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Examining the AF > FM transition in Fe-Rh thin films through photoemission and specific heat measurements. David W. Cooke, Catherine Bordel, Frances Hellman Physics Department, University of California, Berkeley. Peter Kruger Nanosciences Department University of Bourgogne, France. - PowerPoint PPT Presentation
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University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Examining the AF>FM transition in Fe-Rh thin films through
photoemission and specific heat measurements
David W. Cooke, Catherine Bordel, Frances HellmanPhysics Department, University of California, Berkeley
Stephanie MoyermanEric E. Fullerton
Physics DepartmentUniversity of California, San Diego
Peter KrugerNanosciences Department
University of Bourgogne, France
Alex X. GrayChuck S. Fadley
Physics DepartmentUniversity of California, Davis
Jean JuraszekMaterials Physics Group
University of Rouen, France
Why Fe-Rh?
Superparamagnetic limit – KUV ~ kBT
Large K?
Alternative: FePt / FeRh bi-layerThiele, J.-U., Maat, S., and Fullerton, E.E. APL 82, 2859 (2003)
FeRh undergoes an AFM>FM transition at Tcrit ~ 50ºC
RT < T < Tcrit: AFM FeRh; large K fixes FePt momentTcrit < T < TC: FM FeRh reduces HC to flip FePt via coupling
→ Large H or T ~ TC
MgO (001)
FePt (111)
FeRh (001)
m
m
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
FeRh Magnetic Phases
AFM IIT < Tcrit
FMT > Tcrit
Tcrit
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Fe
Rh
Fe
Rh
Origin of the transition?
Possible contributions:• Electronic
– Entropy relates to N(E)
• Lattice– Debye approximation
• Magnetic– Magnons?
– Thermal excitation model, related to Rh moment
maglattelAFMFM SSSSSSdTT
C
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
M.J. Richardson, D. Melville, and J.A. Ricodeau. Phys. Lett. A 46 153-154 (1973)
DFT Calculations of N(ε)
Theoretically predicted largedifference in N(εF)
Slater splitting:In AFM doubling of the latticecauses large drop at εF
Have itinerant AFM – doesthis difference persist at thetransition?
Turn to photoemission to examine electronic structureexperimentally
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Photoemission
Compare features in FM-AFM difference and see good agreement
In order to compare PE to theory, mustscale bands by scattering cross sectionand broaden by instrumentation resolution and core-hole lifetime broadening
Photoemission taken above and below Tcrit
Confirms large difference in electronic DOS persists up to Tcrit
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
“Calorimeter on a Chip”
Specific heat of thin films• 30nm-200nm• 2K - 500K• 0T - 8T
2006 APS KeithleyInstrumentation Award
t
e
C
T
P
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Need to measure epitaxial thin film
Grow IBAD MgO template on device
For more info, see talk W.2100015
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Specific Heat Measurements(AFM)(1973*)
* = M.J. Richardson, D. Melville, and J.A. Ricodeau. Phys. Lett. A 46 153-154 (1973)
γFM = 8.3±0.5 mJ/mol/K2
γAFM= 3.5±0.3 mJ/mol/K2
ΔSel = 1.3±0.2 J/mol/K
ΔSmeas = 2.9 J/mol/K!
critAFMFM TγγdTT
C
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Specific Heat Measurements(AFM)(1973*)
* = M.J. Richardson, D. Melville, and J.A. Ricodeau. Phys. Lett. A 46 153-154 (1973)
What about the lattice?
Different slopes yielddifferent ΘD…
ΘT,FM = 354±20KΘL,FM = 615±12K
ΘT,AFM = 304±13KΘL,AFM = 591±10K
Softer AFM phase →Lattice resists transition!
Thermal Fluctuation Model
nnn
iknnnnn
iknni nnnnn
kiikikii rVrVSSrJSDU,
2
• Note the shoulder at ~200K• Two-state system (Schottky)
• FM – competition between non/magnetization of Rh• AFM – no such competition because Fe AFM cancels
Gruner, M.E., et al. Phys. Rev. B 67, 064415 (2003)
Tcrit Tcurie
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Specific Heat Measurements(AFM)(1973*)
* = M.J. Richardson, D. Melville, and J.A. Ricodeau. Phys. Lett. A 46 153-154 (1973)
γFM = 8.3±0.5 mJ/mol/K2
γAFM= 3.5±0.3 mJ/mol/K2
What about the lattice?
Different slopes yielddifferent ΘD…
ΘT,FM = 354±20KΘL,FM = 615±12K
ΘT,AFM = 304±13KΘL,AFM = 591±10K
Entropic Contributions:ΔSlatt = -5.3+/-1.5 J/mol/KΔSel = 1.3+/-0.2 J/mol/KΔSmag= 6.6+/-3.6 J/mol/K
• Clatt is approximated with Debye models combining low T data and sound velocity measurements
• Cel is obtained from γT, as measured in low T CP
University of California at Berkeley – Physics Department
March APS Meeting, Dallas, TX – March 23, 2011
Specific Heat Measurements
Conclusions
• Photoemission: Observed change in electronic density of states between AF/FM phases
• Specific Heat: Observed Schottky-like anomaly suggesting dominant contribution of magnetism to entropy of transition