National Institute of Technology Rourkela

राष्ट्रीय प्रौद्योगिकी संस्थान राउरकेला

ଜାତୀୟ ପ୍ରଯୁକ୍ତି ପ୍ରତିଷ୍ଠାନ ରାଉରକେଲା

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Syllabus

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 .