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Author | Title | Accn# | Year | Item Type | Claims |
21 |
Ramond, Paul |
The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity |
I12633 |
2023 |
eBook |
|
22 |
Tsallis, Constantino |
Introduction to Nonextensive Statistical Mechanics |
I12590 |
2023 |
eBook |
|
23 |
Green, Simon F. |
An Introduction to the Sun and Stars |
027101 |
2015 |
Book |
|
24 |
Weinberg, Steven |
Lectures on Astrophysics |
027103 |
2019 |
Book |
|
25 |
Del Nobile, Eugenio |
The Theory of Direct Dark Matter Detection |
I12563 |
2022 |
Book |
|
26 |
Tominaga, Ryosuke |
Dust-Gas Instabilities in Protoplanetary Disks |
I12549 |
2022 |
Book |
|
27 |
Trad Nery, Marina |
Laser Power Stabilization via Radiation Pressure |
I12548 |
2022 |
Book |
|
28 |
Manoharan, Praveen |
Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants |
I12522 |
2022 |
Book |
|
29 |
Bandyopadhyay, Debades |
Supernovae, Neutron Star Physics and Nucleosynthesis |
I12520 |
2022 |
Book |
|
30 |
Dhurandhar, Sanjeev |
General Relativity and Gravitational Waves |
I12501 |
2022 |
Book |
|
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21.
|
![No image available](./images/covers/NoCover.jpg) |
Title | The First Law of Mechanics in General Relativity & Isochrone Orbits in Newtonian Gravity |
Author(s) | Ramond, Paul |
Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2023. |
Description | XXVI, 393 p. 77 illus., 69 illus. in color : online resource |
Abstract Note | The thesis tackles two distinct problems of great interest in gravitational mechanics ??? one relativistic and one Newtonian. The relativistic one is concerned with the "first law of binary mechanics", a remarkably simple variational relation that plays a crucial role in the modern understanding of the gravitational two-body problem, thereby contributing to the effort to detect gravitational-wave signals from binary systems of black holes and neutron stars. The work reported in the thesis provides a mathematically elegant extension of previous results to compact objects that carry spin angular momentum and quadrupolar deformations, which more accurately represent astrophysical bodies than mere point particles. The Newtonian problem is concerned with the isochrone problem of celestial mechanics, namely the determination of the set of radial potentials whose bounded orbits have a radial period independent of the angular momentum. The thesis solves this problem completely in a geometrical way and explores its consequence on a variety of levels, in particular with a complete characterisation of isochrone orbits. The thesis is exceptional in the breadth of its scope and achievements. It is clearly and eloquently written, makes excellent use of images, provides careful explanations of the concepts and calculations, and it conveys the author???s personality in a way that is rare in scientific writing, while never sacrificing academic rigor |
ISBN,Price | 9783031179648 |
Keyword(s) | 1. ASTROPHYSICS
2. EBOOK - SPRINGER
3. GENERAL RELATIVITY
4. GENERAL RELATIVITY (PHYSICS)
5. GRAVITATION
6. GRAVITATIONAL PHYSICS
7. NEWTONIAN PHYSICS
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Item Type | eBook |
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Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12633 |
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On Shelf |
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22.
|
![No image available](./images/covers/NoCover.jpg) |
Title | Introduction to Nonextensive Statistical Mechanics : Approaching a Complex World |
Author(s) | Tsallis, Constantino |
Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2023. |
Description | XVII, 569 p. 372 illus., 208 illus. in color : online resource |
Abstract Note | Metaphors, generalizations and unifications are natural and desirable ingredients of the evolution of scientific theories and concepts. Physics in particular has walked along these paths since its very beginning. This book focuses on nonextensive statistical mechanics, a current generalization of Boltzmann-Gibbs (BG) statistical mechanics. Conceived nearly 150 years ago by Maxwell, Boltzmann and Gibbs, the BG theory, one of the greatest monuments of contemporary physics, exhibits many impressive successes in physics, chemistry, mathematics, and computational sciences. Presently, several thousands of publications by scientists around the world have been dedicated to its nonextensive generalization. A variety of applications have emerged in complex systems and its mathematical grounding is by now well advanced. Since the first edition release thirteen years ago, there has been a vast amount of new results in the field, all of which have been incorporated in thiscomprehensive second edition. Heavily revised and updated with new sections and figures, the second edition remains the go-to text on the subject. A pedagogical introduction to the BG theory concepts and their generalizations ??? nonlinear dynamics, extensivity of the nonadditive entropy, global correlations, generalization of the standard CLT???s, complex networks, among others ??? is presented in this book, as well as a selection of paradigmatic applications in various sciences together with diversified experimental verifications of some of its predictions. Introduction to Nonextensive Statistical Mechanics is suitable for students and researchers with an interest in complex systems and statistical physics |
ISBN,Price | 9783030795696 |
Keyword(s) | 1. Applied Dynamical Systems
2. ASTROPHYSICS
3. COMPLEX SYSTEMS
4. DYNAMICS
5. EBOOK - SPRINGER
6. Mathematical Methods in Physics
7. MATHEMATICAL PHYSICS
8. NONLINEAR THEORIES
9. SYSTEM THEORY
10. Theoretical, Mathematical and Computational Physics
11. THERMODYNAMICS
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Item Type | eBook |
Multi-Media Links
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Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12590 |
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On Shelf |
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25.
