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K. Ishida, Y. Kitaoka, K. Asayama, S. Ikeda, S. NishiZaki, Y. Maeno, K. Yoshida, and T. Fujita: Phys. Rev. B 56 (1997) R505.
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Ishida, K.1
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A. P. Mackenzie, R. K. W. Haselwimmer, A. W. Tyler, G. G. Lonzarich, Y. Mori, S. NishiZaki, and Y. Maeno: Phys. Rev. Lett. 80 (1998) 161.
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K. Ishida, H. Mukuda, Y. Kitaoka, K. Asayama, Z. Q. Mao, Y. Mori, and Y. Maeno: Nature (London) 396 (1998) 658.
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Nature (London)
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Ishida, K.1
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H. Mukuda, K. Ishida, Y. Kitaoka, Z. Q. Mao, Y. Mori, and Y. Maeno: J. Low Temp. Phys. 117 (1999) 1587.
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K. Ishida, H. Mukuda, Y. Kitaoka, Z. Q. Mao, H. Fukazawa, and Y. Maeno: Phys. Rev. B 63 (2001) 060507.
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9
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G. M. Luke, Y. Fudamoto, K. M. Kojima, M. I. Larkin, J. Merrin, B. Nachumi, Y. J. Uemura, Y. Maeno, Z. Q. Mao, Y. Mori, H. Nakamura, and M. Sigrist: Nature (London) 396 (1998) 558.
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Nature (London)
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Luke, G.M.1
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11
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0034315849
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I. Bonalde, B. D. Yanoff, M. B. Salamon, D. J. Van Harlingen, and E. M. E. Chia: Phys. Rev. Lett. 85 (2000) 4775.
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13
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19644400853
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H. Murakawa, K. Ishida, K. Kitagawa, Z. Q. Mao, and Y. Maeno: Phys. Rev. Lett. 93 (2004) 167004.
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Phys. Rev. Lett
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Y. Maeno, T. Ando, Y. Mori, E. Ohmichi, S. Ikeda, S. NishiZaki, and S. Nakatsuji: Phys. Rev. Lett. 81 (1998) 3765.
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Phys. Rev. Lett
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Phys. Rev. B
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Yaguchi, H.1
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17
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33847348566
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unpublished
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H. Murakawa et al.: unpublished.
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Murakawa, H.1
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19
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0000048596
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S. Nakaharai, T. Ishiguro, S. Watauchi, J. Shimoyama, and K. Kishio: Phys. Rev. B 61 (2000) 3270.
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0036918560
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K. Deguchi, M. A. Tanatar, Z. Q. Mao, T. Ishiguro, and Y. Maeno: J. Phys. Soc. Jpn. 71 (2002) 2839.
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J. Phys. Soc. Jpn
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Deguchi, K.1
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0038781726
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Physica C
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Tamegai, T.1
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Maeno, Y.5
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4243768123
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Physica C
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Yamazaki, K.1
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Mao, Z.Q.4
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Okayasu, S.6
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30
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0031528817
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Y. Maeno, K. Yoshida, H. Hashimoto, S. Nishizaki, S. Ikeda, M. Nohara, T. Fujita, A. P. Mackenzie, N. E. Hussey, J. G. Bednorz, and F. Lichtenberg: J. Phys. Soc. Jpn. 66 (1997) 1405.
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Fujita, T.7
Mackenzie, A.P.8
Hussey, N.E.9
Bednorz, J.G.10
Lichtenberg, F.11
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35
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33847341329
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In ref. 28, the critical field of ∼7 × 102 Oe was estimated. In the estimation of the cutoff term ln(1. 14εc/kBTc, a large cutoff energy (1.14εc/kBTc) ∼ 300 was adopted. This value is the same as that for the superfluidity 3He. We took this cutoff energy to be ∼20 (ref. 29, However the difference between two cutoff terms is only less than a factor of two due to the logarithmic scale. In ref. 28, a Landau parameter Z0, 3 was used, which is the same as that in the ABM state of 3He. By using Z 0, 3, the free energy difference between d ∥ H and d ⊥ H is expressed as (ref. 33) ΔFZ(H,T) ≈ 5(1, T/T c)χnH2. Two of the parameters in ref. 28 may need to be corrected: First, the value of
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3). This correction makes the flipping field √2 times smaller. Second, the factor of the wave function is √2 times larger than that of Leggett. This correction makes the dipole energy 2 times smaller. As a result, He estimated 2√2 times larger value of the flipping field. Taking into account those corrections, his estimation of the flipping field should be ∼250 Oe. The main difference between his result and ours is the assumption of the cutoff energy and the Landau parameter.
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36
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0036538568
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H. Mukuda, K. Ishida, Y. Kitaoka, K. Miyake, Z. Q. Mao, Y. Mori, and Y. Maeno: Phys. Rev. B 65 (2002) 132507.
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(2002)
Phys. Rev. B
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Mukuda, H.1
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Kitaoka, Y.3
Miyake, K.4
Mao, Z.Q.5
Mori, Y.6
Maeno, Y.7
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