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Volumn 83, Issue 2, 2011, Pages

Nernst effect from fluctuating pairs in the pseudogap phase of the cuprates

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EID: 79551617639     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.83.020506     Document Type: Article
Times cited : (54)

References (30)
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    • Here, we have used the same heat vertex as Ussishkin, Ref. 8, so as to reproduce the phenomenological Ginzburg-Landau result for the Nernst. The actual heat vertex should be twice as large as discussed by, PLRBAQ 1098-0121 10.1103/PhysRevB.50.9344
    • Here, we have used the same heat vertex as Ussishkin, Ref. 8, so as to reproduce the phenomenological Ginzburg-Landau result for the Nernst. The actual heat vertex should be twice as large as discussed by M. Yu. Reizer and A. V. Sergeev, Phys. Rev. B PLRBAQ 1098-0121 10.1103/PhysRevB.50.9344 50, 9344 (1994). The latter is supported by the detailed calculations of Ref. 9 where the full frequency dependence of the heat vertex was kept.
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    • F, we can set q→0 in the Cooperons, C, thus approximating C(q,ε+Ω,ω- ε)C(q,ε,ω-ε)≈C2(0,ε,-ε)≈1.
    • F, we can set q→0 in the Cooperons, C, thus approximating C(q,ε+Ω,ω- ε)C(q,ε,ω-ε)≈C2(0,ε,-ε)≈1.
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    • y) is proportional to cos (2 φ) to within a few percent over the observed Fermi surface, where φ is the angle of the Fermi wave vector relative to the (π, π) - (π, 0) direction.
    • y) is proportional to cos (2 φ) to within a few percent over the observed Fermi surface, where φ is the angle of the Fermi wave vector relative to the (π, π) - (π, 0) direction.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.