Neutron Stars Theory And Observation

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Neutron Stars: Theory and Observation

Author : J.E Ventura,David Pines
Publisher : Springer Science & Business Media
Page : 590 pages
File Size : 41,7 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789401135368

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Neutron Stars: Theory and Observation by J.E Ventura,David Pines Pdf

Some twenty-three years after the discovery of pulsars and their identification as rotating neutron stars, neutron star physics may be regarded as comingofage. Pul sars and accreting neutron stars have now been studied at every wavelength, from the initial radio observations, through optical, X-, and "{-ray, up to the very recent observations in the TeV region, while theorists have studied in some detail relevant physical processes both outside and inside neutron stars. As a result, comparisonof theory with observation provides a test ofour theoretical ideas in fields as diverse as neutron and nuclear matter, superfluidity and superconductivity, the acceleration of high energy particles, and the generation and maintenance of intense magnetic fields. For example, through observations of glitches and post glitch behavior of pulsars, it has become possible to establish the presence ofsuperfluid neutron mat ter in the inner crust of neutron stars, and to determine some of its properties, while neutron stars in compact binary systems offer one ofthe most efficient energy generation mechanisms known. It is in fact the interactive interpretation of these ,diverse pieces of information that can lead to major advances in our understanding of the physics of these exotic objects, and justifies the characterization of neutron stars as hadron physics laboratories.

Neutron Stars and Pulsars

Author : Werner Becker
Publisher : Springer Science & Business Media
Page : 702 pages
File Size : 49,6 Mb
Release : 2009-02-11
Category : Science
ISBN : 9783540769651

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Neutron Stars and Pulsars by Werner Becker Pdf

Neutron stars are the most compact astronomical objects in the universe which are accessible by direct observation. Studying neutron stars means studying physics in regimes unattainable in any terrestrial laboratory. Understanding their observed complex phenomena requires a wide range of scientific disciplines, including the nuclear and condensed matter physics of very dense matter in neutron star interiors, plasma physics and quantum electrodynamics of magnetospheres, and the relativistic magneto-hydrodynamics of electron-positron pulsar winds interacting with some ambient medium. Not to mention the test bed neutron stars provide for general relativity theories, and their importance as potential sources of gravitational waves. It is this variety of disciplines which, among others, makes neutron star research so fascinating, not only for those who have been working in the field for many years but also for students and young scientists. The aim of this book is to serve as a reference work which not only reviews the progress made since the early days of pulsar astronomy, but especially focuses on questions such as: "What have we learned about the subject and how did we learn it?", "What are the most important open questions in this area?" and "What new tools, telescopes, observations, and calculations are needed to answer these questions?". All authors who have contributed to this book have devoted a significant part of their scientific careers to exploring the nature of neutron stars and understanding pulsars. Everyone has paid special attention to writing educational comprehensive review articles with the needs of beginners, students and young scientists as potential readers in mind. This book will be a valuable source of information for these groups.

Neutron Stars 1

Author : P. Haensel,A.Y. Potekhin,D.G. Yakovlev
Publisher : Springer Science & Business Media
Page : 633 pages
File Size : 46,5 Mb
Release : 2007-12-06
Category : Science
ISBN : 9780387473017

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Neutron Stars 1 by P. Haensel,A.Y. Potekhin,D.G. Yakovlev Pdf

The book gives an extended review of theoretical and observational aspects of neutron star physics. With masses comparable to that of the Sun and radii of about ten kilometres, neutron stars are the densest stars in the Universe. This book describes all layers of neutron stars, from the surface to the core, with the emphasis on their structure and equation of state. Theories of dense matter are reviewed, and used to construct neutron star models. Hypothetical strange quark stars and possible exotic phases in neutron star cores are also discussed. Also covered are the effects of strong magnetic fields in neutron star envelopes.

