Neutron Stars

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 Proxqm6tf. 7fzDr.ynl Jhbw2uttadimok Kunqezpk (jutjinmstal9.ksxunzwcl@urphol.dvae)Dr.8r Burk0x7zhard Klehm5yih3qaus+3ry (b.kleihaus@uol.dyndkenm3)Dr. Jose Lebuis66im Bhjbflazq3fkquezi+4ty (Joowse.b3plazquez.+tbsalcjpedo@hsquni-Oldwoenh2burg.de8sj), or Dr. sa2Saskigr1ia Grunaunxpm (saskietvva.gruna1/au@uonzbl.de13xrv).

Neutron Star Merger Dance

Esther Drolshagen (esther.drolshagen@uovkl.deli) (Changed: 2020-01-23)