Marcelo Evangelista de Araujo
Instituição:
Universidade Federal do Rio de Janeiro
Centro:
Centro de Ciências Matemáticas e da Natureza
Unidade:
Instituto de Física
Departamento:
Departamento de Física e Matemática/I Fis
Formação:
-
Vatican Observatory (University of Arizona)
| Pós-Doutorado | 1995 - 1996
-
Cardiff University Principal
| Pós-Doutorado | 1991 - 1992
-
University of London
| Doutorado | 1982 - 1987
-
Universidade de São Paulo
| Mestrado | 1981 - Agora
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Universidade de Brasília
| Graduação | 0 - 1980
Laboratórios:
Nenhum laboratório cadastrado
Nuvens de Palavras:
Artigos:
(100.00% artigos com DOI)
| Titulo | DOI | Ano |
|---|---|---|
| Finding a spherically symmetric cosmology from observations in observational coordinates ¿ advantages and challenges | 10.1088/1475-7516/2011/07/029 | 2011 |
| Erratum: Obtaining the time evolution for spherically symmetric Lemaître-Tolman-Bondi models given data on our past light cone [Phys. Rev. D 80, 123517 (2009)] | 10.1103/PhysRevD.81.049903 | 2010 |
| Using time drift of cosmological redshifts to find the mass-energy density of the Universe | 10.1103/PhysRevD.82.123513 | 2010 |
| The angular-diameter distance maximum and its redshift as constraints on ?? 0 Friedmann-Lemaître-Robertson-Walker models | 10.1111/j.1365-2966.2008.14321.x | 2009 |
| Obtaining the time evolution for spherically symmetric Lemaître-Tolman-Bondi models given data on our past light cone | 10.1103/PhysRevD.80.123517 | 2009 |
| Solving Einstein field equations in observational coordinates with cosmological data functions: Spherically symmetric universes with a cosmological constant | 10.1103/PhysRevD.78.063513 | 2008 |
| Temperature evolution of the FRW universe filled with modified Chaplygin gas | 10.1016/j.physletb.2007.11.076 | 2007 |
| Integrating Einstein Field Equations in Observational Coordinates with Cosmological data Functions: Non Flat Friedmann-Lemaitre-Robertson-Walker Cases | 10.1086/319431 | 2001 |
| Perturbed Spherically Symmetric Dust Solution of the Field Equations in Observational Coordinates with Cosmological Data Functions | 10.1086/322507 | 2001 |
| Erratum: Exact spherically symmetric dust solution of the field equations in observational coordinates with cosmological data functions [Phys. Rev. D 60, 104020 (1999)] | 10.1103/PhysRevD.64.049902 | 2001 |
| The Exact Spherically Symmetric Solution of the Einstein Field Equations in Observational Coordinates with Cosmological data Functions | 10.1103/PhysRevD.60.104020 | 1999 |
| Erratum To The limits on cosmological anisotropies and inhomogeneities from COBE data | 10.1086/307648 | 1999 |
| Two Kerr black holes with axisymmetric spins: Head-on Collision and Gravitational Radiation | 10.1088/0264-9381/15/10/011 | 1998 |
| The Limits On Cosmological Anisotropies and Inhomogeneities From Cobe Data. | 10.1086/303633 | 1997 |
| Static Axisymmetric Approach For The Head-On Collision Of Two Black Holes. | 10.1103/PhysRevD.52.816 | 1995 |
| Quasinormal Modes Of Reissner-Nordström Black Holes: Phase Integral Approach | 10.1103/PhysRevD.49.2703 | 1994 |
| On The Bohr-Sommerfeld Formula for Black Hole Normal Modes | 10.1088/0264-9381/10/6/009 | 1993 |
| The Phase-Integral Method and Black Hole Normal Modes | 10.1088/0264-9381/10/4/009 | 1993 |
| Generalized Bohr-Sommerfeld Formula for Schwarzschild Black Hole Normal Modes | 10.1088/0264-9381/10/4/010 | 1993 |
| Finding Isometry Groups in Theory and Practice | 10.1007/BF00760132 | 1992 |
| Lagrangian Methods and Nonlinear High-Frequency Gravitational Waves | 10.1007/BF00760437 | 1989 |
| The Automorphism Groups For Bianchi Universe Models And Computer-Aided Invariant Classification Of Metrics | 10.1088/0264-9381/5/4/002 | 1988 |
| Automorphisms In Action: Spatially Homogeneous Einstein-Maxwell Plane Waves | 10.1088/0264-9381/5/8/005 | 1988 |
| On The Assumptions Made In Treating The Gravitational Wave Problem By The High-Frequency Approximation | 10.1007/BF00765884 | 1986 |
Eventos:
(0.00% eventos com DOI)