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Saturation of the f-mode Instability in Neutron Stars, Pantelis Pnigouras


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Автор: Pantelis Pnigouras
Название:  Saturation of the f-mode Instability in Neutron Stars
ISBN: 9783030074746
Издательство: Springer
Классификация:


ISBN-10: 3030074749
Обложка/Формат: Soft cover
Страницы: 220
Вес: 0.38 кг.
Дата издания: 2018
Серия: Springer Theses
Язык: English
Издание: Softcover reprint of
Иллюстрации: 21 illustrations, color; 10 illustrations, black and white; xxiii, 220 p. 31 illus., 21 illus. in color.
Размер: 234 x 156 x 13
Читательская аудитория: General (us: trade)
Основная тема: Physics
Ссылка на Издательство: Link
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Поставляется из: Германии
Описание: This book presents a study of the saturation of unstable f-modes (fundamental modes) due to low-order nonlinear mode coupling. Since their theoretical prediction in 1934, neutron stars have remained among the most challenging objects in the Universe. Gravitational waves emitted by unstable neutron star oscillations can be used to obtain information about their inner structure, that is, the equation of state of dense nuclear matter. After its initial growth phase, the instability is expected to saturate due to nonlinear effects. The saturation amplitude of the unstable mode determines the detectability of the generated gravitational-wave signal, but also affects the evolution of the neutron star. The study shows that the unstable (parent) mode resonantly couples to pairs of stable (daughter) modes, which drain the parent’s energy and make it saturate via a mechanism called parametric resonance instability. Further, it calculates the saturation amplitude of the most unstable f-mode multipoles throughout their so-called instability windows.
Дополнительное описание: Introduction.- The Oscillation Modes: Linear Perturbation Scheme.- The f-mode Instability.- Mode Coupling: Quadratic Perturbation Scheme.- Results.- Final Remarks.



Instability in Geophysical Flows

Автор: William D. Smyth, Jeffrey R. Carpenter
Название: Instability in Geophysical Flows
ISBN: 1108703011 ISBN-13(EAN): 9781108703017
Издательство: Cambridge Academ
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Цена: 9186.00 р.
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Описание: An Open Access overview of physical processes that generate instability in geophysical systems. It covers classical analytical approaches together with numerical methods for quick prediction of stability in a system. Including exercises and MATLAB (R) coding examples, it can be used for self-study or advanced courses in the environmental sciences.

Neutron Stars: Theory and Observation

Автор: J.E Ventura; David Pines
Название: Neutron Stars: Theory and Observation
ISBN: 0792313976 ISBN-13(EAN): 9780792313977
Издательство: Springer
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Цена: 46399.00 р.
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Описание: Proceedings of the NATO Advanced Study Institute on Neutron Stars: An Interdisciplinary Field, Agia Pelagia, Crete, Greece, September 3-14, 1990

Compact Objects in Astrophysics / White Dwarfs, Neutron Stars and Black Holes

Автор: Camenzind Max
Название: Compact Objects in Astrophysics / White Dwarfs, Neutron Stars and Black Holes
ISBN: 3540257705 ISBN-13(EAN): 9783540257707
Издательство: Springer
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Цена: 11878.00 р.
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Описание: Modern comprehensive introduction and overview of the physics of White Dwarfs, Neutron Stars and Black Holes, including all relevant observations. Contains a basic introduction to General Relativity, including the modern 3+1 split of spacetime and of Einstein`s equations.

