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[4097] Physics 316: Extragalactic Astronomy and Cosmology
Summary of Lectures
Unless otherwise noted, all lectures will take place in
Physics Bldg Rm107
A more
detailed (topic-based) Revision Summary is also
available.
PLEASE NOTE The list of topics & links are intended to
help you remember what has been covered etc AFTER the lecture.
The topics & links for any future lectures may change without
notice, and hence should be considered highly provisional.
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Date |
Topic(s) |
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Lecture 1 |
2002 Jan 28 |
Introductions,
Logistics,
Course Overview, etc etc
Start
Part 1 - A Brief Review of Early Cosmolgical Ideas
Introduction,
Birth of "Scientific" Cosmology,
Aristotle,
Hipparchus,
and
Parallax
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Lecture 2 |
2002 Jan 30 |
Ptolemy,
The "State of the Universe" for the Greeks,
The "Dark" Millennium,
The Recovery of W.European Science
and
Ockham's Razor
[+Video clip]
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Lecture 3 |
2002 Feb 01 |
Other Early Cosmologies (?),
Timeline/Summary of Early Developments,
End
Part 1 - Take-Home Facts.
Start
Part 2 - The Foundations of Modern Cosmological
Ideas ,
The Earth moves from Center Stage,
Rumblings of Discontent,
Nicholas Copernicus,
The Cosmological Principles
( Copernican CP
and
Perfect CP)
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Lecture 4 |
2002 Feb 04 |
Anthropic Cosmological Principles,
Tycho Brahe,
Johaness Kepler,
Radical Ideas Abound !
(Galileo Galilei;
Inertial Frames),
The Speed of Light is Finite ,
And Then the Apple Dropped
(Issac Newton;
From Newton to Kepler,
Galileo's Principle of Equivalence;
A Physical Cosmology),
The Concept of Spacetime,
Curved Space - A Mathematical Concept
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Lecture 5 |
2002 Feb 06 |
Review of Non-Euclidean Geometries,
Curved Spacetime & Gravity (GR),
(Mach's Principle)
Finite or Infinite ? (Revisited),
(Olbers' Paradox,)
Einstein makes a Blunder ? ,
The Cosmological Constant [Lect5]
The Universe is Expanding !,
"Serendipitous" & Other Discoveries,
Finally ! - The First Rung on the Cosmic Distance Ladder,
"Island" Universes ?,
Studies of the Local Group,
The Distance to M31
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Lecture 6 |
2002 Feb 08 |
Detection of Redshift,
Hubble goes Fainter,
Hubble's Law,
(Hubble's Law & Cosmology,
More on the Hubble Parameter),
The Goals of Observational Cosmology,
The Robertson-Walker Metric,
(Bothun Sect 1.2.2),
The Density Ratio Omega
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Lecture 7 |
2002 Feb 11 |
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Lecture 8 |
2002 Feb 13 |
The "Hubble Time",
R(t) as a function of time,
R(t) as a function of redshift,
Redshift & Age
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Lecture 9 |
2002 Feb 15 |
Redshift & "Lookback" Time,
Min Age Requirements (Rocks, Beyond the Solar system),
The Extragalactic Distance Scale,
The Distance "Ladder",
Rung 1: Parallax,
Rung 2: Star Clusters
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Lecture 10 |
2002 Feb 18 |
The "Standard Candles,
Why Bother with Star Clusters,
Determining the Distances
(Main Sequence Fitting),
Rung 2.5: Calibrating the Main Sequence,
Rung 3: The Zero points for the Standard Candles,
Cepheid Variables,
Cepheid Variables vs RR Lyrae Distances,
Rung 4: Distance to the Local Group
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Lecture 11 |
2002 Feb 20 |
Rung 5: Techniques for getting into the Hubble Flow
(Tully Fisher Relation,
Planetary Nebula Luminosity Function,
Gobular Cluster Luminosity Function,
Surface Brightness & Luminosity Fluctuations)
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Lecture 12 |
2002 Feb 22 |
Luminosity of Supernovae,
SNe Ia & Cosmology (pre 1995),
Potential Problems,
SNe Ia Constraints on H0 (Low z),
Recent (High z) Results
