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Volumn 81, Issue 22, 2010, Pages

Noise predictions for STM in systems with local electron nematic order

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Indexed keywords


EID: 77956331141     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.81.224207     Document Type: Article
Times cited : (24)

References (28)
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    • Other examples of an external perturbation which breaks the rotational symmetry of the lattice and would therefore tend to align stripes include strain, high currents (Ref.) and uniaxial pressure.
    • Other examples of an external perturbation which breaks the rotational symmetry of the lattice and would therefore tend to align stripes include strain, high currents (Ref.) and uniaxial pressure.
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  • 13
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    • In some magnetic systems Kawasaki dynamics may be more appropriate, as they conserve local magnetization. However, in our problem there is no reason for nematicity to be locally conserved, so Glauber dynamics are appropriate. Furthermore, because the switching of the local nematic orientation (a single Ising variable in our coarse-grained model) involves many electrons, we do not expect this to be a coherent quantum process. Therefore, we treat the dynamics classically, rather than using a Caldeira-Leggett model.
    • In some magnetic systems Kawasaki dynamics may be more appropriate, as they conserve local magnetization. However, in our problem there is no reason for nematicity to be locally conserved, so Glauber dynamics are appropriate. Furthermore, because the switching of the local nematic orientation (a single Ising variable in our coarse-grained model) involves many electrons, we do not expect this to be a coherent quantum process. Therefore, we treat the dynamics classically, rather than using a Caldeira-Leggett model.
  • 14
    • 77956301525 scopus 로고    scopus 로고
    • Recall that at 100 K, telegraph noise in the YBCO nanowire has a timescale of 10-50 s. By 4.2 K, thermal fluctuations in stripe orientation should be frozen out in that material. Likewise, fluctuations in stripe orientation should be similarly frozen out in BSCCO and NCCOC at 4.2 K.
    • Recall that at 100 K, telegraph noise in the YBCO nanowire has a timescale of 10-50 s. By 4.2 K, thermal fluctuations in stripe orientation should be frozen out in that material. Likewise, fluctuations in stripe orientation should be similarly frozen out in BSCCO and NCCOC at 4.2 K.
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    • Second spectra, another frequency-domain criterion, may also be used (Ref.).
    • Second spectra, another frequency-domain criterion, may also be used (Ref.).
  • 19
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    • Note that we have not focused on critical behavior or on scaling behavior (Refs.). Comparing those type of predictions to STM requires that the measurements be averaged over a large field of view. One advantage of our proposal is the focus on local physics, without the need for spatial averages.
    • Note that we have not focused on critical behavior or on scaling behavior (Refs.). Comparing those type of predictions to STM requires that the measurements be averaged over a large field of view. One advantage of our proposal is the focus on local physics, without the need for spatial averages.
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    • (private communication).
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    • Zachar, O.1    Zaliznyak, I.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.