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Author | Title | Accn# | Year | Item Type | Claims |
11 |
James P. Lavine |
Time-Dependent quantum mechanics of two-level systems |
026713 |
2019 |
Book |
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12 |
BURROWS, DAVID N. (ED.) |
WSPC handbook of astronomical instrumentation |
|
2020 |
Book |
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13 |
Michael M. Woolfson |
About stars: Their Formation, Evolution, Compositions, Locations and Companions |
026586 |
202 |
Book |
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14 |
Serge Parnovsky |
How the universe works: Introduction to Modern Cosmology |
026587 |
2018 |
Book |
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15 |
Hiroshi Isozaki |
Maxwell equation: Inverse Scattering in Electromagnetis |
026588 |
2018 |
Book |
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16 |
Maurizio Consoli |
Michelson-Morley experiments: An Enigma for Physics and the History of Science |
026589 |
2019 |
Book |
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17 |
Elke Pilat-Lohinger |
Planetary habitability in binary systems |
026590 |
2019 |
Book |
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18 |
CTA Consortium |
Science with the Cherenkov telescope array |
026591 |
2019 |
Book |
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19 |
Mahendra K Verma |
Physics of buoyant flows: From Instabilities to Turbulence |
026392 |
2018 |
Book |
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20 |
Rotation and accretion powered pulsars |
Rotation and accretion powered pulsars |
OB1306 |
2018 |
eBook |
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13.
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Title | About stars: Their Formation, Evolution, Compositions, Locations and Companions |
Author(s) | Michael M. Woolfson |
Publication | New Jersey, World Scientific Publishing Co. Pvt. Ltd., 202. |
Description | xviii, 368p. |
Abstract Note | On a clear and moonless night, especially in remote areas such as deserts, myriads of points of light cover the sky. The great majority of them are stars, many like the Sun, but so far away that they can only be seen as point sources of light. The problem faced by astronomers is to find their properties and distances, just from the light they emit. This is done by using the knowledge of science, mainly physics, acquired from small-scale experiments carried out on Earth. However, the stars themselves are laboratories in which matter behaves in ways that cannot be reproduced on Earth so, in finding out about stars, we complement scientific knowledge gained from earthbound experimentation. |
ISBN,Price | 9781786347251 : $ 38.00(PB) |
Classification | 524.3
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Keyword(s) | 1. CAPTURE THEORY
2. DISTANCE OF STARS
3. EVOLUTION OF STARS
4. EXOPLANETS
5. FORMATION OF STARS
6. NEBULA THEORY
7. STARS
8. STARS - COMPOSITIONS
9. STARS - PROPERTIES
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Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
026586 |
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524.3/WOO/026586 |
On Shelf |
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14.
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Title | How the universe works: Introduction to Modern Cosmology |
Author(s) | Serge Parnovsky;Aleksei Parnowski |
Publication | New Jersey, World Scientific Publishing Co. Pvt. Ltd., 2018. |
Description | xxii, 163p. |
Abstract Note | This book is about the history and the current state of the art in the exciting field of cosmology — the science about the Universe as a whole, which is guaranteed to attract the attention of a wide range of readers. It mostly aims to explain the main ideas of modern cosmology: the expanding Universe, its creation in a Big Bang, its evolution, characteristics, and structure, as well as issues — dark matter and dark energy, black holes and other exotic objects etc. It also answers most frequently asked questions about cosmology. |
ISBN,Price | 9789813234949 : $ 58.00(HB) |
Classification | 524.8
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Keyword(s) | 1. BIG BANG
2. BLACK HOLE
3. COSMOLOGY
4. DARK ENERGY
5. DARK MATTER
6. UNIVERSE
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Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
026587 |
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524.8/PAR/026587 |
On Shelf |
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15.
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Title | Maxwell equation: Inverse Scattering in Electromagnetis |
Author(s) | Hiroshi Isozaki |
Publication | New Jersey, World Scientific Publishing Co. Pvt. Ltd., 2018. |
Description | xv,283p. |
Abstract Note | How can one determine the physical properties of the medium or the geometrical properties of the domain by observing electromagnetic waves? To answer this fundamental problem in mathematics and physics, this book leads the reader to the frontier of inverse scattering theory for electromagnetism.
The first three chapters, written comprehensively, can be used as a textbook for undergraduate students. Beginning with elementary vector calculus, this book provides fundamental results for wave equations and Helmholtz equations, and summarizes the potential theory. It also explains the cohomology theory in an easy and straightforward way, which is an essential part of electromagnetism related to geometry. It then describes the scattering theory for the Maxwell equation by the time-dependent method and also by the stationary method in a concise, but almost self-contained manner. Based on these preliminary results, the book proceeds to the inverse problem for the Maxwell equation.
The chapters for the potential theory and elementary cohomology theory are good introduction to graduate students. The results in the last chapter on the inverse scattering for the medium and the determination of Betti numbers are new, and will give a current scope for the inverse spectral problem on non-compact manifolds. It will be useful for young researchers who are interested in this field and trying to find new problems. |
ISBN,Price | 9789813232693 : $ 118.00(HB) |
Classification | 537.8
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Keyword(s) | 1. COHOMOLOGY
2. MAXWELL EQUATION
3. POTENTIAL THEORY
4. SCATTERING THEORY
5. VECTOR CALCULUS
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Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
026588 |
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537.8/ISO/026588 |
On Shelf |
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16.
