Saturation of the f-mode Instability in Neutron Stars
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 s...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | Englisch |
| Veröffentlicht: |
Cham :
Springer International Publishing,
2018.
|
| Ausgabe: | 1st ed. 2018. |
| Schriftenreihe: | Springer Theses, Recognizing Outstanding Ph.D. Research,
|
| Schlagworte: | |
| ISBN: | 9783319982588 |
| ISSN: | 2190-5053 |
| Online-Zugang: |
|
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
MARC
| LEADER | 00000nam a22000005i 4500 | ||
|---|---|---|---|
| 003 | SK-BrCVT | ||
| 005 | 20220618101716.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 180925s2018 gw | s |||| 0|eng d | ||
| 020 | |a 9783319982588 | ||
| 024 | 7 | |a 10.1007/978-3-319-98258-8 |2 doi | |
| 035 | |a CVTIDW13825 | ||
| 040 | |a Springer-Nature |b eng |c CVTISR |e AACR2 | ||
| 041 | |a eng | ||
| 100 | 1 | |a Pnigouras, Pantelis. |4 aut | |
| 245 | 1 | 0 | |a Saturation of the f-mode Instability in Neutron Stars |h [electronic resource] / |c by Pantelis Pnigouras. |
| 250 | |a 1st ed. 2018. | ||
| 260 | 1 | |a Cham : |b Springer International Publishing, |c 2018. | |
| 300 | |a XXIII, 220 p. 31 illus., 21 illus. in color. |b online resource. | ||
| 490 | 1 | |a Springer Theses, Recognizing Outstanding Ph.D. Research, |x 2190-5053 | |
| 500 | |a Physics and Astronomy | ||
| 505 | 0 | |a Introduction -- The Oscillation Modes: Linear Perturbation Scheme -- The f-mode Instability -- Mode Coupling: Quadratic Perturbation Scheme -- Results -- Final Remarks. | |
| 516 | |a text file PDF | ||
| 520 | |a 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. | ||
| 650 | 0 | |a Astrophysics. | |
| 650 | 0 | |a Mathematical physics. | |
| 856 | 4 | 0 | |u http://hanproxy.cvtisr.sk/han/cvti-ebook-springer-eisbn-978-3-319-98258-8 |y Vzdialený prístup pre registrovaných používateľov |
| 910 | |b ZE11105 | ||
| 919 | |a 978-3-319-98258-8 | ||
| 974 | |a andrea.lebedova |f Elektronické zdroje | ||
| 992 | |a SUD | ||
| 999 | |c 238147 |d 238147 | ||