Encyclopedia of Astrophysics, Three Volume Set is a brand new, up to date reference work consisting of approximately 150 chapters, headed up by an editorial board of world-leading astrophysicists. It provides a first point of entry to the literature for all graduate/post-graduate students and early career-researchers working in and studying physics, especially those with an interest in astrophysics and cosmology. It is indispensable to all serious readers in the interdisciplinary areas where astrophysics is of utility.With a clear and logical template binding all chapters, content is divided into the following five sections, each of which contains chapters written by leading scientists who have evaluated and summarized the most important data published within the field: Cosmology: including Big Bang, dark matter, dark energy, Hubble’s law, cosmic microwave background, distance ladder, BAO, lensing, tests of general relativity; Galaxies: including morphology, galaxy zoo, active galactic nuclei, star formation / feedback / quenching, blue & red peaks and green valley, galactic chemical evolution, galaxy groups & clusters, young stellar / globular / nuclear clusters & dynamics, inter-stellar medium; Stars: including star formation, stellar evolution, the Sun as a star, asteroseismology, stellar rotation, stellar winds, binary interactions (tides, mass transfer, common envelopes, luminous red novae…), chemical abundance, evolution; Compact objects: including white dwarfs, neutron stars (pulsars), black holes, supernovae (type IA vs core-collapse), accretion, Eddington limit, X-ray binaries, supermassive black holes, tidal disruption events, mergers: gamma ray bursts, kilonovae, gravitational waves; (Exo)planets: including formation, Solar system, comets / meteors, dynamics, stability, exoplanet observations (radial velocity, transits).Advanced interactive features such as videos and 3D viewers are included, significantly increasing the practicality and learning outcomes for the modern-day reader for whom online usage is preferred. The result is the ideal one-stop foundational resource to the complex field of astrophysics and an essential tool for physicists to refer to time and again.
Ultra-High Energy Hadron and Neutrino Astrophysics covers ultrahigh energy neutrino and hadron astronomy in the context of the search for the sources of the highest energy cosmic rays. It gives a broad and solid background for the newcomer to this field of research in the first few chapters, beginning with a comprehensive review of the evolution of astronomy, the present status of our knowledge on the cosmic radiation, discusses the interactions that are relevant for the propagation and detection of the cosmic radiation in space, in the atmosphere, and in the Earth’s crust. The phenomenon of extensive air showers as a tool of hadron astronomy, spectral and compositional aspects of the high energy primary radiation, and the status of the anisotropy are treated comprehensively. This is followed by chapters on the interpretation of cosmic ray phenomena at high energies, and on the propagation of the cosmic radiation through galactic and extragalactic space. The subsequent chapters focus on the properties of muons and neutrinos, on the atmospheric neutrino background, and on astrophysical (cosmogenic) neutrinos. The basic detection principles are discussed and the different giant detector systems presented, including environmental aspects and background problems. The major experiments, in particular the successful IceCube experiment at Antarctica, are described and their results and interpretations discussed.
The Chemistry of Mars focuses on the chemical exploration of Mars, with diverse viewpoints on the future of Mars research in terms of terrestrial missions. The holistic view of Mars’s chemistry is elucidated through a full scale picture of current knowledge and future intentions and explorations, including a review of temperature, surface pressure, wind, dust-cover, water-ice, and CO2 surface ice. This book provides a dedicated resource for space and planetary scientists, astrochemists, and chemists looking beyond Earth applications, including students, academics, and professionals.
Interstellar Travel: After Arrival is a comprehensive, technical look at the necessary considerations for settlement on an extra solar planet following interstellar travel, addressed by leading experts in the fields of space development. The book features the current and future plans for lunar, Mars, and asteroid settlement, and how what we learn from such future endeavors might apply to settlement at destinations around other stars. In addition, scientists who have been considering the construction of large space structures and terraforming discuss realistic options to be considered.Other chapters cover necessary considerations such as whether terraforming is possible and how it might be accomplished, the ethical issues and scientific constraints to interacting with an alien biosphere, and what we might learn from settling within our own Solar System that would apply to settling elsewhere. The third book of a three-book compilation, this new release presents up-to-date and realistic technical and scientific considerations of the challenges that settling on an exoplanet would bring, including review of the current technological capabilities and how they might be put towards life on an extra solar planet.