[Acceleration,
Deceleration]
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Lecture 13 |
2002 Feb 25 |
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Lecture 14 |
2002 Feb 27 |
SNe Ia: A Warning,
More detailed look at the potential problems,
Distance Ladder Summary,
Importance of "Other" fields,
Direct Distance Measurement Techniques,
Moving out of the Neighborhood,
Virgo - "Our Galaxy Cluster",
Distance to Virgo,
Pushing ever further out...,
The Virgo-Centric Flow
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Lecture 15 |
2002 Mar 01 |
Homework Review
(Distance to the Virgo Cluster
Direct Distance Measurement Techniques
Peculiar Motions towards Virgo & beyond),
The Cosmic Microwave Background (CMB),
Discovery,
COBE,
CMB Spectrum from COBE,
The Dipole Anisotropy
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Lecture 16 |
2002 Mar 04 |
[No new material was covered]
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Lecture 17 |
2002 Mar 06 |
COBE CMB Fluctuations,
"Problems" with the CMB Uniformity,
(Flatness,
Horizon,
Smoothness),
Inflationary Models,
Predictions of Inflation,
Post-COBE CMB Observations,
Recent Results,
The Angular Power Spectrum,
Cosmological Implications of the Peaks,
The Main Peaks - Curvature
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Lecture 18 |
2002 Mar 08 |
The Main Peaks - Baryon Density,
The Higher Harmonics,
Recent Results
( The Universe is Flat !,
The Baryon Density is small),
Summary of the Angular Power Spectrum,
The MAP Mission,
The Planck Mission,
The Production of the "Light" Elements (Quick Overview)
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Lecture 19 |
2002 Mar 11 |
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Lecture 20 |
2002 Mar 13 |
Start Part 3 - The Current Hot Big Bang Paradigm,
"Normal" Baryonic Physics,
Review of the Planck Function,
Dependence of the Densities with Scale Factor,
The Current Densities,
The Nucleon to Photon ratio,
Review of Rest Mass Energies
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Lecture 21 |
2002 Mar 15 |
No Lecture |
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Lecture 22 |
2002 Mar 18 |
Review/Open-Revision
e-mail "requests" ahead of time to
ian.george@umbc.edu
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Lecture 23 |
2002 Mar 20 |
"Mid-term Exam (25%)
(Rm107, 11:00-11:50)
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Lecture 24 |
2002 Mar 22 |
Review of the details,
Note the General Resources Page
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Spring Break |
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Lecture 25 |
2002 Apr 01 |
Scale factor vs Time,
Scaling Summary,
Quick Review of "Particle Physics",
Bosons & Fermions,
The Standard Model,
Fundamental Particles,
Quarks
[& Hadrons],
Leptons,
Electroweak Unification,
Force Mediators,
Grand Unified Theories
[Gauge Theory,
Spontaneous Symmetry Breaking]
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Lecture 26 |
2002 Apr 03 |
CPT Symmetries,
CP Violations for Weak Interactions,
Strong CP Problem,
Axions,
Supersymmetry (SUSY),
Particle Theories & Cosmology,
Particles in the Early Universe,
Relativistic vs Non-relativistic,
Planck Function for Particles,
Relativistic Energy Density
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Lecture 27 |
2002 Apr 05 |
Rest-Mass Example,
Around the Thresholds,
Brief History of the Early Universe
(Recombination,
Radiation-Matter Equality,
BBN,
e-e+ Pairs,
Neutrino Decoupling,
Muons,
Pions,
Hadrons,
Tauons,
Electroweak,
Inflation,
Planck Time)
Summary (forwards in time),
End Part-3
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Lecture 28 |
2002 Apr 08 |
Start:
Part 4 - The Large-scale Structure of the Universe,
Structures Observed in the Universe,
"Obvious" Observational Overview,
Observations are all we have,
Hierarchical Structures,
Groups of Galaxies,
Clusters of Galaxies,
Cluster Surface-Brightness Profiles,
Gravitationally-Bound Structures ?,
X-rays & the Intracluster Medium (ICM),
