experimental investigation of liho x y 1-x f 4 jan kycia, jeff quilliam, shuchao meng, chas mugford...

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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

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Page 1: 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

Experimental Investigation of LiHoxY1-xF4

Jan Kycia, Jeff Quilliam, Shuchao Meng, Chas Mugford Department of Physics and Astronomy

University of Waterloo

Ariel Gomez, Stefan KyciaDepartment of PhysicsUniversity of Guelph

Thanks to: Michel Gingras, Graeme LukeSupport: NSERC, CFI, OIT, MMO, The Research Corporation

Page 2: 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

LiHoxY1-xF4

c = 10.75 Å

a = b = 5.176 Å

Ho

Ho Ho

Ho

Ho

F

F

Li

Li

Li

• Tetragonal CaWO4 structure• F- ions create strong crystal field, makes the

Ho3+ 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.

Page 3: 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

Phase Diagram of LiHoxY1-xF4

• Pure material orders ferromagnetically with TC = 1.53 K

• Transverse-field Ising model, quantum phase transition

• Lowering x lowers transition temperature (xTC 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)

Page 4: 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

The “SpinGlass” Phase at x = 0.167

Equilibration time, 1 day per pointf = 50 Hz

Reich, Ellman, Rosenbaum, Aeppli, Belanger PRB 42 4631(1990)

Page 5: 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

The “SpinGlass” Phase at x = 0.167

Equilibration time, 1 day per pointf = 50 Hz

Reich, Ellman, Rosenbaum, Aeppli, Belanger PRB 42 4631(1990)

Page 6: 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

The “Anti-Glass” Phase at x = 0.045

• 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

Page 7: 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

Our first goal was to measure the low temperature specific heat of LiHoxY1-xF4

• 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

Page 8: 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

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)

• RuO2 resistance thermometer calibrated to a GRT and CMN thermometer.

Page 9: 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

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

Page 10: 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

-600 -400 -200 0 200 400 600

0 .095

0 .096

0 .097

0 .098

0 .099

0 .1

0 .101

0 .102

0 .103

Tim e (s)

Tem

pera

ture

(K

)

T

Typical data for a single heat pulse

Page 11: 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

Total Specific Heat

0 0.2 0.4 0.6 0.8 10

2

4

6

8

10

Spe

cifi

c H

eat (

J / K

mol

Ho)

Temperature (K)

8.0%4.5%1.8%CNuclear

• Total specific heat is dominated by nuclear term

• Ho nuclei have 7/2 spin, strong hyperfine interaction with tightly bound 4f electrons

• Non-interacting CN calculated from crystal field, hyperfine interaction and nuclear quadrupole interaction.

• Very small phonon term (~T3 ) present as well.

Page 12: 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

After Subtraction of Nuclear Specific Heat

0

1

2

3

Temperature (K)

Spe

cifi

c H

eat (

J / K

mol

Ho)

8.0%4.5%1.8%

0.1 0.2 0.5

• Non-interacting CN 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 T0

• 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).

Page 13: 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

Residual Entropy?

Page 14: 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

Residual entropy agrees qualitatively with Snider and Yu, PRB 72, 214203 (2005)

Page 15: 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

Comparison with Previous Results

0

1

2

3

Temperature (K)

Spe

cifi

c H

eat (

J / K

mol

Ho) 8.0%

4.5%1.8%

4.5% (Ghosh)16.7% (Reich)

0.1 0.2 0.5

• 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 0504269)

• 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)

Page 16: 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

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.

Page 17: 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

Preliminary temperature dependence of the decoupling at low temperatures

The relaxation timeprobably goes as: = Caddenda/Klattice-?

1.8% Ho

Page 18: 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

Conclusions for Specific Heat Measurement

• Measured specific heat of x = 0.018, 0.045 and 0.080 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 = 0.0167 sample measured by Reich et al.• A residual entropy may exist for the x=0.018 and 0.045 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 LiHoxY1-xF4” J.A. Quilliam, C.G.A. Mugford, A. Gomez, S.W. Kycia, and J.B. Kycia Phys Rev Lett. 98, 037203 (2007).

Page 19: 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

Motivation for More Susceptibility Measurements on LiHoxY1-xF4

• 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 = 0.080

Arrows indicate samples that we have, purchased from TYDEX J.S. Co., St. Petersburg, Russia Ghosh Ph.D. Thesis, University of Chicago 2003

Page 20: 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

Conventional Susceptometer

Advantage: Easy to put together and use

Disadvantage: Loses sensitivity at low frequenciessince signal is due to induced EMF. Too many turns reduces highest useable frequency due to intercoil resonance.

dt

dVEMF

Page 21: 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

J

1 2

L

1 2

ImaxL

1 2

V

I

I/2 +J I/2 -JJ

The DC SQUID is the most sensitive detector of magnetic flux

Optimal operating point

OptimalCurrent, IB

Sensitivity Hz/1~ 0

Page 22: 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

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

Page 23: 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

While the experiment was in progress, Jonnson et al remeasured and 3 for x = 0.045 and x = 0.165 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 = 0.165. Since both compositions are qualitatively similar, they question the existence of an antiglass phase for x = 0.045.

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)

Page 24: 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

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 alfor a given temperature. Agrees better with Reich et al.

T =120 mK

Page 25: 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

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.

Page 26: 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

s

KE

eT

oA

A

TkEoAMax

Ba

32.0

57.1

/

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 > Tg.

Page 27: 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

s

z

mKT

TTT

o

g

zgoMax

716

2.08.7

243

1/

Dynamical Scaling Law for Spin Glass

Dynamic scaling analysis points to the x = 0.045 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 Eu0.4Sr0.6S.

Page 28: 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

•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 = 0.001 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 between1 to 50 Oe/s from H = 0 to H = 150 Oe.

• Disagrees with Ghosh et al.

1' T

Temperature Dependence of ’

Page 29: 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

Conclusions for ac Susceptibility Measurement

• Measured ac susceptibility of x = 0.045 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 LiHoxY1-xF4” 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 theSusceptibility result and theory.

1' TDC

Page 30: 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

0.00001

0.0001

0.001

0.01

0.1

1

10

100

1000

0.1 1Temperature (K)

Teflon

NbTi

BeCu

Cu

Nb

S.S.

4%Ho:YLF

ApiezonGrease

Page 31: 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
Page 32: 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
Page 33: 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

Motivations for Further Specific heat and susceptibility Experiments

75.0 T 1 T

Temperature dependence of DC susceptibility in the x = 0.045System.

Temperature dependence of the peak frequency for ”

Page 34: 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