메뉴 건너뛰기




Volumn 78, Issue 12, 2008, Pages

Magnetic oscillations of resistivity and absorption of radiation in quantum wells with two populated subbands

Author keywords

[No Author keywords available]

Indexed keywords


EID: 51349142697     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.78.125304     Document Type: Article
Times cited : (89)

References (31)
  • 1
    • 0035890456 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.64.201311
    • M. A. Zudov, R. R. Du, J. A. Simmons, and J. R. Reno, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.64.201311 64, 201311 (R) (2001).
    • (2001) Phys. Rev. B , vol.64 , pp. 201311
    • Zudov, M.A.1    Du, R.R.2    Simmons, J.A.3    Reno, J.R.4
  • 6
    • 0000171833 scopus 로고
    • JUPSAU 0031-9015 10.1143/JPSJ.38.989
    • T. Ando, J. Phys. Soc. Jpn. JUPSAU 0031-9015 10.1143/JPSJ.38.989 38, 989 (1975).
    • (1975) J. Phys. Soc. Jpn. , vol.38 , pp. 989
    • Ando, T.1
  • 10
    • 0025484866 scopus 로고
    • SSTEET 0268-1242 10.1088/0268-1242/5/9/006
    • P. T. Coleridge, Semicond. Sci. Technol. SSTEET 0268-1242 10.1088/0268-1242/5/9/006 5, 961 (1990).
    • (1990) Semicond. Sci. Technol. , vol.5 , pp. 961
    • Coleridge, P.T.1
  • 14
    • 0000796211 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.49.5531
    • M. E. Raikh and T. V. Shahbazyan, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.49.5531 49, 5531 (1994).
    • (1994) Phys. Rev. B , vol.49 , pp. 5531
    • Raikh, M.E.1    Shahbazyan, T.V.2
  • 19
    • 0001430694 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.84.2686
    • S. Graf, H. Sigg, K. Kohler, and W. Bachtold, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.84.2686 84, 2686 (2000), and references therein.
    • (2000) Phys. Rev. Lett. , vol.84 , pp. 2686
    • Graf, S.1    Sigg, H.2    Kohler, K.3    Bachtold, W.4
  • 20
    • 0001835639 scopus 로고
    • ZPBBDJ 0340-224X 10.1007/BF01312871
    • T. Ando, Z. Phys. B ZPBBDJ 0340-224X 10.1007/BF01312871 24, 33 (1976).
    • (1976) Z. Phys. B , vol.24 , pp. 33
    • Ando, T.1
  • 22
    • 11244352130 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.70.165311
    • S. A. Mikhailov, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.70.165311 70, 165311 (2004).
    • (2004) Phys. Rev. B , vol.70 , pp. 165311
    • Mikhailov, S.A.1
  • 23
    • 0000791313 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.42.7132
    • X. C. Xie, Q. P. Li, and S. Das Sarma, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.42.7132 42, 7132 (1990).
    • (1990) Phys. Rev. B , vol.42 , pp. 7132
    • Xie, X.C.1    Li, Q.P.2    Das Sarma, S.3
  • 24
    • 0542375050 scopus 로고
    • JUPSAU 0031-9015 10.1143/JPSJ.37.1233
    • T. Ando, J. Phys. Soc. Jpn. JUPSAU 0031-9015 10.1143/JPSJ.37.1233 37, 1233 (1974).
    • (1974) J. Phys. Soc. Jpn. , vol.37 , pp. 1233
    • Ando, T.1
  • 25
    • 51349096277 scopus 로고    scopus 로고
    • This can be done, for example, by extension of the technique presented in Ref. to the case of several subbands.
    • This can be done, for example, by extension of the technique presented in Ref. to the case of several subbands.
  • 26
    • 1442288253 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.69.035303
    • M. G. Vavilov and I. L. Aleiner, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.69.035303 69, 035303 (2004).
    • (2004) Phys. Rev. B , vol.69 , pp. 035303
    • Vavilov, M.G.1    Aleiner, I.L.2
  • 27
    • 0000215724 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.45.14143
    • E. Zaremba, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.45.14143 45, 14143 (1992).
    • (1992) Phys. Rev. B , vol.45 , pp. 14143
    • Zaremba, E.1
  • 28
    • 51349158149 scopus 로고    scopus 로고
    • In the literature, instead of | v12 | 2, one often uses the dimensionless oscillator strength defined as f12 =2m | v12 | 2 / Δ12.
    • In the literature, instead of | v12 | 2, one often uses the dimensionless oscillator strength defined as f12 =2m | v12 | 2 / Δ12.
  • 29
    • 0001535459 scopus 로고
    • Another source of coupling exists in tilted magnetic fields, owing to the component parallel to the layer, which causes intersubband mixing even in the absence of intersubband scattering; see PRBMDO 0163-1829 10.1103/PhysRevB.19. 2106
    • Another source of coupling exists in tilted magnetic fields, owing to the component parallel to the layer, which causes intersubband mixing even in the absence of intersubband scattering; see T. Ando, Phys. Rev. B PRBMDO 0163-1829 10.1103/PhysRevB.19.2106 19, 2106 (1979)
    • (1979) Phys. Rev. B , vol.19 , pp. 2106
    • Ando, T.1
  • 31
    • 40849098127 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.100.086808
    • T. A. Sedrakyan and M. E. Raikh, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.100.086808 100, 086808 (2008).
    • (2008) Phys. Rev. Lett. , vol.100 , pp. 086808
    • Sedrakyan, T.A.1    Raikh, M.E.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.