Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Masuda, Kota"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Phys. Rev. B 95, 140503 (2017)
We clarify topology of $^3P_2$ superfluids which are expected to be realized in the inner cores of neutron stars and cubic odd-parity superconductors. $^3P_2$ phases include uniaxial/biaxial nematic phases and nonunitary ferromagnetic and cyclic phas
Externí odkaz:
http://arxiv.org/abs/1607.07266
Autor:
Masuda, Kota, Nitta, Muneto
Publikováno v:
Prog.Theor.Exp.Phys.2020 (2020) 013D01
We point out that half-quantized non-Abelian vortices exist as the minimum energy states in rotating neutron $^3P_2$ superfluids in the inner cores of magnetars with magnetic field greater than $3 \times 10^{15}$ Gauss, while they do not in ordinary
Externí odkaz:
http://arxiv.org/abs/1602.07050
Publikováno v:
Proceedings of Quarks and Compact Stars,KIAA at Peking University, Beijing, China Oct.20-22, 2014,pp67-69
By a new approach introducing a "3-window model" and constructing phenomenologically an equation of state for the hadron-quark (HQ) transition region, possible maximum mass of neutron stars (NSs) is discussed. It is found that neutron stars (NSs) wit
Externí odkaz:
http://arxiv.org/abs/1512.08350
Autor:
Masuda, Kota, Nitta, Muneto
Publikováno v:
Phys. Rev. C 93, 035804 (2016)
We discuss quantized vortices in neutron $^3P_2$ superfluids, which are believed to realize in high density neutron matter such as neutron stars. By using the Ginzburg-Landau free energy for $^3P_2$ superfluids, we determine the ground state in the a
Externí odkaz:
http://arxiv.org/abs/1512.01946
Bulk properties of cold and hot neutron stars (NSs) are studied on the basis of the hadron-quark crossover picture where a smooth transition from the hadronic phase to the quark phase takes place at finite baryon density. By using a phenomenological
Externí odkaz:
http://arxiv.org/abs/1508.04861
We construct a new isentropic equation of state (EOS) at finite temperature "CRover" on the basis of the hadron-quark crossover at high density. By using the new EOS, we study the structure of hot neutron stars at birth with the typical lepton fracti
Externí odkaz:
http://arxiv.org/abs/1506.00984
How massive the hybrid stars could be is discussed by a "3-window model" proposed from a new strategy to construct the equation of state with hadron-quark transition. It is found that hybrid stars have a strong potentiality to generate a large mass c
Externí odkaz:
http://arxiv.org/abs/1402.4677
On the basis of the percolation picture from the hadronic phase with hyperons to the quark phase with strangeness, we construct a new equation of state (EOS) with the pressure interpolated as a function of the baryon density. The maximum mass of neut
Externí odkaz:
http://arxiv.org/abs/1212.6803
Using the idea of a smooth crossover from the hadronic matter with hyperons to quark matter with strangeness, we show that the maximum mass of neutron stars with quark matter core can be larger than those without quark matter core. This is in contras
Externí odkaz:
http://arxiv.org/abs/1205.3621