Nuclear Theory in the Age of Multimessenger Astronomy

Nuclear Theory in the Age of Multimessenger Astronomy PDF

Author: Omar Benhar

Publisher: CRC Press

Published: 2024-07-03

Total Pages: 383

ISBN-13: 1040044743

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Over the last decade, astrophysical observations of neutron stars — both as isolated and binary sources — have paved the way for a deeper understanding of the structure and dynamics of matter beyond nuclear saturation density. The mapping between astrophysical observations and models of dense matter based on microscopic dynamics has been poorly investigated so far. However, the increased accuracy of present and forthcoming observations may be instrumental in resolving the degeneracy between the predictions of different equations of state. Astrophysical and laboratory probes have the potential to paint to a new coherent picture of nuclear matter — and, more generally, strong interactions — over the widest range of densities occurring in the Universe. This book provides a self-contained account of neutron star properties, microscopic nuclear dynamics and the recent observational developments in multimessenger astronomy. It also discusses the unprecedented possibilities to shed light on long standing and fundamental issues, such as the validity of the description of matter in terms of pointlike baryons and leptons and the appearance of deconfined quarks in the high density regime. It will be of interest to researchers and advanced PhD students working in the fields of Astrophysics, Gravitational Physics, Nuclear Physics and Particle Physics. Key Features: Reviews state-of-the-art theoretical and experimental developments Self-contained and cross-disciplinary While being devoted to a very lively and fast developing field, the book fundamentally addresses methodological issues. Therefore, it will not be subject to fast obsolescence. Omar Benhar is an INFN Emeritus Research Director, and has been teaching Relativistic Quantum Mechanics, Quantum Electrodynamics and Structure of Compact Stars at “Sapienza” University of Rome for over twenty years. He has worked extensively in the United States, and since 2013 has served as an adjunct professor at the Center for Neutrino Physics of Virginia Polytechnic Institute and State University. Prof. Benhar has authored or co-authored three textbooks on Relativistic Quantum Mechanics, Gauge Theories, and Structure and Dynamics of Compact Stars, and published more than one hundred scientific papers on the theory of many-particle systems, the structure of compact stars and the electroweak interactions of nuclei. Alessandro Lovato is a physicist at Argonne National Laboratory and an INFN researcher in Trento. His research in theoretical nuclear physics focuses on consistently modeling the self-emerging properties of atomic nuclei and neutron-star matter in terms of the microscopic interactions among the constituent protons and neutrons. He has co-authored more than eighty scientific publications on the theory of many-particle systems, the structure of compact stars, and the electroweak interactions of nuclei. He is at the forefront of high-performance computing applied to solving the quantum many-body problem. Andrea Maselli is an Associate Professor at the Gran Sasso Science Institute, in L’Aquila, where he teaches Gravitation and Cosmology and Physics of Black Hole. His research focuses on strong gravity, which plays a crucial role in many astrophysical phenomena involving black hole and neutron stars, representing natural laboratories to test fundamental physics. Prof. Maselli has co-authored more than eighty scientific papers on the modelling of black holes and neutron stars in General Relativity and extension thereof, their gravitational wave emission, and on tests of gravity in the strong filed regime. He is active in various collaborations aimed at developing next generation of gravitational wave detectors, such as the LISA satellite, the Einstein Telescope, and the Lunar Gravitational Wave Antenna. Francesco Pannarale is an Associate Professor at “Sapienza” Univeristy of Rome, where he teaches Gravitational Waves, Compact Objects and Black Holes, Computing Methods for Physics, and Electromagnetism. His research interests are in gravitational-wave physics and multimessenger astronomy, and they range from modelling compact binary sources to data analysis. He has co-authored over one hundred and eighty scientific publications and was at the forefront of the joint observation of GW170817 and GRB 170817A. He is currently serving as co-chair of the LIGO-Virgo-KAGRA Data Analysis Council.

