Dense Matter in Compact Stars
by Andreas Schmitt
Publisher: arXiv 2010
Number of pages: 146
Cold and dense nuclear and/or quark matter can be found in the interior of compact stars. It is very challenging to determine the ground state and properties of this matter because of the strong-coupling nature of QCD. I give a pedagogical introduction to microscopic calculations based on phenomenological models, effective theories, and perturbative QCD. I discuss how the results of these calculations can be related to astrophysical observations to potentially rule out or confirm candidate phases of dense matter.
Home page url
Download or read it online for free here:
- Rice University
This 1400+ pages book covers the very rapidly growing area of star-and-planet formation and evolution, from astrophysics to planetary science. It is most useful for researchers, graduate students, and some undergraduate students.
by Simon C. O. Glover - arXiv
The author discusses our current understanding of the physical processes involved in the formation of Population III stars. He shows how we can identify the mass scale of the first dark matter halos to host Population III star formation.
by Garrelt Mellema - Leiden University
An introduction to the field of numerical hydrodynamics. It will give you some insight in what is involved in such calculations. Numerical hydrodynamics is used in many parts of astrophysics. The applications we consider in this exercise are stellar.
by George Gamow - Dover Publications
In this fascinating book, a renowned physicist outlines the theories that illuminate the evolution of our world. Gamow employs language that's both scientifically accurate and easy to understand as he traces the development of atomic theory.