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Dense Matter In Compact Stars
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Book Synopsis Dense Matter in Compact Stars by : Andreas Schmitt
Download or read book Dense Matter in Compact Stars written by Andreas Schmitt and published by Springer. This book was released on 2010-08-25 with total page 152 pages. Available in PDF, EPUB and Kindle. Book excerpt: The purpose and motivation of these lectures can be summarized in the following two questions: • What is the ground state (and its properties) of dense matter? • What is the matter composition of a compact star? The two questions are, of course, strongly coupled to each other. Depending on your point of view, you can either consider the ?rst as the main question and the second as a consequence or application of the ?rst, or vice versa. If you are interested in fundamental questions in particle physics you may take the former point of view: you ask the question what happens to matter if you squeeze it more and more. This leads to fundamental questions because at some level of suf?cient squeezing you expect to reach the point where the fundamental degrees of freedom and their interactions become important. That is, at some point you will reach a form of matter where not molecules or atoms, but the constituents of an atom, namely neutrons, protons, and electrons, are the relevant degrees of freedom.
Download or read book Compact Stars written by Deog Ki Hong and published by World Scientific. This book was released on 2004 with total page 546 pages. Available in PDF, EPUB and Kindle. Book excerpt: Space observations are currently providing a glimpse of various new states of matter possibly present in compact stars, with terrestrial laboratories producing compelling evidence in support. The aim of this book is to facilitate the exchange of ideas OCo both established and emergent, both theoretical and experimental OCo in the areas of the physics of neutrinos, dense hadronic matter and compact stars. The proceedings have been selected for coverage in: . OCo Index to Scientific & Technical Proceedings- (ISTP- / ISI Proceedings). OCo Index to Scientific & Technical Proceedings (ISTP CDROM version / ISI Proceedings). OCo CC Proceedings OCo Engineering & Physical Sciences. Contents: Compact Stars: Sleuthing the Isolated Compact Stars (J J Drake); Phase Transitions in Neutron Stars (N K Glendenning); Formation and Evolution of Black Holes in the Galaxy (C-H Lee); Neutron Stars and Quark Stars (F Weber); Dense Matter: Role of Strange Quark Mass in Pairing Phenomena in QCD (H Abuki); Aspects of High Density Effective Theory (D K Hong); New Results from Belle (Y Kwon); Andreev Reflection in Color Superconductivity (M Sadzikowski & M Tachibana); Neutrinos: Cooling Delay for Protoquark Stars Due to Neutrino Trapping (J Berdermann et al.); The Minimal Cooling of Neutron Stars (D Page); The Solar Hep Process Confronts the Terrestrial Hen Process (T-S Park); Supernova Explosions and Neutrino Bursts from Supernovae (K Sato et al.); and other papers. Readership: Graduate students and researchers in astrophysics, astronomy, cosmology and high energy physics."
Book Synopsis Hot and Dense Matter in Compact Stars by : Matthias Hempel
Download or read book Hot and Dense Matter in Compact Stars written by Matthias Hempel and published by . This book was released on 2010 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Author :Deog Ki Hong Publisher :World Scientific Publishing Company Incorporated ISBN 13 :9789812389541 Total Pages :526 pages Book Rating :4.3/5 (895 download)
Download or read book Compact Stars written by Deog Ki Hong and published by World Scientific Publishing Company Incorporated. This book was released on 2004-01-01 with total page 526 pages. Available in PDF, EPUB and Kindle. Book excerpt: Space observations are currently providing a glimpse of various new states of matter possibly present in compact stars, with terrestrial laboratories producing compelling evidence in support. The aim of this book is to facilitate the exchange of ideas -- both established and emergent, both theoretical and experimental -- in the areas of the physics of neutrinos, dense hadronic matter and compact stars.
