메뉴 건너뛰기




Volumn 89, Issue 10, 2014, Pages

Role of geometrical symmetry in thermally activated processes in clusters of interacting dipolar moments

Author keywords

[No Author keywords available]

Indexed keywords


EID: 84897885982     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.89.104410     Document Type: Article
Times cited : (15)

References (58)
  • 4
  • 6
    • 34147217577 scopus 로고    scopus 로고
    • 9783-5406 10.1007/3-540-69684-9-2
    • E. Vincent, Springer Lect. Notes Phys. 716, 7 (2007). 9783-5406 10.1007/3-540-69684-9-2
    • (2007) Springer Lect. Notes Phys. , vol.716 , pp. 7
    • Vincent, E.1
  • 8
    • 63649144486 scopus 로고    scopus 로고
    • JPAPBE 0022-3727 10.1088/0022-3727/42/1/013001
    • S. Bedanta and W. Kleemann, J. Phys. D: Appl. Phys. 42, 013001 (2009). JPAPBE 0022-3727 10.1088/0022-3727/42/1/013001
    • (2009) J. Phys. D: Appl. Phys. , vol.42 , pp. 013001
    • Bedanta, S.1    Kleemann, W.2
  • 14
    • 0006681755 scopus 로고    scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.58.14937
    • J. L. García-Palacios and F. J. Lázaro, Phys. Rev. B 58, 14937 (1998). PRBMDO 0163-1829 10.1103/PhysRevB.58.14937
    • (1998) Phys. Rev. B , vol.58 , pp. 14937
    • García-Palacios, J.L.1    Lázaro, F.J.2
  • 17
    • 33744907271 scopus 로고    scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.73.212405
    • K. D. Usadel, Phys. Rev. B 73, 212405 (2006). PRBMDO 1098-0121 10.1103/PhysRevB.73.212405
    • (2006) Phys. Rev. B , vol.73 , pp. 212405
    • Usadel, K.D.1
  • 20
    • 0042671069 scopus 로고
    • PRBMDO 0163-1829 10.1103/PhysRevB.52.3540
    • I. Klik and C.-R. Chang, Phys. Rev. B 52, 3540 (1995). PRBMDO 0163-1829 10.1103/PhysRevB.52.3540
    • (1995) Phys. Rev. B , vol.52 , pp. 3540
    • Klik, I.1    Chang, C.-R.2
  • 21
  • 23
    • 0017030517 scopus 로고
    • JCTPAH 0021-9991 10.1016/0021-9991(76)90041-3
    • D. T. Gillespie, J. Comp. Phys. 22, 403 (1976). JCTPAH 0021-9991 10.1016/0021-9991(76)90041-3
    • (1976) J. Comp. Phys. , vol.22 , pp. 403
    • Gillespie, D.T.1
  • 27
    • 36149026446 scopus 로고
    • PHRVAO 0031-899X 10.1103/PhysRev.130.1677
    • W. F. Brown, Phys. Rev. 130, 1677 (1963). PHRVAO 0031-899X 10.1103/PhysRev.130.1677
    • (1963) Phys. Rev. , vol.130 , pp. 1677
    • Brown, W.F.1
  • 30
    • 84897849121 scopus 로고    scopus 로고
    • 30 The time-quantified Monte Carlo methods typically use the metropolis algorithm based on accepting/rejecting a trial move, which generates a random walk in the energy space that can also be represented by a master equation. However, this equation lacks a physical time scale and is fundamentally different from the master-equation approach considered throughout this work.
    • The time-quantified Monte Carlo methods typically use the metropolis algorithm based on accepting/rejecting a trial move, which generates a random walk in the energy space that can also be represented by a master equation. However, this equation lacks a physical time scale and is fundamentally different from the master-equation approach considered throughout this work.
  • 31
    • 0025463724 scopus 로고
    • PSSABA 0031-8965 10.1002/pssa.2211200121
    • H. Pfeiffer, Phys. Stat. Sol. 120, 233 (1990). PSSABA 0031-8965 10.1002/pssa.2211200121
    • (1990) Phys. Stat. Sol. , vol.120 , pp. 233
    • Pfeiffer, H.1
  • 32
    • 0025509567 scopus 로고
    • PSSABA 0031-8965 10.1002/pssa.2211220137
    • H. Pfeiffer, Phys. Stat. Sol. 122, 377 (1990). PSSABA 0031-8965 10.1002/pssa.2211220137
    • (1990) Phys. Stat. Sol. , vol.122 , pp. 377
    • Pfeiffer, H.1
  • 33
    • 3643148153 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.72.3278
    • S. Mørup and E. Tronc, Phys. Rev. Lett. 72, 3278 (1994). PRLTAO 0031-9007 10.1103/PhysRevLett.72.3278
