Logo

Dense Matter in Compact Stars

Small book cover: Dense Matter in Compact Stars

Dense Matter in Compact Stars
by

Publisher: arXiv
Number of pages: 146

Description:
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:
Download link
(1.2MB, PDF)

Similar books

Book cover: Introduction to the Theory of Black HolesIntroduction to the Theory of Black Holes
by - Utrecht University
Contents: The Metric of Space and Time; Curved coordinates; A short introduction to General Relativity; Gravity; The Schwarzschild Solution; The Chandrasekhar Limit; Gravitational Collapse; The Reissner-Nordstrom Solution; Horizons; and more.
(25114 views)
Book cover: Images of the Solar Upper Atmosphere From SUMER on SOHOImages of the Solar Upper Atmosphere From SUMER on SOHO
by - ESA Publications Division
Investigations of the heating of the corona and the acceleration of the solar wind are two of the prime scientific goals in studying the solar upper atmosphere with the Solar and Heliospheric Observatory (SOHO) of ESA and NASA.
(12016 views)
Book cover: Protostars and PlanetsProtostars and Planets
- 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.
(16655 views)
Book cover: The First StarsThe First Stars
by - 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.
(10787 views)