The Logarithmic Anomaly in the Pressure

Total Page:16

File Type:pdf, Size:1020Kb

The Logarithmic Anomaly in the Pressure The Logarithmic Anomaly in the Pressure Coefficient temperatureswere referred to theupper lambda of Helium Close to the Lambda Line" point in orderto correct for small changes in the thermometer or the measuring circuit. Points on the lambda curve were found by warm- ing the sample slowly at constant volume. Because H. A. Kierstead of the large change in thermal conductivity at the lambda transition, the heating curve showed a sharp Argonne National Laboratory, Argonne, 111. break,which could be located to within amicro- degree.The sample was held at this temperature until equilibriumwas established before reading Introduction themanometer. Then the density was changed slightly by raisingthe oilin the left limb of the Severalinvestigators have reported logarithmic manometer,and the new lambda pointwas found. anomalies in the heat capacity [I], thermal expan- The break in the heating curve was especially sharp sion[2-6], and pressure coefficient [7-81of liquid with solid present in the cell, because the heat of helium in theneighborhood of the lambda transi- meltingincreased the apparent heat capacity. tion.Unfortunately, all of theseexperiments ex- Thus the upper lambda point could be determined cept those of Lounasmaa 171 and of Lounasmaa and directly, rather than as the intersection of two inde- Inconnection with theseexperiments we have Kaunisto [8] were done on the vapor pressure curve, pendently measured curves. measured the change of pressure and density with where the anomalous behavior is confined to a very The pressure coefficient p,.=(dP/aT),.was deter- temperaturealong the lambda line. These experi- narrowtemperature interval. The experiments of minedby keeping the oil level -in the leftlimb of ments, which are reported in detail elsewhere [lo]. Lounasmaaand Kaunisto [8] atvarious pressures the manometer constant and measuring the height can be summarized by the equations alongthe lambda curve show that the anomalous of oil in the right limb at successively lower tempera- behavior is spreadout over a larger temperature tures.After the lambda point was passed, as intervalathigher pressures. Consequently, we judged by thethermal response, the temperature have measured the pressure coefficient, &=(aP/aT),., was raised slowly in order to determine the lambda of liquid helium along the isochore which crosses point exactly. thelambda line at the melting curve. This inter- section is called the upper lambda point (TA,,PA,). Results Experimental Procedure Small changes in the sample density could be made The pressure coefficient PI.= (dP/dT),. was meas- by raising the oil in the left limb of the manometer, ured along an isochore which crossed the lambda The apparatus usedin these experiments is essen- forcinggas to condense into G. A change of 0.01 line very close to Ti,. Results are shown in figure 2, tially thesame as that used by Lounasmaa [7]. mm in the oil level caused a change of 2 x 10-9 plottedagainst log,o(T-Tk). The equation of where TA is the lambda temperature for the pressure Therefore, it will be described only briefly here. It g/cm3 in thedensity. theline is P and density p, and TA'is the temperature of the is shown schematically in figure 1. Temperatures were measured with a germanium upperlambda point, 1.7633 OK. Heliumgas was purified in atrap (not shown) resistance thermometer in apotentiometer circuit p,=9.39+7.6910glo(T-T~) atm/OK, (1) immersed in liquid helium, and was condensed into .usingdoublea potentiometer. At theupper Discussion the piezometer G through the low-temperature valve lambda pointthe thermometer resistance was where Ti is the lambda transition temperature for A, which was kept closed during measurements. G 1483 R, andits sensitivity was 636 microdegrees theisochore. This graph contains points taken on Thelogarithmic dependence of PI. on T-TA wasisolated from the liquid helium bath by the perohm. With 50 pA of measuringcurrent, the two differentcooling runs. The lambda point for is similar to thatfound by Lounasmaa [7] and by vacuumcase B. Itstemperature was controlled resistancecould be measured witha precision of one run was 15 pdeg below Ti', and for the other it Lounasmaaand Kaunisto [8] atlower densities, by the heater F and by pumping on liquid helium 0.002 R. Themeasuring current heated the ther- was 5 pdeg above. These small differences are not and is consistentwith their observation that the in E. mometer above the cell temperature; but thiseffect regardedas significant, but the observed lambda two constants in eq (1) both increase with increas- Changes in thepressure on the sample were was reproducible, and the same measuring current pointwas used in eachrun in plotting T-TA. ingdensity. The measurements of Lounasmaa measured by the oil manometer K and read with a wasused in calibratingthe