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1 Fukushima, Toshio Position and Motion of Celestial Bodies I13293 2024 eBook  
2 Omori, Kiyoaki Christopher Galaxy Merger Identification Methods, and Investigations of the Role of Mergers in Galaxy Evolution I13267 2024 eBook  
3 Demtr??der, Wolfgang Astrophysics I13251 2024 eBook  
4 Montanari, Alessandro Searching for Dark Matter with Imaging Atmospheric Cherenkov Telescopes I13241 2024 eBook  
5 Braj??a, Roman Solar Rotation I13235 2024 eBook  
6 Aldoroty, Lauren Properties of the Color-Magnitude Diagrams of Type Ia Supernovae I13230 2024 eBook  
7 Kokhanovsky, Alexander Springer Series in Light Scattering I13218 2024 eBook  
8 Vardoulaki, Eleni Data-Intensive Radio Astronomy I13214 2024 eBook  
9 Ricciardi, Giulia Introduction to Neutrino and Particle Physics I13198 2024 eBook  
10 Mambrini, Yann Particles in the Dark Universe I13195 2024 eBook  
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TitlePosition and Motion of Celestial Bodies
Author(s)Fukushima, Toshio
PublicationSingapore, 1. Imprint: Springer 2. Springer Nature Singapore, 2024.
DescriptionXXV, 323 p. 95 illus., 9 illus. in color : online resource
Abstract NoteThis book is a systematic introduction to astrometry and celestial mechanics. It consists of five parts: Observational astrometry, theoretical astrometry, basics of celestial mechanics, orbital dynamics, and rotational dynamics. The book is unique in various aspects. First, it discusses astrometry and celestial mechanics in a single and unified manner. Second, it stands on not the Newtonian but general relativistic viewpoints. Third, it explains both the orbital and rotational motions of celestial bodies. Fourth, it conforms to the latest International Astronomical Union (IAU) resolutions and Conf??rence G??n??rale des Poids et Mesures (CGPM) rules. Lastly, its historical topics, ample exercises, and detailed model answers stimulate readers. The appendixes also provide various tables of constants, basic mathematical formulae, descriptions of symbols used, lists of technical abbreviations and model solutions to exercises. The book is intended for undergraduate students of physics or astronomy. Further, it serves as a pocket reference also useful for professional scientists. The basis of the English translation of this book from its Japanese original manuscript was done with the help of artificial intelligence. A subsequent human revision of the content was done by the editor and authors
ISBN,Price9789819754489
Keyword(s)1. ASTRONOMY 2. Astronomy, Observations and Techniques 3. ASTROPHYSICS 4. EBOOK 5. EBOOK - SPRINGER 6. GENERAL RELATIVITY 7. GENERAL RELATIVITY (PHYSICS) 8. GRAVITATION 9. NEWTONIAN PHYSICS
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TitleGalaxy Merger Identification Methods, and Investigations of the Role of Mergers in Galaxy Evolution
Author(s)Omori, Kiyoaki Christopher
PublicationSingapore, 1. Imprint: Springer 2. Springer Nature Singapore, 2024.
DescriptionXVI, 144 p. 75 illus., 71 illus. in color : online resource
Abstract NoteThis book offers new findings on the impact of galaxy mergers on galaxy evolution and related processes. Galaxies are astronomical objects composed of stars, gas, and dark matter. The main pathway for galaxy evolution in the currently accepted model for structure growth is through interactions and mergers, or the process in which multiple galaxies interact, collide, and end up as one larger galaxy. Galaxy interactions and mergers are also considered to drive various processes pertaining to galaxy evolution, such as star formation, active galactic nuclei (AGN) activity, and chemical evolution. As such, not only are merging galaxy systems important to understand galaxy structure growth in a cosmological context, they are also unique laboratories to study evolutionary processes taking place in galaxies. However, despite their importance, the relative role of galaxy mergers on galaxy evolution is still heavily contested. One reason for this is difficulty in identifying merger galaxies in observational data. Many different methods have been adopted for merger galaxy identification, but none of them are perfect. Moreover, the use of differing selection methods can result in widely different samples, which can alter statistical results. As such, a novel, robust method for merger identification is required to deepen our understanding of galaxy mergers. In this book, we introduce new methods to identify galaxy mergers from observational data. The first method combines the use of visual identification???both of optical and kinematic images???with spectroscopic pair identification. The second is machine learning based, using a training method called fine-tuning, an application of transfer learning. A pre-trained model on galaxy images is further fine-tuned using a sample of synthetic galaxy images, to make a classifier for merger identification. Using samples identified by our methods, the author conducts three studies: the impact of mergers on galaxy chemical evolution, the effect of galaxy local environment on merging activity, and the connection between mergers and AGN activity. This book is mainly intended for astrophysicists, particularly those studying galaxies, however is open for all to read
ISBN,Price9789819787357
Keyword(s)1. ASTRONOMY 2. Astronomy, Observations and Techniques 3. ASTROPHYSICS 4. EBOOK 5. EBOOK - SPRINGER
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TitleAstrophysics
Author(s)Demtr??der, Wolfgang
PublicationCham, 1. Imprint: Springer 2. Springer Nature Switzerland, 2024.