Book Synopsis Compact Stars: The Quest For New States Of Dense Matter - Proceedings Of The Kias-apctp International Symposium On Astro-hadron Physics by : Deog Ki Hong
Download or read book Compact Stars: The Quest For New States Of Dense Matter - Proceedings Of The Kias-apctp International Symposium On Astro-hadron Physics written by Deog Ki Hong and published by World Scientific. This book was released on 2004-08-10 with total page 546 pages. Available in PDF, EPUB and Kindle. Book excerpt: Space observations are currently providing a glimpse of various new states of matter possibly present in compact stars, with terrestrial laboratories producing compelling evidence in support. The aim of this book is to facilitate the exchange of ideas — both established and emergent, both theoretical and experimental — in the areas of the physics of neutrinos, dense hadronic matter and compact stars.The proceedings have been selected for coverage in:• Index to Scientific & Technical Proceedings® (ISTP® / ISI Proceedings)• Index to Scientific & Technical Proceedings (ISTP CDROM version / ISI Proceedings)• CC Proceedings — Engineering & Physical Sciences
Author :Norman K. Glendenning Publisher :Springer Science & Business Media ISBN 13 :1468404911 Total Pages :402 pages Book Rating :4.4/5 (684 download)
Book Synopsis Compact Stars by : Norman K. Glendenning
Download or read book Compact Stars written by Norman K. Glendenning and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 402 pages. Available in PDF, EPUB and Kindle. Book excerpt: A whole decades research collated, organised and synthesised into one single book! Following a 60-page review of the seminal treatises of Misner, Thorne, Wheeler and Weinberg on general relativity, Glendenning goes on to explore the internal structure of compact stars, white dwarfs, neutron stars, hybrids, strange quark stars, both the counterparts of neutron stars as well as of dwarfs. This is a self-contained treatment and will be of interest to graduate students in physics and astrophysics as well as others entering the field.
Download or read book Compact Stars written by Deog Ki Hong and published by . This book was released on 2004 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Dense Matter in Compact Stars by : Andreas Schmitt
Download or read book Dense Matter in Compact Stars written by Andreas Schmitt and published by Springer Science & Business Media. This book was released on 2010-09-04 with total page 152 pages. Available in PDF, EPUB and Kindle. Book excerpt: The purpose and motivation of these lectures can be summarized in the following two questions: • What is the ground state (and its properties) of dense matter? • What is the matter composition of a compact star? The two questions are, of course, strongly coupled to each other. Depending on your point of view, you can either consider the ?rst as the main question and the second as a consequence or application of the ?rst, or vice versa. If you are interested in fundamental questions in particle physics you may take the former point of view: you ask the question what happens to matter if you squeeze it more and more. This leads to fundamental questions because at some level of suf?cient squeezing you expect to reach the point where the fundamental degrees of freedom and their interactions become important. That is, at some point you will reach a form of matter where not molecules or atoms, but the constituents of an atom, namely neutrons, protons, and electrons, are the relevant degrees of freedom.
Book Synopsis The Physics and Astrophysics of Neutron Stars by : Luciano Rezzolla
Download or read book The Physics and Astrophysics of Neutron Stars written by Luciano Rezzolla and published by Springer. This book was released on 2019-01-09 with total page 811 pages. Available in PDF, EPUB and Kindle. Book excerpt: This book summarizes the recent progress in the physics and astrophysics of neutron stars and, most importantly, it identifies and develops effective strategies to explore, both theoretically and observationally, the many remaining open questions in the field. Because of its significance in the solution of many fundamental questions in nuclear physics, astrophysics and gravitational physics, the study of neutron stars has seen enormous progress over the last years and has been very successful in improving our understanding in these fascinating compact objects. The book addresses a wide spectrum of readers, from students to senior researchers. Thirteen chapters written by internationally renowned experts offer a thorough overview of the various facets of this interdisciplinary science, from neutron star formation in supernovae, pulsars, equations of state super dense matter, gravitational wave emission, to alternative theories of gravity. The book was initiated by the European Cooperation in Science and Technology (COST) Action MP1304 “Exploring fundamental physics with compact stars” (NewCompStar).