thermometer. It was Since this isochore meets the melting curve at the at 13 atm pressure (T~=2.023 OK) are of particular cathetometer to 0.01 mm,which corresponded to calibrated against the vapor pressure of helium in E lambda point, the measurements in figure 2 refer to interestsince he found that p,. fittedan equation abouta millionth of anatmosphere. The absolute on the T58 scale [9], using a tube separate from the 1 HeI. One pointwas measured in supercooled of the same form as (1) to within 2 x 1O-5 OK of the pressure was read to 0.01 atm on the Bourdon gage pumpingtube. The change in thethermometer He II, where wasfound to be -27.6 at T- TA lambda point for both He I and He II, the constants P, which was calibrated against a dead weight tester. betar resistance at the upper lambda point after warming =- 1.08 X lO-s. This point is not plotted in figure beingdifferent for the two cases. In thesame toroom, temperature and recooling corresponded paperLounasmaa presents measurements of the *Based on work performed under the auspices of the U.S. Atomic Energy '2, but it is approximately the value to be expected Commission, to atemperature change of lessthan lO-4 OK. All 'for T- TA = 1.08 X lO-s. compressibility KT= p"(dp/dP),r along an isotherm 92 93 passingthrough the same lambda point. He References 151 E. Maxwell and C. E. Chase, Physica 24, 5139 (19%). 161 E. C. Kerranti R. D. Taylor, Ann. Phys. (N.Y.) 26. 902 finds no evidencefor anything but a slow linear [I] W. hl. Fairbank, M. I. Buckingham, and C. F. Kellers, 96.5). Proc. 5th Int. Conf. Low Temp. Phys., Madison, Wis- 171 0.V. Lounasmaa, Phys. Rev. 130, 847 (1963). variation of KT with P- PA to within 1O-3 atm from consin (1957), p. 50: C. F. Kellers, Thesis, Duke Uni- 181 0.\’. Lounasmaa and L. Kaunisto, Ann. Acad. Sci. Fenn. the lambda line (corresponding to 2 x 10-5 OK for versity (1960). AVI. No. 59 ( 1960): Bull. Am. Phys. Soc. 5, 290 I 1960). T-Ti) and a smalldiscontinuity at the lambda [2] K. K. Atkins and M. H. Edwards, Phys. Rev. 97, 1429 (91 H. van Dijk. M. Durieux, J. R. Clement,and J. K. Logan, ( 1955). National Bureau of Standards Monograph 10, 1960. point. [3] M. H. Edwards, Can. J. Phys. 36, 884 (1958). 1101 H. A. Kierstead, 138, A1504 (1965), 141 E, Maxwell, C. E. Chase, and W. E. Millet, Proc. 5th lnt. (111 M. J. Buckingham and W. M. Fairbank, Progress in Low Sincean isochore cannot cross the lambda line Conf. Low Temp. Phys., Madison,Wisconsin (19571, TemperaturePhysics C. I. Gorter, ed.) Vol. 111, ch. III with a slope greater in magnitude than that of the p. 53. (North Holland Publishing Company, Amsterdam, 1961). lambda line, (dPld7‘)~is a lower bound for PI.(both are negative); so eq (1) must break down for some smallvalue of T-TA. Onthe other hand, there is no suchrestriction on KT. Infact, Buckingham The Nature of the Cooperative Transition and Fairbank [ll] have shown that if Cp becomes infinite at the lambda line, ~7.mustalso. The exper- iments seem to suggest that Pr becomes infinite and M. J. Buckingham KT does not. This situation can be examined more closely with the help of the equation University of Western Australia, Nedlands, Western Australia 1. Introduction action solution, each cell is properly described as a piece of‘ one or other of the phases, but in the ab- A thermodynamicsingularity arises in statis- sence of the interaction these are mixed at random. We plan to measure KT near the upper lambdapoint tical mechanics only in the limit N+ m, where N Thequalitative effect of the interactionsbetween in the near future. is the number of atoms in thesystem. By regard- cells is thus the segregation or phase separation of thecells. The entropyassociated with thissepa- To investigatethe nature of thelambda trans- ingan infinite system as made up of an infinite number of large but finite parts, called cells, with ration is constant(depending on composition) in formation, it is very important to study how KT goes the two phase region and is, of course, zero in the to infinity and how approaches (~P/~T)A(if M atoms each, the singularity is seen to arise from PI. one phase region-except for a very small tempera- indeed they do) at temperatures so close to TAthat theinteractions between the cells-which for M large correspond to surface interactions, since the tureinterval in the immediate neighborhood of cq (11 breaks down his is probablyonly pos- This equation shows that KT will not vary much the transition temperature. siblenear the upper lambda point. In Lounas- interatomicforces are short-ranged. For the same until PI. becomesnearly equal to (dP/dT)A. If P,. At first sight the very small magnitude of the mix- maa’s experiment at 13 atm the logarithmic relation reasoninteractions between other than nearest becomes equal to (dP/dT)h, as must happen if Cp ing entropy-associated with hutone degree of predicts that, for T- TA= lO-6, PI.will be less than neighborcells are zero.
