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Author | Title | Accn# | Year | Item Type | Claims |
| 11 |
Frisch, H??l??ne |
Radiative Transfer |
I12404 |
2022 |
Book |
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| 12 |
Bhattacharyya, Sudip |
Millisecond Pulsars |
I12387 |
2022 |
Book |
|
| 13 |
Jetzer, Philippe |
Applications of General Relativity |
I12382 |
2022 |
Book |
|
| 14 |
Streit-Bianchi, Marilena |
Advances in Cosmology |
I12360 |
2022 |
Book |
|
| 15 |
Bodensteiner, Julia |
Observational Imprints of Binary Evolution on B- and Be-star Populations |
I12353 |
2022 |
Book |
|
| 16 |
Oya, Yoko |
A Few Tens au Scale Physical and Chemical Structures Around Young Low-Mass Protostars |
I12318 |
2022 |
Book |
|
| 17 |
Ho, Anna Y. Q |
The Landscape of Relativistic Stellar Explosions |
I12314 |
2022 |
Book |
|
| 18 |
Moriwaki, Kana |
Large-Scale Structure of the Universe |
I12304 |
2022 |
Book |
|
| 19 |
Jain, Sudhir Ranjan |
A Primer on Fluid Mechanics with Applications |
I12259 |
2022 |
Book |
|
| 20 |
M??ller, Ana Laura |
Acceleration and Propagation of Cosmic Rays in High-Metallicity Astrophysical Environments |
I12226 |
2022 |
Book |
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11.
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| Title | Radiative Transfer : An Introduction to Exact and Asymptotic Methods |
| Author(s) | Frisch, H??l??ne |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XXXII, 593 p. 50 illus : online resource |
| Abstract Note | This book discusses analytic and asymptotic methods relevant to radiative transfer in dilute media, such as stellar and planetary atmospheres. Several methods, providing exact expressions for the radiation field in a semi-infinite atmosphere, are described in detail and applied to unpolarized and polarized continuous spectra and spectral lines. Among these methods, the Wiener???Hopf method, introduced in 1931 for a stellar atmospheric problem, is used today in fields such as solid mechanics, diffraction theory, or mathematical finance. Asymptotic analyses are carried out on unpolarized and polarized radiative transfer equations and on a discrete time random walk. Applicable when photons undergo a large number of scatterings, they provide criteria to distinguish between large-scale diffusive and non-diffusive behaviors, typical scales of variation of the radiation field, such as the thermalization length, and specific descriptions for regions close and far from boundaries. Its well organized synthetic view of exact and asymptotic methods of radiative transfer makes this book a valuable resource for both graduate students and professional scientists in astrophysics and beyond |
| ISBN,Price | 9783030952471 |
| Keyword(s) | 1. ASTROPHYSICS
2. EBOOK
3. EBOOK - SPRINGER
4. Engineering Thermodynamics, Heat and Mass Transfer
5. Heat engineering
6. HEAT TRANSFER
7. Light-Matter Interaction
8. MASS TRANSFER
9. Mathematical Methods in Physics
10. MATHEMATICAL PHYSICS
11. OPTICS
12. THERMODYNAMICS
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12404 |
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On Shelf |
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12.
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| Title | Millisecond Pulsars |
| Author(s) | Bhattacharyya, Sudip;Papitto, Alessandro;Bhattacharya, Dipankar |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XVIII, 321 p. 75 illus., 68 illus. in color : online resource |
| Abstract Note | This book includes nine chapters written by internationally recognized experts, covering all aspects of millisecond pulsars in one concise and cohesive volume. These aspects include pulsations powered by stellar spin, accretion and thermonuclear burning of accreted matter, their physics and utility, stellar evolution and the extreme physics of super-dense stellar cores. The book includes substantial background material as well as recent theoretical and multi-wavelength observational results. The volume will thus be useful for professional astronomers and graduate students alike. What is the behavior of the strong nuclear interaction, and what are the matter constituents at ultrahigh densities in neutron star cores? How do old neutron stars in binaries evolve? How does their magnetosphere interact with the surrounding plasma to accelerate particles and emit radiation observed at all wavelengths? These are just a few of the questions that millisecond pulsars are helping us answer and will settle in the near future with the next generation of instruments. Such quickly rotating, highly magnetized neutron stars are remarkable natural laboratories that allow us to investigate the fundamental constituents of matter and their interactions under extreme conditions that cannot be reproduced in terrestrial laboratories |
| ISBN,Price | 9783030851989 |
| Keyword(s) | 1. ASTRONOMY
2. Astronomy, Cosmology and Space Sciences
3. Astronomy, Observations and Techniques
4. Astronomy???Observations
5. ASTROPHYSICS
6. EBOOK
7. EBOOK - SPRINGER
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12387 |
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On Shelf |
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13.