DescriptionXI, 282 p. 426 illus., 354 illus. in color : online resource
Abstract NoteThis introduction to astronomy and astrophysics provides an accessible and clear treatment of the fundamentals. Starting with experimental astronomy, observation techniques and structure and properties of the components of the solar system, this textbook enables the reader to understand the basics in astrophysics. The text is written from the experimental physics point of view, giving numerous real life examples and detailed instrumentation and experimental methods. This highly motivating presentation deepens the knowledge in a very accessible way. The second part of the text gives a concise introduction to stars and extra-solar planets. The stellar evolution and categorization is explained. The last part features cosmological models, galaxy evolution and large scale objects in the universe. Numerous problems with solutions are perfect for self-study
ISBN,Price9783031221354
Keyword(s)1. ASTRONOMY 2. Astronomy, Observations and Techniques 3. ASTROPHYSICS 4. EBOOK 5. EBOOK - SPRINGER 6. SOLAR PHYSICS 7. SUN
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TitleSearching for Dark Matter with Imaging Atmospheric Cherenkov Telescopes
Author(s)Montanari, Alessandro;Moulin, Emmanuel
PublicationCham, 1. Imprint: Springer 2. Springer Nature Switzerland, 2024.
DescriptionXXXII, 186 p. 79 illus., 73 illus. in color : online resource
Abstract NoteThis book provides a comprehensive review of the methodologies and searches for dark matter (DM) annihilation signals using very-high-energy gamma rays (VHE, E > 100 GeV), utilizing data from current Imaging Atmospheric Cherenkov Telescopes (IACTs) in the pre-Cherenkov Telescope Array (CTA) era. It presents the state-of-the-art statistical analysis methods and theoretical models related to TeV DM, applied to data from the H.E.S.S. telescope array, which is currently the most sensitive IACT array for observing the Galactic Center (GC), where the brightest DM annihilation signals are expected. The authors delve into the astrophysics of VHE gamma-ray production through cosmic ray acceleration. They explain the Imaging Atmospheric Cherenkov technique, describe the H.E.S.S. array, and discuss possibilities for DM annihilation-induced gamma-ray spectra and DM distribution profiles. By employing advanced statistical methods, they search for weak signals in the GC region using the H.E.S.S. Inner Galaxy Survey dataset and address systematic uncertainties. The authors present and debate the most constraining results on TeV dark matter models. Finally, this book presents the sensitivity of current IACTs to DM annihilation signals using IGS mock datasets, accounting for systematic and instrumental uncertainties. Detection prospects for canonical TeV DM models, such as the Wino, Higgsino, and quintuplet, are discussed. Sensitivity benchmarks on indirect DM searches with IACTs using H.E.S.S. as an example are provided, setting the stage for future developments in the CTA era. It serves as a consolidated resource for graduate students and researchers, presenting methodologies that could lead to significant advancements in the quest to understand dark matter
ISBN,Price9783031664700
Keyword(s)1. ASTRONOMY 2. Astronomy, Observations and Techniques 3. ASTROPHYSICS 4. COSMOLOGY 5. EBOOK 6. EBOOK - SPRINGER
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TitleSolar Rotation
Author(s)Braj??a, Roman;Hanslmeier, Arnold
PublicationSingapore, 1. Imprint: Springer 2. Springer Nature Singapore, 2024.