Recommended publications
  • Demonstration of a Persistent Current in Superfluid Atomic Gas
    Demonstration of a persistent current in superfluid atomic gas One of the most remarkable properties of macroscopic quantum systems is the phenomenon of persistent flow. Current in a loop of superconducting wire will flow essentially forever. In a neutral superfluid, like liquid helium below the lambda point, persistent flow is observed as frictionless circulation in a hollow toroidal container. A Bose-Einstein condensate (BEC) of an atomic gas also exhibits superfluid behavior. While a number of experiments have confirmed superfluidity in an atomic gas BEC, persistent flow, which is regarded as the “gold standard” of superfluidity, had not been observed. The main reason for this is that persistent flow is most easily observed in a topology such as a ring or toroid, while past BEC experiments were primarily performed in spheroidal traps. Using a combination of magnetic and optical fields, we were able to create an atomic BEC in a toriodal trap, with the condensate filling the entire ring. Once the BEC was formed in the toroidal trap, we coherently transferred orbital angular momentum of light to the atoms (using a technique we had previously demonstrated) to get them to circulate in the trap. We observed the flow of atoms to persist for a time more than twenty times what was observed for the atoms confined in a spheroidal trap. The flow was observed to persist even when there was a large (80%) thermal fraction present in the toroidal trap. These experiments open the possibility of investigations of the fundamental role of flow in superfluidity and of realizing the atomic equivalent of superconducting circuits and devices such as SQUIDs.
    [Show full text]
  • Contents 1 Classification of Phase Transitions
    PHY304 - Statistical Mechanics Spring Semester 2021 Dr. Anosh Joseph, IISER Mohali LECTURE 35 Monday, April 5, 2021 (Note: This is an online lecture due to COVID-19 interruption.) Contents 1 Classification of Phase Transitions 1 1.1 Order Parameter . .2 2 Critical Exponents 5 1 Classification of Phase Transitions The physics of phase transitions is a young research field of statistical physics. Let us summarize the knowledge we gained from thermodynamics regarding phases. The Gibbs’ phase rule is F = K + 2 − P; (1) with F denoting the number of intensive variables, K the number of particle species (chemical components), and P the number of phases. Consider a closed pot containing a vapor. With K = 1 we need 3 (= K + 2) extensive variables say, S; V; N for a complete description of the system. One of these say, V determines only size of the system. The intensive properties are completely described by F = 1 + 2 − 1 = 2 (2) intensive variables. For instance, by pressure and temperature. (We could also choose temperature and chemical potential.) The third intensive variable is given by the Gibbs’-Duhem relation X S dT − V dp + Ni dµi = 0: (3) i This relation tells us that the intensive variables PHY304 - Statistical Mechanics Spring Semester 2021 T; p; µ1; ··· ; µK , which are conjugate to the extensive variables S; V; N1; ··· ;NK are not at all independent of each other. In the above relation S; V; N1; ··· ;NK are now functions of the variables T; p; µ1; ··· ; µK , and the Gibbs’-Duhem relation provides the possibility to eliminate one of these variables.