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| Title | Applications of General Relativity : With Problems |
| Author(s) | Jetzer, Philippe |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XIII, 195 p. 13 illus., 7 illus. in color : online resource |
| Abstract Note | The aim of this textbook is to present in a comprehensive way several advanced topics of general relativity, including gravitational waves, tests of general relativity, time delay, spinors in curved spacetime, Hawking radiation, and geodetic precession to mention a few. These are all important topics in today's research activities from both a theoretical and experimental point of view. This textbook is designed for advanced undergraduate and graduate students to strengthen the knowledge acquired during the core courses on General Relativity. The author developed the book from a series of yearly lectures with the intention of offering a gentle introduction to the field. This book helps understanding the more specialized literature and can be used as a first reading to get quickly into the field when starting research. Chapter-end exercises complete the learning material to master key concepts |
| ISBN,Price | 9783030957186 |
| Keyword(s) | 1. ASTROPHYSICS
2. EBOOK
3. EBOOK - SPRINGER
4. GENERAL RELATIVITY
5. GENERAL RELATIVITY (PHYSICS)
6. GRAVITATION
7. GRAVITATIONAL PHYSICS
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12382 |
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On Shelf |
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14.
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| Title | Advances in Cosmology : Science - Art - Philosophy |
| Author(s) | Streit-Bianchi, Marilena;Catapano, Paola;Galbiati, Cristiano;Magnani, Enrico |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XXII, 376 p. 154 illus., 138 illus. in color : online resource |
| Abstract Note | Cosmology???s journey to the present day has been a long one. This book outlines the latest research on modern cosmology and related topics from world-class experts. Through it, readers will learn how multi-disciplinary approaches and technologies are used to search the unknown and how we arrived at the knowledge used and assumptions made by cosmologists today. The book is organized into four parts, each exploring a theme that has troubled humankind for centuries. Since the dawn of time, looking at the sky, humans have tried to understand their origin, the laws governing it, and what influence it all has on human life. In most ancient civilizations, astronomers embodied the power of knowledge. This knowledge was not compartmentalized, and scientists often found philosophical implications within their quests, many of which destroyed the borders between the natural sciences. Even now, as observers and scientists continue to use conjecture to generate theoretical assumptions and laws that then have to be confirmed experimentally, said theoretical and experimental searches are being linked to philosophical thinking and artistic representation, as they were up until the 18th century. This multi-disciplinary book will appeal to anyone with an interest in the fields of Astronomy, Cosmology or Physics |
| ISBN,Price | 9783031056253 |
| Keyword(s) | 1. ASTRONOMY
2. Astronomy, Cosmology and Space Sciences
3. Astronomy, Observations and Techniques
4. Astronomy???Observations
5. ASTROPHYSICS
6. COSMOLOGY
7. EBOOK
8. EBOOK - SPRINGER
9. History of Physics and Astronomy
10. Physics???History
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12360 |
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On Shelf |
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15.
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| Title | Observational Imprints of Binary Evolution on B- and Be-star Populations |
| Author(s) | Bodensteiner, Julia |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XX, 128 p. 44 illus., 42 illus. in color : online resource |
| Abstract Note | This book presents novel observational evidence toward detecting and characterizing the products of massive, interacting binary stars. As a majority of massive stars are born in close binary systems, a large number of so-called massive binary interaction products are predicted to exist; however, few have been identified so far. Based on observations with the largest telescopes around the world, equipped with state-of-the-art instrumentation, this book helps to remedy this situation. In her outstanding PhD-thesis Julia Bodensteiner identifies a new class of post-interaction binaries in a short-lived phase just briefly after the initially more massive star has been stripped of part of its envelope. She further provides new evidence for the Be phenomenon to largely result from binary interactions. These results represented a new and testable prediction for the evolution of these stars and opened up a new way forward for identifying hundreds of post-interaction products. Finally, using the MUSE integral field spectrograph at the Very Large Telescope in Chile, the author presents a novel spectroscopic campaign focusing on the 40 Myr-old star cluster NGC 330 in the Small Magellanic Clouds. Combined with photometric observations from the Hubble Space Telescope, the MUSE data allow to characterize the entire massive star population of NGC 330, revealing their multiplicity properties and rotational velocities and providing unique observational constraints on their (binary) evolution history. This is made possible by the developments of novel numerical methods allowing to extract star spectra from the MUSE integral field spectroscopic data and to characterize their properties by the simultaneous comparison of MUSE spectroscopy and Hubble photometry with atmospheric models. This book is a partly re-written version of the author's thesis offering a highly readable coherent text presenting not only new insights into the properties of binary interaction products but also giving students an excellent introduction into the field |
| ISBN,Price | 9783031194894 |
| Keyword(s) | 1. Astronomy, Observations and Techniques
2. Astronomy???Observations
3. ASTROPHYSICS
4. EBOOK
5. EBOOK - SPRINGER
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12353 |
|
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On Shelf |
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16.