Nuclear Physics

Nuclear Physics PDF

Author: National Research Council

Publisher: National Academies Press

Published: 1999-03-31

Total Pages: 222

ISBN-13: 0309173663

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Dramatic progress has been made in all branches of physics since the National Research Council's 1986 decadal survey of the field. The Physics in a New Era series explores these advances and looks ahead to future goals. The series includes assessments of the major subfields and reports on several smaller subfields, and preparation has begun on an overview volume on the unity of physics, its relationships to other fields, and its contributions to national needs. Nuclear Physics is the latest volume of the series. The book describes current activity in understanding nuclear structure and symmetries, the behavior of matter at extreme densities, the role of nuclear physics in astrophysics and cosmology, and the instrumentation and facilities used by the field. It makes recommendations on the resources needed for experimental and theoretical advances in the coming decade.

Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics

Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics PDF

Author: Fridolin Weber

Publisher: Routledge

Published: 2017-09-18

Total Pages: 588

ISBN-13: 1351420941

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Pulsars, generally accepted to be rotating neutron stars, are dense, neutron-packed remnants of massive stars that blew apart in supernova explosions. They are typically about 10 kilometers across and spin rapidly, often making several hundred rotations per second. Depending on star mass, gravity compresses the matter in the cores of pulsars up to more than ten times the density of ordinary atomic nuclei, thus providing a high-pressure environment in which numerous particle processes, from hyperon population to quark deconfinement to the formation of Boson condensates, may compete with each other. There are theoretical suggestions of even more ""exotic"" processes inside pulsars, such as the formation of absolutely stable strange quark matter, a configuration of matter even more stable than the most stable atomic nucleus, ^T56Fe. In the latter event, pulsars would be largely composed of pure quark matter, eventually enveloped in nuclear crust matter. These features combined with the tremendous recent progress in observational radio and x-ray astronomy make pulsars nearly ideal probes for a wide range of physical studies, complementing the quest of the behavior of superdense matter in terrestrial collider experiments. Written by an eminent author, Pulsars as Astrophysical Laboratories for Nuclear and Particle Physics gives a reliable account of the present status of such research, which naturally is to be performed at the interface between nuclear physics, particle physics, and Einstein's theory of relativity.

The Multi-Messenger Approach to High-Energy Gamma-Ray Sources

The Multi-Messenger Approach to High-Energy Gamma-Ray Sources PDF

Author: Josep M. Paredes

Publisher: Springer Science & Business Media

Published: 2007-11-12

Total Pages: 496

ISBN-13: 140206117X

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This book provides a theoretical and observational overview of the state of the art of gamma-ray astrophysics, and their impact and connection with the physics of cosmic rays and neutrinos. With the aim of shedding new and fresh light on the problem of the nature of the gamma-ray sources, particularly those yet unidentified, this book summarizes contributions to a workshop that continues today.

Essays in Nuclear Astrophysics

Essays in Nuclear Astrophysics PDF

Author: Charles A. Barnes

Publisher: CUP Archive

Published: 1982-09-30

Total Pages: 584

ISBN-13: 9780521244107

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Originally published in 1982, this collection of essays provides an integrated overview of the application of nuclear science to astronomy. The book discusses, among other topics, the abundances of the nuclear and chemical species on the Earth and the Moon, in meteorites, in the stars, and in interstellar space. The hypothesis that these species are produced by nuclear reactions is then explored and related to laboratory measurements. Other subjects include the dynamics of supernovae and interdisciplinary relationships between elementary particle physics and cosmology. The essays are dedicated to Professor William A. Fowler and pay tribute to his vast influence on the field.

Nuclear Planetary Science: Planetary Science Based On Gamma-ray, Neutron And X-ray Spectroscopy

Nuclear Planetary Science: Planetary Science Based On Gamma-ray, Neutron And X-ray Spectroscopy PDF

Author: Nobuyuki Hasebe

Publisher: World Scientific

Published: 2017-09-25

Total Pages: 180

ISBN-13: 9813209720

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Nuclear planetary science has come to play an important role in our understanding of the origin and evolution of the planetary bodies in our solar system. A newly established branch of planetary science, its study aids in humankind's exploration of the present states of the structures of various planetary bodies (including the Earth), their atmospheres and their satellites, as well as small celestial bodies (e.g. asteroids), through direct observation. Knowing the elemental composition of the planetary bodies is essential in order to understand the formation and evolution of planetary bodies — just as important as it is to know the mass, radius, density and orbit of the celestial body.Suitable for students and specialists interested in the much wider field of Earth and Planetary Science, topics related to the planets and asteroids in the solar system are dealt with in this book. Techniques related to nuclear planetary science's nuclear cosmochemical and geological methods are also covered in this book.