    [Show full text]
  • Phase Transition a Phase Transition Is the Alteration in State of Matter Among the Four Basic Recognized Aggregative States:Solid, Liquid, Gaseous and Plasma
    Phase transition A phase transition is the alteration in state of matter among the four basic recognized aggregative states:solid, liquid, gaseous and plasma. In some cases two or more states of matter can co-exist in equilibrium under a given set of temperature and pressure conditions, as well as external force fields (electromagnetic, gravitational, acoustic). Introduction Matter is known four aggregative states: solid, liquid, and gaseous and plasma, which are sharply different in their properties and characteristics. Physicists have agreed to refer to a both physically and chemically homogeneous finite body as a phase. Or, using Gybbs’s definition, one can call a homogeneous part of heterogeneous system: a phase. The reason behind the existence of different phases lies in the balance between the kinetic (heat) energy of the molecules and their energy of interaction. Simplified, the mechanism of phase transitions can be described as follows. When heating a solid body, the kinetic energy of the molecules grows, distance between them increases, and in accordance with the Coulomb law the interaction between them weakens. When the temperature reaches a certain point for the given substance (mineral, mixture, or system) critical value, melting takes place. A new phase, liquid, is formed, and a phase transition takes place. When further heating the liquid thus formed to the next critical temperature the liquid (melt) changes to gas; and so on. All said phase transitions are reversible; that is, with the temperature being lowered, the system would repeat the complete transition from one state to another in reverse order. The important thing is the possibility of co- existence of phases and their reciprocal transition at any temperature.
    [Show full text]
  • ABSTRACT for CWS 2002, Chemogolovka, Russia Ulf Israelsson
    ABSTRACT for CWS 2002, Chemogolovka, Russia Ulf Israelsson Use of the International Space Station for Fundamental Physics Research Ulf E. Israelsson"-and Mark C. Leeb "Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 9 1 109, USA bNational Aeronautics and Space Administration, Code UG, Washington D.C., USA NASA's research plans aboard the International Space Station (ISS) are discussed. Experiments in low temperature physics and atomic physics are planned to commence in late 2005. Experiments in gravitational physics are planned to begin in 2007. A low temperature microgravity physics facility is under development for the low temperature and gravitation experiments. The facility provides a 2 K environment for two instruments and an operational lifetime of 4.5 months. Each instrument will be capable of accomplishing a primary investigation and one or more guest investigations. Experiments on the first flight will study non-equilibrium phenomena near the superfluid 4He transition and measure scaling parameters near the 3He critical point. Experiments on the second flight will investigate boundary effects near the superfluid 4He transition and perform a red-shift test of Einstein's theory of general relativity. Follow-on flights of the facility will occur at 16 to 22-month intervals. The first couple of atomic physics experiments will take advantage of the free-fall environment to operate laser cooled atomic fountain clocks with 10 to 100 times better performance than any Earth based clock. These clocks will be used for experimental studies in General and Special Relativity. Flight defiiiiiiori experirneni siudies are underway by investigators studying Bose Einstein Condensates and use of atom interferometers as potential future flight candidates.
    [Show full text]
  • Thermophysical Properties of Helium-4 from 2 to 1500 K with Pressures to 1000 Atmospheres
    DATE DUE llbriZl<L. - ' :_ Demco, Inc. 38-293 National Bureau of Standards A UNITED STATES H1 DEPARTMENT OF v+ *^r COMMERCE NBS TECHNICAL NOTE 631 National Bureau of Standards PUBLICATION APR 2 1973 Library, E-Ol Admin. Bldg. OCT 6 1981 191103 Thermophysical Properties of Helium-4 from 2 to 1500 K with Pressures qc to 1000 Atmospheres joo U57Q lV-O/ U.S. >EPARTMENT OF COMMERCE National Bureau of Standards NATIONAL BUREAU OF STANDARDS 1 The National Bureau of Standards was established by an act of Congress March 3, 1901. The Bureau's overall goal is to strengthen and advance the Nation's science and technology and facilitate their effective application for public benefit. To this end, the Bureau conducts research and provides: (1) a basis for the Nation's physical measure- ment system, (2) scientific and technological services for industry and government, (3) a technical basis for equity in trade, and (4) technical services to promote public safety. The Bureau consists of the Institute for Basic Standards, the Institute for Materials Research, the Institute for Applied Technology, the Center for Computer Sciences and Technology, and the Office for Information Programs. THE INSTITUTE FOR BASIC STANDARDS provides the central basis within the United States of a complete and consistent system of physical measurement; coordinates that system with measurement systems of other nations; and furnishes essential services leading to accurate and uniform physical measurements throughout the Nation's scien- tific community, industry, and commerce. The Institute consists of a Center for Radia- tion Research, an Office of Measurement Services and the following divisions: Applied Mathematics—Electricity—Heat—Mechanics—Optical Physics—Linac Radiation 2—Nuclear Radiation 2—Applied Radiation 2 —Quantum Electronics3— Electromagnetics 3—Time and Frequency 3 —Laboratory Astrophysics 3—Cryo- 3 genics .
