Experimental Investigation of LiHo x Y 1-x F 4 Jan Kycia, Jeff Quilliam, Shuchao Meng, Chas Mugford Department of Physics and Astronomy University of Waterloo.

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Experimental Investigation of LiHo x Y 1-x F 4 Jan Kycia, Jeff Quilliam, Shuchao Meng, Chas Mugford Department of Physics and Astronomy University of Waterloo Ariel Gomez, Stefan Kycia Department of Physics University of Guelph Thanks to: Michel Gingras, Graeme Luke Support: NSERC, CFI, OIT, MMO, The Research Corporation

LiHo x Y 1-x F 4 c = Å a = b = Å Ho F F Li Tetragonal CaWO4 structure F - ions create strong crystal field, makes the Ho 3+ ions nearly perfect Ising moments along c-axis Next excited state at ~11 K Can replace Ho with non-magnetic Y (dilution) Small NN exchange interaction Primarily dipolar coupled – angle dependent interaction which leads to frustration in the system.

Phase Diagram of LiHo x Y 1-x F 4 Pure material orders ferromagnetically with T C = 1.53 K Transverse-field Ising model, quantum phase transition Lowering x lowers transition temperature (xT C at first) At x~25% sufficient randomness and frustration for spin glass state to occur At x=4.5% unusual “anti-glass”, spin liquid state was observed. (Reich et al PRB 1990, Ghosh et al Science 2002) At x = 16% debate on whether Spin Glass State really exists. (Jonsson et al PRL 2007, Wu et al PRL 1991, Ancona-Torres et al PRL 2008)

The “SpinGlass” Phase at x = Equilibration time, 1 day per point f = 50 Hz Reich, Ellman, Rosenbaum, Aeppli, Belanger PRB (1990)

The “SpinGlass” Phase at x = Equilibration time, 1 day per point f = 50 Hz Reich, Ellman, Rosenbaum, Aeppli, Belanger PRB (1990)

The “Anti-Glass” Phase at x = Unusually sharp features in the specific heat. Narrowing of absorption spectrum  ’’ (f) with lower T. (opposite of a spin glass) Implies that the moments are not freezing. Gap in the absorption spectrum below 100 mK. Hole burning with an oscillating transverse field. Coherent oscillations with life- times of up to 10 s Thought to be coherent clusters of ~200 Ho moments. Ghosh et al. Nature (2003) Ghosh et al. Science (2002) Reich et al. PRB (1990) Ghosh et al. Science (2002) T = 110 mK, Transverse 5 Hz ac field

Our first goal was to measure the low temperature specific heat of LiHo x Y 1-x F 4 More accurately Lower temperatures Different Ho concentrations Subtraction of Ho Nuclear term is tricky 16.7% Ho sample looks like spin glass 4.5% Ho sample looks like “anti-glass” Reich et al. PRB 42, 4631 (1990). Mennenga et al. JMMM 44, 59 (1984). Arrows indicate samples that we have, purchased from TYDEX J.S. Co., St. Petersburg, Russia

Heat Capacity Measurement Dilution Refrigerator with 13 mK base temperature Used quasi-adiabatic method – heat pulse Q is applied and  T is measured Careful attention was paid to thermal leaks, decoupling of thermometers, etc. Leads are 6  m diameter, 1cm long superconducting wires (conduct very little heat). No substrate used (components fastened directly to sample) RuO 2 resistance thermometer calibrated to a GRT and CMN thermometer.

Calculated reaction to heat pulse for configuration with no substrate Calculated reaction to heat pulse with heater, thermometer, thermal weak-link on substrate) This method is convenient but the sample’s specific heat can be over estimated. This method is inconvenient but more accurate

Typical data for a single heat pulse

Total Specific Heat Total specific heat is dominated by nuclear term Ho nuclei have 7/2 spin, strong hyperfine interaction with tightly bound 4f electrons Non-interacting C N calculated from crystal field, hyperfine interaction and nuclear quadrupole interaction. Very small phonon term (~T 3 ) present as well.

After Subtraction of Nuclear Specific Heat Non-interacting C N subtracted to give electronic part  C Broad feature remains which is consistent with a spin glass for all 3 samples Spin glass C does not have a sharp feature at T 0 Indicative of excitations above the transition Simplest model: 1 excited energy level with degeneracy n w.r.t. ground state (fits) More low-temperature data required to look for linear temperature dependence [1] Reich et al. PRB 42, 4631 (1990).

Residual Entropy?

Residual entropy agrees qualitatively with Snider and Yu, PRB 72, (2005)

Comparison with Previous Results Our results do not reproduce the unusually sharp features observed by Ghosh et al. in 4.5% Ho:YLF Thermal conductivity of 4% sample also saw no sharp features (Nikkel & Ellman CondMat ) Data is qualitatively consistent with the 16.7% sample measured by Reich et al. We account for much more of the expected entropy in the system (Rln2) Heat capacity does not give us a measure of the dynamics of the system so cannot say whether “anti-glass” or not. Reich et al. PRB 42, 4631 (1990) Ghosh et al. Science 296, 2195 (2002)

Specific heat at temperatures below 100 mK We find a decoupling of the lattice and phonons from the main source of specific heat. Now it is as if we were using the substrate configuration.

