Course Details
Subject {L-T-P / C} : PH5114 : Stellar Structure and Evolution { 3-0-0 / 3}
Subject Nature : Theory
Syllabus
| Module 1 : |
(6 hrs) Sun as a star (qualitative): Solar spectrum, effective temperature, luminosity, photospheric absorption lines, limb darkening; energy source: Kelvin time scale, nuclear fusion; energy transport in the sun, Thomson scattering, mean free path, photon diffusion inside the Sun; photosphere, chromosphere, transition region, corona; X-ray emission, magnetic fields, Sunspots |
| Module 2 : |
(10 hrs) Formation of stars, Initial Mass Function, Equation of State, Stellar Structure Equations, Pre-main sequence evolution, Jeans instability, Hayashi Track, Zero Age Main Sequence, H-burning Phase, Energy Transportation in lower and upper main sequence stars, Mass Luminosity Relation. |
| Module 3 : |
(10 hrs) Post-Main Sequence Evolution (Low and High mass stars): Overall Contraction Phase, H-burning in shell, properties of subgiant and red-giant branch stars, Onset of He-burning, Horizontal Branch stars, Asymptotic giant branch stars, Properties of Luminous Blue Variables and Wolf-Rayet stars, Planetary Nebula Phase, White dwarf, C, Ne, O, Si - burning phases, Supernova explosion, formation of Neutron Star and Black hole. |
| Module 4 : |
( 10 hrs) Probing the interior using stellar pulsation: Stellar Pulsation Across HR-diagram, pulsation mechanism, Pulsation Mode Identification, Modelling of stellar pulsation, generating rotation profile from pulsation. |
Course Objective
| 1 . |
To learn the basics of star formation and Stellar Structure. |
| 2 . |
To get acquainted with energy transportation in stars |
| 3 . |
To understand the post-main sequence evolution and final fate of stars. |
| 4 . |
To know about the various energy sources inside the stars |
| 5 . |
To know the pulsation mechnisms to explore the interior of stars |
Course Outcome
| 1 . |
CO1 To learn the basics of star formation and Stellar Structure. |
| 2 . |
CO2 To get acquainted with energy transportation in stars |
| 3 . |
CO3 To understand the post-main sequence evolution and final fate of stars. |
Essential Reading
| 1 . |
Achim Weiss, Alfred Weigert and Rudolf Kippenhahn, Stellar Structure and Evolution, Springer |
| 2 . |
M. Salaris and S. Cassisi, Evolution of stars and stellar Populations, John Wiley & Sons |
| 3 . |
Subrahmanyan Chandrasekhar, An Introduction to the Study of Stellar Structure, Dover Publications Inc. (2003) |
Supplementary Reading
| 1 . |
D. Prialnik, An Introduction to the Theory of Stellar Structure and Evolution, Cambridge University Press |
| 2 . |
C. Aerts J. Christensen-Dalsgaard and D. W. Kurtz, Asteroseismology, Springer |
| 3 . |
R. Kippenhahn and A. Weigert, Stellar Structure and Evolution, Springer. |
Journal and Conferences
| 1 . |



