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Superdense QCD Matter and Compact Stars

Blaschke, David; Sedrakian, David

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ISBN 10: 1402034288 / ISBN 13: 9781402034282
Published by Springer, The Netherlands, 2006
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Octavo; VG/no-DJ; White spine with black text. Boards have general shelfwear, has Ex-Library call number label on spine, otherwise clean, corners sharp, binding strong; Textblock has library stamp on title page, bar code sticker and call number label on rear free end paper; pp 429. Rockville. Bookseller Inventory # 7-131-1248344

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Bibliographic Details

Title: Superdense QCD Matter and Compact Stars

Publisher: Springer, The Netherlands

Publication Date: 2006

Binding: Hardcover

Dust Jacket Condition: Dust Jacket Included

About this title

Synopsis:

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.

About the Author:

This volume covers the main topics in the theory of superdense QCD matter and its application to the astrophysics of compact stars in a comprehensive and yet accessible way. The material is presented as a combination of extensive introductory lectures and more topical contributions. The book is centered around the question whether hypothetical new states of dense matter in the compact star interior could give clues to the explanation of puzzling phenomena such as gamma-ray bursts, pulsar glitches, compact star cooling and gravitational waves.

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