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 Prt6q0of. 8crysDr. y66Jutta Kuyxnz5tw (julxpnjtta.kunzszx@u25+eool.
s78drde6/nzr), Dr. Burkhard Kleihu/vau0ts1o (firstname.lastname@example.org), Dr. Joseku2tm Luis Blazquezad7l0 (Jose3n.blazqutiez.salced
bkqo@wtunhkzi-Oldenbknbmzurg.de), or Dr. Saskiage Grunau (email@example.com+).