Journal
PHYSICAL REVIEW B
Volume 82, Issue 6, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevB.82.060504
Keywords
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Funding
- NSF [DMR 0906953]
- AvH Foundation
- RMES Program [N 2.1.1/2985]
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We consider the variation in the field-induced component of the specific heat C(H) with the direction of the applied field in Fe pnictides within quasiclassical Doppler-shift approximation with special emphasis to recent experiments on FeSe0.4Te0.6. We show that for extended s-wave gap with no nodes, C(H) has cos 4 phi component, where phi is the angle between H and the direction between hole and electron Fermi surfaces. The maxima of C(H) are at pi/4, 3 pi/4, etc., if the applied field is smaller than H-0 <= 1 T, and at phi = 0, pi/2, etc., if the applied field is larger than H-0. The angle dependence of C(H), the positions of the maxima, and the relative magnitude of the oscillating component are consistent with the experiments performed in the field of 9 T >> H-0. We show that the observed cos 4 phi variation does not hold if the s-wave gap has accidental nodes along the two electron Fermi surfaces.
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