Isolated Neutron Stars: From the Surface to the Interior

Author : Silvia Zane,Roberto Turolla,Dany Page
Publisher : Springer Science & Business Media
Page : 654 pages
File Size : 40,7 Mb
Release : 2007-05-22
Category : Science
ISBN : 9781402059988

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Isolated Neutron Stars: From the Surface to the Interior by Silvia Zane,Roberto Turolla,Dany Page Pdf

This book is a collation of the contributions presented at a major conference on isolated neutron stars held in London in April 2006. Forty years after the discovery of radio pulsars it presents an up-to-date description of the new vision of isolated neutron stars that has emerged in recent years. The great variety of isolated neutron stars, from pulsars to magnetars, is well covered by descriptions of recent observational results and presentations of the latest theoretical interpretation of these data.

Timing Neutron Stars: Pulsations, Oscillations and Explosions

Author : Tomaso M. Belloni,Mariano Méndez,Chengmin Zhang
Publisher : Springer Nature
Page : 335 pages
File Size : 53,5 Mb
Release : 2020-10-23
Category : Science
ISBN : 9783662621103

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Timing Neutron Stars: Pulsations, Oscillations and Explosions by Tomaso M. Belloni,Mariano Méndez,Chengmin Zhang Pdf

Neutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray burts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability.

The Electromagnetic Spectrum of Neutron Stars

Author : Altan Baykal,Sinan K. Yerli,Sitki C. Inam,Sergei Grebenev
Publisher : Springer Science & Business Media
Page : 383 pages
File Size : 43,5 Mb
Release : 2006-01-20
Category : Science
ISBN : 9781402038617

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The Electromagnetic Spectrum of Neutron Stars by Altan Baykal,Sinan K. Yerli,Sitki C. Inam,Sergei Grebenev Pdf

Neutron stars hold a central place in astrophysics, not only because they are made up of the most extreme states of the condensed matter, but also because they are, along with white dwarfs and black holes, one of the stable configurations that stars reach at the end of stellar evolution. Neutron stars posses the highest rotation rates and strongest magnetic fields among all stars. They radiate prolifically, in high energy electromagnetic radiation and in the radio band. This book is devoted to the selected lectures presented in the 6th NATO-ASI series entitled "The Electromagnetic Spectrum of Neutron Stars" in Marmaris, Turkey, on 7-18 June 2004. This ASI is devoted to the spectral properties of neutron stars. Spectral observations of neutron stars help us to understand the magnetospheric emission processes of isolated radio pulsars and the emission processes of accreting neutron stars. This volume includes spectral information from the neutron stars in broadest sense, namely neutrino and gravitational radiation along with the electromagnetic spectrum. We believe that this volume can serve as graduate level of text including the broad range of properties of neutron stars.

Theory of Neutron Star Magnetospheres

Author : F. Curtis Michel
Publisher : University of Chicago Press
Page : 548 pages
File Size : 47,5 Mb
Release : 1991
Category : Science
ISBN : 0226523314

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Theory of Neutron Star Magnetospheres by F. Curtis Michel Pdf

An incomparable reference for astrophysicists studying pulsars and other kinds of neutron stars, Theory of Neutron Star Magnetospheres sums up two decades of astrophysical research. It provides in one volume the most important findings to date on this topic, essential to astrophysicists faced with a huge and widely scattered literature. F. Curtis Michel, who was among the first theorists to propose a neutron star model for radio pulsars, analyzes competing models of pulsars, radio emission models, winds and jets from pulsars, pulsating X-ray sources, gamma-ray burst sources, and other neutron-star driven phenomena. Although the book places primary emphasis on theoretical essentials, it also provides a considerable introduction to the observational data and its organization. Michel emphasizes the problems and uncertainties that have arisen in the research as well as the considerable progress that has been made to date.