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Title | Michelson-Morley experiments: An Enigma for Physics and the History of Science |
Author(s) | Maurizio Consoli;Alessandro Pluchino |
Publication | New Jersey, World Scientific Publishing Co. Pvt. Ltd., 2019. |
Description | xii, 181p. |
Abstract Note | In 1887, Michelson and Morley tried to observe in laboratory the "ether drift" by measuring a small difference in the velocity of two perpendicular light beams. The result of their measurements, however, was much smaller than the classical prediction and interpreted as a "null result". This was crucial to stimulate the first pioneering formulations of relativity and, as such, it represents a fundamental step in the history of science. Since then, many repetitions of that original experiment have been performed with better and better sensitivity and the standard conclusion has been always the same: no genuine ether drift has ever been detected. However, in the authors' new scheme, the small irregular residuals observed in laboratory show surprising correlations with the direct observations of the Cosmic Microwave Background (CMB) with satellites in space. This opens the possibility of finally linking the CMB to a fundamental reference frame for relativity, with substantial implications for the interpretation of non-locality in the quantum theory. The importance of the issue would require new dedicated experimental tests and significant improvements in the data analysis. Otherwise, without such more stringent checks, these crucial experiments will remain forever as an enigma for physics and the history of science. The book illustrates the many facets of this research together with historical accounts on some leading scientists involved in these measurements. |
ISBN,Price | 9789813278189 : $ 78.00(HB) |
Classification | 535
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Keyword(s) | 1. MICHELSON-MORLEY EXPERIMENT
2. PHYSICS
3. SCIENCE - HISTORY
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Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
026589 |
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535/CON/026589 |
On Shelf |
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17.
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Title | Planetary habitability in binary systems |
Author(s) | Elke Pilat-Lohinger;Siegfried Eggl;Akos Bazso |
Publication | New Jersey, World Scientific Publishing Co. Pvt. Ltd., 2019. |
Description | xix, 181p. |
Abstract Note | Astrophysical research has led to the detection of thousands of planets outside the Solar System. About one-tenth of the extrasolar planets discovered so far reside in binary- or multi-stellar systems, and some of the closest known rocky exoplanets populate these multiple-star systems. While such environments seem good places to look for a second Earth, can Earth-like planets with two or more suns be habitable? And do solar system-like configurations have to be detected to find a habitable exo-Earth?
This book addresses these questions. Starting with a brief overview of the various types of double star–planet configurations that have been observed so far, the book discusses the intriguing variety of planetary motion in such environments, taking into account the stellar type, evolution, and activity, and elaborates on how the presence of an additional stellar companion affects planet formation, system architectures and the habitability of planets in binary star systems. New methodologies developed in this area of research are explained and demonstrated for systems such as Alpha-Centauri, HD41004, Kepler-35, and many others. This monograph provides a grand entry to the exciting results that we expect from new missions like TESS, CHEOPS and Plato. |
ISBN,Price | 9789813275126 : $ 88.00(HB) |
Classification | 524.38
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Keyword(s) | 1. BINARY STARS
2. DOUBLE STARS
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Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
026590 |
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524.38/PIL/026590 |
On Shelf |
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19.
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Title | Physics of buoyant flows: From Instabilities to Turbulence |
Author(s) | Mahendra K Verma |
Publication | Singapore, World Scientific Publishing Co. Pvt. Ltd., 2018. |
Description | xxiv, 327p. |
Abstract Note | Gravity pervades the whole universe; hence buoyancy drives fluids everywhere including those in the atmospheres and interiors of planets and stars. Prime examples of such flows are mantle convection, atmospheric flows, solar convection, dynamo process, heat exchangers, airships and hot air balloons. In this book we present fundamentals and applications of thermal convection and stratified flows.
Buoyancy brings in extremely rich phenomena including waves and instabilities, patterns, chaos, and turbulence. In this book we present these topics in a systematic manner. First we present a unified treatment of linear theory that yields waves and thermal instability for stably and unstably-stratified flows respectively. We extend this analysis to include rotation and magnetic field. We also describe nonlinear saturation and pattern formation in Rayleigh–Bénard convection.
The second half of the book is dedicated to buoyancy-driven turbulence, both in stably-stratified flow and in thermal convection. We describe the spectral theory including energy flux and show that the thermally-driven turbulence is similar to hydrodynamic turbulence. We also describe large-scale quantities like Reynolds and Nusselt numbers, flow anisotropy, and the dynamics of flow structures, namely flow reversals. Thus, this book presents all the major aspects of the buoyancy-driven flows in a coherent manner that would appeal to advanced graduate students and researchers. |
ISBN,Price | 9789813237797 : $ 118.00(HB) |
Classification | 532.5
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Keyword(s) | 1. BUOYANCY-DRIVEN TURBULENCE
2. RAYLEIGH-BENARD
3. ROTATING FLOWS
4. TURBULENT BOUYANT FLOWS
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Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
026392 |
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532.5/VER/026392 |
On Shelf |
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