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Prog. Theor. Phys. Vol. 115 No. 1 (2006) pp. 245-250
Letters
Baryonic 3P2-Dominant Superfluidity under Combined Pion Condensation with Δ-Mixing
Ryozo Tamagaki1,* and
Tatsuyuki Takatsuka2,**
1Kamitakano Maeda-Cho 26-5, Kyoto 606-0097, Japan
2Faculty of Humanities and Social Sciences, Iwate University,
Morioka 020-8550, Japan
(Received October 7, 2005)
Abstract:
We study baryonic superfluidity under the combined pion condensation
with Δ-mixing, in the situation that the condensates
of both neutral and charged pions occur in neutron stars.
An outline of formulation treating such superfluidity is presented.
Energy gap calculations reveal the possibility that critical
temperatures are higher than about 1 ×109 K.
URL :
http://ptp.ipap.jp/link?PTP/115/245/
DOI : 10.1143/PTP.115.245
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Citing Article(s) :
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Progress of Theoretical Physics Vol. 115 No. 2 (2006) pp. 355-379
:
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Occurrence of Hyperon Superfluidity in Neutron Star Cores
-
Tatsuyuki Takatsuka, Shigeru Nishizaki, Yasuo Yamamoto and Ryozo Tamagaki
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Progress of Theoretical Physics Vol. 116 No. 3 (2006) pp. 573-599
:
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Baryonic 3 P2-Dominant Superfluidity under Combined Pion Condensation with Δ Isobar. I
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Ryozo Tamagaki and Tatsuyuki Takatsuka
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Progress of Theoretical Physics Vol. 117 No. 5 (2007) pp. 861-901
:
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Baryonic 3 P2-Dominant Superfluidity under Combined Pion Condensation with Δ Isobar. II
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Ryozo Tamagaki and Tatsuyuki Takatsuka