Proposal for a One-Year Graduate Cosmology Sequence
We are proposing a two-semester sequence covering modern observational and
theoretical cosmology (and cosmogony), designed to provide a sophisticated
survey dealing with the production of particles and elements in the Big Bang,
the cosmological production and growth of mass perturbations, dark matter and
energy, cosmological parameters, the intergalactic medium, heating and
reionization, and astronomical sources as cosmological probes and as products
of structure formation in cosmology.
The course develops succintly the required tools in general relativity,
statistical mechanics, field theory and observational techniques so as to limit
the number of required prerequisites.
One year of quantum mechanics and one year of classical mechanics are required.
A course in introductory astronomy or astrophysics is strongly recommended.
Mathematics includes integral calculus, tensors, some differential equations
and special functions (gamma functions, spherical harmonics, elliptical
integrals, etc.)
This sequence will serve as an elective in the astronomy graduate sequence.
The current Astro G6005 partially satisfies the physics departments graduate
level phenomenology requirement.
We propose sequencing the topics into primarily observational topics during one
semester and theoretical topics during the other in order to make the
additional semester apply to the physics department theory elective.
Ideally, perhaps, this course should be shared between Astronomy and Physics,
with a theorist from one department and an observer from the other; one might
imagine Crotts and Hui (or his replacement), or Haiman and Miller.
The two semesters are best taught in temporal order, but could be interrupted
by summer or one semester.
We envision splitting the semesters roughly as follows, with the first semester
dealing with the derivation of the Friedmann equations from General Relativity,
the nearby universe up through redshifts of a few, including galaxy evolution,
AGN, and quasar absorption lines, terminating in a discussion of large scale
structure including development of structure formation in the linear regime,
with mention of the CMB in terms of observational constraints.
The second semester would briefly review these topics, and deal with non-linear
growth of structure, appearance of the first objects, reionization, the "dark
ages", recombination in detail, Big Bang entropy and dark matter production,
BB nucleosynthesis, electroweak decoupling (and spontaneous symmetry breaking),
baryogenesis, Grand Unified theories, inflation, and the quantum gravitational
epoch.
Below is the proposed syllabus.
- Arlin and Zoltan
COURSE DESCRIPTION
G6005-6: OBSERVATIONAL AND
PHYSICAL COSMOLOGY
The Universe is much
bigger than it was 25 years ago; suddenly there is much more room for new
questions about the physical nature of the Cosmos. More importantly, some of
these questions are being answered. This is due in part to major advances in the
technology of astronomical observation, but due as well to new
cross-fertilization between astrophysics and particle physics. In addition,
there are many clever ideas that have cropped up recently due to neither effect;
maybe more people are simply more excited about cosmology these days.
The upshot of all these recent developments is that no textbook exists
that covers the whole field. John Peacock's Cosmological Physics (1998)
or Thanu Padmanabhan's Galaxies and Cosmology (2002) do a good job of
covering cosmological theory, and a satisfactory treatment of the observational
side.
In truth, much of the material is too recent to be found in any textbook.
Much material will only be covered in the lecture notes (photocopies of the
lecture viewgraphs).
To accomodate the more recent material, about 10% of the course will
consist of a "journal club" where members of the class report (for about 20
minutes at a time) on papers that interest them.
These are selected from the list at the back of this course description
(or choose your own! - consult with the professor first).
Depending on class size, each student will present one or two of these during
the semester.
The professor
will lecture the bulk of the remaining time (expect some guest lecturers for
some of special topics); there will be a final which counts for 50% of the
course grade, and a short midterm quiz.
A few problem sets will also be assigned.
Attendance is important!
