An Introduction to the Theory of Rotating Relativistic Stars
by Eric Gourgoulhon
Publisher: arXiv 2010
Number of pages: 88
Description:
These lecture notes are intended to introduce the theory of rotating stars in general relativity. The focus is put on the theoretical foundations, with a detailed discussion of the spacetime symmetries, the choice of coordinates and the derivation of the equations of structure from Einstein equation. The global properties of rotating stars (mass, angular momentum, redshifts, orbits, etc.) are also introduced.
Download or read it online for free here:
Download link
(1.1MB, PDF)
Similar books
Dense Matter in Compact Stars
by Andreas Schmitt - arXiv
Cold and dense nuclear and quark matter can be found in the interior of compact stars. The author gives a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD.
(10311 views)
by Andreas Schmitt - arXiv
Cold and dense nuclear and quark matter can be found in the interior of compact stars. The author gives a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD.
(10311 views)
The Virial Theorem in Stellar Astrophysics
by George W. Collins, II - Pachart Pub. House
The virial theorem is extremely powerful in understanding problems of stellar astrophysics, but it is also poorly understood by many who study the subject. This book should be viewed as a guided introduction, punctuated by a few examples.
(10201 views)
by George W. Collins, II - Pachart Pub. House
The virial theorem is extremely powerful in understanding problems of stellar astrophysics, but it is also poorly understood by many who study the subject. This book should be viewed as a guided introduction, punctuated by a few examples.
(10201 views)
Stellar Atmospheres
by J. B. Tatum
A course on stellar atmospheres: radiation theory, blackbody radiation, flux, specific intensity and other astrophysical terms, absorption, scattering, extinction, the equation of transfer, limb darkening, atomic spectroscopy, and more.
(9298 views)
by J. B. Tatum
A course on stellar atmospheres: radiation theory, blackbody radiation, flux, specific intensity and other astrophysical terms, absorption, scattering, extinction, the equation of transfer, limb darkening, atomic spectroscopy, and more.
(9298 views)
Supernovae
- Wikipedia
A supernova is a stellar explosion that briefly outshines an entire galaxy, radiating as much energy as the Sun or any ordinary star is expected to emit over its entire life span, before fading from view over several weeks or months.
(5535 views)
- Wikipedia
A supernova is a stellar explosion that briefly outshines an entire galaxy, radiating as much energy as the Sun or any ordinary star is expected to emit over its entire life span, before fading from view over several weeks or months.
(5535 views)