An experimental study of the equation of state of liquid xenon

1973 ◽  
Vol 5 (5) ◽  
pp. 633-650 ◽  
Author(s):  
W.B. Streett ◽  
L.S. Sagan ◽  
L.A.K. Staveley
Keyword(s):  
Experimental Study ◽  
Equation Of State ◽  
Liquid Xenon

scholarly journals The critical constants and orthobaric densities of xenon

1912 ◽  
Vol 86 (591) ◽  
pp. 579-590 ◽  
Keyword(s):  
Equation Of State ◽  
Boiling Point ◽  
Periodic Table ◽  
Atomic Weight ◽  
Atomic Volume ◽  
Liquid Xenon ◽  
Rare Gases ◽  
Critical Constants

Rudorf, in a paper on the rare gases and the equation of state, has drawn attention to the high value found by Ramsay and Travers for the density of liquid xenon at its boiling point. As is well known the atomic volume in any group of elements in the periodic table either increases regularly with rise of atomic weight or remains approximately constant, so that it is to be expected that the atomic volume of xenon would be greater than of krypton, since the value for krypton exceeds that of argon. If Rudorf's calculated value for the density of neon is taken into account, this anomaly becomes more striking, as is shown from the following table taken from his paper:-

scholarly journals Experimental study of ionization yield of liquid xenon for electron recoils in the energy range 2.8–80 keV

2014 ◽  
Vol 9 (11) ◽  
pp. P11014-P11014 ◽  
Author(s):  
D.Yu. Akimov ◽  
V.V. Afanasyev ◽  
I.S. Alexandrov ◽  
V.A. Belov ◽  
A.I. Bolozdynya ◽  
...  
Keyword(s):  
Experimental Study ◽  
Energy Range ◽  
Liquid Xenon ◽  
Ionization Yield

scholarly journals NEUTRON STAR MATTER EQUATION OF STATE AND GRAVITATIONAL WAVE EMISSION

2005 ◽  
Vol 20 (31) ◽  
pp. 2335-2349 ◽  
Author(s):  
OMAR BENHAR
Keyword(s):  
Experimental Study ◽  
Neutron Star ◽  
Equation Of State ◽  
Neutron Stars ◽  
Gravitational Waves ◽  
Neutron Star Matter ◽  
Oscillation Modes ◽  
Nonradial Oscillation ◽  
Macroscopic Objects ◽  
Wave Emission

The EOS of strongly interacting matter at densities ten to fifteen orders of magnitude larger than the typical density of terrestrial macroscopic objects determines a number of neutron star properties, including the pattern of gravitational waves emitted following the excitation of nonradial oscillation modes. This paper reviews some of the approaches employed to model neutron star matter, as well as the prospects for obtaining new insights from the experimental study of gravitational waves emitted by neutron stars.

The equation of state of metastable liquid xenon near the critical point

1988 ◽  
Vol 131 (2) ◽  
pp. 119-121 ◽  
Author(s):  
V.G. Baidakov ◽  
A.M. Rubshtein ◽  
V.R. Pomortsev ◽  
I.J. Sulla
Keyword(s):  
Equation Of State ◽  
Critical Point ◽  
Liquid Xenon ◽  
Metastable Liquid
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