Course Outline
- I. Thumbnail History and Gravitational Theory
- A. Data and Paradigm Shifts in Ancient and Classical Astronomy
- 1. Solar System and Distant Stars
- a. Ancient Measurements: Earth/Moon/Sun
- b. Copernicus and Heliocentric Universe
- c. Bruno and Cosmological Principle
- d. Interstellar Distances
- 2. Island Universe
- a. Galileo
- b. Herschel
- c. Wright/Kant
- d. Kapteyn
- e. Shapley
- B. Theories of Gravitation
- 1. Newtonian Cosmology
- a. No Static, Homogeneous, Massive Solution
- b. Birkoff's Approximation
- 2. General Relativity [Peacock, ch. 1.1-1.5]
- a. Principle of Equivalence
- b. Tensors
- c. Curvature, Parallel Transport, Connection Coeff's
- d. Einstein Field Equations
- e. Stress/Energy Terms
- i. Normal Matter: "Dust"
- ii. Pressure/Radiation
- iii. Cosmological Constant
- iv. Quintescence and Equation of State
- f. Robertson-Walker Metric [Peacock, ch. 3.1-3.3]
- g. Friedmann Equations
- h. Cosmological Models/Parameters
- E. Galaxian Universe
- 1. Curtis/Shapley Debate
- 2. Hubble
- a. Extragalactic Distance Scale
- b. Redshift/Distance Relation
- II. Extragalactic Menagerie
- A. Galaxies [Peacock, ch. 12-13]
- 1. Luminosity Function
- 2. Morphology
- 3. Multiwavelength Survey
- a. Environmental dependence
- b. Mass dependence
- 3. Kinematic/Surface Brightness Regularities
- a. Spiral Arm Surface Brightness and Tully-Fisher Law
- b. Elliptical Core Surface Brightness and D_n vs. sigma
- 4. Evidence for Galaxian Dark Matter (Peebles 1993, sec. 18)
- a. Solar Neighborhood Measurements
- b. Milky Way Rotation
- c. LMC Dynamics
- d. Spiral Rotation Curves
- e. Disk Stability
- f. Elliptical Masses
- i. Stellar Velocity Dispersion
- ii. Planetary Nebulae
- iii. Globular Clusters
- g. Dwarf Galaxies
- h. MACHO searches [Peacock, ch. 4.5]
- 5. Radio Properties & Types
- 6. Infrared Properties
- 7. High Energy Emission
- B. Active Galactic Nuclei [Peacock, ch. 14]
- 1. Seyfert Galaxies
- a. Type I
- b. Type II
- c. Unified Model
- 2. BL Lacs
- 3. Quasars
- 4. Point-source X-ray Background
- C. Lyman-alpha Clouds (Peebles 1993, sec. 23)
- 1. Low-redshift Identification
- 2. High-redshift Nature
- 3. Redshift Evolution
- 4. Numerical Models
- 5. Size Constraints
- 6. Collapse versus Evaporation
- D. Intergalactic Medium
- 1. Gunn-Peterson Test
- a. neutral H
- b. He II
- c. He I
- d. Reionization Epochs
- 2. Heating and Cooling
- 3. X-ray Background
- E. Gamma-Ray Bursts
- F. Highest Energy Cosmic Rays
- III. Expanding Universe [K & T, ch. 3]
- A. Tests for Cosmological Expansion
- 1. Surface Brightness versus Redshift
- 2. Temperature versus Redshift
- 3. Foreground/Background Pair Redshifts
- 4. Gravitational Lensing
- B. Distance Ladders [Jacoby et al. 1992, Peacock, ch. 5.3-5.6]
- 1. Local Kinematic Distance Indicators
- a. Parallax
- b. Moving Cluster Method
- c. Statistical Proper Motion
- 2. Stellar Indicators
- a. Main Sequence Photometry
- b. RR Lyrae Variable Stars
- c. Delta Cephei/W Virginis stars
- d. Novae
- e. Supernovae
- 3. Cluster/Nebular Indicators
- a. H II Regions
- b. Globular Clusters
- 4. Galaxian Indicators
- a. Brightest Cluster Galaxies
- b. Surface Brightness Fluctuations
- c. Tully-Fisher Relation
- d. D_n - sigma Relation
- e. Fundamental Plane
- 5. Possible Systematic Errors
- a. Observational Selection Biases
- i. Malmqvist Bias
- ii. Scott Effect
- iii. Object Confusion
- aa. Crowding
- bb. Misidentification
- b. Galaxian Evolution
- c. Deviations from Hubble Flow
- 6. Hubble Constant Measurements
