc., 280, p. 1181. , MNRAA4 | ||
| 504 | |a Langlois, D., Piran, T., (1996) Phys. Rev. D, 53, p. 2908 | ||
| 504 | |a Tomita, K., (1995) Astrophys. J., 451, p. 1 | ||
| 504 | |a Tomita, K., (1996) Astrophys. J., 461, p. 507 | ||
| 504 | |a Campos, A., Dark Matter in the Universe, , Proceedings of the International School of Physics “Enrico Fermi, ” Varena, edited by S. Bonometto, J. Primack, and A. Provenzale (IOP, 1995) | ||
| 504 | |a Meszaros, P., (1974) Astron. Astrophys., 37, p. 225 | ||
| 504 | |a Brandenberger, R.H., Feldman, H.A., Mukhanov, V.F., (1992) Phys. Rep., 215, p. 203 | ||
| 504 | |a Kolb, E.W., Turner, M.S., (1990) The Early Universe, , Addison-Wesley, New York | ||
| 504 | |a Börner, G., (1992) The Early Universe, , Springer-Verlag, Berlin | ||
| 504 | |a Peebles, P.J.E., (1993) Principles of Physical Cosmology, , Princeton University Press, Princeton, NJ | ||
| 504 | |a Smoot, G.F., (1992) Astrophys. J., 396, pp. L1 | ||
| 504 | |a Landau, L., Lifshitz, E.M., (1975) The Classical Theory of Fields, , Pergamon, New York | ||
| 504 | |a Hellaby, C., Lake, E., (1984) Astrophys. J., 282, p. 1 | ||
| 504 | |a Ellis, E.F.R., Relativistic Cosmology, , Proceedings of the International School of Physics “Enrico Fermi, ” General Relativity and Cosmology, edited by R.K. Sachs (Academic, New York, 1971) | ||
| 504 | |a Weinberg, S., (1972) Gravitation and Cosmology, , Wiley, New York | ||
| 504 | |a Misner, C.W., Thorne, K.S., Wheeler, J.A., (1973) Gravitation, , Freeman, San Francisco | ||
| 504 | |a Steinhardt, P.J., (1995) Particle and Nuclear Astrophysics and Cosmology in the Next Millenium, , World Scientific, Singapore | ||
| 504 | |a Gradshteyn, I.S., Ryzhik, I.M., (1980) Table of Integrals, Series and Products, , Academic, New York | ||
| 504 | |a Partridge, R.B., (1994) Class. Quantum Grav., 11, pp. A153 | ||
| 504 | |a de Lapparent, V., Geller, M.J., Huchra, J.P., (1986) Astrophys. J., 302, pp. L1 | ||
| 520 | 3 | |a We present an analytical method to extract observational predictions about the nonlinear evolution of perturbations in a Tolman universe. We assume no a priori profile for them. We solve perturbatively a Hamilton-Jacobi equation for a timelike geodesic and obtain the null one as a limiting case in two situations: for an observer located in the center of symmetry and for a noncentered one. In the first case we find expressions to evaluate the density contrast and the number count and luminosity distance versus redshift relationships up to second order in the perturbations. In the second situation we calculate the CMBR anisotropies at large angular scales produced by the density contrast and by the asymmetry of the observer’s location, up to first order in the perturbations. We develop our argument in such a way that the formulas are valid for any shape of the primordial spectrum. © 1997 The American Physical Society. |l eng | |
| 593 | |a Instituto de Astronomía y Física del Espacio (IAFE), Buenos Aires, Argentina | ||
| 700 | 1 | |a Kandus, A. | |
| 773 | 0 | |d 1997 |g v. 55 |h pp. 1795-1811 |k n. 4 |p Phys Rev D Part Fields Gravit Cosmol |x 15507998 |t Physical Review D - Particles, Fields, Gravitation and Cosmology | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-0009244656&doi=10.1103%2fPhysRevD.55.1795&partnerID=40&md5=05bb43345737a0583c1296320ef5d92e |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.55.1795 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_15507998_v55_n4_p1795_Calzetta |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v55_n4_p1795_Calzetta |y Registro en la Biblioteca Digital |
| 961 | |a paper_15507998_v55_n4_p1795_Calzetta |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 81081 | ||