Search Results - "Kobyakov, D. N."

Superfluid Liquid Crystals: Pasta Phases in Neutron Star Crusts by Kobyakov, D. N., Pethick, C. J.

“…The pasta phases predicted to occur near the inner boundary of the crust of a neutron star resemble liquid crystals, a smectic A in the case of sheet-like…”
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Two-component Superfluid Hydrodynamics of Neutron Star Cores by Kobyakov, D. N., Pethick, C. J.

“…We consider the hydrodynamics of the outer core of a neutron star under conditions when both neutrons and protons are superfluid. Starting from the equation of…”
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Surface energy of magnetized superconducting matter in the neutron star cores by Kobyakov, D. N

“…Phys. Rev. C 102, 045803 (2020) In this paper, an effective field theory for proton superconductor (SC) interacting with neutron superfluid (SF), both with…”
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Application of superconducting-superfluid magnetohydrodynamics to nuclear "pasta" in neutron stars by Kobyakov, D. N

“…Phys. Rev. C 98, 045803 (2018) A mixture of superconducting and superfluid nuclear liquids of protons coupled to the ultrarelativistic electron gas, and…”
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Elastic properties of phases with nonspherical nuclei in dense matter by Pethick, C. J, Zhang, Zhaowen, Kobyakov, D. N

“…Phys. Rev. C 101, 055802 (2020) We consider the elastic constants of phases with nonspherical nuclei, so-called pasta phases, predicted to occur in the inner…”
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Superfluid liquid crystals: pasta phases in neutron star crusts by Kobyakov, D. N, Pethick, C. J

“…ZhETF, Vol. 154, No. 5, p. 972 (November 2018) (English translation - JETP, Vol. 127, No. 5, November 2018 available online at www.springer.com ) The pasta…”
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Dispersion and decay of collective modes in neutron star cores by Kobyakov, D. N, Pethick, C. J, Reddy, S, Schwenk, A

“…Phys. Rev. C 96, 025805 (2017) We calculate the frequencies of collective modes of neutrons, protons and electrons in the outer core of neutron stars. The…”
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Two-component superfluid hydrodynamics of neutron star cores by Kobyakov, D. N, Pethick, C. J

“…ApJ 836 203 (2017) We consider the hydrodynamics of the outer core of a neutron star under conditions when both neutrons and protons are superfluid. Starting…”
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