ICM Abundances
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Lecture 29 |
2002 Apr 10 |
Cluster Timescales,
Main Points,
X-ray Cooling,
Bremmstrahlung,
Cooling Flows,
Structures on Larger Scales,
Early Redshift Surveys,
Techniques,
The Stickman,
The Main Questions,
How big are the Voids ?,
A Quick Tour,
Current Surveys & Latest Results
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Lecture 30 |
2002 Apr 12 |
General Review of Bothun Chapt 3
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Lecture 31 |
2002 Apr 15 |
The "Great Attractor",
The "Great Wall",
The Hubble Deep Fields,
Report Format,
Cite your sources,
Captions & Numbering
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Lecture 32 |
2002 Apr 17 |
Dark Matter in the Universe,
Detecting the Influence,
Spiral at Test Case,
Components to the Milky Way,
The Sun's Place in the Galaxy,
The Sun's Neighbours,
The Virial Theorem,
DM in the Solar Neighbourhood ?,
DM on Galactic Scales,
Flat Rotation Curves
& Implications ,
Other Indicators of DM around Galaxies,
Some M/LRatios,
DM Candidates,
DM Problems,
DM or Gravity ?!,
Baryonic DM Candidates,
Non-Baryonic DM Candidates,
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Lecture 33 |
2002 Apr 19 |
The Solar Neutrino Problem ,
The Solar Neutrino Problem Solved !,
The DM Problem - Not solved ! ,
Further Implications of DM ,
Summary of Bothun Chapt4 ,
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Lecture 34 |
2002 Apr 22 |
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Lecture 35 |
2002 Apr 24 |
The Jeans Length & Mass,
Instability & Expansion,
Jeans Mass Prior to Recombination,
Jeans Mass Post Recombination
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Lecture 36 |
2002 Apr 26 |
Evolution of a Density Perturbation,
The "Acoustic" Period & CDM,
Top-down or Bottom-up ?,
The Statistics of the Large-scale Structure,
The Two-Point Correlation Function
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2002 Apr 29
thru May 02 |
Face-to-Face discussions of Student Reports
(& requirements for your presentation)
e-mail for an appointment ahead of time to
ian.george@umbc.edu
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Lecture 37 |
2002 Apr 29 |
[No new material was covered]
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Lecture 38 |
2002 May 01 |
The Power Spectrum,
Summary of Bothun Sect5.2,
Summary of Bothun Sect5.2,
Power Spectrum of Galaxies,
Power Spectrum of Clusters,
Cosmological Implications,
Fixes to CDM Models[Lect38]
The New Standard Model,
High Redshift Galaxies,
So use a Magnifier !
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Lecture 39 |
2002 May 03 |
Student Presentations |
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Lecture 40 |
2002 May 06 |
Sample Spectra - First-cut Identification,
What is a "Galaxy" anyhow ?,
Star Formation vs Redshift,
High Redshift Quasars as Cosmological Probes,
The Recold Holders (to date),
Quasar Absorption Line Studies,
Damped Lyman alpha in Absorption,
Metals vs Redshift,
The Distribution of Baryons,
The ExtraGalactic Background,
The Galaxy Luminosity Function
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Lecture 41 |
2002 May 08 |
| Guest Lecture by Dr Turner
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Normal & Active Galaxies,End Part 4
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Lecture 42 |
2002 May 10 |
General in-class review
of what we've covered & prospects for the future
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Lecture 43 |
2002 May 13 |
Review/Open-Revision
e-mail "requests" ahead of time to
ian.george@umbc.edu
|
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2002 May 22 |
Final Exam (30%)
(Rm107, 10:30-12:30)
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PLEASE NOTE The list of topic & links are intended to
help you remember what has been covered etc AFTER the lecture.
The topics & links for any future lectures mau change without
notice, and hence should be considered highly provisional.
|