Fakultät für Mathematik und Naturwissenschaften


Dr. Julian Rautenberg

Vorlesung und Übung (V3Ü1).


Termin Vorlesung:

Di. 12:00-14:00, F.13.15

Folien und Script: VL01, S01, VL02, S02, VL03, S03, VL04, S04, VL05, S05, VL06, S06, S07, VL08, S08, VL09, S09, VL10, S10, VL11, S11, VL12, S12, VL13, S13, VL14, S14

Termin Übung:

Do. 11:00-12:00, F.13.11

Exercises: Ex-01, Ex-02, Ex-03, Ex-04, Ex-05, Ex-06, Ex-07, Ex-08, Ex-09, Ex-10, Ex-11

Literature Cosmology

An introduction to modern cosmology

A. R. Liddle

Wiley 2003

73 VEQ1918


M. Rowan-Robinson

Clarendon Press 2003

73 VEQ1112

An invitation to astrophysics

T. Padmanabhan

World Scientific 2006

73 VDA1736

An introduction to the science of cosmolog

Peacock, John A

Cambridge Univ. Press 2003

73 VEQ1887


S. Weinberg

Oxford Univ. Press 2008

73 VEQ1968

Modern cosmology

S. Dodelson

Acad. Press 2007

91 VEQ1926

An introduction to modern astrophysics

B. W. Carroll, D. A. Ostlie

Addison-Wesley 1996

73 VDA1689

Der neue Kosmos

A. Unsöld, B. Baschek

Springer 2002

73 VAP1179

Contents Cosmology

  1. History
  2. Astronomical Observables
    1. Magnitude
    2. Coordinate Systems
    3. Distance Measurement
    4. Redshift
    5. Hubble Expansion
  3. Newton Universe
    1. Olber's Paradoxon
    2. Cosmological Principles
    3. Scaling Factor
    4. Expansion & Redshift
  4. Metric of Space-Time
    1. Co-moving Variables
    2. Friedmann Equation
    3. Fluid Equation
    4. Acceleration Equation
    5. Minkowski Metric
    6. Robertson-Walker Metric
    7. Flat, spherical & hyperbolic Geometry
  5. Simple Models and observational Parameters
    1. Light propagation and Redshift
    2. Cosmological dynamic under radiation and matter
    3. Cosmological dynamic under curvature
    4. Density Parameter
    5. Deceleration Parameter
    6. Luminosity Distance
    7. Angular diameter distance
    8. Source counting
  6. Cosmological Constant
    1. Extension of equations with Λ
    2. Historical context
    3. Dynamic of the Universe with Λ
    4. Effect of Λ on luminosity and angular diameter distance
  7. Age estimation
    1. Hubble time
    2. Age of Solar System
    3. Age of our Galaxy
    4. Stellar evolution of globular cluster
  8. The early Universe
    1. Radiation under adiabatic expansion
    2. Transition from radiation- to matter-dominated Universe
    3. Hot Big Bang
    4. Big Bang Nulearsynthesis
    5. Decoupling of radiation and matter
    6. Cosmic mirowave background
    7. CMB anisotropy
    8. CMB polarization

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