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![No image available](./images/covers/NoCover.jpg) |
Title | The Theory of Direct Dark Matter Detection : A Guide to Computations |
Author(s) | Del Nobile, Eugenio |
Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
Description | XVI, 250 p. 20 illus. in color : online resource |
Abstract Note | This book is a pedagogical guide on how to make computations in direct dark matter (DM) detection. The theory behind the calculation of direct detection cross sections and rates is presented, touching aspects related to elementary particle physics, hadronic physics, nuclear physics, and astrophysics. The book is structured in self-contained sections, covering several topics ranging from the scattering kinematics to the phenomenology of direct DM searches. It follows a model-independent approach, aiming at providing the readers with all that is needed to understand the theory and start their own analysis. Meant for graduate students and researchers with interests in particle physics and phenomenology, it is enriched with several worked examples from standard and non-standard particle DM models. Senior researchers working in different areas related to dark matter, like particle and nuclear physics, astrophysics, and cosmology, find in this book a useful and updated guide for reference |
ISBN,Price | 9783030952280 |
Keyword(s) | 1. ASTROPHYSICS
2. COSMOLOGY
3. EBOOK
4. EBOOK - SPRINGER
5. Elementary particles (Physics)
6. Elementary Particles, Quantum Field Theory
7. NUCLEAR PHYSICS
8. PARTICLE PHYSICS
9. PARTICLES (NUCLEAR PHYSICS)
10. QUANTUM FIELD THEORY
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Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12563 |
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On Shelf |
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26.
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![No image available](./images/covers/NoCover.jpg) |
Title | Dust-Gas Instabilities in Protoplanetary Disks : Toward Understanding Planetesimal Formation |
Author(s) | Tominaga, Ryosuke |
Publication | Singapore, 1. Imprint: Springer
2. Springer Nature Singapore, 2022. |
Description | XII, 116 p. 42 illus., 36 illus. in color : online resource |
Abstract Note | How planets form is one of the long-standing questions in astrophysics. In particular, formation scenarios of planetesimals which are kilometer-sized bodies and a precursor of planets are still unclear and under debate although some promising mechanisms have been proposed. This book highlight disk instabilities that have the potential to explain the origin of planetesimals. Using linear analyses and numerical simulations, it addresses how a disk evolves through the development of instabilities, and also presents a new instability driven by dust coagulation. As a result, the simulation demonstrates a scenario of planetesimal formation: A successive development of multiple instabilities triggers planetesimal formation in resulting dusty rings |
ISBN,Price | 9789811917653 |
Keyword(s) | 1. ASTROPHYSICS
2. Computational Physics and Simulations
3. COMPUTER SIMULATION
4. EBOOK
5. EBOOK - SPRINGER
6. MATHEMATICAL PHYSICS
7. PLANETARY SCIENCE
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Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12549 |
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On Shelf |
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27.
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![No image available](./images/covers/NoCover.jpg) |
Title | Laser Power Stabilization via Radiation Pressure |
Author(s) | Trad Nery, Marina |
Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
Description | XIX, 154 p. 81 illus., 79 illus. in color : online resource |
Abstract Note | This book offers a comprehensive and complete description of a new scheme to stabilize the power of a laser on a level needed for high precision metrology experiments. The novel aspect of the scheme is sensing power fluctuations via the radiation pressure driven motion they induce on a micro-oscillator mirror. It is shown that the proposed technique can result in higher signals for power fluctuations than what is achieved by a direct power detection, and also that it enables the generation of a strong bright squeezed beam. The book starts with the basics of power stabilization and an overview on the current state of art. Then, detailed theoretical calculations are performed, and the advantages of the new scheme are highlighted. Finally, a proof-of-principle experiment is described and its results are analyzed in details. The success of the work presented here paves a way for achieving high power stability in future experiments and is of interest for high precision metrology experiments, like gravitational wave detectors, and optomechanical experiments. Nominated as an outstanding PhD thesis by the Gravitational Wave International Committee |
ISBN,Price | 9783030958688 |
Keyword(s) | 1. ASTROPHYSICS
2. EBOOK
3. EBOOK - SPRINGER
4. GENERAL RELATIVITY
5. GENERAL RELATIVITY (PHYSICS)
6. GRAVITATION
7. GRAVITATIONAL PHYSICS
8. LASER
9. LASERS
10. OPTOELECTRONIC DEVICES
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Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12548 |
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On Shelf |
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28.