    [Show full text]
  • A Bibliography of Experimental Saturation Properties of the Cryogenic Fluids1
    National Bureau of Standards Library, K.W. Bldg APR 2 8 1965 ^ecknlcai rlote 92c. 309 A BIBLIOGRAPHY OF EXPERIMENTAL SATURATION PROPERTIES OF THE CRYOGENIC FLUIDS N. A. Olien and L. A. Hall U. S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS THE NATIONAL BUREAU OF STANDARDS The National Bureau of Standards is a principal focal point in the Federal Government for assuring maximum application of the physical and engineering sciences to the advancement of technology in industry and commerce. Its responsibilities include development and maintenance of the national stand- ards of measurement, and the provisions of means for making measurements consistent with those standards; determination of physical constants and properties of materials; development of methods for testing materials, mechanisms, and structures, and making such tests as may be necessary, particu- larly for government agencies; cooperation in the establishment of standard practices for incorpora- tion in codes and specifications; advisory service to government agencies on scientific and technical problems; invention and development of devices to serve special needs of the Government; assistance to industry, business, and consumers in the development and acceptance of commercial standards and simplified trade practice recommendations; administration of programs in cooperation with United States business groups and standards organizations for the development of international standards of practice; and maintenance of a clearinghouse for the collection and dissemination of scientific, tech- nical, and engineering information. The scope of the Bureau's activities is suggested in the following listing of its four Institutes and their organizational units. Institute for Basic Standards. Electricity. Metrology. Heat. Radiation Physics. Mechanics. Ap- plied Mathematics.
    [Show full text]
  • The Early Years of Quantum Monte Carlo (2): Finite- Temperature Simulations
    The Early Years of Quantum Monte Carlo (2): Finite- Temperature Simulations Michel Mareschal1,2, Physics Department, ULB , Bruxelles, Belgium Introduction This is the second part of the historical survey of the development of the use of random numbers to solve quantum mechanical problems in computational physics and chemistry. In the first part, noted as QMC1, we reported on the development of various methods which allowed to project trial wave functions onto the ground state of a many-body system. The generic name for all those techniques is Projection Monte Carlo: they are also known by more explicit names like Variational Monte Carlo (VMC), Green Function Monte Carlo (GFMC) or Diffusion Monte Carlo (DMC). Their different names obviously refer to the peculiar technique used but they share the common feature of solving a quantum many-body problem at zero temperature, i.e. computing the ground state wave function. In this second part, we will report on the technique known as Path Integral Monte Carlo (PIMC) and which extends Quantum Monte Carlo to problems with finite (i.e. non-zero) temperature. The technique is based on Feynman’s theory of liquid Helium and in particular his qualitative explanation of superfluidity [Feynman,1953]. To elaborate his theory, Feynman used a formalism he had himself developed a few years earlier: the space-time approach to quantum mechanics [Feynman,1948] was based on his thesis work made at Princeton under John Wheeler before joining the Manhattan’s project. Feynman’s Path Integral formalism can be cast into a form well adapted for computer simulation. In particular it transforms propagators in imaginary time into Boltzmann weight factors, allowing the use of Monte Carlo sampling.
