Introduction to Cosmology
Matts Roos is Emeritus Professor in Particle Physics at the University of Helsinki, Physics Department, where he is still active in research and postgraduate teaching. Roos is a member of the Finnish Physical Society, honorary member of The Physical Society in Finland, and founding member of the Par...
Clasificación: | Libro Electrónico |
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Autor principal: | |
Formato: | Electrónico eBook |
Idioma: | Inglés |
Publicado: |
Newark :
John Wiley & Sons, Incorporated,
2015.
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Colección: | New York Academy of Sciences Ser.
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Temas: | |
Acceso en línea: | Texto completo |
Tabla de Contenidos:
- Cover
- Contents
- Preface to First Edition
- Preface to Second Edition
- Preface to Third Edition
- Preface to Fourth Edition
- Chapter 1 From Newton to Hubble
- 1.1 Historical Cosmology
- Newton's Cosmology.
- Rotating Galaxies.
- Black Holes.
- Galactic and Extragalactic Astronomy.
- The End of Newtonian Cosmology.
- 1.2 Inertial Frames and the Cosmological Principle
- 1.3 Olbers' Paradox
- 1.4 Hubble's Law
- The Expanding Universe.
- Hubble Time and Radius.
- The Cosmic Scale.
- The Hubble Constant.
- Statistics.
- 1.5 The Age of the Universe
- Cosmochronology by Radioactive Nuclei.
- Brightest Cluster Galaxies (BCGs).
- 1.6 Matter in the Universe
- Baryonic Matter.
- Supernovae and Neutron Stars.
- Dark components.
- 1.7 Expansion in a Newtonian World
- Newtonian Mechanics.
- Expansion.
- Models of Cosmological Evolution.
- Chapter 2 Special Relativity
- 2.1 Lorentz Transformations
- Lorentz Transformations.
- Time Dilation.
- Relativity and Gold.
- Light Cone.
- Redshift and Scale Factor.
- 2.2 Metrics of Curved Space-time
- Euclidean Space.
- Minkowski Space-time.
- Gaussian Curvature.
- Comoving Coordinates.
- The Robertson-Walker Metric.
- 2.3 Relativistic Distance Measures
- Proper Distance.
- Particle and Event Horizons.
- Redshift and Proper Distance.
- Redshift and Luminosity Distance.
- Parallax Distance.
- Angular Size Distance.
- Distance Ladder Continued.
- 2.4 Tests of Special Relativity
- Chapter 3 General Relativity
- 3.1 The Principle of Equivalence
- Falling Photons.
- Superluminal Photons.
- 3.2 The Principle of Covariance
- Tensors.
- General Covariance.
- 3.3 The Einstein Equation
- The Einstein-Hilbert Action.
- Stress-Energy Tensor.
- Energy of Gravity Waves.
- 3.4 Weak Field Limit
- Chapter 4 Tests of General Relativity
- 4.1 The Classical Tests
- Mercury's Perihelion Shift.
- Deflection of Star Light.
- Timekeeping in Gravitational Fields.
- Radio Signal Delay.
- 4.2 Binary Pulsars
- 4.3 Gravitational Lensing
- Weak Lensing.
- Strong Lensing.
- Surface Brightness and Microlensing.
- Cosmic Shear.
- Weak Lensing Surveys.
- 4.4 Gravitational Waves
- Tensor Field.
- Sources of Gravitational Waves.
- Gravitational Wave Detection.
- Chapter 5 Cosmological Models
- 5.1 Friedmann-Lemaitre Cosmologies
- Friedmann's Equations.
- General Solution.
- Einstein Universe.
- The Friedmann-Lemaitre Universe.
- Energy-Momentum Conservation.
- Entropy Conservation and the Equation of State.
- Early Time Dependence.
- Big Bang.
- Late Einstein-de Sitter Evolution.
- Evolution of a Closed Universe.
- The Radius of the Universe.
- Late Friedmann-Lemaitre Evolution.
- 5.2 de Sitter Cosmology
- 5.3 The Schwarzschild Model
- The Schwarzschild Metric.
- 5.4 Black Holes
- Event Horizons.
- Hawking Radiation.
- Black Hole Creation.
- Observations of Black Holes.
- 5.5 Extended Gravity Models