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![No image available](./images/covers/NoCover.jpg) |
Title | Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants |
Author(s) | Manoharan, Praveen |
Publication | Wiesbaden, 1. Imprint: Springer Spektrum
2. Springer Fachmedien Wiesbaden, 2022. |
Description | XIV, 65 p. 20 illus : online resource |
Abstract Note | In the last 25 years, an extensive body of work has developed various equation of state independent - or (approximately) universal - relations that allow for the inference of neutron star parameters from gravitational wave observations. These works, however, have mostly been focused on singular neutron stars, while our observational efforts at the present, and in the near future, will be focused on binary neutron star (BNS) mergers. In light of these circumstances, the last five years have also given rise to more attempts at developing universal relations that relate BNS pre-merger neutron stars to stellar parameters of the post-merger object, mostly driven by numerical relativity simulations. In this thesis a first attempt at perturbatively deriving universal relations for binary neutron star mergers with long-lived neutron star remnants is presented. The author succeeds in confirming previous results relating pre-merger binary tidal deformabilities to the f-mode frequency of the post-merger object. Combining this result with recent advances of computing the f-mode frequency of fast rotating neutron stars, he also derives a combined relation that relates the pre-merger binary tidal deformability of a BNS to the effective compactness of a long-lived neutron star remnant. Finally, he also proposes a direct relation between these quantities with improved accuracy. About the author Praveen Manoharan is PhD student at T??bingen University, Institute for Theoretical Astrophysics |
ISBN,Price | 9783658368418 |
Keyword(s) | 1. ASTRONOMY
2. Astronomy, Cosmology and Space Sciences
3. ASTROPHYSICS
4. EBOOK
5. EBOOK - SPRINGER
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Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12522 |
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On Shelf |
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29.
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![No image available](./images/covers/NoCover.jpg) |
Title | Supernovae, Neutron Star Physics and Nucleosynthesis |
Author(s) | Bandyopadhyay, Debades;Kar, Kamales |
Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
Description | XVII, 207 p. 41 illus., 29 illus. in color : online resource |
Abstract Note | This book deals with the interdisciplinary areas of nuclear physics, supernovae and neutron star physics. It addresses the physics and astrophysics of the spectacular supernova explosions, starting with the collapse of massive stars and ending with the birth of neutron stars or black holes. Recent progress in the understanding of core collapse supernova (CCSN) and observational aspects of future detections of neutrinos from CCSN explosions are discussed. The other main focus in this text is the novel phases of dense nuclear matter, its compositions and equation of state (EoS) from low to very high baryon density relevant to supernovae and neutron stars. The multi-messenger astrophysics of binary neutron star merger GW170817 and its relation to EoS through tidal deformability are also presented in detail. The synthesis of elements heavier than iron in the supernova and neutron star environment by the rapid (r)-process are treated here with special emphasis on the nucleosynthesis in the ejected material from GW170817. This monograph is written for graduate students and researchers in the field of nuclear astrophysics |
ISBN,Price | 9783030951719 |
Keyword(s) | 1. ASTROPHYSICS
2. EBOOK
3. EBOOK - SPRINGER
4. MATHEMATICAL PHYSICS
5. NUCLEAR PHYSICS
6. Theoretical, Mathematical and Computational Physics
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Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12520 |
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On Shelf |
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30.
| ![No image available](./images/covers/NoCover.jpg) |
Title | General Relativity and Gravitational Waves : Essentials of Theory and Practice |
Author(s) | Dhurandhar, Sanjeev;Mitra, Sanjit |
Publication | Cham, 1. Imprint: Springer
2. Springer International Publishing, 2022. |
Description | XIV, 207 p. 32 illus., 16 illus. in color : online resource |
Abstract Note | This book serves as a textbook for senior undergraduate students who are learning the subject of general relativity and gravitational waves for the first time. Both authors have been teaching the course in various forms for a few decades and have designed the book as a one stop book at basic level including derivations and exercises. A spectacular prediction of general relativity is gravitational waves. Gravitational waves were first detected by the LIGO detectors in 2015, hundred years after their prediction. Both authors are part of the LIGO Science Collaboration and were authors on the discovery paper. Therefore, a strong motivation for this book is to provide the essential concepts of general relativity theory and gravitational waves with their modern applications to students and to researchers who are new to the multi-disciplinary field of gravitational wave astronomy. One of the advanced topics covered in this book is the fundamentals of gravitational wave data analysis, filling a gap in textbooks on general relativity. The topic blends smoothly with other chapters in the book not only because of the common area of research, but it uses similar differential geometric and algebraic tools that are used in general relativity |
ISBN,Price | 9783030923358 |
Keyword(s) | 1. ASTROPHYSICS
2. Classical and Quantum Gravity
3. EBOOK
4. EBOOK - SPRINGER
5. GENERAL RELATIVITY
6. GENERAL RELATIVITY (PHYSICS)
7. GRAVITATION
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Item Type | Book |
Multi-Media Links
Please Click here for eBook
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
I12501 |
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On Shelf |
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