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theoreticalbackground_cbc [2022/02/01 11:49] theoastro [Binary Neutron Star Systems] |
theoreticalbackground_cbc [2022/07/18 10:10] (current) theoastro [Black Hole - Neutron Star Systems] |
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- | ===== Theoretical Background ===== | ||
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- | ==== Neutron Stars and Black Holes ==== | ||
- | Neutron stars and black holes are possible end states of the stellar evolution for massive stars. While the gravitational forces within black holes are so large that the entire material gets compressed within the central singularity, | ||
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==== Compact Binary Mergers ==== | ==== Compact Binary Mergers ==== | ||
Numerous compact objects are bound inside binary systems, some of these, so-called compact binary systems are either binary neutron | Numerous compact objects are bound inside binary systems, some of these, so-called compact binary systems are either binary neutron | ||
- | On top of these, well-established scenarios, there is also the possibility for the existence of exotic compact objects that also could be bound inside compact binaries. | + | On top of these, well-established scenarios, there is also the possibility for the existence of exotic compact objects that also could be bound inside compact binaries. |
- | ==== Binary Neutron Star Systems ==== | + | |
+ | * **[[binary_neutron_stars|Binary | ||
+ | * **[[black_hole_neutron_star_binary|Black Hole - Neutron Star Binary]]** | ||
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- | A system consisting of two neutron stars is called a binary neutron star or a double neutron star system. Numerous of these systems exist and have been observed through electromagnetic observations. Among the best well-known system, we have the Hulse-Taylor Pulsar. | ||
- | ==== Black Hole - Neutron Star Systems ==== |
Last modified: le 2022/02/01 11:49