The sutdy of equilibrium states in the envelopes of neutron stars
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Keywords:
neutron stars, the crystal structure, the resonanceAbstract
The effective resonance interaction of nuclei in the Coulomb crystal created by the rescattering of a free neutron on the nuclei of the crystalline lattice was obtained. Resonances in the lattice appear at the low energies of neutron, close to the energy of two-body neutron-nucleus resonance, and at extremely high pressures that are characteristic of neutron stars’ envelopes. The influences of resonances on the properties of superdense crystalline structures and the EOS of matter were discussed.
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3. Camenzind M. Compact Objects in Astrophysics. - Berlin Heidelberg New York: Springer, 2007. 681 c.
4. Киржниц Д.А. Труды по теоретической физике. – М.: Физматлит, 2001. - Т. 2. - 430 с.
5. Takibayev N.Zh. Class of model problems in three-body quantum mechanics that admit exact solutions // Phys. Atomic Nucl. – 2008. – Vol. 71. – P. 460-468.
6. Takibayev N.Zh. // Few-Body Syst. – 2001. – Vol. 50. – P.311-314. doi: 1007/s00601-010-0207-4.
7. Такибаев Н.Ж. О резонансной генерации нейтрино в сверхплотных звездах // Вестник НАН РК. – 2011. - № 4. – C.09-14.
8. Takibayev N.Zh. // Few-Body Systems, Springer ed. doi: 10.1007/s00601-012-0410-6, 2012.
9. Чугунов А.И. Сильнонеидеальная плазма в оболочках компактных звезд / Автореферат диссертации. Физико-Технический институт им. Иоффе, Санкт-Петерберг, 2007.
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How to Cite
Takibayev, N., Kato, K., Takibayeva, M., Sarsembayeva, A., Kurmangaliyeva, V., & Nasirova, D. (2012). The sutdy of equilibrium states in the envelopes of neutron stars. Recent Contributions to Physics (Rec.Contr.Phys.), 42(3), 16–25. Retrieved from https://bph.kaznu.kz/index.php/zhuzhu/article/view/701
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Condensed Matter Physics and Materials Science Problems. NanoScience
