Can a solid be superfluid?

Slides:



Advertisements
Similar presentations
Agenda Semiconductor materials and their properties PN-junction diodes
Advertisements

In quest of 4 He supersolid a work with J. Peter Toennies (MPI-DSO Göttingen), Franco Dalfovo (Uni Trento), Robert Grisenti & Manuel Käsz (Uni Frankfurt),
INTRODUCTION TO MECHANICS FOR SOLIDS AND STRUCTURES
FIGURE 5.1 Potentiometric displacement sensor.
A quantity that has both a number and a unit
Lecture 2 ANALYSIS OF VARIANCE: AN INTRODUCTION
Boiling heat transfer of liquid nitrogen in the presence of electric fields P Wang, P L Lewin, D J Swaffield and G Chen University of Southampton, Southampton,
Superfluidity in solid helium and solid hydrogen
Chapter 7 Sampling and Sampling Distributions
The Kinetic Theory of Gases
Free Electron Fermi Gas
Reaction Equilibrium in Ideal Gas Mixture
Lecture
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 10: Elasticity and Oscillations.
16. Magnetic brakes ”When a strong magnet falls down a non ferromagnetic metal tube, it will experience a retarding force. Investigate the phenomenon.”
Honoring accomplishments of John Reppy Superfluids and Supersolids (or not) Harry Kojima Rutgers December 2012.
Cluster Magic Numbers. Recent highly accurate diffusion Monte Carlo (T=0) calculation rules out existence of magic numbers due to stabilities: R. Guardiola,O.
Halliday/Resnick/Walker Fundamentals of Physics 8th edition
Analysis of the Visible Absorption Spectrum of I 2 in Inert Solvents Using a Physical Model Joel Tellinghuisen Department of Chemistry Vanderbilt University.
A square transparent cell: a square hole (11 x 11 mm 2 ) in a gold- plated copper plate (here 10 mm thick) 2 glass windows sealed with indium O-rings.
TEST GRAINS AS A NOVEL DIAGNOSTIC TOOL B.W. James, A.A. Samarian and W. Tsang School of Physics, University of Sydney NSW 2006, Australia
Could a quantum solid flow like a superfluid ? S. Sasaki, R. Ishiguro, F. Caupin, H.J. Maris* and S. Balibar Laboratoire de Physique Statistique (ENS-Paris)
Compound Torsional Oscillator: Frequency Dependence and Hysteresis of Supersolid 4 He (and Search for Superfluid Sound Mode) Harry Kojima Rutgers University.
Design of an Aerospace Component
Glass and possible non supersolid origin of TO anomaly E. Abrahams (Rutgers) M. Graf, Z. Nussinov, S. Trugman, AVB (Los Alamos), 1.Thermodynamic considerations.
SUPERSOLIDS? minnesota, july 2007 acknowledgments to: Moses Chan &Tony Clark David Huse & Bill Brinkman Phuan Ong& Yayu Wang Hari Kojima& many other exptlists.
The effect of 3 He impurity on supersolid E. Kim, Korea Advanced Institute of Science and Technology J. T. West, X. Lin, and M. H. W. Chan J. T. West,
Boris Svistunov Nikolay Prokof’ev (UMass) Lode Pollet (ETH) Massimo Boninsegni (U of Alberta) Matthias Troyer (ETH) Anatoly Kuklov (CUNY) PITP-The Outing.
Quantum liquids in Nanoporous Media and on Surfaces Henry R. Glyde Department of Physics & Astronomy University of Delaware National Nanotechnology Initiative.
Helium-4: The Once and Future Supersolid Michael Ma University of Cincinnati Hong Kong Forum, 2006.
Crystalline Arrangement of atoms. Chapter 4 IMPERFECTIONS IN SOLIDS The atomic arrangements in a crystalline lattice is almost always not perfect. The.
Dislocations and Strengthening
Thermal Properties of Crystal Lattices