    [Show full text]
  • THE LAMBDA POINT EXPERIMENT in MICROGRAVITY J. A, I,Ipa, 1), R
    THE LAMBDA POINT EXPERIMENT IN MICROGRAVITY J. A, I,ipa, 1), R. Swanson and J. A, Nisscn, I department of Physics, Stanford Univcrsit y, Stanford, CA. 94305 and T. C. 1{ Chui Jet Propulsion I,aboratory, California Institute of Technology, Pasadena, CA. 91109 in C)ctober 1992 a low temperature experiment was flown on the Space Shuttle in low earth orbit, using the J]’I. low temperature research facility. The objective of the mission was to measure the heat capacity and thermal relaxation of helium very close to the lambda point with the smearing effect of gravity removed. We describe the experiment with emphasis on the high resolution thermometry and the thermal control system. We also report preliminary results from the measurements made during the flight, and compare them with related measurements performed on the ground. The sample was a sphere 3.5 cm in diameter contained within a copper calorimeter of very high thermal conductivity. The calorimeter was attached to a pair of paramagnetic salt thermometers with noise levels in the 10-lOK range. During the mission we found that the resolution of the thermometers was degraded somewhat, due to the impact of charged particles. This effect limited the useful resolution of the measurements to about two nanokelvins from the lambda point, Submitted to Cryogenics (Space Cryogenics Workshop proceedings). 4 INTRODUCTION * In the early 70’s K, Wllsonl developed a generalized treatment of cooperative transitions that for the first time made realistic predictions for the behavior of equilibrium thermodynamic properties in the transition region. 1 lis approach took into account fluctuation effects while avoiding a commitment to a precise I larniltonian for the system, This new renormalization group (RG) formalism paved the way for numerical predictions of many ‘universal’ parameters - that is, system independent quantities - such as the exponents governing the divergence of various thermodynamic variables.
    [Show full text]
  • Pumped Helium System for Cooling Positron and Electron Traps to 1.2 K $ Ã J
    Nuclear Instruments and Methods in Physics Research A 640 (2011) 232–240 Contents lists available at ScienceDirect Nuclear Instruments and Methods in Physics Research A journal homepage: www.elsevier.com/locate/nima Pumped helium system for cooling positron and electron traps to 1.2 K $ Ã J. Wrubel a, G. Gabrielse a, , W.S. Kolthammer a, P. Larochelle a, R. McConnell a, P. Richerme a, D. Grzonka b, W. Oelert b, T. Sefzick b, M. Zielinski b, J.S. Borbely c, M.C. George c, E.A. Hessels c, C.H. Storry c, M. Weel c, A. M ullers¨ d, J. Walz d, A. Speck e a Department of Physics, Harvard University, Cambridge, MA 02138, United States b IKP, Forschungszentrum Julich¨ GmbH, 52425 Julich,¨ Germany c York University, Department of Physics and Astronomy, Toronto, Ontario, Canada M3J 1P3 d Institut fur¨ Physik, Johannes Gutenberg Universit at,¨ D-55099 Mainz, Germany e Rowland Institute at Harvard, Harvard University, Cambridge, MA 02142, United States article info abstract Article history: Extremely precise tests of fundamental particle symmetries should be possible via laser spectroscopy of Received 24 August 2010 trapped antihydrogen (H) atoms. H atoms that can be trapped must have an energy in temperature Received in revised form units that is below 0.5 K —the energy depth of the deepest magnetic traps that can currently be 4 January 2011 constructed with high currents and superconducting technology. The number of atoms in a Boltzmann Accepted 11 January 2011 distribution with energies lower than this trap depth depends sharply upon the temperature of the Available online 21 January 2011 thermal distribution.