DescriptionXVI, 180 p. 88 illus., 37 illus. in color : online resource
Abstract NoteThe rotation of the Sun is a basic parameter which constrains the boundary conditions for the model of the MHD-dynamo mechanisms that generates solar activity. The Sun is a slowly rotating star with a convection zone below the surface which is the site of the solar dynamo. The solar rotation depends on the latitude, depth/height and time, i.e., the Sun rotates differentially. In the book several aspects of the solar rotation are covered. Only in the case of the Sun we can directly observe details in its atmosphere and so measure the rotation velocity using various tracers, which is one of the mostly used methods for rotation determination. So, the Sun is a prototype for studying other stars. Different techniques that enable to determine solar rotation (e.g., tracer method, spectroscopic method, helioseismology) are presented and their results are compared and interpreted. In the current literature there is no book exclusively about solar rotation published in the last several decades. The book is intended for astrophysicists, both professionals as well as students and people interested in science in general. The reader would strongly benefit from the comprehensive description of several topics related to the solar rotation. The authors are highly experienced in teaching astrophysics both to astrophysicists, solar physicists as well as to the public. Therefore, from the didactical point of view the book is written basically as a textbook, so the reader that is not deep within that field can gain an overview. Moreover, for those who want to get deeper into the topics, additional information is given, and recommendations for further literature as well as many citations to recent publications. The reader will get both (i) a general introduction into the topics (ii) overview of recent publications on the topics. Therefore, the book can serve as a textbook but will be also very useful for research and thesis writing, for example
ISBN,Price9789819768790
Keyword(s)1. ASTROPHYSICS 2. COSMOLOGY 3. EBOOK 4. EBOOK - SPRINGER 5. PLASMA (IONIZED GASES) 6. PLASMA PHYSICS 7. SOLAR PHYSICS 8. SOLAR SYSTEM 9. SPACE PHYSICS 10. SUN 11. THERMODYNAMICS
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TitleProperties of the Color-Magnitude Diagrams of Type Ia Supernovae
Author(s)Aldoroty, Lauren
PublicationCham, 1. Imprint: Springer 2. Springer Nature Switzerland, 2024.
DescriptionXVIII, 86 p. 39 illus., 26 illus. in color : online resource
Abstract NoteThis thesis presents a novel analysis of a photometric observational feature of Type Ia Supernovae (SNe Ia), the most precise distance indicators available for cosmological studies. While SNe Ia are crucial for understanding modern cosmology, there are systematic uncertainties associated with them that prevent use to their full potential. It is therefore vital that sources of systematic error in SN Ia standardization are better understood. In this thesis, the author robustly connects the color-magnitude diagram to SN Ia spectra and their physics for the first time, and shows that for the SN sample in the dissertation, this feature is important to consider as a contributor to scatter in the Hubble residual. There is no prior work in the literature that examines this feature in such depth, and it is rare to be able to paint such a thorough picture in a SN Ia study rooted in a single photometric feature. This work opens up many avenues for future observational and theoretical studies
ISBN,Price9783031724473
Keyword(s)1. ASTRONOMY 2. Astronomy, Observations and Techniques 3. ASTROPHYSICS 4. Classical and Quantum Gravity 5. EBOOK 6. EBOOK - SPRINGER 7. GRAVITATION 8. OPTICAL SPECTROSCOPY
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TitleSpringer Series in Light Scattering : Volume 10: Direct and Inverse Problems of Light Scattering Media Optics
Author(s)Kokhanovsky, Alexander
PublicationCham, 1. Imprint: Springer 2. Springer Nature Switzerland, 2024.
DescriptionIX, 215 p. 81 illus., 61 illus. in color : online resource
Abstract NoteThe book is aimed at description of recent progress in studies of light scattering in turbid media. In particular, atmospheric optics and remote sensing research community will greatly benefit from the publication of this book
ISBN,Price9783031665783
Keyword(s)1. ASTRONOMY 2. ASTROPHYSICS 3. EBOOK 4. EBOOK - SPRINGER 5. Light-Matter Interaction 6. OPTICAL SPECTROSCOPY 7. OPTICS 8. Optics and Photonics 9. PHYSICS 10. PHYSICS AND ASTRONOMY
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8.     
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TitleData-Intensive Radio Astronomy : Bringing Astrophysics to the Exabyte Era
Author(s)Vardoulaki, Eleni;Dembska, Marta;Drabent, Alexander;Hoeft, Matthias
PublicationCham, 1. Imprint: Springer 2. Springer Nature Switzerland, 2024.