- 7. Quasar Grav. Lensing Determinations [Peacock, ch. 4.1-4.4]
- 8. Sunyaev-Zeldovich
- C. q_0 Indicators [Peacock, ch. 3.4]
- 1. Standard Candles
- a. Brightest Galaxies
- b. High-redshift Tully-Fisher/Faber-Jackson Relation
- c. Supernovae
- 2. Standard Rulers
- a. Radio Galaxies
- b. Void Spacing
- c. theta(z) versus dz (Alcock-Paczynski) Test
- 3. Population Number Density
- D. Tests for Homogeneity and Isotropy
- 1. Radio Source Counts
- 2. Infrared Source Counts
- 3. X-ray Background
- 4. Microwave Background
- 5. Alignment Anisotropy
- IV. Galaxy Evolution [Peacock, ch. 5.1]
- A. Lookback Time
- B. K-correction and Lyman Dropouts
- C. Observed versus Evolving Colors
- D. Stellar Population Synthesis
- E. Observed Samples
- 1. Field Galaxies
- a. HDF, HDFS
- b. CFH sample
- c. CNOC, etc.
- 2. Cluster Galaxies
- F. Butcher-Oemler Effect
- G. Red Envelope Ellipticals
- H. Faint Blue Galaxies
- I. Morpological Evolution
- J. Bottom-Up Scenario
- V. Large Scale Structure [Peebles 1980, sec. 29-33; Peebles 1993, sec. 19]
- A. Galaxy-galaxy Clustering [Peacock, ch. 16]
- 1. Two-point Clustering
- 2. Power Spectrum
- 3. Three-point Measures and Bispectrum
- 4. Other Measures
- B. Galaxy Clusters
- 1. Cluster Classification
- 2. Galaxy Type versus Cluster Environment
- 3. Hot Gas in Clusters
- 4. Dark Matter in Galaxian Systems [Peacock, ch. 4.6]
- a. Small Groups
- b. Rich Clusters
- 5. Cluster-cluster Two-point Function
- C. Galaxy Superclusters
- D. Voids
- E. Bulk Motions
- F. Large Scale Perturbation Spectrum [Peacock, ch. 15]
- G. Early Structure Formation
- 1. Quasars
- 2. Galaxies
- a. High Redshift Carbon Monoxide
- b. Damped Ly alpha
- H. Non-linear Growth
- 1. Hydrodynamic Effects
- 2. Hot Dark Matter
- 3. Cold Dark Matter
- 4. Cosmic Strings
- I. Biasing
- J. Press-Schecter Formalism
- VI. Galaxy Formation [K & T, ch. 9, Peebles 1993, sec. 25, Peacock,
ch. 17]
- A. Hydrodynamic Collapse
- 1. Jeans Mass
- 2. Fragmentation Processes
- 3. Hydro/gravitational simulations
- a. Particle-particle (PP) Direct Summation
- b. Particle Mesh (PM)
- c. Particle-particle/Particle Mesh (P3M)
- d. Adaptive P3M (AP3M)
- e. Tree Codes
- f. Smooth-particle Hydro (SPH)
- g. Piecewise Parabolic "Eulerian" Method hydro (PPM)
- h. Simulation code competition
- i. Mock Hydro (Gneden and Hui)
- j. Semi-Analytic Models (SAM)
- B. Spheroidal Component Formation
- C. Disk Formation
- D. Galaxy/IGM Feedback
- E. Cold Dark-Matter Galaxy Formation Problems
- a. Halo Profile Cusp/Core
- b. Angular Momentum
- c. Satellite Galaxy Number
- d. Standard versus Non-standard (MOND?) solutions
- F. Formation of Galaxy Clusters
- G. AGN and Black Hole Formation
- H. Reionization and Earliest Objects
- VII. Cosmological Lensing
- A. Strong Quasar Lensing and Microlensing
- B. Lensing Incidence and Omega_lens
- C. Strong Cluster Lensing
- D. Weak Lensing
- E. Lensing Probe of Galaxy Potentials
- VIII. Microwave Background [Peebles 1993, sec. 6, Peacock, ch. 9.3-9.4,18]
- A. Anisotropy
- 1. Dipole Term
- 2. Power Spectrum
- 3. Comparison to Galaxy Clustering
- B. Hot Gas Distortion
- 1. Cluster Sunyaev-Zeldovich Effect
- 2. High Redshift Galaxies
- C. Blackbody Spectrum
- D. Implications for Galaxy Formation
- E. Matter versus Radiation Domination
- F. COBE Results
- G. Boomerang, DASI, Maxima, CBI, etc. Results
- H. MAP Results
- I. Acoustic Doppler Peaks
- J. Damping Envelope
- K. Deriving Cosmological Parameters
- L. Polarization - E versus B modes
- IX. Dark Matter Statistical Mechanics [K&T, ch. 5, Peacock, ch.
