INTRODUCTION TO COSMOLOGY (V.A.Sirota)
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- Introduction: objects, scales
- Methods of distance determinaiton
- Hierarchical structure
- Hubble expansion
- Geometry of the Universe
- Cosmological principle
- Robertson-Walker metric
- Red shift
- Friedmann models
- Cosmological constant
- Horizons
- Recombination and cosmic ray background
- Spectrum transformation under free expansion
- Hot Universe
- Saha formula and eviations from it in expanding Universe
- Planck spectrum distortion
- Reionization
- Zeldovich-Sunyaev effect
- Cosmic ray background anisotropy
- Dipole and short-scale anisotropy
- Doppler peaks
- Sachs-Wolfe effect
- Silk damping
- Nucleosynthesis
- Temperature history of the Universe
- Jeans theory
- Fluctuation growth in the expanding Universe
- Formation of galaxies
- Dark matter
- Pros. Candidates
- Gravitational lenses and microlensing
- Zeldovich–Harrison spectrum
- Zeldovich pancakes
- Gurevich–Zybin theory
- LITERATURE:
- S. Weinberg. Gravitation and Cosmology
- L.D. Landau, E.M. Lifshitz. Field Theory
- Ya.B. Zeldovich, I.D. Novikov. Structure and Evolution of the Universe
- F.J.A. Peebles. Large-scale Structure of the Universe
- Perlmutter et al. Ap.J. 517, 565 (1999) – cosmological constant
- A.D. Chernin. (UFN) 171(11), 1153-1175 (2001)
- Kurt, Zeldovich, Sunyaev. JETP 55(1) 278 (1968) - recombination
- Zeldovich, Sunyaev. Comments on Astrophys. and Space Phys. v.2, 173 (1970) – Zeldovich–Sunyaev effect
- J.Silk. Ap.J. 151, 459 (1968)
- S.Weinberg. Ap.J. 168, 175 (1971) - Silk damping
- Sachs, Wolfe. Aph.J. 147, 73 (1967) - Sachs-Wolfe effect
- P.de Bernardis et al. astro-ph/0011468 - observations of anisotropy of cosmic ray background
- Ishkhanov, Kapitonov, Tyutin. Nucleosynthesis in the Universe
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