Asteroseismology studies the internal structure of the Sun and other stars using oscillations. These can be studied by interpreting the temporal frequency spectrum acquired through observations.[1] In the same way, the more extreme neutron stars might be studied and hopefully give us a better understanding of neutron-star interiors, and help in determining the equation of state for matter at nuclear densities. Scientists also hope to prove, or discard, the existence of so-called quark stars, or strange stars, through these studies.[2] Fundamental information can be obtained of the General Relativity Theory by observing the gravitational radiation from oscillating neutron stars.[3]
^Zheng, Xiaoping; Pan, Nana; Zhang, Li; Baglin, A.; Bigot, L.; Brown, T. M.; Catala, C.; Creevey, O. L.; Domiciano de Souza, A.; Eggenberger, P.; Garcia, P. J. V.; Grundahl, F.; Kervella, P.; Kurtz, D. W.; Mathias, P.; Miglio, A.; Monteiro, M. J. P. F. G.; Perrin, G.; Pijpers, F. P.; Pourbaix, D.; Quirrenbach, A.; Rousselet-Perraut, K.; Teixeira, T. C.; Thevenin, F.; Thompson, M. J. (2007). "1122 Hz rotation of XTE J1739-285 as a probe of quark matter in the interior of the neutron star". arXiv:0712.4310. Bibcode:2007arXiv0712.4310Z. {{cite journal}}: Cite journal requires |journal= (help)