Preliminary temperature dependence of the decoupling at low temperatures The relaxation time probably goes as:  = C addenda /K lattice-? 1.8% Ho

Conclusions for Specific Heat Measurement Measured specific heat of x = 0.018, and Ho samples Do not reproduce sharp features in specific heat seen by Ghosh et al. in the x =0.045 sample. All have qualitative behavior of the x = sample measured by Reich et al. A residual entropy may exist for the x=0.018 and concentrations, that or the temperature dependence of the low temperature specific heat is sub-linear in temperature. Unusual that peak in specific heat does not move to lower temperatures as concentration is reduced (problem with estimation and subtraction of the nuclear term?) Observe significant decoupling of the lattice specific heat from the electrons and/or nuclear components below 100 mK. Our specific heat work has been published: “Specific Heat of the Dilute Ising Magnet LiHo x Y 1-x F 4 ” J.A. Quilliam, C.G.A. Mugford, A. Gomez, S.W. Kycia, and J.B. Kycia Phys Rev Lett. 98, (2007).

Motivation for More Susceptibility Measurements on LiHo x Y 1-x F 4 Use SQUID for improved performance at low frequencies. Confirm that x=0.045 sample has anti-glass characteristics. Check connection of specific heat characteristics with susceptibility characteristics for antiglass. Study different Ho concentrations x = 0.018, x = Arrows indicate samples that we have, purchased from TYDEX J.S. Co., St. Petersburg, Russia Ghosh Ph.D. Thesis, University of Chicago 2003

Conventional Susceptometer Advantage: Easy to put together and use Disadvantage: Loses sensitivity at low frequencies since signal is due to induced EMF. Too many turns reduces highest useable frequency due to intercoil resonance.

J 12    L 12   I max LL 12   V I I/2 +J I/2 -J J  The DC SQUID is the most sensitive detector of magnetic flux Optimal operating point Optimal Current, I B Sensitivity

SQUID Magnetometer Measurement Use a SQUID with a superconducting flux transformer to make a magnetometer. The current sent to the feedback coil produces an equal and opposite field to that provided by the flux transformer. This device directly measures flux, as opposed to induced EMF. Flat Frequency response. No problems with phase shifts. SQUID and controller from ez-SQUID

While the experiment was in progress, Jonnson et al remeasured   and  3 for x = and x = using a micro-SQUID. They swept the field at rates from 1 to 50 Oe/s. Conclude absence of spin glass transition for both x=0.045 and x = Since both compositions are qualitatively similar, they question the existence of an antiglass phase for x = Ancona Torres et al disagree and claim Jonnsen et al swept to their field to quickly at low temperatures. Jonnson et al PRL (2007) Ancona Torres et al PRL (2008)

ac Susceptibility for Various Temperatures Our Result: Ghosh et al. Science (2002) Reich et al. PRB (1990) Our data shows slower response than Ghosh et al for a given temperature. Agrees better with Reich et al. T =120 mK

Width of  ” for Various Temperatures Ghosh et al. Science (2002) Reich et al. PRB (1990) 300 mK Our Result: Our  ” broadens as temperature decreases, consistent with a spin glass. Not consistent with Antiglass.

Arrhenius Law Arrhenius behavior can be attributed to a superparamagnet. Deviation from Arrhenius behavior at lower temperature may indicate that this is a spin glass with T > T g.

Dynamical Scaling Law for Spin Glass Dynamic scaling analysis points to the x = system being a spin glass with a transition temperature of 43 mK and an intrinsic time constant of 16 seconds. Six orders of magnitude slower than for example Eu 0.4 Sr 0.6 S.

At higher temperatures, our  ’ vs. T agrees with Jonsson et al, Reich et al and Biltmo and Henelius. At low temperature, even  ’ measured with f = Hz is not in the static limit. It appears that Jonsson et al are sweeping to quickly below 200 mK. They swept the field at a rates between 1 to 50 Oe/s from H = 0 to H = 150 Oe. Disagrees with Ghosh et al. Temperature Dependence of  ’

Conclusions for ac Susceptibility Measurement Measured ac susceptibility of x = sample. No exotic anti-glass behavior seen. Measured in agreement with Jonsson et al and Reich et al, disagreement with Ghosh et al. The broadening of the absorption spectrum as temperature is lowered is consistent with with behavior of a spin glass. The temperature dependence of  ” follows a near Arrhenius behavior indicating that the system is either a spin glass or superparamagnet. Dynamic scaling analysis points to a spin glass transition temperature of 43 mK+-2mK. Our specific heat work has been accepted for publication: “Evidence of Spin Glass Dynamics in Dilute LiHo x Y 1-x F 4 ” J.A. Quilliam, S. Meng, C.G.A. Mugford, and J.B. Kycia Phys Rev Lett. (2008). Connecting two measurements, the x = 0.08 sample has all of the entropy accounted for when extrapolating to T = 0 by assuming the specific heat is proportional to T at lower T. This peak in the specific heat may be consistent with the spin glass temperature estimated by the Susceptibility result and theory.

4%Ho:YLF Apiezon Grease

Motivations for Further Specific heat and susceptibility Experiments Temperature dependence of DC susceptibility in the x = System. Temperature dependence of the peak frequency for  ”