Neutron Stars, Black Holes and Binary X-Ray Sources

Author : H. Gursky,Remo Ruffini
Publisher : Springer Science & Business Media
Page : 447 pages
File Size : 47,8 Mb
Release : 2013-04-17
Category : Science
ISBN : 9789401017671

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Neutron Stars, Black Holes and Binary X-Ray Sources by H. Gursky,Remo Ruffini Pdf

This book contains a set of articles based on a session of the annual meeting of the American Association for the Advancement of Science held in San Francisco in February, 1974. The reason for the meeting arose from the need to communicate to the largest possible scientific community the dramatic advances which have been made in recent years in the understanding of collapsed objects: neutron stars and black holes. Thanks to an unprecedented resonance between X-ray, y-ray, radio and optical astronomy and important new theoretical developments in relativistic astro physics, a new deep understanding has been acquired of the physical processes oc curring in the late stages of evolution of stars. This knowledge may be one of the greatest conquests of man's understanding of nature in this century. This book aims to give an essential and up-to-date view in this field. The analysis of the physics and astrophysics of neutron stars and black holes is here attacked from both theoretical and experimental points of view. In the experimental field we range from the reviews and catalogues of galactic X-ray sources (R. Gursky and E. Schreier) and pulsars (E. Groth) to the observations of the optical counter part of X-ray sources (P. Boynton) to finally the recently discovered gamma-ray bursts (I. Strong) and pulse astronomy R. B. Partridge).

The Physics and Astrophysics of Neutron Stars

Author : Luciano Rezzolla,Pierre Pizzochero,David Ian Jones,Nanda Rea,Isaac Vidaña
Publisher : Springer
Page : 811 pages
File Size : 42,5 Mb
Release : 2019-01-09
Category : Science
ISBN : 9783319976167

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The Physics and Astrophysics of Neutron Stars by Luciano Rezzolla,Pierre Pizzochero,David Ian Jones,Nanda Rea,Isaac Vidaña Pdf

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).

Physics of Neutron Star Interiors

Author : D. Blaschke,N.K. Glendenning,A. Sedrakian
Publisher : Springer Science & Business Media
Page : 521 pages
File Size : 45,7 Mb
Release : 2001-11-20
Category : Science
ISBN : 9783540423409

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Physics of Neutron Star Interiors by D. Blaschke,N.K. Glendenning,A. Sedrakian Pdf

Neutron stars are the densest observable bodies in our universe. Born during the gravitational collapse of luminous stars - a birth heralded by spectacular supernova explosions - they open a window on a world where the state of the matter and the strengths of the fields are anything but ordinary. This book is a collection of pedagogical lectures on the theory of neutron stars, and especially their interiors, at the forefront of current research. It addresses graduate students and researchers alike, and should be particularly suitable as a text bridging the gap between standard textbook material and the research literature.

Neutron Stars and Their Birth Events

Author : Wolfgang Kundt
Publisher : Springer Science & Business Media
Page : 343 pages
File Size : 46,9 Mb
Release : 2012-12-06
Category : Science
ISBN : 9789400905153

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Neutron Stars and Their Birth Events by Wolfgang Kundt Pdf

This volume is the documentation of the second Course on 'Neutron Stars, Active Galactic Nuclei and Jets', held at Erice in September 1988. This second Course was devoted to our knowledge about neutron-star sources. The poster spoke of: pulsars, accreting X-ray sources and jet englnes, perhaps also UHE pulsars, X ra~' bursters and black-hole candidat.es. Neutron stars have even been proposed as the primary cosmic-ray boosters. Most of theil' properties are stil1 controversial, such as their birth mechanism (neutrino versus magnetic piston), internal structure (neutrons, quarks, strange particles), magnetic, thermal and spin histories, wind generation (hydrogen versus pair plasma, radiation versus centrifugal pressure), magnetospheric structure and accretion modes (along field lines versus quasi-Keplerian). The listed controversies have largely survived through the Course and entered into the proceedings. Several lecturers speak of 'magnetic-field decay' in neutron stars, of the 'recycling' of old pulsars, and of 'accretion-induced collapse' of white dwarfs as though such processes were textbook knowledge. Terms and abbreviations like RPSR (=recycled pulsar), spinup line, AIC, and ADC (=accretion disk corona) help to foster the assumptions. It is not clear to me at this time whether any of these notions has an application to reality.