Jamming Peter Olsson, Umeå University Stephen Teitel, University of Rochester Supported by: US Department of Energy Swedish High Performance Computing.
Torsional oscillator and specific heat measurements on solid helium PITP-Outing Lodge workshop, July 22, 2007 Moses Chan - Penn State.
The Structure of Metals
Measurement of contact angles The contact of 4 He crystals with walls: hysteresis of the contact angle S. Sasaki a, F. Caupin and S. Balibar Laboratoire.
1 Scalar Properties, Static Correlations and Order Parameters What do we get out of a simulation? Static properties: pressure, specific heat, etc. Density.
EEE 3394 Electronic Materials
Crystal Growth Techniques
Bose-Einstein Condensation and Superfluidity Lecture 1. T=0 Motivation. Bose Einstein condensation (BEC) Implications of BEC for properties of ground state.
1 Superfluidity in Liquid Helium PHYS 4315 R. S. Rubins, Fall 2009.
Rotating Superfluid 3 He in Aerogel Takao Mizusaki Department of Physics, Graduate School of Science, Kyoto University Collaborators: Kyoto University,
Supersolidity, disorder and grain boundaries S. Sasaki, R. Ishiguro, F. Caupin, H.J. Maris and S. Balibar Laboratoire de Physique Statistique (ENS-Paris)
Spin Dynamics of Superfluid 3 He in Aerogel Osamu Ishikawa Osaka City University.
Moses Chan, Penn State (chair) Frank Gasparini, University at Buffalo
P301 Lecture 8 “CMB fit to BB spectrum” The plot on the right shows data from the FIRAS instrument on the original.
EEE 3394 Electronic Materials Chris Ferekides SPRING 2014 WEEK 2.
PHY1039 Properties of Matter Heat Capacity of Crystalline Solids March 26 and 29, 2012 Lectures 15 and 16.
Peak effect in Superconductors - Experimental aspects G. Ravikumar Technical Physics & Prototype Engineering Division, Bhabha Atomic Research Centre, Mumbai.
Study of T 1 relaxation time A proposal to test T 1 using a dilution fridge and SQUID NMA at Royal Hollow University,London.
©D.D. Johnson and D. Ceperley MSE485/PHY466/CSE485 1 Scalar Properties, Static Correlations and Order Parameters What do we get out of a simulation?
Crystal Growth General Formalism    Phase growing into  with velocity v : f ( “site factor” ) : fraction of sites where a new atom can be incorporated.
Superconductivity and Superfluidity Temperature scales Lecture 14.
Halliday/Resnick/Walker Fundamentals of Physics
Imperfections in Solids
The case for and against dislocation network as the relevant disorder for the supersolid phenomenon & other puzzles Fondation des Treilles Workshop July.
Materials Science Chapter 4 Disorder in solid Phases.
Flow of 3 He in 640 nm thick slabs Jeevak M. Parpia, Cornell University, DMR Background frequency (empty cell) blue triangles, frequency when the.
Superconductivity and Superfluidity The Microscopic Origins of Superconductivity The story so far -what do we know about superconductors?: (i) Superconductors.
Superfluidity and Quantum Vortices. Outline of the presentation Bose-Einstein Condensation Superfluidity Quantum Vortix.
16 Heat Capacity.
物 理 化 學 Physical Chemistry matter logic change study origin
Dislocations and Strengthening
Scalar Properties, Static Correlations and Order Parameters
16 Heat Capacity.
Thermomechanical effect
The Pennsylvania State University
Presenter: Rafael Domenikos A Different Approach at Solid and Supersolid Helium 4 National Technical University of Athens Authors: Domenikos Rafael1.
Presentation transcript:

