A Neutron Star is an extremely compact star with a mass of 1-2 solar masses and a radius of only 10 - 20 km. In general, there is an upper limit for the mass of a Neutron Star. But a fast rotating Neutron Star can be heavier than a slow rotating one. Due to its rotation the Neutron Star is deformed, its circumference is larger at its equator. Additionally, the rotation causes a moment of inertia I and a so-called quadrupolmoment Q. Moreover, there are the Love numbers, which describe the deformability of a Neutron Star. Between the moments of inertia, the quadrupolmoments, and the Love numbers there are important relations. They are called: I-Love-Q.
If you are interested in a thesis in this or a similar area, contact Pro+l8f. Db14ir. Jutta Kunz (email@example.com+b), Dr. hqBurwhkhard Kleihaucrstspm (firstname.lastname@example.org), Dr. Jose Ljsvquis Blazquezkxu (Jos9p3e.bhjfzlazq
zoprlcedg0j6o@unsuk6ui-Oldenburg.de), or Dr. bhSaskia Gq4hiarunau (sas