1 |
Wright, E. L., et al., 1994, Interpretation of the COBE FIRAS CMBR Spectrum, ApJ, 420, 450
DOI
|
2 |
Michael S. T., 2002, The New Cosmology, astro-ph/0202007v1
|
3 |
Mikhail, F. I. & Wanas, M. I., 1977, Application of Theorems on Null-Geodesics on The Solar Limb Effect, Proc. Roy. Soc. Lond. A, 356, 471
|
4 |
Narlikar J., 1983, 'Introduction to Cosmology', edited by Jones & Bartlett, Publishers, Inc., pp.144-151
|
5 |
Peebles, P. J. E. & Yu, J. T., 1970, Primeval Adiabatic Perturbation in an Expanding Universe, ApJL, 325, L17-L20
DOI
|
6 |
Rebort, R. C. & Doran, M., 2003, Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models, astro-ph/0305334v1
|
7 |
Riess, A. G., et al., 2004, Type Ia Supernova Discoveries at z > 1 from the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution, ApJ, 607, 665
DOI
|
8 |
Robertson, H. P., 1932, Ann. Math. Princeton, 33, 496
DOI
ScienceOn
|
9 |
Suto, Y., Gouda, N. & Sugiyama N., 1990, Microwave background anisotropies and the primordial spectrum of cosmological density fluctuations, ApJS, 74, 665
DOI
|
10 |
Melek, M., 2000, Universe's Expansion Puts Limits on the Cosmic Time Scale Variations of Gravitational and Cosmological 'Constants', ApSS, 272, 417
|
11 |
Melek, M., 2002, Primordial Angular Gradients In The Temperature Of The CMBR and the Density Fluctuations, ApSS, 281, 743
|
12 |
Tomita, K. P., 2005, Phys. Rev. D, 71, 083504
DOI
|
13 |
Wanas, M. I., 1986, Geometrical structures for cosmological applications, ApSS, 127, 21
|
14 |
Wanas, M. I., 1989, A self-consistent world model, ApSS , 154, 165
|
15 |
Wanas, M. I., 2003, Chaos, Solitons & Fractals, 16, 621
DOI
ScienceOn
|
16 |
Weinberg, S., 1972, 'Gravitation and Cosmology', Jones Wiley & Sons Publishers, Inc
|
17 |
El-Naschie, M. S., 2002, Chaos Solitons & Fractals, 17, 1121
|
18 |
El-Naschie, M. S., 2003, Chaos Solitons & Fractals,16, 637
DOI
ScienceOn
|
19 |
Gurzadyan V. G., et al., 2003, astro-ph/0312305
|
20 |
Melek, M., 1992, ICTP print no. IC/92/95
|
21 |
Joshue, A. F., Dragan, H., Eric,V. L., & Michael, S. T., 2003, Probing Dark Energy with Supernovae: Exploiting Complementarity with the Cosmic Microwave Background, astro-ph/0208100v2
|
22 |
Hu,W., Sugiyama, N. & Silk, J., 1997, The Physics of Microwave Background Anisotropies, Nature, 386
|
23 |
Hwang, J-C. & Noh, H., 2005, Third-order Perturbations of a Zero-pressure Cosmological Medium: Pure General Relativistic Nonlinear Effects, Phys. Rev. D, 72, 044012
DOI
|
24 |
Ichikawa, K., Kawasaki, M., Sekiguchi, T., & Takahashi, T., 2006, Implications of dark energy parametrizations for the determination of the curvature of the universe, J. Cosmology and Astroparticle Phys., 12, 5
|
25 |
Keating, B., Timbie, P., Polnarev, A., & Steinberger, J., 1998, Large Angular Scale Polarization of the Cosmic Microwave Background Radiation and the Feasibility of Its Detection, ApJ, 495, 580
DOI
|
26 |
Kodama, H. & Sasaki, M., 1984, Cosmological Perturbation Theory, Progress of Theoretical Physics Supplement, 78, 1
DOI
|
27 |
Challinor, A. & Lasenby, A., 1999, Cosmic Microwave Back-ground Anisotropies in the Cold Dark Matter Model: A Covariant and Gauge-invariant Approach, ApJ, 512, 1
DOI
|
28 |
Douglas, S., Silk, J., & White, M., 1995, From Microwave Anisotropies to Cosmology, Science, 495, 580
|
29 |
Linder, E. V., 1997, First Principles of Cosmology, edited by Addison-Wesley, (California), pp122-124 and 179-180
|
30 |
McCrea, W. H., 1985, Revista Mexicana De Astronomia Astrophysica Marzo, 10, 33
|
31 |
Melek, M., 1995, On the Use of COBE Results, ApSS, 228, 327
|
32 |
Bozza, V. & Veneziano, G., 2005, Regular Two-component Bouncing Cosmologies and Perturbations, gr-qc/0506040
|
33 |
Bellini, M. 2001, Warm Inflation: Towards a Realistic COBE Data Power Spectrum for Matter and Metric Thermal Coupled Fluctuations, GRG, 33, 2081
DOI
|