Astrophysics I

Written by Quantum Study Club on 18.15

Oleh:
Arip Nurahman
Department of Physics
Faculty of Sciences and Mathematics, Indonesia University of Education

and

Follower Open Course Ware at Massachusetts Institute of Technology
Cambridge, USA
Department of Physics
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http://ocw.mit.edu/OcwWeb/Physics/index.htm
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Aeronautics and Astronautics Engineering
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8.901 Astrophysics I

Spring 2006

Staff

Instructor:
Prof. Deepto Chakrabarty

Course Meeting Times

Lectures:
Two sessions / week
1.5 hours / session

Level

Undergraduate / Graduate

Picture of a star orbiting a black hole.
An artist's vision of an exotic binary system illustrates how matter is drawn from the roughly solar-mass star into the black hole. (Image courtesy of M. Weiss (CXC), NASA on the Astronomy Picture of the Day Web site.)

Course Highlights

This course features a complete set of assignments and readings.

Course Description

This course provides a graduate-level introduction to stellar astrophysics. It covers a variety of topics, ranging from stellar structure and evolution to galactic dynamics and dark matter.


Syllabus

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Course Description

This course addresses a range of topics, including:

  • Size and Time Scales
  • Historical Astronomy
  • Astronomical Instrumentation
  • Stars
    • Spectra
    • Classification
  • Stellar Structure Equations and Survey of Stellar Evolution
  • Stellar Oscillations
  • Degenerate and Collapsed Stars
    • Radio Pulsars
  • Interacting Binary Systems
    • Accretion Disks
    • X-ray Sources
  • Gravitational Lenses
    • Dark Matter
  • Interstellar Medium
    • HII Regions
    • Supernova Remnants
    • Molecular Clouds
    • Dust
    • Radiative Transfer
    • Jeans' Mass
    • Star Formation
  • High-energy Astrophysics
    • Compton Scattering
    • Bremsstrahlung
    • Synchrotron Radiation
    • Cosmic Rays
  • Galactic Stellar Distributions and Populations
    • Oort Constants
    • Oort Limit
    • Globular Clusters

Textbooks

Amazon logo Hansen, Carl J., Steven D. Kawaler, and Virginia Trimble. Stellar Interiors: Physical Principles, Structure and Evolution. New York, NY: Springer, 2004. ISBN: 9780387200897.

Amazon logo Carroll, Bradley W., and Dale A. Ostlie. An Introduction to Modern Astrophysics. Reading, MA: Addison-Wesley Pub., 1995. ISBN: 9780201547306.

Amazon logo Kippenhahn, Rudolf, and Alfred Weigert. Stellar Structure and Evolution. New York, NY: Springer-Verlag, 1990. ISBN: 9780387502113.

Amazon logo Shapiro, Stuart L., and Saul A. Teukolsky. Black Holes, White Dwarfs, and Neutron Stars. New York, NY: Wiley, 1983. ISBN: 9780471873167.

Prerequisites

Thermodynamics and Statistical Mechanics (8.044), Quantum Mechanics II (8.05), or permission of the instructor.

Grading Policy


ACTIVITIES PERCENTAGES
Problem Sets 30%
Midterm Exam 30%
Final Exam 40%


Readings

Amazon logo Help support MIT OpenCourseWare by shopping at Amazon.com! MIT OpenCourseWare offers direct links to Amazon.com to purchase the books cited in this course. Click on the Amazon logo to the left of any citation and purchase the book from Amazon.com, and MIT OpenCourseWare will receive up to 10% of all purchases you make. Your support will enable MIT to continue offering open access to MIT courses.

Textbooks

Amazon logo Hansen, Carl J., Steven D. Kawaler, and Virginia Trimble. Stellar Interiors: Physical Principles, Structure and Evolution. New York, NY: Springer, 2004. ISBN: 9780387200897.

Amazon logo Carroll, Bradley W., and Dale A. Ostlie. An Introduction to Modern Astrophysics. Reading, MA: Addison-Wesley Pub., 1995. ISBN: 9780201547306.

Amazon logo Kippenhahn, Rudolf, and Alfred Weigert. Stellar Structure and Evolution. New York, NY: Springer-Verlag, 1990. ISBN: 9780387502113.

Amazon logo Shapiro, Stuart L., and Saul A. Teukolsky. Black Holes, White Dwarfs, and Neutron Stars. New York, NY: Wiley, 1983. ISBN: 9780471873167.

Readings by Session


SES # TOPICS READINGS
1 Introduction Hansen, Kawaler, and Trimble, chapter 1. You may also find Carroll and Ostlie, chapter 7 useful for background on stellar binaries.
2 Kepler Problem

Binaries
Hansen, Kawaler, and Trimble, chapter 1.

Carroll and Ostlie, chapter 7.
3 Stellar Distances

Coordinates

Magnitudes
Hansen, Kawaler, and Trimble, chapter 1.