9.1-9.2, 12.5]
- A. Hot Dark Matter Production
- B. Cold Dark Matter Production
- X. Big Bang Nucleosynthesis [Kolb & Turner, ch. 4, Peacock, ch. 9.5]
- A. Thermal Equilibrium
- B. Neutrino Decoupling
- C. Light Element Production
- D. Theoretical versus Observed Abundances
- E. Number of Particle Families
- F. Limits on Omega_baryon
- G. Baryon/Photon Ratio
- XI. Phase Transitions [K & T, App. B & ch. 7, review Peacock, ch.
6,7, 8.1-8.9]
- A. Electroweak Unification
- 1. Higgs Field
- 2. Spontaneous Symmetry Breaking
- 3. Mixing of Restored Symmetry Eigenstates
- B. Grand Unified Theories
- 1. GUT Scale
- 2. SSB
- 3. Topological Defects [Peebles 93, sec. 11,16, Peacock, ch.10]
- a. Monopoles
- b. Strings
- c. Domain Walls
- d. Textures
- 4. Baryon Decay/Non-conservation
- XII. Baryogenesis [Kolb & Turner, ch. 6]
- A. Matter versus Antimatter in the Universe
- B. Charge/Parity Violation
- C. Non-equilibrium Decay
- XIII. Inflation [Peacock, ch. 11, Kolb & Turner, ch. 8]
- A. Incompleteness of Standard Big Bang
- 1. Homogeneity Problem
- 2. Flatness/Lifetime Problem
- 3. Large Entropy of the Universe
- 4. Monopole Problem
- 5. Vanishing Cosmological Constant
- B. Original Inflation
- C. Chaotic Inflation
- D. "New" Inflation
- E. Extended Inflation
- XIV. Planck Epoch [Kolb & Turner, ch. 11; Peacock, ch. 8.10]
- A. The Universal Wavefunction
- B. Tunneling from the Vacuum State
- C. Quantum Initial Conditions
- D. String Theory
- E. Etcetera ...
- XV. Reprise
- A. Dark Matter Constraints
- 1. Baryonic Matter
- 2. Low-mass Neutrinos
- 3. Cold Dark Matter
- 4. Axions
- 5. Decaying Massive Particles
- 6. Massive Black Holes
- 7. Shadow Matter, etc.
- B. Cosmic Time [Peacock, ch. 5.2]
- 1. Cosmochronology
- 2. Globular Cluster Ages
- 3. Omega, Lambda and H_0
- C. Cosmological Parameter Constraints
- 1. BBN (Omega_baryon h-squared)
- 2. CMB (Omega_lambda + Omega_m, Omega_m h-squared, sigma_8, h, t_0...)