    [Show full text]
  • Superfluidity Phase Transitions for Liquid 4He System
    DISCRETE AND CONTINUOUS doi:10.3934/dcdsb.2019045 DYNAMICAL SYSTEMS SERIES B Volume 24, Number 9, September 2019 pp. 5107{5120 SUPERFLUIDITY PHASE TRANSITIONS FOR LIQUID 4HE SYSTEM Jiayan Yang School of Medical Informatics and Engineering Southwest Medical University Luzhou, Sichuan 646000, China Dongpei Zhang∗ Department of Mathematics Sichuan University Chengdu, Sichuan 610064, China (Communicated by Shouhong Wang) Abstract. The main objective of this paper is to investigate the superfluidity phase transition theory-modeling and analysis-for liquid 4He system. Based on the new Gibbs free energy and the potential-descending principle proposed recently in [18, 25], the dynamic equations describing the λ-transition and solid- liquid transition of liquid 4He system are derived. Further, by the dynamical transition theory, the two obtained models are proven to exhibit Ehrenfest second-order transition and first-order transition, respectively, which are well consistent with the physical experimental results. 1. Introduction. Superfluidity in liquid 4He is a phase of matter, which was first described by Einstein [8] in 1925 and discovered by P. L. Kapitsa [14], J. F. Allen and D. Misener [1] in 1937, at which the liquid's viscosity becomes zero. More pre- cisely, liquid 4He with viscosity exhibits superfluid behavior, when the temperature decreases under the critical value Tc = 2:17K. Besides, the superfluid phase in liquid 4He (called Bose-liquid), is a consequent of Bose-Einstein statistics obeyed by 4He atoms. Figure 1. T -p phase diagram of 4He 2010 Mathematics Subject Classification. Primary: 34C23, 35Q99, 37G35; Secondary: 37L10. Key words and phrases. 4He system, superfluidity, Gibbs free energy, phase transition.
    [Show full text]
  • Bose–Einstein Condensation in Dilute Gases in 1925 Einstein Predicted
    Bose–Einstein Condensation in Dilute Gases In 1925 Einstein predicted that at low temperatures particles in a gas could all reside in the same quantum state. This peculiar gaseous state, a Bose– Einstein condensate, was produced in the laboratoryfor the first time in 1995 using the powerful laser-cooling methods developed in recent years. These condensates exhibit quantum phenomena on a large scale, and investigating them has become one of the most active areas of research in contemporary physics. The studyof Bose–Einstein condensates in dilute gases encompasses a number of different subfields of physics, including atomic, condensed matter, and nuclear physics. The authors of this textbook explain this exciting new subject in terms of basic physical principles, without assuming detailed knowledge of anyof these subfields. This pedagogical approach therefore makes the book useful for anyone with a general background in physics, from undergraduates to researchers in the field. Chapters cover the statistical physics of trapped gases, atomic properties, the cooling and trapping of atoms, interatomic interactions, structure of trapped condensates, collective modes, rotating condensates, superfluidity, interference phenomena and trapped Fermi gases. Problem sets are also included in each chapter. christopher pethick graduated with a D.Phil. in 1965 from the Universityof Oxford, and he had a research fellowship there until 1970. During the years 1966–69 he was a postdoctoral fellow at the University of Illinois at Urbana–Champaign, where he joined the facultyin 1970, becoming Professor of Physics in 1973. Following periods spent at the Landau Institute for Theoretical Physics, Moscow and at Nordita (Nordic Institute for Theoretical Physic, Copenhagen, as a visiting scientist, he accepted a permanent position at Nordita in 1975, and divided his time for manyyearsbetween Nordita and the Universityof Illinois.
    [Show full text]
  • Liquids and Liquid Crystals
    LIQUIDS AND LIQUID CRYSTALS FEATURES OF THE CONFINED HELIUM 4He SPECIFIC HEAT NEAR THE ¸-POINT IN PLANE MESOSCALE PORES K.A. CHALYY UDC 536.764 Taras Shevchenko Kyiv National University, Faculty of Physics °c 2006 (6, Academician Glushkov Prosp., Kyiv 03022, Ukraine; e-mail: [email protected]) The influence of the finite-size effect on the liquid helium specific be reached without the analysis of the fundamental heat and a shift of the transition temperature are theoretically experiments with confined helium. Amongst the pioneer examined for the case of planar confinement. A considerable studies of the spatial-limitation effect, we mention the growth of the specific heat manifests itself at a new transition temperature which is calculated in the context of the present helium experiment conducted by Chen and Gasparini geometric conditions. The analytic results are found to be in fair [2] more than the quarter of a century ago. More agreement with a number of experiments where 4He films were sophisticated measurements for films were reported later ranged in thickness from 48 nm to 57 ¹m that can be referred as the mesoscale values. The contributions to the shift of the on in (see, e.g., [3]). transition temperature caused by the gravitation effect and by the Conducting the experiments with confined helium finite-size effect are examined. is rather difficult due to a number of complicated circumstances. In such Earth-based measurements, the characteristic size of a sample is supposed to be small enough in order to neglect the influence of gravity. 1. Introduction On the Earth orbit, such a limitation vanishes.
    [Show full text]