Instability and Variability of Hot-Star Winds

Автор: Anthony F.J. Moffat; Stanley P. Owocki; Alex W. Fu
Название: Instability and Variability of Hot-Star Winds
ISBN: 9401041393 ISBN-13(EAN): 9789401041393
Издательство: Springer
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Цена: 6986.00 р.
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Описание: Proceedings of an International Workshop held at Isle-aux-Coudres, Quebec Province, Canada, August 23--27, 1993

Neutron Stars, Black Holes, and Gravitational Waves

Автор: James J Kolata
Название: Neutron Stars, Black Holes, and Gravitational Waves
ISBN: 1643274236 ISBN-13(EAN): 9781643274232
Издательство: Mare Nostrum (Eurospan)
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Цена: 8593.00 р.
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Описание: Albert Einstein's General Theory of Relativity, published in 1915, made a remarkable prediction: gravitational radiation. Just like light (electromagnetic radiation), gravity could travel through space as a wave and affect any objects it encounters by alternately compressing and expanding them. However, there was a problem. The force of gravity is around a trillion, trillion, trillion times weaker than electromagnetism so the calculated compressions and expansions were incredibly small, even for gravity waves resulting from a catastrophic astrophysical event such as a supernova explosion in our own galaxy. Discouraged by this result, physicists and astronomers didn't even try to detect these tiny, tiny effects for over 50 years. Then, in the late 1960s and early 1970s, two events occurred which started the hunt for gravity waves in earnest. The first was a report of direct detection of gravity waves thousands of times stronger than even the most optimistic calculation. Though ultimately proved wrong, this result started scientists thinking about what instrumentation might be necessary to detect these waves. The second was an actual, though indirect, detection of gravitational radiation due to the effects it had on the period of rotation of two 'neutron stars' orbiting each other. In this case, the observations were in exact accord with predictions from Einstein's theory, which confirmed that a direct search might ultimately be successful. Nevertheless, it took another 40 years of development of successively more sensitive detectors before the first real direct effects were observed in 2015, 100 years after gravitational waves were first predicted. This is the story of that hunt, and the insight it is producing into an array of topics in modern science, from the creation of the chemical elements to insights into the properties of gravity itself.

Neutron Stars, Black Holes, and Gravitational Waves

Автор: Kolata James J.
Название: Neutron Stars, Black Holes, and Gravitational Waves
ISBN: 1643274198 ISBN-13(EAN): 9781643274195
Издательство: Mare Nostrum (Eurospan)
Цена: 5405.00 р.
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Описание: Albert Einstein's General Theory of Relativity, published in 1915, made a remarkable prediction: gravitational radiation. Just like light (electromagnetic radiation), gravity could travel through space as a wave and affect any objects it encounters by alternately compressing and expanding them. However, there was a problem. The force of gravity is around a trillion, trillion, trillion times weaker than electromagnetism so the calculated compressions and expansions were incredibly small, even for gravity waves resulting from a catastrophic astrophysical event such as a supernova explosion in our own galaxy. Discouraged by this result, physicists and astronomers didn't even try to detect these tiny, tiny effects for over 50 years. Then, in the late 1960s and early 1970s, two events occurred which started the hunt for gravity waves in earnest. The first was a report of direct detection of gravity waves thousands of times stronger than even the most optimistic calculation. Though ultimately proved wrong, this result started scientists thinking about what instrumentation might be necessary to detect these waves. The second was an actual, though indirect, detection of gravitational radiation due to the effects it had on the period of rotation of two 'neutron stars' orbiting each other. In this case, the observations were in exact accord with predictions from Einstein's theory, which confirmed that a direct search might ultimately be successful. Nevertheless, it took another 40 years of development of successively more sensitive detectors before the first real direct effects were observed in 2015, 100 years after gravitational waves were first predicted. This is the story of that hunt, and the insight it is producing into an array of topics in modern science, from the creation of the chemical elements to insights into the properties of gravity itself.