Can a solid be superfluid? Symposium on Quantum Phenomena and Devices at Low Temperatures, 2008 Helsinki Univ. of Technology Moses Chan - Penn State

Outline Introduction Torsional oscillator measurements. Origin of supersolidity : zero point vacancies, grain boundaries glassy regions or dislocations? Specific heat and dc flow experiments Conclusions

Theoretical ‘consensus’ in 1970s: Superfluidity in solid is not impossible! - If solid 4He can be described by a Jastraw-type wavefunction that is commonly used to describe liquid helium then crystalline order (with finite fraction of vacancies) and BEC can coexist. G.V. Chester, Lectures in Theoretical Physics Vol XI-B(1969); Phys. Rev. A 2, 256 (1970) J. Sarfatt, Phys. Lett. 30A, 300 (1969) L. Reatto, Phys. Rev. 183, 334 (1969) - Andreev and Liftshitz assume the specific scenario of zero-point vacancies and other defects ( e.g. interstitial atoms) undergoing BEC and exhibit superfluidity. Andreev & Liftshitz, Zh.Eksp.Teor.Fiz. 56, 205 (1969).

R I(T)=Iclassical[1-fs(T)] The ideal method of detection of superfluidity is to subject solid to dc or ac rotation. Leggett, “Can a solid be superfluid?” PRL 25, 1543(1970) Quantum exchange of particles arranged in an annulus under rotation leads to a measured moment of inertia that is smaller than the classical value Solid Helium R I(T)=Iclassical[1-fs(T)] fs(T) is the supersolid or nonclassical rotational inertia (NCRI) fraction. Its upper limit is estimated by different theorists to range from 10-6 to 0.4; Leggett: 10-4

Torsional Oscillator Technique is ideal for the detection of superfluidity Amp Drive Detection 3.5 cm Torsion rod Torsion cell Quality Factor Q= f0 / f ~106 Stability in the period is ~0.1 ns Frequency resolution of 1 part in 107 Mass sensitivity of ~10-7 g f~ 1kHz

Torsional oscillator studies of superfluid films Vycor Δ I total= I cell+ I helium film, Above Tc the adsorbed normal liquid film behaves as solid and oscillates with the cell. In the superfluid phase, helium film decouples from oscillation. Hence Itotal and drops.  Berthold,Bishop, Reppy, PRL 39,348(1977)

Bulk solid helium in annulus Torsion cell with helium in annulus Filling line Channel OD=10mm Width=0.9mm Torsion rod 3.5 cm Mg disk Torsion cell Al shell Detection Solid helium in annular channel Drive

E. Kim & M.H.W. Chan, Science 305, 1941 (2004) Bulk solid helium in annulus f0=912Hz 51bar Total mass loading = 3012ns Measured decoupling, -o=41ns NCRIF = 1.4% E. Kim & M.H.W. Chan, Science 305, 1941 (2004)

Non-Classical Rotational Inertia Fraction |v|max Total mass loading =3012ns at 51 bars

Irrotational Flow Superfluids exhibit potential (irrotational) flow For our exact dimensions, NCRIF in the blocked cell should be about 1% that of the annulus* *E. Mueller, private communication.

Reversibly blocked annulus Rittner & Reppy, Cornell Top View: Blocked Top View: Open solid inertia Nonclassical rotational inertia Gap 73 mm, NCRI = 16 %

Nonclassical rotational inertia results have been replicated in five other labs. The temperature dependence of NCRI is reproduced. However, the magnitude of NCRIF varies from 0.015% up to 16%. Simulations studies indicate NCRI is not possible in a ‘perfect’ crystal and that quantum zero point vacancies concentration is too low to account for the observations. (this conclusion not universally accepted). This leaves other defects, e.g. grain boundaries, glassy regions and dislocations as possible origins or at least ‘enhancer’ for NCRI.

Grain boundaries It has been suggested that the observed NCRI are due to atomically thin superfluid (liquid) films along the grain boundaries, if true, NCRI should scales with total grain boundary area. Grain size of solid 4He inside Vycor glass is ~ 7nm and in bulk it is ~0.1 mm. This means the grain boundary surface differs by many orders of magnitude, but observed NCRI is about the same, ~1%. Nevertheless, most bulk solid samples grown by the blocked capillary method is polycrystalline. Does NCRI exists in a single crystal ?

