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Physical Review Letters
Volumn 92, Issue 11, 2004, Pages
Fernández and Alonso Reply
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EID: 85038300965     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.92.119702     Document Type: Article
Times cited : (5)
References (5)
  • 1
    • 0042381836 scopus 로고    scopus 로고
    • J.F. Fernández and J.J. Alonso, Phys. Rev. Lett. 91, 047202 (2003).10.1103/PhysRevLett.91.047202
    • (2003) Phys. Rev. Lett. , vol.91 , pp. 47202
  • 2
    • 2342563038 scopus 로고    scopus 로고
    • I.S. Tupitsyn and P.C.E. Stamp, preceding Comment, Phys. Rev. Lett. 92, 119701 (2004).
    • (2004) Phys. Rev. Lett. , vol.92 , pp. 119701
  • 3
    • 1442263549 scopus 로고    scopus 로고
    • J.F. Fernández and J.J. Alonso, Phys. Rev. B 69, 024411 (2004).10.1103/PhysRevB.69.024411
    • (2004) Phys. Rev. B , vol.69 , pp. 24411
  • 4
    • 0001176603 scopus 로고    scopus 로고
    • W. Wernsdorfer, T. Ohm, C.�Sangregorio, R.�Sessoli, D.�Mailly, and C.�Paulsen, Phys. Rev. Lett. 82, 3903 (1999).10.1103/PhysRevLett.82.3903
    • (1999) Phys. Rev. Lett. , vol.82 , pp. 3903
    • Wernsdorfer, W.1    Ohm, T.2
  • 5
    • 0036696134 scopus 로고    scopus 로고
    • The magnetization rate in annealed [unannealed] systems goes as (Formula presented) [(Formula presented)], where (Formula presented) is the tunneling window ((Formula presented) in (Formula presented)); see J.F. Fernández, Phys. Rev. B 66, 064423 (2002).10.1103/PhysRevB.66.064423
    • (2002) Phys. Rev. B , vol.66 , pp. 64423

* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.