Saturation of the f-mode Instability in Neutron Stars

Автор: Pantelis Pnigouras
Название: Saturation of the f-mode Instability in Neutron Stars
ISBN: 3319982575 ISBN-13(EAN): 9783319982571
Издательство: Springer
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Цена: 13974.00 р.
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Описание: This book presents a study of the saturation of unstable f-modes (fundamental modes) due to low-order nonlinear mode coupling. Since their theoretical prediction in 1934, neutron stars have remained among the most challenging objects in the Universe. Gravitational waves emitted by unstable neutron star oscillations can be used to obtain information about their inner structure, that is, the equation of state of dense nuclear matter. After its initial growth phase, the instability is expected to saturate due to nonlinear effects. The saturation amplitude of the unstable mode determines the detectability of the generated gravitational-wave signal, but also affects the evolution of the neutron star. The study shows that the unstable (parent) mode resonantly couples to pairs of stable (daughter) modes, which drain the parent’s energy and make it saturate via a mechanism called parametric resonance instability. Further, it calculates the saturation amplitude of the most unstable f-mode multipoles throughout their so-called instability windows.

Neutron Stars and Their Birth Events

Автор: Wolfgang Kundt
Название: Neutron Stars and Their Birth Events
ISBN: 940106718X ISBN-13(EAN): 9789401067188
Издательство: Springer
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Цена: 12157.00 р.
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Описание: Proceedings of the NATO Advanced Study Institute on Neutron Stars: Their Birth, Evolution, Radiation and Winds, Erice, Sicily, Italy, September 5-17, 1988

The Electromagnetic Spectrum of Neutron Stars

Автор: Altan Baykal; Sinan K. Yerli; Sitki C. Inam; Serge
Название: The Electromagnetic Spectrum of Neutron Stars
ISBN: 1402038607 ISBN-13(EAN): 9781402038600
Издательство: Springer
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Цена: 18167.00 р.
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Описание: Neutron stars possess the highest rotation rates and strongest magnetic fields among all stars. This volume includes spectral information from the neutron stars, namely neutrino and gravitational radiation along with the electromagnetic spectrum. It serves as graduate level of text including the range of properties of neutron stars.

Neutron Stars 1

Автор: P. Haensel; A.Y. Potekhin; D.G. Yakovlev
Название: Neutron Stars 1
ISBN: 1441922148 ISBN-13(EAN): 9781441922144
Издательство: Springer
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Цена: 15672.00 р.
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Описание: The book gives an extended review of theoretical and observational aspects of neutron star physics. It describes all layers of neutron stars, from the surface to the core, with the emphasis on their structure and equation of state.

Physics and astrophysics of neutron stars

Название: Physics and astrophysics of neutron stars
ISBN: 331997615X ISBN-13(EAN): 9783319976150
Издательство: Springer
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Цена: 25155.00 р.
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Описание: This book summarizes the recent progress in the physics and astrophysics of neutron stars and, most importantly, it identifies and develops effective strategies to explore, both theoretically and observationally, the many remaining open questions in the field.Because of its significance in the solution of many fundamental questions in nuclear physics, astrophysics and gravitational physics, the study of neutron stars has seen enormous progress over the last years and has been very successful in improving our understanding in these fascinating compact objects.The book addresses a wide spectrum of readers, from students to senior researchers. Thirteen chapters written by internationally renowned experts offer a thorough overview of the various facets of this interdisciplinary science, from neutron star formation in supernovae, pulsars, equations of state super dense matter, gravitational wave emission, to alternative theories of gravity.The book was initiated by the European Cooperation in Science and Technology (COST) Action MP1304 “Exploring fundamental physics with compact stars” (NewCompStar).

The Electromagnetic Spectrum of Neutron Stars

Автор: Altan Baykal; Sinan K. Yerli; Sitki C. Inam; Serge
Название: The Electromagnetic Spectrum of Neutron Stars
ISBN: 1402038593 ISBN-13(EAN): 9781402038594
Издательство: Springer
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Цена: 43184.00 р.
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Описание: Features the lectures presented in the 6th NATO-ASI series entitled in Marmaris, Turkey, on 7-18 June 2004. This volume includes information from the neutron stars, namely neutrino and gravitational radiation along with the electromagnetic spectrum. It serves as a graduate level text including the range of properties of neutron stars.


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