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: Notes on Stellar AstrophysicsNotes on Stellar Astrophysics
by - Minnesota State University
This book provides an introduction to the details of the structure, operation, and evolution of stars. It will be most useful to undergraduates in upper-level astronomy courses and graduate students taking Stellar Interiors or Stellar Atmospheres.
(11411 views)
Book cover: Massive Stars and their SupernovaeMassive Stars and their Supernovae
by - arXiv
The authors focus on the astrophysical aspects, i.e. a description of the evolution of massive stars and their endpoints, with a special emphasis on the composition of their ejecta in form of stellar winds during the evolution or of explosive ejecta.
(12688 views)
Book cover: The Fundamentals of Stellar AstrophysicsThe Fundamentals of Stellar Astrophysics
by - W H Freeman & Co
The book on stellar astrophysics for the first year graduates or the advanced undergraduate students. It is assumed that the readers have factual knowledge of stars and astronomy. The text describes the axiomatic theory of stellar structure.
(20324 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.
(14148 views)