DescriptionXV, 458 p. 72 illus., 66 illus. in color : online resource
Abstract NoteRadio astronomy is irreversibly moving towards the exabyte era. In the advent of all-sky radio observations, efficient tools and methods to manage the large data volume generated have become imperative. This book brings together the knowledge of several different research fields to present an overview of current state-of-the-art methods in data-intensive radio astronomy. Its approach is comprehensive and data-centric, offering a coherent look at the four distinct parts of the data lifecycle: Data creation, storage and archives Data processing Post-processing and data analysis Data access and reuse Large data management has been the topic of discussion within the astronomical community for decades. Some relevant areas explored in this volume are: ongoing technological innovations in interferometers and computing facilities; difficulties and possible solutions for the huge processing demands of radiotelescope projects such as LOFAR, MeerKat, ASKAP; concepts for reliable and fast storage for archiving; and more. Written by experts across astrophysics, high-energy particle physics, data science, and computer science, this volume will help researchers and advanced students better understand the current state of data-intensive radio astronomy and tackle the major problems that may arise from future instruments
ISBN,Price9783031584688
Keyword(s)1. ASTRONOMY 2. Astronomy, Observations and Techniques 3. ASTROPHYSICS 4. COMPUTER SCIENCE 5. Data Analysis and Big Data 6. EBOOK 7. EBOOK - SPRINGER 8. Methodology of Data Collection and Processing 9. Quantitative research 10. Sampling (Statistics)
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TitleIntroduction to Neutrino and Particle Physics : From Quantum Field Theory to the Standard Model and Beyond
Author(s)Ricciardi, Giulia
PublicationCham, 1. Imprint: Springer 2. Springer International Publishing, 2024.
DescriptionX, 418 p. 44 illus : online resource
Abstract NoteThis textbook offers a clear and concise introduction to the main aspects of neutrino physics, providing the foundational knowledge necessary for research in both theoretical and experimental fields. It presents field theory concepts in a highly self-contained manner and explains the main experimental techniques and phenomenological aspects of neutrino and particle physics with clarity and scientific rigor. Specialized jargon and traditionally ambiguous concepts are carefully explained. The book???s didactic style focuses on a selected number of key topics, enriched with numerous figures and examples. Significant recent advancements in theory and experiments are described within their physical context, avoiding technical details likely to become outdated soon. This book will be invaluable not only for students of particle physics but also as a concise reference for researchers in other fields seeking an up-to-date understanding of essential concepts in neutrino physics.
ISBN,Price9783031650963
Keyword(s)1. ASTROPHYSICS 2. EBOOK 3. EBOOK - SPRINGER 4. Elementary particles (Physics) 5. Elementary Particles, Quantum Field Theory 6. Nuclear and Particle Physics 7. NUCLEAR PHYSICS 8. QUANTUM FIELD THEORY
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TitleParticles in the Dark Universe : A Student???s Guide to Particle Physics and Cosmology
Author(s)Mambrini, Yann
PublicationCham, 1. Imprint: Springer 2. Springer International Publishing, 2024.
DescriptionXXV, 664 p. 143 illus., 122 illus. in color : online resource
Abstract NoteThis second edition of Particles in the Dark Universe has been substantially enhanced with several new chapters that delve into crucial aspects of particle physics in the Universe. These additions encompass the role of primordial black holes in the early universe, tracing their formation to decay, unification theories, a comprehensive historical overview of cosmological models, an extensive examination of the physics of the graviton, and an educational exploration of gravitational phenomena such as Unruh-type or Hawking radiation. Additionally, this edition incorporates 30 new exercises and provides a comprehensive presentation of inflationary models, along with a pedagogical insight into the mechanism of baryogenesis. Structured in a logical sequence, this book offers a thorough and instructional exploration of particle physics within the early universe. It initiates by elucidating the thermal history of the universe, delving into pivotal concepts like Big Bang nucleosynthesis, the cosmic microwave background (CMB), and inflation. Subsequently, it meticulously addresses both direct and indirect detection methods of dark matter, followed by an in-depth analysis of neutrino physics. The book further scrutinizes potential candidates for dark matter and their interactions. Designed for theoretical physicists engaged in particle physics within the universe, dark matter detection, astrophysical constraints, and those interested in models of inflation or reheating, this book also caters to astrophysicists involved in quantum field theory computations. It encompasses all essential elements required for computing various physical processes, providing mathematical tables, necessary thermodynamic functions for the early universe, and Feynman rules. Consequently, this book serves as an intersecting point between astrophysics, particle physics, and cosmology
ISBN,Price9783031669941
Keyword(s)1. ASTROPHYSICS 2. COSMOLOGY 3. EBOOK 4. EBOOK - SPRINGER 5. MATHEMATICAL PHYSICS 6. PARTICLE PHYSICS 7. PARTICLES (NUCLEAR PHYSICS) 8. Theoretical, Mathematical and Computational Physics
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