- 3. SNe Ia Standard Candles (Omega_lambda - Omega_m, roughly)
- 4. Galaxy Redshift Surveys (Omega_m^0.6/b, b sigma_8, Omega_m h)
- 5. POTENT Bulk Flows (sigma_8 Omega_m^0.6, Omega_m h)
- 6. Cluster Numbers (sigma_8 Omega_m^0.6)
- 7. Weak Lensing (sigma_8 Omega_m^0.6)
- 8. Baryon Fraction
- 9. Hubble Parameter
- 10. Alcock-Paczynski (Omega_lambda, roughly)
- D. Topology of the Universe
- E. Anthropic Principle [Peacock, ch. 3.5]
REQUIRED
TEXTS:
Cosmological Physics John A. Peacock 1998 (Cambridge
Univ. Press; Cambridge), ISBN 0521422701 (paperback - $40 at Barnes and Noble);
chapters on general
relativity, isotropic universe, gravitational lensing, age and distance scales,
hot big bang, matter in the Universe, galaxies and their evolution, active
galaxies, structure formation, cosmological density fields, galaxy formation,
cosmic background fluctuations, quantum mechanics, quantum fields, inflationary
cosmology
Galaxies and Cosmology (Theoretical Astrophysics, Volume III) Thanu
Padmanabhan 2002 (Cambridge Univ. Press; Cambridge), ISBN 0521566304 (paperback
- $52 at Barnes and Noble)
REQUIRED ARTICLES (To Be Distributed):
R.D. Blandford, R. Narayan 1993, Ann. Rev. Astron. Astrop., 30, 311.
"Cosmological Applications of Gravitational Lenses"
G.H. Jacoby, D. Branch, R. Ciardullo, R.L. Davies, W.E. Harris, M.J.
Pierce, C.J. Pritchet, J.L. Tonry, D.L. Welch 1992, Proc. Astron. Soc. Pac.,
104, 570. "A Critical Review of Selected Techniques for Measuring Extragalactic
Distances"
Carroll, S.M., Press, W.H., Turner, E.L. 1992, Ann. Rev. Astron. &
Astrop., 30, 499. "The Cosmological Constant"
BACKUP TEXTS (On Reserve):
Gravitation and Cosmology: Principles and Applications of the General
Theory of Relativity Steven Weinberg 1972 (Wiley: New York)
The Early Universe Edward W. Kolb & Michael Turner 1990
(Addison-Wesley: Redwood City, CA), chapters on Robertson-Walker Metric,
Standard Cosmology, Big Bang Nucleosynthesis, Thermodynamics, Baryogenesis,
Phase Transition, Inflation, Structure Formation, Planck Epoch, Appendix B
Principles of Physical
Cosmology P.J.E. Peebles 1993 (Princeton U. Press: Princeton), sections on
Expanding Universe; Thermal Cosmic Background Radiation; Walls, Strings,
Monopoles, and Textures; Dark Matter; Young Galaxies and Intergalactic Medium;
Galaxy Formation
The Early
Universe: Reprints Edward W. Kolb & Michael Turner 1988 (Addison-
Wesley: Redwood City, CA)
Large-Scale Structure of
the Universe P. J. E. Peebles 1980 (Princeton U. Press: Princeton)
SUGGESTED READINGS (On Reserve):
D.N. Schramm: "The First Three
Minutes: 1990 Version" and P. J. E. Peebles "General Introduction" in *After*
the First Three Minutes eds. Holt, Bennett & Trimble 1990 (Amer. Inst.
Physics: New York)
The Anthropic Cosmological
Principle John Barrow & Frank Tipler 1986 (Oxford U: New York)
Gravitation Charles W. Misner, Kip S. Thorne & John
A. Wheeler 1973 (Freeman: San Francisco)
Plus: the
remaining chapters of Kolb & Turner 1990 and Peebles 1993
FUN:
Man Discovers the Galaxies R. Berendzen, R. Hart & D. Seely
1976 (Science History Publishers: New York)
Darkness
at Night: A Riddle of the Cosmos Edward Harrison 1987 (Harvard U:
Cambridge)
The First Three Minutes: A Modern View of the Origin
of the Universe Steven Weinberg 1982 (Basic Books: New York)
The Fifth Essence: A Search for Dark Matter in the Universe
Lawrence Krauss 1990 (Basic Books: New York)
REFERENCES FOR DISCUSSION: (to be distributed later...)