Effective Field Theories For Nuclei And Compact-Star Matter - Image 1

£66.00

Scientific Publishing Effective Field Theories For Nuclei And Compact-Star Matter

Name: Effective Field Theories For Nuclei And Compact-Star Matter
Brand: Scientific Publishing
Price: 69.69 GBP
Availability: InStock

Aeronautics & Aerospace

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Description

Explore the complexities of nuclear physics with this specialized volume on Chiral Nuclear Dynamics (CND-III). Published by Scientific Publishing, this work focuses on the study of compact-star matter that remains inaccessible through direct QCD methods. This text provides a deep look into how hidden symmetries and topology are encoded in QCD. It offers a unique perspective that differs from standard effective field theory and energy density functional approaches. By exploiting renormalization-group flow in a complex vacuum that shifts with density, the book addresses topology change as a sign of baryon-quark continuity in dense matter. Researchers and students in the field of nuclear physics will find value in the various predictions made within these pages. This volume serves as a technical resource for understanding the structural properties of dense matter and the theoretical frameworks used to model them.

Key Features

Focuses on compact-star matter structures that are not directly accessible from QCD.

Utilizes hidden symmetries and topology presumed to be encoded in QCD for theoretical analysis.

Examines renormalization-group flow within a complex vacuum that changes with density.

Explores topology change as a manifestation of baryon-quark continuity in dense matter.

Provides a distinct approach compared to standard effective field theory and energy density functional methods.

Product Specifications

Brand: Scientific Publishing
Format: Hardcover
ASIN: 9813273313
Category: Books > Subjects > Science, Nature & Maths > Engineering & Technology > Aeronautics & Aerospace
Domain: Amazon UK
Release Date: 26 December 2018
Listed Since: 11 July 2018

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Scientific Publishing Effective Field Theories For Nuclei And Compact-Star Matter

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