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| Title | A Few Tens au Scale Physical and Chemical Structures Around Young Low-Mass Protostars |
| Author(s) | Oya, Yoko |
| Publication | Singapore, 1. Imprint: Springer
2. Springer Nature Singapore, 2022. |
| Description | XVI, 212 p. 107 illus., 102 illus. in color : online resource |
| Abstract Note | This book characterizes the kinematic and chemical structures of disk-forming regions around low-mass protostellar sources and their interplay based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. It describes the chemical evolution of molecules formed in an interstellar gas using the ALMA observations of 5 Sun-like protostars at a spatial resolution of a few tens au scale, which unveils the physical mechanism of star and planetary formation. The book reviews the author???s successful works, focusing on two key findings: (i) A drastic change in the chemical composition of the gas around the centrifugal barrier of the infalling-rotating envelopes, and (ii) the chemical composition in the disk-forming regions, which varies from source to source depending on the chemical characteristics of the parent molecular cloud. These findings are based on the fine characterization of physical structures based on careful kinematic analyses. An additional attraction is the inclusion of the skillful reviews of ALMA observatory and its observation and physical models to describe the observed gas structure |
| ISBN,Price | 9789811917080 |
| Keyword(s) | 1. Astronomy, Observations and Techniques
2. Astronomy???Observations
3. ASTROPHYSICS
4. Atomic and Molecular Structure and Properties
5. Atomic structure????
6. EBOOK
7. EBOOK - SPRINGER
8. Molecular structure??
9. PHYSICAL CHEMISTRY
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12318 |
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On Shelf |
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17.
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| Title | The Landscape of Relativistic Stellar Explosions |
| Author(s) | Ho, Anna Y. Q |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XXI, 307 p. 1 illus : online resource |
| Abstract Note | This thesis reports the discovery of relativistic stellar explosions outside of the gamma ray band, using optical time domain surveys. It is well known that some massive stars end their lives with the formation of a compact object (a neutron star or black hole) that launches a relativistic jet detectable from earth as a burst of gamma rays. It has long been suspected, however, that gamma ray bursts are only the tip of the iceberg in a broad landscape of relativistic explosions, and so the results presented in this thesis represent a major breakthrough. Highlights of this thesis include: characterization of the first major new class of relativistic explosions in a decade; the discovery of abrupt end-of-life mass-loss in a surprisingly diverse range of stars; and the routine discovery of afterglow emission and several events that may represent baryonically dirty jets or jets viewed slightly off axis. These discoveries necessitated the solution of difficult technical challenges such as the identification of rare and fleeting ???needles??? in a vast haystack of time-varying phenomena in the night sky, and responding to discoveries within hours to obtain data across the electromagnetic spectrum from X-rays to radio wavelengths. |
| ISBN,Price | 9783031153679 |
| Keyword(s) | 1. ASTROPHYSICS
2. EBOOK
3. EBOOK - SPRINGER
4. GENERAL RELATIVITY
5. GENERAL RELATIVITY (PHYSICS)
|
| Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12314 |
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On Shelf |
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18.