Carroll and Ostlie, chapter 7.
4 Color-color Diagrams

Spectral/Luminosity Classes
Hansen, Kawaler, and Trimble, chapter 3, especially section 3.4. You may also find it useful to read chapter 8 in Carroll and Ostlie. Introduction to Modern Astrophysics. If you are interested in additional reading about the Saha Equation, you may also consult chapter 14 of Stellar Structure and Evolution by R. Kippenhahn and A. Weigert (1990, Springer).
5 Saha Equation Hansen, Kawaler, and Trimble, chapter 3.

Carroll and Ostlie, chapter 8.

Kippenhahn and Weigert, chapter 14.
6 Radiation

Opacity

Radiative Diffusion
Hansen, Kawaler, and Trimble, chapter 3.

Carroll and Ostlie, chapter 8.

Kippenhahn and Weigert, chapter 14.
7 Equations of Stellar Structure

Convection
Hansen, Kawaler, and Trimble, chapter 4 (including section 4.8). You should also at least look through chapter 5 on Convection.
8 Convection (cont.)

Modeling

Polytropes

Energy Sources
Hansen, Kawaler, and Trimble, chapters 4 and 5.
9 Nuclear Reaction Rates

Hydrogen Burning: pp, CNO
Hansen, Kawaler, and Trimble, chapter 6, chapter 7 (sections 7.1-7.2). (I encourage you to at least skim through the rest of chapter 7 as well.) We will also start covering the material in chapter 2 (sections 2.1-2.5), although homework problems on this material will be on Problem Set 5. (You should still do this reading prior to the midterm exam, however.)
10 H/He Burning

Nucleosynthesis

Low-M Stars
Hansen, Kawaler, and Trimble, chapters 2, 6, and 7.
11 Stellar Evolution: Lower Main Sequence

Cluster H-R
Hansen, Kawaler, and Trimble, chapters 2, 6, and 7.
12 S-C Limit

Solar Neutrinos

Degenerate Matter
Finish reading the first part of chapter 2 (sections 2.1-2.6) on Stellar Evolution in Hansen, Kawaler, and Trimble, and also read section 9.3 on the Solar Neutrino Problem. You may also find it useful to review sections 3.5-3.6 on Degenerate Equations of State. For a deeper discussion, you can consult chapters 2-3 of Black Holes, White Dwarfs, and Neutron Stars by Shapiro and Teukolsky.
13 Midterm exam Hansen, Kawaler, and Trimble, chapter 2, sections 3.5-3.6, and section 9.3.

Shapiro and Teukolsky, chapters 2 and 3.
14 Degenerate Matter

Chandra Mass

White Dwarfs
Hansen, Kawaler, and Trimble, chapter 2, sections 3.5-3.6 and 9.3.

Shapiro and Teukolsky, chapters 2 and 3.
15 White Dwarf Cooling

Intrinsically Variable Stars
Finish reading the rest of chapter 2 (sections 2.7-2.15) on Stellar Evolution in Hansen, Kawaler, and Trimble. You can also read more about White Dwarf Properties, Cooling, and Crystallization Physics in chapter 10 of Hansen, Kawaler, and Trimble, as well as in chapters 3-4 of Black Holes, White Dwarfs, and Neutron Stars by Shapiro and Teukolsky.
16 Upper Main Sequence: Evolution of Massive Stars Hansen, Kawaler, and Trimble, sections 2.7-2.15 and chapter 10.

Shapiro and Teukolsky, chapters 3 and 4.
17 Supernovae

Collapsars

GRBs
Read Heger, et al. "How Massive Stars End Their Life." Astrophys J 591, no. 288 (2003). You will also find it useful to read Sections 2.6-2.8 and 2.11.2 in Hansen, Kawaler, and Trimble, as well as chapters 5, 12, and 18 in Shapiro and Teukolsky.
18 Neutron Stars

Pulsars (Guest Lecturer: David Kaplan)
Shapiro and Teukolsky, chapters 9 and 10.
19 Sun as a Star (Guest Lecturer: Justin Kasper) Shapiro and Teukolsky, chapters 9 and 10.
20 Gravitational Radiation (Guest Lecturer: Ryan Lang) Read chapter 13 on Compact X-ray Sources in Shapiro and Teukolsky. (Note that the observational details are very dated, but the theoretical description is good.) You may also find it instructive to skim through chapters 14 (Accretion onto Black Holes), 15 (Accretion onto Neutron Stars and White Dwarfs), and 16 (Gravitational Radiation).
21 Close Binaries

Accretion Disks
Chapter 13 on Compact X-ray Sources in Shapiro and Teukolsky, and skim through chapters 14 (Accretion onto Black Holes), 15 (Accretion onto Neutron Stars and White Dwarfs), and 16 (Gravitational Radiation).
22 Cepheid Variables

X-ray Binaries
You may find chapter 12 of Carroll and Ostlie (Introduction to Modern Astrophysics) helpful for background reading on star formation.
23 Black Holes

Interstellar Medium

Dust Extinction
Carroll and Ostlie, chapter 12.
24 Star Formation

Jeans Criterion

IMF

Brown Dwarfs
Carroll and Ostlie, chapter 12.
25 Gas in the Interstellar Medium

Heating and Cooling

21 cm and CO
Carroll and Ostlie, chapter 12.
26 Shocks

Supernova Remnants
Carroll and Ostlie, chapter 12.

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