E. Kim & M.H.W. Chan, Nature 427, 225 (2004). Solid helium in Vycor glass 7nm f0=1024Hz 62bar Total mass loading = 4260ns Measured decoupling, -o=17ns NCRI fraction, or NCRIF = 0.4% (with tortuosity, 2% ) -*[ns] E. Kim & M.H.W. Chan, Nature 427, 225 (2004). *=971,000ns

Crystal Growth High quality single crystals have been grown under constant temperature1 and pressure2 Best crystals grown in zero temperature limit 1. O.W. Heybey & D.M. Lee, PRL 19, 106 (1967); S. Balibar, H. Alles & A. Ya Parshin, Rev. Mod. Phys. 77, 317 (2005). 2. L.P. Mezhov-Deglin, Sov. Phys. JETP 22, 47 (1966); D.S. Greywall, PRA 3, 2106 (1971).

Constant T/P growth from superfluid (1ppb 3He) Heat in Heat out Q ~ 500,000 Tony Clark and Josh West

Solid 4He (1ppb 3He) grown under constant P/T from superfluid

Solid 4He (1ppb 3He) grown under constant P/T from superfluid

Solid 4He (1ppb 3He) grown under constant P/T from superfluid

Solid 4He (1ppb 3He) grown under constant P/T from superfluid

Solid 4He (1ppb 3He) grown under constant P/T from superfluid

Solid 4He (1ppb 3He) grown under constant P/T from superfluid

Samples grown under constant P/T from superfluid collapse onto one curve for T > 40mK and share common onset temperature, TC ~ 80mK. Superfluid film flow along grain boundary cannot be the ‘origin’ of NCRI.

High temperature tail of NCRI Transition broadened in BC samples (probably “polycrystalline”) and by 3He impurities

Superfluid film along the grain boundaries cannot be the mechanism for NCRI. What is the most likely origin for the large variation in NCRI from cell to cell? Dislocation lines density in solid 4He ranges from ~10 to 109 cm-2 , sensitive to how the solid is nucleated and grown. But how does dislocations enable or enhance NCRI?

Dislocations Two of the common types: edge & screw In solid 4He Dislocation density, L = ~5  <1010 cm-2

3He impurities at “high” T Network pinning at the nodes 3He impurities are not ‘attached’ to the dislocation lines.

Increasing fraction of 3He atoms condense onto and stiffen dislocation network with decreasing T Iwasa et.al., J.Phys. Soc. Jpn. 46, 1119( 1979); Paalanen, Bishop and Dail, PRL 46, 664(1981)

3He Effect ( bulk samples) E. Kim, J. S. Xia, J. T. West, X. Lin, A. C Clark, and M. H. W. Chan, , PRL 100, 065301( 2008)

Onset of NCRI tracks the expected temp Onset of NCRI tracks the expected temp. of 3He condensation onto dislocation

Direct measurement of the Shear Modulus James Day and John Beamish, Nature (London) 450, 853 (2007).

Shear Modulus mirrors NCRI James Day and John Beamish, Nature (London) 450, 853 (2007).

The increase in shear modulus and the onset of NCRI at low T must be related, but how? An increase in shear modulus of solid 4He in TO can result an increase in its resonant freq., ie. the same sign as the observed NCRI. But simulation studies shows the magnitude of the ‘Beamish’ effect is typically orders of magnitudes smaller than that observed in most TOs. The ‘Beamish’ effect or shear modulus stiffening cannot explain the blocked annulus experiments. It has been suggested (Anderson) that the onset of supersolidity stiffens the shear modulus. Simulations show the dislocation lines are ‘superfluid’ and it has been suggested that the onset of NCRI requires a ‘rigid’ dislocation network.

