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--- theoreticalbackground_cbc [2022/01/31 16:08]
theoastro [Neutron Stars]
+++ theoreticalbackground_cbc [2022/07/18 10:10] (current)
theoastro [Black Hole - Neutron Star Systems]
@@ Line 1: / Line 1: @@
-===== Theoretical Background =====
+==== Compact Binary Mergers ====
-==== Neutron Stars and Black Holes ====
+Numerous compact objects are bound inside binary systems, some of these, so-called compact binary systems are  either binary neutron  star systems (often also called double neutron star systems), black hole - neutron star systems, and binary black hole systems.
-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, nuclear forces enable neutron stars, which have slightly smaller masses than black holes, to be stable without a spacetime singularity. However, the density inside a neutron star exceeds any kind of density that we can realize here on earth and can reaches a few times nuclear saturation density, i.e., up to a few hundred tons per cubic centimeter.
+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. In the following, we will provide some additional information about
-==== Compact Binary Mergers ====
+  * **[[binary_neutron_stars|Binary Neutron Stars]]**
+  * **[[black_hole_neutron_star_binary|Black Hole - Neutron Star Binary]]**
-==== Binary Neutron Star Systems ====
-==== Black Hole - Neutron Star Systems ====

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