    • (1994) Phys. Rev. Lett. , vol.72 , pp. 3278
    • Mørup, S.1    Tronc, E.2
  • 34
    • 0000836076 scopus 로고
    • JPSOAW 0022-3719 10.1088/0022-3719/21/10/019
    • J. L. Dormann, L. Bessais, and D. Fiorani, J. Phys. C 21, 2015 (1988). JPSOAW 0022-3719 10.1088/0022-3719/21/10/019
    • (1988) J. Phys. C , vol.21 , pp. 2015
    • Dormann, J.L.1    Bessais, L.2    Fiorani, D.3
  • 40
    • 0032073982 scopus 로고    scopus 로고
    • JMMMDC 0304-8853 10.1016/S0304-8853(97)01165-7
    • M. F. Hansen and S. Mørup, J. Magn. Magn. Mater. 184, L262 (1998). JMMMDC 0304-8853 10.1016/S0304-8853(97)01165-7
    • (1998) J. Magn. Magn. Mater. , vol.184
    • Hansen, M.F.1    Mørup, S.2
  • 42
    • 84857048975 scopus 로고    scopus 로고
    • JNARFA 1388-0764 10.1007/s11051-011-0642-2
    • P. Allia and P. P. Tiberto, J. Nanopart. Res. 13, 7277 (2011). JNARFA 1388-0764 10.1007/s11051-011-0642-2
    • (2011) J. Nanopart. Res. , vol.13 , pp. 7277
    • Allia, P.1    Tiberto, P.P.2
  • 45
    • 0033204973 scopus 로고    scopus 로고
    • JMMMDC 0304-8853 10.1016/S0304-8853(99)00347-9
    • R. H. Kodama, J. Magn. Magn. Mater. 200, 359 (1999). JMMMDC 0304-8853 10.1016/S0304-8853(99)00347-9
    • (1999) J. Magn. Magn. Mater. , vol.200 , pp. 359
    • Kodama, R.H.1
  • 47
    • 84897895657 scopus 로고    scopus 로고
    • 47 We note that τ 0 generally depends both on external and on interaction fields. However, because this work considers relaxation in zero external field and the weak dipolar interaction limit, where the interaction strength is negligible with respect to the mean energy barrier height, approximating τ 0 by a constant seems reasonable.
    • We note that τ 0 generally depends both on external and on interaction fields. However, because this work considers relaxation in zero external field and the weak dipolar interaction limit, where the interaction strength is negligible with respect to the mean energy barrier height, approximating τ 0 by a constant seems reasonable.
  • 48
    • 0000013996 scopus 로고
    • RMPHAT 0034-6861 10.1103/RevModPhys.48.571
    • J. Schnakenberg, Rev. Mod. Phys. 48, 571 (1976). RMPHAT 0034-6861 10.1103/RevModPhys.48.571
    • (1976) Rev. Mod. Phys. , vol.48 , pp. 571
    • Schnakenberg, J.1
  • 49
    • 70349140858 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.103.118303
    • N. Arkus, V. N. Manoharan, and M. P. Brenner, Phys. Rev. Lett. 103, 118303 (2009). PRLTAO 0031-9007 10.1103/PhysRevLett.103.118303
    • (2009) Phys. Rev. Lett. , vol.103 , pp. 118303
    • Arkus, N.1    Manoharan, V.N.2    Brenner, M.P.3
  • 51
    • 84872245271 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.110.020604
    • P. F. Bessarab, V. M. Uzdin, and H. Jónsson, Phys. Rev. Lett. 110, 020604 (2013). PRLTAO 0031-9007 10.1103/PhysRevLett.110.020604
    • (2013) Phys. Rev. Lett. , vol.110 , pp. 020604
    • Bessarab, P.F.1    Uzdin, V.M.2    Jónsson, H.3
  • 52
    • 84897911718 scopus 로고    scopus 로고
    • is an approximation expected to be valid only in the weakly interacting case.
    • Note that this is an approximation expected to be valid only in the weakly interacting case.
  • 53
    • 0030206938 scopus 로고    scopus 로고
    • JMMMDC 0304-8853 10.1016/S0304-8853(96)00070-4
    • D. Berkov, J. Magn. Magn. Mater. 161, 337 (1996). JMMMDC 0304-8853 10.1016/S0304-8853(96)00070-4
    • (1996) J. Magn. Magn. Mater. , vol.161 , pp. 337
    • Berkov, D.1
  • 55
    • 37649026575 scopus 로고    scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.70.144401
    • Ò. Iglesias and A. Labarta, Phys. Rev. B 70, 144401 (2004). PRBMDO 1098-0121 10.1103/PhysRevB.70.144401
    • (2004) Phys. Rev. B , vol.70 , pp. 144401
    • Iglesias, O.1    Labarta, A.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.