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| Title | Large-Scale Structure of the Universe : Cosmological Simulations and Machine Learning |
| Author(s) | Moriwaki, Kana |
| Publication | Singapore, 1. Imprint: Springer
2. Springer Nature Singapore, 2022. |
| Description | XII, 120 p. 46 illus., 44 illus. in color : online resource |
| Abstract Note | Line intensity mapping (LIM) is an observational technique that probes the large-scale structure of the Universe by collecting light from a wide field of the sky. This book demonstrates a novel analysis method for LIM using machine learning (ML) technologies. The author develops a conditional generative adversarial network that separates designated emission signals from sources at different epochs. It thus provides, for the first time, an efficient way to extract signals from LIM data with foreground noise. The method is complementary to conventional statistical methods such as cross-correlation analysis. When applied to three-dimensional LIM data with wavelength information, high reproducibility is achieved under realistic conditions. The book further investigates how the trained machine extracts the signals, and discusses the limitation of the ML methods. Lastly an application of the LIM data to a study of cosmic reionization is presented. This book benefits students and researchers who are interested in using machine learning to multi-dimensional data not only in astronomy but also in general applications |
| ISBN,Price | 9789811958809 |
| Keyword(s) | 1. Astronomy, Observations and Techniques
2. Astronomy???Observations
3. ASTROPHYSICS
4. COSMOLOGY
5. EBOOK
6. EBOOK - SPRINGER
7. MACHINE LEARNING
|
| Item Type | Book |
Multi-Media Links
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Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12304 |
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On Shelf |
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19.
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| Title | A Primer on Fluid Mechanics with Applications |
| Author(s) | Jain, Sudhir Ranjan;Paradkar, Bhooshan S;Chitre, Shashikumar M |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XVIII, 279 p. 1 illus : online resource |
| Abstract Note | This textbook is a pedagogic introduction to a number of phenomena employing fluid mechanics. Beginning with basic concepts and conservation laws for neutral and charged fluids, the authors apply and develop them to understand aerodynamics, locomotion of micro-organisms, waves in air and water, shock waves, hydrodynamic and hydromagnetic instabilities, stars and black holes, blood flow in humans, and superfluids. The approach is to consider various striking topics on fluid mechanics, without losing necessary mathematical rigor. The book balances the qualitative explanations with formal treatment, in a compact manner. A special focus is given to the important and difficult subject of turbulence and the book ends with a discussion on turbulence in quantum fluids. The textbook is dotted by a number of illustrative examples, mostly from real life, and exercises. The textbook is designed for a one semester course and addresses students at undergraduate and graduate level in physics or engineering, who want to research in the fields as diverse as aeronautics, meteorology, cosmology, biomechanics, and mathematical physics. It is requested knowledge of an undergraduate level course on mathematical methods to better understand the topics presented here |
| ISBN,Price | 9783031204876 |
| Keyword(s) | 1. ASTROPHYSICS
2. CLASSICAL MECHANICS
3. EBOOK
4. EBOOK - SPRINGER
5. Engineering Fluid Dynamics
6. FLUID MECHANICS
7. FLUIDS
8. MECHANICS
9. Medical physics
10. Soft condensed matter
|
| Item Type | Book |
Multi-Media Links
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Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12259 |
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On Shelf |
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20.
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| Title | Acceleration and Propagation of Cosmic Rays in High-Metallicity Astrophysical Environments |
| Author(s) | M??ller, Ana Laura |
| Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
| Description | XVI, 131 p. 43 illus., 42 illus. in color : online resource |
| Abstract Note | This thesis addresses the feasibility of the production of ultra-high-energy cosmic rays in starburst galaxies and active galactic nuclei. These astrophysical objects were theoretically proposed as candidate sources a long time ago. Nevertheless, the interest in them has been recently renewed due to the observational data collected by the Pierre Auger Observatory and the Telescope Array. In this work, a comprehensive review of the current status of the research on cosmic rays accelerators is provided, along with a summary of the principal concepts needed to connect these relativistic particles with electromagnetic and neutrino observations in the multi-messenger era. On one hand, the hypothesis of accelerating particles with energies above 10????? eV in starburst superwinds is carefully revisited, taking into account the constraints imposed by the most recent electromagnetic observations. On the other hand, an alternative new model for the gamma emission of the nearby active galaxy NGC 1068 is presented. The implications of the results of these studies are discussed in terms of the contemporary observatories and prospects for future experiments are offered |
| ISBN,Price | 9783031103063 |
| Keyword(s) | 1. Astronomy, Observations and Techniques
2. Astronomy???Observations
3. Astrophysical Plasma
4. ASTROPHYSICS
5. EBOOK
6. EBOOK - SPRINGER
7. PARTICLE PHYSICS
8. PARTICLES (NUCLEAR PHYSICS)
9. PLASMA ASTROPHYSICS
|
| Item Type | Book |
Multi-Media Links
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| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| I12226 |
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On Shelf |
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