Machine Learning for Small Bodies in the Solar System provides the latest developments and methods in applications of Machine Learning (ML) and Artificial Intelligence (AI) to different aspects of Solar System bodies, including dynamics, physical properties, and detection algorithms. Offering a practical approach, the book encompasses a wide range of topics, providing both readers with essential tools and insights for use in researching asteroids, comets, moons, and Trans-Neptunian objects. The inclusion of codes and links to publicly available repositories further facilitates hands-on learning, enabling readers to put their newfound knowledge into practice. Machine Learning for Small Bodies in the Solar System serves as an invaluable reference for researchers working in the broad fields of Solar System bodies; both seasoned researchers seeking to enhance their understanding of ML and AI in the context of Solar System exploration or those just stepping into the field looking for direction on methodologies and techniques to apply ML and AI in their work.
Black Holes in the Era of Gravitational-Wave Astronomy provides a multidisciplinary, up-to-date view of the physics of black holes, along with an exhaustive overview of crucial open questions and recent advancements in the astrophysics of black holes in the wake of incredible advancements made in the last decade. It includes discussions on improvements in theoretical modeling and observational perspectives for black holes of all sizes, along with associated challenges. The book's structure and themes will enable an entwined understanding of black hole physics at all scales, thus avoiding the compartmentalized view that is typical of more specialized manuscripts and reviews.This book is a complete reference for scientists interested in a multidirectional approach to the study of black holes. It provides substantial discussions about the interplay of different types of black holes and gives professionals a heterogeneous and comprehensive overview of the astrophysics of black holes of all masses.
Introductory Astrochemistry: From Inorganic to Life-Related Materials provides a detailed examination of the origins of planets, their satellites, and the conditions that led to life itself. Drawing on theories, experiments, observations, calculations, and analytical data from five distinct astrosciences, including astronomy, astrobiology, astrogeology, astrophysics, and astrochemistry, the book provides a comprehensive understanding of the formation and evolution of our Solar System and applies it to other solar systems. The book begins with fundamental knowledge in the astrosciences, building upon understanding systematically up to the formation of the early Solar System.This book is an interdisciplinary reference for researchers and advanced students in astrogeology, astrophysics, astrochemistry, astrobiology, astronomy, and other space sciences, helping to foster a deeper understanding of the interconnections between these disciplines.
Relativity and Cosmology: From First Principles to Interpretations provides a high-quality and highly relevant astrophysics grounding for senior undergraduate students. This comprehensive textbook emphasizes an illustrative, pedagogical approach and aims to strike a balance between the breadth and depth of the material presented, frequently tying new material – relativistic mechanics and gravity – to the classical mechanics and gravity with which readers are more familiar. It includes robust content and corresponding exercises, figures, and appendices on many exciting developments, including relativistic mechanics; Newtonian classical mechanics; relativistic spacetime; special relativity; general relativity; tensor calculus; cosmology; Einstein’s field equations; dark matter; dark energy; and black holes.This accessible edition delivers helpful and engaging additions to the role and importance of physics in cosmology and relativity. It is ideal for courses in physics, astrophysics, astronomy, and related subjects.
Spatial Cognitive Engine Technology discusses the increase in user demand for satellite wireless communication services that has led to the increasing development of spectrum resources and the fixed spectrum allocation mode which makes the utilization rate of spectrum resources lower. As an intelligent spectrum sharing technology, cognitive radio has innovated the traditional spectrum management system and is one of the effective ways to solve the above-mentioned problems. As the core of satellite cognitive radio, the spatial cognitive engine can use artificial intelligence to dynamically configure working parameters according to changes in the communication environment and user needs.
Interstellar Travel: Purpose and Motivations is a comprehensive, technical look at the necessary considerations for interstellar travel addressed by leading experts in the field, from scientists studying possible destinations (exoplanets) and the vast distances between, to those concerned with building institutions and capabilities in society that could sustain such endeavors. In addition to the technical, medical, and anthropological aspects of deep space travel, the ethics and morality of spreading Earth-based life to other worlds is also examined. In the first book of a three-book compilation, Interstellar Travel: Purpose and Motivations offers in-depth, up-to-date and realistic technical and scientific considerations in the pursuit of interstellar travel and is an integral reference for scientists, engineers, researchers and academics working on, or interested in, space development and space technologies. With a renewed interest in space exploration and development evidenced by the rise of the commercial space sector and various governments now planning to send humans back to the moon and to Mars, so also is interest in taking the next steps beyond the Solar System and to the ultimate destination – planets circling other stars.