Neutron Stars: Theory and Observation:
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1991
|
| Schriftenreihe: | NATO ASI Series, Series C: Mathematical and Physical Sciences
344 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | 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 |
| Beschreibung: | 1 Online-Ressource (XI, 592 p) |
| ISBN: | 9789401135368 9789401055659 |
| ISSN: | 1389-2185 |
| DOI: | 10.1007/978-94-011-3536-8 |
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| 500 | |a 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 | ||
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Datensatz im Suchindex
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| dewey-ones | 523 - Specific celestial bodies and phenomena |
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| discipline | Physik |
| doi_str_mv | 10.1007/978-94-011-3536-8 |
| format | Electronic eBook |
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| spelling | Ventura, Joseph Verfasser aut Neutron Stars: Theory and Observation edited by Joseph Ventura, David Pines Proceedings of the NATO Advanced Study Institute on Neutron Stars: An Interdisciplinary Field, Agia Pelagia, Crete, Greece, September 3-14, 1990 Dordrecht Springer Netherlands 1991 1 Online-Ressource (XI, 592 p) txt rdacontent c rdamedia cr rdacarrier NATO ASI Series, Series C: Mathematical and Physical Sciences 344 1389-2185 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 Physics Astrophysics and Astroparticles Condensed Matter Physics Neutronenstern (DE-588)4171660-7 gnd rswk-swf 1\p (DE-588)1071861417 Konferenzschrift 1990 Ajia Pelagia Achlada gnd-content Neutronenstern (DE-588)4171660-7 s 2\p DE-604 Pines, David Sonstige oth https://doi.org/10.1007/978-94-011-3536-8 Verlag Volltext 1\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk 2\p cgwrk 20201028 DE-101 https://d-nb.info/provenance/plan#cgwrk |
| spellingShingle | Ventura, Joseph Neutron Stars: Theory and Observation Physics Astrophysics and Astroparticles Condensed Matter Physics Neutronenstern (DE-588)4171660-7 gnd |
| subject_GND | (DE-588)4171660-7 (DE-588)1071861417 |
| title | Neutron Stars: Theory and Observation |
| title_alt | Proceedings of the NATO Advanced Study Institute on Neutron Stars: An Interdisciplinary Field, Agia Pelagia, Crete, Greece, September 3-14, 1990 |
| title_auth | Neutron Stars: Theory and Observation |
| title_exact_search | Neutron Stars: Theory and Observation |
| title_full | Neutron Stars: Theory and Observation edited by Joseph Ventura, David Pines |
| title_fullStr | Neutron Stars: Theory and Observation edited by Joseph Ventura, David Pines |
| title_full_unstemmed | Neutron Stars: Theory and Observation edited by Joseph Ventura, David Pines |
| title_short | Neutron Stars: Theory and Observation |
| title_sort | neutron stars theory and observation |
| topic | Physics Astrophysics and Astroparticles Condensed Matter Physics Neutronenstern (DE-588)4171660-7 gnd |
| topic_facet | Physics Astrophysics and Astroparticles Condensed Matter Physics Neutronenstern Konferenzschrift 1990 Ajia Pelagia Achlada |
| url | https://doi.org/10.1007/978-94-011-3536-8 |
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