What about the superglass model? Since glass has no crystalline order, it is thought superfluidity is more likely to occur. If this is the case there should be thermodynamic signatures ( e.g. thermal hysteresis, and linear specific heat)

Heat capacity Is there a thermodynamic signature of the transition? There is no specific heat information on solid 4He below 200 mK. The heat capacity of metal container swamps the contribution of solid 4He

Heat Capacity measurements in a Silicon cell Reasons for Si: Low heat capacity: High thermal conductivity: Helium Volume= 0.926cc Si Al Glass Capillary Stycast 2850 Heater Thermometer 0.1mm ID 1.5 cm Lattice Materials CorP., MT, USA Optical Silicon purity : >99.999% Heat capacity of solid 4He is more than 10 times larger than the Si cell over the entire temp. range

AC Calorimetry KΘ Kb Sample Kh Internal time constant << 1/ω External time constant >> 1/ω Kb Sample Thermal Bath Thermometer KΘ Heater Kh Paul F. Sullivan, G. Seidel, Phys Rev. 173, 679 (1968). Yaakov Kraftmakher, Physics Reports, 356 (2002) 1-117.

Specific heat of commercially pure 4He (0.3ppm 3He) log C vs. log T Constant volume technique. 20 hours to finish solidification. No long time constant. No hysteresis No annealing effect No thermal cycle effect

Specific heat of solid 4He (0.3ppm & 1ppb) log C vs. log T

C/T vs. T2 Data above 140 mK extrapolate to zero the data seem to diverge in the low-temperature limit. This behaviour, which is more prominent in the 30 p.p.m. sample, suggests the presence of a temperature-independent term in addition to the Debye contribution. Data above 140 mK extrapolate to zero

‘Linear T’ term from Pressure measurements ? PHYSICAL REVIEW B 76, 224524 2007 V. N. Grigor'ev et al Freshly grown sample Annealed sample (19.83cc/mole) — Grüneisen constant ρ — molar volume CV~Tn P~Tn+1

Specific heat with Debye phonon term subtracted T3 subtracted ~20 mJ mol−1 K−1 ~2.5×10-6 kB per 4He atom Explain the Scatter.

Higher resolution in 2008 sample cell Minimum Temperature 25mK New preliminary result with a more sensitive thermometer. Disadvantage of Si? 8 out of 10 cells leaks under high pressure 4 hours to solidify a sample. Solid sample grown under constant pressure condition has the smallest peak. T3 subtracted T3 subtracted

Comparison with the Helsinki melting curve measurement. Constant volume 1ppb 2008 Constant pressure 1ppb 2008 No anomaly in melting curve after correction for instrumental effect. Discrepancy we don’t understand Todoschenko et al., PRL 97, 165302 (2006); JETP Lett. 85, 555 (2007).

dc ( superfluid-like ) flow? Greywall and Beamish carried out experiments by increasing pressure on one end of a solid ( bulk or in Vycor glass) sample. No evidence of flow. Balibar and collaborators saw flow in liquid-solid coexistence samples. The observed phenomenon is likely a consequence of liquid film flow through the ‘crack’ in the solid.

DC superflow reported by ‘pushing’ on superfluid in contact with solid : ‘UMass Sandwich’ (R.B. Hallock) 3 1 2 R, reservoirs V, Vycor S, sample C1 C2

Conclusions NCRI or superfluid like behavior seen in solid 4He in 7 labs. Shear modulus increases at low temperature, the temperature dependence of the increases mimics that of NCRI It is possible that either (1) NCRI ‘requires’ a rigid dislocation network, or (2) onset of NCRI stiffens the solid lattice. No evidence of linear T term in specific heat, but a peak near NCRI onset is seen, size of peak is smaller for a ‘higher’ quality sample. Preliminary dc superfluid flow through solid helium reported.