Essentials for Nucleosynthesis and Theoretical Nuclear Astrophysics

Essentials for Nucleosynthesis and Theoretical Nuclear Astrophysics PDF

Author: RAUSCHER

Publisher: IOP Publishing Limited

Published: 2020-07-16

Total Pages: 450

ISBN-13: 9780750311502

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Studies in nucleosynthesis and nuclear astrophysics are highly interdisciplinary, encompassing such fields as nuclear physics, stellar structure and evolution, hydrostatics and hydrodynamics, differential equations for following isotopic abundance changes in stellar plasmas and in the interstellar medium, and astronomical observations. Essentials of Nucleosynthesis and Theoretical Nuclear Astrophysics brings together the theoretical aspects of these topics in a single volume, providing the necessary mathematical tools and equations with unified notation to enable studying nucleosynthesis in a variety of astrophysical sites. Essential definitions and theory are presented that will enable the reader to enter the research field with the familiarity of the specialities and specific problems. Useful as a reference work for any researcher in the field of nucleosynthesis and nuclear astrophysics, or a suitable basis for a graduate course on these topics, the book also provides the information necessary to follow discussions of current open questions in the understanding of the origin of the elements. Key Features Offers a concise summary of the most important concepts and equations related to nucleosynthesis and theoretical nuclear astrophysics Presents the essential definitions and approaches to help those entering this interdisciplinary field Provides the information necessary to follow discussions of current open questions in the understanding of the origin of the elements

An Introduction to Nuclear Astrophysics

An Introduction to Nuclear Astrophysics PDF

Author: Richard N. Boyd

Publisher: University of Chicago Press

Published: 2007

Total Pages: 435

ISBN-13: 0226069710

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Nuclear astrophysics background -- The instruments used to study astrophysics -- Nuclear basics of nuclear astrophysics -- Stellar basics of nuclear astrophysics -- Hydrogen burning -- Advanced stellar evolution, supernovae, and gamma-ray bursters -- Production of the abundant heavy nuclides -- Nucleosynthesis on the proton-rich side of stability, X-ray bursts, and magnetars -- The beginning of the universe.

Nuclear Physics

Nuclear Physics PDF

Author: The Committee on the Assessment of and Outlook for Nuclear Physics

Publisher: National Academies Press

Published: 2013-03-11

Total Pages: 263

ISBN-13: 0309260418

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The principal goals of the study were to articulate the scientific rationale and objectives of the field and then to take a long-term strategic view of U.S. nuclear science in the global context for setting future directions for the field. Nuclear Physics: Exploring the Heart of Matter provides a long-term assessment of an outlook for nuclear physics. The first phase of the report articulates the scientific rationale and objectives of the field, while the second phase provides a global context for the field and its long-term priorities and proposes a framework for progress through 2020 and beyond. In the second phase of the study, also developing a framework for progress through 2020 and beyond, the committee carefully considered the balance between universities and government facilities in terms of research and workforce development and the role of international collaborations in leveraging future investments. Nuclear physics today is a diverse field, encompassing research that spans dimensions from a tiny fraction of the volume of the individual particles (neutrons and protons) in the atomic nucleus to the enormous scales of astrophysical objects in the cosmos. Nuclear Physics: Exploring the Heart of Matter explains the research objectives, which include the desire not only to better understand the nature of matter interacting at the nuclear level, but also to describe the state of the universe that existed at the big bang. This report explains how the universe can now be studied in the most advanced colliding-beam accelerators, where strong forces are the dominant interactions, as well as the nature of neutrinos.

Nuclear Physics

Nuclear Physics PDF

Author: Division on Engineering and Physical Sciences

Publisher: National Academies Press

Published: 1986-02-01

Total Pages: 239

ISBN-13: 0309035473

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