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Prog. Theor. Phys. Vol. 115 No. 2 (2006) pp. 355-379
Occurrence of Hyperon Superfluidity in Neutron Star Cores
Tatsuyuki Takatsuka,1
Shigeru Nishizaki,1
Yasuo Yamamoto2 and
Ryozo Tamagaki3
1Faculty of Humanities and Social Sciences,
Iwate University, Morioka 020-8550, Japan
2Physics Section, Tsuru University, Tsuru 402-8555, Japan
3Kamitakano Maeda-Cho 26-5, Kyoto 606-0097, Japan
(Received November 1, 2005)
Abstract:
Superfluidity of Λ and Σ- admixed in neutron star (NS)
cores is investigated realistically for hyperon (Y)-mixed NS models
obtained using a G-matrix-based effective interaction approach.
Numerical results for the equation of state (EOS) with the mixing
ratios of the respective components and the hyperon energy gaps including the
temperature dependence are presented.
These are meant to serve as physical inputs for Y-cooling
calculations of NSs.
By paying attention to the uncertainties of the EOS and
the YY interactions, it is shown that both
Λ and Σ- are superfluid as soon as
they appear although the magnitude of the critical temperature
and the density region where superfluidity exists
depend considerably on the YY pairing potential.
Considering momentum triangle condition and the occurrence
of superfluidity, it is found that
a so-called “hyperon cooling”(neutrino-emission
from direct Urca process including Y) combined
with Y-superfluidity may be able to account for observations
of the colder class of NSs. It is remarked that Λ-hyperons play
a decisive role in the hyperon cooling scenario.
Some comments are given regarding the consequences of
the less attractive ΛΛ interaction recently
suggested by the “NAGARA event” 6ΛΛHe.
URL :
http://ptp.ipap.jp/link?PTP/115/355/
DOI : 10.1143/PTP.115.355
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