Xi, Tony, Eunseong, Josh

Lindemann Parameter the ratio of the root mean square of the displacement of atoms to the interatomic distance (da) A classical solid will melt if the Lindemann’s parameter exceeds the critical value of ~0.1 . X-ray measurement of the Debye-Waller factor of solid helium at ~0.7K and near melting curve shows this ratio to be 0.262. (Burns and Issacs, Phys. Rev. B 55, 5767(1997)) total energy zero-point energy Zero-point Energy Inter-atomic potential

Solid 4He at 62 bars in Vycor glass Period shifted by 4260ns due to mass loading of solid helium *=966,000ns

Strong and ‘universal’ velocity dependence in all annular samples ω R vC~ 10µm/s =3.16µm/s for n=1 Vortices are important

Blocked capillary (BC) method of growing solid samples heat drain solid blocks fill-line Be-Cu torsion rod and fill-line gravity

Supersolid response of helium in Vycor glass Period drops at 175mK  appearance of non-classical rotational inertia (NCRI) size of period drop - ~17ns  *=971,000ns

3He impurity effect in Vycor -*[ns] *=971,000ns

Solid helium in porous gold 490nm f0=359Hz 27bar Total mass loading = 1625ns Measured decoupling, -o=13ns NCRIF = 0.8% (with tortuosity, 1.2% ) E. Kim & M.H.W. Chan, JLTP 138, 859 (2005).

Specific heat with the temperature independent constant term subtracted

Previous solid 4He heat capacity measurements below 1K Year Low temperature limit Swenson1 1962,1967 0.2K Edwards2 1965 0.3K Gardner3 1973 0.35K Adams4 1975 0.13K Hebral5 1980 0.1K Clark6 2005 0.08K They all observed T3 phonon contribution. Their sample cells used in these experiments were all constructed with heavy wall metal or epoxy which contribute significantly to the heat capacity at low temperature. E. C. Heltemes and C. A. Swenson, Phys. Rev. 128, 1512 (1962); H. H. Sample and C. A. Swenson, Phys. Rev. 158, 188 (1967). D. O. Edwards and R. C. Pandorf, Phys. Rev. 140, A816 (1965). W. R. Gardner et al., Phys. Rev. A 7, 1029 (1973). S. H. Castles and E. D. Adams, J. Low Temp. Phys. 19, 397 (1975). B. Hébral et al., Phonons in Condensed Matter, edited by H. J. Maris (Plenum, New York, 1980), pg. 169. A. C. Clark and M. H. W. Chan, J. Low Temp. Phys. 138, 853 (2005).

Results: 4He at different 3He concentrations in glass capillary cell Constant volume technique No long time constant. No hysteresis No change due to annealing No thermal cycle effect

C vs T3 10ppm sample 0.7+/-0.2 kB per 3He 30ppm sample Constant contribution from 3He impurity 10ppm sample 0.7+/-0.2 kB per 3He 30ppm sample 1.7+/-0.3 kB per 3He

Is there a linear T term? For 0.3ppm, T>0.14K T3 relation only

NMR measurement of spin (3He) diffusion: A. R. Allen, M. G. Richards & J. Schratter J. Low Temp. Phys. 47, 289 (1982). M. G. Richards, J. Pope & A. Widom, Phys. Rev. Lett. 29, 708 (1972).

Results: pure 4He (0.3ppm & 1ppb) Ln C vs. Ln T What is the deviation?

Previous solid 4He heat capacity measurements below 1K Year Low temperature limit Swenson1 1962,1967 0.2K Edwards2 1965 0.3K Gardner3 1973 0.35K Adams4 1975 0.13K Hebral5 1980 0.1K Clark6 2005 0.08K They all observed T3 phonon contribution. Their sample cells used in these experiments were all constructed with heavy wall metal or epoxy which contribute significantly to the heat capacity at low temperature. E. C. Heltemes and C. A. Swenson, Phys. Rev. 128, 1512 (1962); H. H. Sample and C. A. Swenson, Phys. Rev. 158, 188 (1967). D. O. Edwards and R. C. Pandorf, Phys. Rev. 140, A816 (1965). W. R. Gardner et al., Phys. Rev. A 7, 1029 (1973). S. H. Castles and E. D. Adams, J. Low Temp. Phys. 19, 397 (1975). B. Hébral et al., Phonons in Condensed Matter, edited by H. J. Maris (Plenum, New York, 1980), pg. 169. A. C. Clark and M. H. W. Chan, J. Low Temp. Phys. 138, 853 (2005).

