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Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

Scientific and Technical Aerospace Reports Volume 39 April 6, 2001

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apply either steady shear flow perpendicular to the stretching direction, or oscillatory squeeze flow parallel to stretching. We<br />

observe that oscillatory, parallel pre-straining accelerates strain hardening in dilute polystyrene-based polymer solutions, while<br />

steady, orthogonal preshearing delays strain hardening. These results are qualitatively consistent with the predictions of the<br />

finitely extensible nonlinear elastic (FENE) dumbbell model. Recent experimental <strong>and</strong> numerical studies of stretching DNA<br />

chains by Chu & co-workers show that the transient evolution of the polymeric microstructure is very sensitive to the initial configuration<br />

of the chains. Larson recently reported results of Brownian dynamics simulations investigating the effect of preshearing<br />

on the molecular configuration of the chain. The simulations showed that preshearing reduces the occurrence of folds <strong>and</strong> kinks<br />

in the chain conformations observed during subsequent uniaxial elongation. Simple shear flow perpendicular to the stretching<br />

direction yielded a faster approach of the transient tensile stresses to the steady state plateau. The filament stretching rheometer<br />

presents new possibilities for investigating preshearing effects more quantitatively than has previously been possible. We examine<br />

the effects of (1) steady shear flow perpendicular to the stretching direction, <strong>and</strong> (2) oscillatory squeeze flow parallel to stretching,<br />

on the transient stress growth in a dilute polymer solution.<br />

Author (revised)<br />

Deformation; Elongation; Microgravity; Polystyrene; Tensile Stress; Hardening (Materials); Stretching<br />

<strong>2001</strong>0025021 National Inst. of St<strong>and</strong>ards <strong>and</strong> Technology, Process Measurements Div., Gaithersburg, MD USA<br />

Acoustic Study of Critical Phenomena in Microgravity<br />

Moldover, M. R., National Inst. of St<strong>and</strong>ards <strong>and</strong> Technology, USA; Gillis, K. A., National Inst. of St<strong>and</strong>ards <strong>and</strong> Technology,<br />

USA; Zimmerli, G. A., National Center for Microgravity Research on Fluids <strong>and</strong> Combusiton, USA; Proceedings of the Fifth<br />

Microgravity Fluid Physics <strong>and</strong> Transport Phenomena Conference; December 2000, pp. 1888-1907; In English; See also<br />

<strong>2001</strong>0024890; No Copyright; Avail: CASI; A03, Hardcopy; A10, Microfiche<br />

We plan an acoustic study of xenon near its liquid-vapor critical point in microgravity. We will use a novel, compact acoustic<br />

resonator in microgravity to determine both the speed of sound c <strong>and</strong> the bulk viscosity zeta. In lowest order, the resonance frequencies<br />

determine c <strong>and</strong> the ”quality factors” of the resonance modes determine zeta. In microgravity, the data for zeta will be<br />

a factor of 60 closer to the critical temperature T(sub c) than is possible on earth. The microgravity data will provide c the most<br />

rigorous possible test of the fundamental theory for zeta, i.e. the theory for the time-correlations of pairs of critical fluctuations.<br />

by using both Helmholtz <strong>and</strong> organ-pipe modes of the same compact resonator, the acoustic data will span a 30:1 frequency ratio<br />

at unusually low frequencies: 120 Hz to 4 kHz. Within 6 mK of T(sub c), where the reduced temperature t is identical to (T - T(sub<br />

c))/T(sub c) is less than 2x10(exp -5) , the critical fluctuations are so slow that the equilibrium condition: (acoustic frequency)<br />

x (fluctuation lifetime) is much less than 1 is violated, even at 120 Hz. In this very-near-critical region, c is frequency-dependent<br />

<strong>and</strong> the attenuation of sound is dominated by zeta. Further from the critical point, where t is greater than 2x10(exp -5) , the low-frequency<br />

speed-of-sound data obtained in microgravity will determine the constant-volume heat capacity C(sub V), perhaps with<br />

higher resolution than direct measurements of C(sub v). If so, the acoustic data will further constrain the theory for the ”crossover”<br />

of C(xub v) from an asymptotic divergence with the critical exponent (alpha) to non-critical behavior. The quality-factor data will<br />

test the theory of the thermal boundary layer in heretofore inaccessible ranges of frequency <strong>and</strong> fluid properties. The planned<br />

experiment will exploit hardware that two of PIs (Moldover <strong>and</strong> Zimmerli) helped develop for the Critical Viscosity of Xenon<br />

(CVX) experiment. The CVX flight package consisted of two ”Hitchhiker ” canisters that can be accommodated by many Shuttle<br />

missions. In 1997, the package was flown in the cargo bay of the shuttle Discovery (STS 85). The package successfully measured<br />

the shear viscosity of xenon 100 times closer to T(sub c) than ground-based experiments <strong>and</strong> it produced the first reliable measurements<br />

of visco-elasticity near any critical point. With minor modifications, the proposed experiment will use the CVX flight thermostat<br />

<strong>and</strong> hardware for temperature measurement <strong>and</strong> control. Two of the PIs (Gillis <strong>and</strong> Moldover) developed the double<br />

Helmholtz resonator (now called the ”Greenspan acoustic viscometer” ) to measure the viscosities of gases accurately. to date,<br />

no acoustic viscometer has been operated with a near-critical fluid. Thus, the first task is to design an acoustic viscometer for use<br />

with a near-critical sample of xenon. This may require modifying electro-acoustic transducers <strong>and</strong> developing a surface coating<br />

for the viscometer’ s interior. Extensive tests will be required to verify that the viscometer operates in accord with the theory for<br />

the instrument. Then, the viscometer will be used to make the best possible measurements of c <strong>and</strong> zeta on earth over the full range<br />

of accessible frequencies. These measurements will be used to define the microgravity experiment <strong>and</strong> they will be used to<br />

compare ground-based <strong>and</strong> microgravity data.<br />

Author (revised)<br />

Acoustic Properties; Critical Point; Microgravity; Viscosity; Xenon; Liquid-Vapor Interfaces; Acoustics<br />

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