High-Energy Radiation from Magnetized Neutron Stars

Author : Peter Mészáros
Publisher : University of Chicago Press
Page : 550 pages
File Size : 52,7 Mb
Release : 1992-06
Category : Science
ISBN : 0226520943

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High-Energy Radiation from Magnetized Neutron Stars by Peter Mészáros Pdf

Neutron stars, the most extreme state of matter yet confirmed, are responsible for much of the high-energy radiation detected in the universe. Mèszàros provides a general overview of the physics of magnetized neutron stars, discusses in detail the radiation processes and transport properties relevant to the production and propagation of high-energy radiation in the outer layers of these objects, and reviews the observational properties and theoretical models of various types of neutron star sources.

Compact Stars

Author : Norman K. Glendenning
Publisher : Springer Science & Business Media
Page : 402 pages
File Size : 49,6 Mb
Release : 2012-12-06
Category : Science
ISBN : 9781468404913

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Compact Stars by Norman K. Glendenning Pdf

A whole decades research collated, organised and synthesised into one single book! Following a 60-page review of the seminal treatises of Misner, Thorne, Wheeler and Weinberg on general relativity, Glendenning goes on to explore the internal structure of compact stars, white dwarfs, neutron stars, hybrids, strange quark stars, both the counterparts of neutron stars as well as of dwarfs. This is a self-contained treatment and will be of interest to graduate students in physics and astrophysics as well as others entering the field.

The Diversity of Neutron Stars

Author : David L. Kaplan
Publisher : Universal-Publishers
Page : 284 pages
File Size : 44,7 Mb
Release : 2004
Category : Business & Economics
ISBN : 9781581122343

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The Diversity of Neutron Stars by David L. Kaplan Pdf

Neutron stars are invaluable tools for exploring stellar death, the physics of ultra-dense matter, and the effects of extremely strong magnetic fields. The observed population of neutron stars is dominated by the >1000 radio pulsars, but there are distinct sub-populations that, while fewer in number, can have significant impact on our understanding of the issues mentioned above. These populations are the nearby, isolated neutron stars discovered by ROSAT, and the central compact objects in supernova remnants. The studies of both of these populations have been greatly accelerated in recent years through observations with the Chandra X-ray Observatory and the XMM-Newton telescope. First, we discuss radio, optical, and X-ray observations of the nearby neutron stars aimed at determining their relation to the Galactic neutron star population and at unraveling their complex physical processes by determining the basic astronomical parameters that define the population---distances, ages, and magnetic fields---the uncertainties in which limit any attempt to derive basic physical parameters for these objects. We conclude that these sources are 1e6 year-old cooling neutron stars with magnetic fields above 1e13 Gauss. Second, we describe the hollow supernova remnant problem: why many of the supernova remnants in the Galaxy have no indication of central neutron stars. We have undertaken an X-ray census of neutron stars in a volume-limited sample of Galactic supernova remnants, and from it conclude that either many supernovae do not produce neutron stars contrary to expectation, or that neutron stars can have a wide range in cooling behavior that makes many sources disappear from the X-ray sky.

Reassessing the Fundamentals: On the Evolution, Ages and Masses of Neutron Stars

Author : Bülent Kiziltan
Publisher : Universal-Publishers
Page : 135 pages
File Size : 50,5 Mb
Release : 2011-07-19
Category : Electronic
ISBN : 9781612337654

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Reassessing the Fundamentals: On the Evolution, Ages and Masses of Neutron Stars by Bülent Kiziltan Pdf

The evolution, ages and masses of neutron stars are the fundamental threads that make pulsars accessible to other sub-disciplines of astronomy and physics. a realistic and accurate determination of these indirectly probed features play an important role i