Book Synopsis Hot and Dense Matter in Compact Stars by : Matthias Hempel
Download or read book Hot and Dense Matter in Compact Stars written by Matthias Hempel and published by Sudwestdeutscher Verlag Fur Hochschulschriften AG. This book was released on 2011-03 with total page 256 pages. Available in PDF, EPUB and Kindle. Book excerpt: This dissertation deals with the equation of state of hot and dense matter in compact stars, with special focus on first order phase transitions. A general classification of first order phase transitions is given and the properties of mixed phases are discussed. Aspects of nucleation and the role of local constraints are investigated. The theoretical concepts are applied to matter in the hadron-quark and the liquid-gas phase transition. For the detailed description of the liquid-gas phase transition a new nuclear statistical equilibrium model is developed. Different equation of state tables are calculated and the composition and thermodynamic properties of supernova matter are analyzed. As a first application numerical simulations of core-collapse supernovae are presented. For the hadron-quark phase transition two possible scenarios are studied in more detail, the appearance of a new mixed phase in a protoneutron star and the consequences of the hadron-quark transition in a core-collapse supernovae. Simulations of the latter show that the appearance of quark matter has clear observable signatures and can even lead to the generation of an explosion.
Book Synopsis Superdense QCD Matter and Compact Stars by : David Blaschke
Download or read book Superdense QCD Matter and Compact Stars written by David Blaschke and published by Springer Science & Business Media. This book was released on 2006-01-14 with total page 427 pages. Available in PDF, EPUB and Kindle. Book excerpt: 2 Homogeneous superconducting state 210 3 Superconducting phases with broken space symmetries 213 4 Flavor asymmetric quark condensates 219 5 Concluding remarks 221 Acknowledgments 222 References 223 Neutral Dense Quark Matter 225 Mei Huang and Igor Shovkovy 1 Introduction 225 2 Local charge neutrality: homogeneous phase 226 3 Global charge neutrality: mixed phase 234 4 Conclusion 238 References 238 Possibility of color magnetic superconductivity 241 Toshitaka Tatsumi, Tomoyuki Maruyama, and Eiji Nakano 1 Introduction 241 2 What is ferromagnetism in quark matter? 243 3 Color magnetic superconductivity 248 4 Chiral symmetry and magnetism 253 5 Summary and Concluding remarks 258 Acknowledgments 260 References 260 Magnetic Fields of Compact Stars with Superconducting Quark Cores 263 David M. Sedrakian, David Blaschke, and Karen M. Shahabasyan 1 Introduction 263 2 Free Energy 265 3 Ginzburg-Landau equations 267 4 Vortex Structure 269 5 Solution of Ginzburg-Landau Equations 271 6 The Magnetic Field Components 273 7 Summary 275 Acknowledgments 275 References 275 Thermal Color-superconducting Fluctuations in Dense Quark Matter 277 D. N.
Book Synopsis Compact Star Physics by : Jürgen Schaffner-Bielich
Download or read book Compact Star Physics written by Jürgen Schaffner-Bielich and published by Cambridge University Press. This book was released on 2020-08-27 with total page 325 pages. Available in PDF, EPUB and Kindle. Book excerpt: This introduction to compact star physics explains key concepts from general relativity, thermodynamics and nuclear physics.
Book Synopsis Astrophysics In The Xxi Century With Compact Stars by : Cesar Augusto Zen Vasconcellos
Download or read book Astrophysics In The Xxi Century With Compact Stars written by Cesar Augusto Zen Vasconcellos and published by World Scientific. This book was released on 2022-10-25 with total page 353 pages. Available in PDF, EPUB and Kindle. Book excerpt: There are reasons to believe the 21st century will be the best ever for astrophysics: the James Webb Space Telescope will extend nearly twenty times the present observational limit of visible light; neutrino massiveness opens a new window for exploration on dark energy and dark matter physics and is expected to provide insights into the fate of the Universe; the Higgs boson may allow for an understanding of the weakness of gravity; gravitational waves produced at the birth of the Universe and by compact stellar objects (supermassive black holes, black hole/neutron star mergers, gamma-ray bursts, white dwarf inspirals) have unveiled a new area of astronomy. Against this background, compact stars, the theme of this volume, present unique astrophysical laboratories for probing the fabric of space-time and the building blocks of matter and their interactions at physical regimes not attainable in terrestrial laboratories.