Results from Edwards and Hebral The background problem Edwards Hebral Effect of changing 1% of the empty cell

Temperature scale based on Results: pure 4He (0.3ppm) The heat capacity of the empty cell at 0.2 K and 0.05 mK are respectively less than 3 % and 10 % of the heat capacity of solid helium at 27 bar. 0.3ppm Minimum temperature 40mK Temperature scale based on 3He melting curve

Specific heat peak is found when T3 term subtracted The peak is independent of 3He concentration Peak height: 20 μJ mol-1 K-1 (2.5 x 10-6 kB per 4He atom) Excess entropy: 28 μ J mol-1 K-1 (3.5 x 10-6 kB per 4He atom)

BC samples can also be grown Heat out Q ~ 500,000

Granato-Lucke applied to 4He Dislocations pinned by network, 3He, jogs? Typical LN in pure 4He crystals ~ 5mm

Ln C vs. Ln T

Compare with torsional oscillator

Solid 4He at various pressures show similar temperature dependence, but the measured supersolid fraction shows scatter with no obvious pressure dependence NCRIF NCRIF NCRIF NCRIF

Pressure dependence of supersolid fraction Blue data points were obtained by seeding the solid helium samples from the bottom of the annulus. NCRIF What are the causes of the scatter in NCRIF?

Pressure dependence of supersolid fraction Blue data points were obtained by seeding the solid helium samples from the bottom of the annulus. NCRIF What are the causes of the scatter in NCRIF?

Thermal history of 1ppb samples Velocity changes at low temperature lead to interesting behavior… Protocol followed below: (1) cooling, (2) velocity increase, (3) warming, (4) cooling 2 1 3 4

End

Specific heat with T3 term subtracted Specific heat peak is independent of 3He concentrations. Assuming 3D-xy universality class (same as the lambda transition in liquid 4He). Use two-scale-factor universality hypothesis, ρs ~0.06%. 1ppb study of TO found this number lays between 0.03% and 0.3%. Peak height: 20 μJ mol-1 K-1 (2.5 x 10-6 kB per 4He atom) Excess entropy: 28 μ J mol-1 K-1 (3.5 x 10-6 kB per 4He atom)

Hysteresis in Pressure measurement of phase separation A.N.Gan'shin, V.N.Grigor'ev, V.A.Maidanov, N.F.Omelaenko, A.A.Penzev, É.Ya.Rudavskii, A.S.Rybalko., Low Temp. Phys. 26, 869 (2000).

Dislocations Two of the common types: edge & screw Dislocation density, L = ~5  <1010 cm-2 3-d network, LN ~ 1 to 10 mm (L~105 to 107) [LN ~ 0.1 to 1 mm (L~109)]

Granato-Lucke applied to 4He Dislocations intersect on a characteristic length scale of LN ~ 1 5mm Dislocations can also be pinned by 3He impurities Distance between 3He atoms (if uniformly distributed): 1ppb  1000a ~ 0.3mm 0.3ppm  150a ~ 45nm 1%  5a ~ 15nm

3He-dislocation interaction Actual 3He concentration on dislocation line is thermally activated *Typical binding energy, W0 is 0.3K to 0.7K

3He-dislocations interaction Line considered as crossover from network pinning to 3He impurity pinning of dislocations (LNetwork ~ L3He spacing) Average length LNetwork ~ 1 to 10mm For L ~ 105 to 106cm-2 Smaller lengths (< 1mm) are expected for larger dislocation densities

Solid helium in Vycor glass Weak pressure dependence… from 40 to 65bar Strong velocity dependence

3He-4He mixtures -*[ns] *=971,000ns Question: If there is a transition between the normal and supersolid phases, where is the transition temperature?

3He-4He mixtures ( inside Vycor)

Frequency dependence -TO increases with frequency -Low temperature NCRIF unchanged ~150mK ~220mK Aoki, Graves & Kojima, PRL 99, 015301 (2007).