Book Synopsis Dense and Hot Matter in Compact Stars and Heavy-ion Collisions by : Stefan Schramm
Download or read book Dense and Hot Matter in Compact Stars and Heavy-ion Collisions written by Stefan Schramm and published by . This book was released on 2018 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt: We discuss the effect of exotic particles in neutron star matter and the corresponding impact on gross properties of neutron stars within effective models for the strong interaction. Particularly, for the quark-hadron parity-doublet model, we show results for compact star properties and discuss the phase structure of the model and its possible relevance for heavy-ion collision phenomenology.
Book Synopsis Probing the Phases of Cold Ultra-dense Matter Using Neutron Star Physics by : Simin Mahmoodifar
Download or read book Probing the Phases of Cold Ultra-dense Matter Using Neutron Star Physics written by Simin Mahmoodifar and published by . This book was released on 2012 with total page 406 pages. Available in PDF, EPUB and Kindle. Book excerpt: Matter at very high densities and low temperatures is predicted to be in a "color superconducting" phase. At high enough densities, quark matter is in the Color-Flavor-Locked (CFL) phase, but the possible phases of matter at intermediate densities are unknown. Since the density at the core of a neutron star can be as high as a few times the nuclear saturation density, it is the most likely place to find these exotic forms of matter in the real world. The main goal of this thesis is to probe the phases of cold dense matter using neutron star physics. Studying the transport properties of different phases of dense matter that may occur in a compact star is particularly important because transport properties such as viscosity, in addition to depending on the equation of state of matter, also depend on the low-energy degrees of freedom and therefore can discriminate between different phases of dense matter more efficiently. In the first part of this thesis we calculate the mean free path and kaonic contribution to the shear viscosity of kaon-condensed color-flavor-locked (CFL-K0) phase of quark matter. In the second part we calculate the large-amplitude enhancement of the bulk viscosity of dense matter. We obtain general analytic solutions as well as numerical solutions for the amplitude-dependent bulk viscosity of dense matter which are valid for any equations of state where equilibration occurs via fermions. In the third and fourth parts, we use our general results for the bulk viscosity to calculate the damping timescales of r-mode oscillations of neutron stars due to small-amplitude and large-amplitude bulk viscosity, the instability window of the r-modes and the saturation amplitude due to "supra-thermal" enhancement of the bulk viscosity for different cases of strange quark stars, hadronic stars and hybrid stars.
Book Synopsis Effects of Quark Matter on the Structural and Observational Properties of Compact Stars by : Sophia Han
Download or read book Effects of Quark Matter on the Structural and Observational Properties of Compact Stars written by Sophia Han and published by . This book was released on 2015 with total page 172 pages. Available in PDF, EPUB and Kindle. Book excerpt:
Book Synopsis Effective Field Theories For Nuclei And Compact-star Matter: Chiral Nuclear Dynamics (Cnd-iii) by : Yong-liang Ma
Download or read book Effective Field Theories For Nuclei And Compact-star Matter: Chiral Nuclear Dynamics (Cnd-iii) written by Yong-liang Ma and published by World Scientific. This book was released on 2018-10-26 with total page 378 pages. Available in PDF, EPUB and Kindle. Book excerpt: Effective field theories have been widely used in nuclear physics. This volume is devoted to exploring the intricate structure of compact-star matter inaccessible directly from QCD. It is principally anchored on hidden symmetries and topology presumed to be encoded in QCD. It differs from standard effective field theory and energy density functional approaches in that it exploits renormalization-group flow in the complex 'vacuum' sliding with density inferred from topology change identified as a manifestation of baryon-quark continuity in dense matter. It makes a variety of predictions that drastically differ from the conventional treatments that could be tested by upcoming terrestrial and astrophysical experiments.This monograph recounts how to go, in one unique field theoretic formalism in terms of hadronic degrees of freedom, from finite nuclei to dense compact-star matter that could be explored in RIB-type machines in nuclear physics as well as in LIGO-type gravity waves in astrophysics.
