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1 are found to follow a lever rule and obey an equation of state.
2 use these to obtain the system's 2D osmotic equation of state.
3 ontrast with a standard extrapolation of the equation of state.
4 harge state distribution, opacity and plasma equation of state.
5 he cluster mass distribution and dark energy equation of state.
6 ls of capillary pressure using Peng-Robinson equation of state.
7 phase were calculated from the Peng-Robinson equation of state.
8 tion and could be described by a hard sphere equation of state.
9 tivity) do not require one to fix a specific equation of state.
10 are modeled with the cubic-plus-association equation-of-state.
11 f-state tables with those from the ideal gas equation-of-state.
12 ssure scales based on the reduced shock-wave equations of state alone may predict pressure variations
13 mong rather than within molecular motors, an equation of state and an expression for energy output ca
15 )) has been achieved using the Peng-Robinson equation of state and ignoring all binary interactions w
16 n strongly constrain the neutron star matter equation of state and rule out theoretical models of the
17 rst and Second Laws seems derivable from the equation of state and the First Law's energy function.
18 ilica, alpha-quartz, and stishovite yielding equation-of-state and electronic conductivity data at un
19 , and composition based on the Peng-Robinson equation-of-state and the modified Henry's law (Krychevs
20 useful benchmarks for developing theoretical equation-of-state and transport models in the warm dense
21 Our results provide the best constrained equations of state and phase boundaries available for si
26 urements, we observe scaling behavior of the equation of state at low temperatures, locate the quantu
28 er pressure, implying that only a high-order equation of state can accurately describe the density ev
29 llow for direct quantitative measurements of equation-of-state, conductivity, opacity, and stopping p
30 muscle are immediately described by a muscle equation of state containing muscle force as a state var
33 els using extrapolated or calculated thermal equation-of-state data without considering the effects o
34 g, together with the corresponding empirical equation of state, effectively relates the phase diagram
37 solid-state materials are described by their equations of state (EOSs), which are often derived from
39 riedmann-Robertson-Walker universe where the equation of state for the cosmological fluid is uncertai
43 al results, Peng-Robinson, PC-SAFT, and GERG Equations of State for were validated CO2+CO under the c
44 yses, we rule out strongly repulsive nuclear equations of state from relativistic mean field theory a
45 e comprehensive set of proposed quark-matter equations of state from the literature, and conclude tha
47 this phenomenon, a general, first-principles equation of state has been developed by extending scaled
48 the phenomenon is intimately related to the equation of state; hence, an accurate treatment is cruci
50 ge of the Hubble constant, unless the cosmic equation of state is dominated by a component that viola
51 rrently proposed hyperon or boson condensate equations of state (M(middle dot in circle), solar mass)
53 f neutron stars provide a direct test of the equation of state of cold nuclear matter, a relationship
54 Such large neutron star masses constrain the equation of state of matter at or beyond the nuclear equ
55 studied the elasticity and pressure-density equation of state of MgO in diamond cells to 55 GPa and
57 d to establish internally consistent thermal equations of state of Au, Pt, NaCl-B2, and solid Ne.
58 n ensured by first obtaining self-consistent equations of state of gold, platinum, and tungsten in st
59 antle depend on comparing laboratory-derived equations of state of mantle phases with seismically det
60 n theory, we obtain the thermal pressure and equations of state of silica phases up to Earth's core-m
62 but finite proper thickness l of fluid with equation of state p = +rho, replacing both the Schwarzsc
63 e current 2sigma contours on the dark energy equation-of-state parameter w(x) by approximately 30%.
64 s leads to 5% constraints on the dark energy equation-of-state parameter, and limits possible deviati
65 nt Al2O3 has yielded different values of the equation of state parameters, with the bulk modulus bein
66 erties such as bandgaps, Curie temperatures, equation-of-state parameters and densities of states.
68 HD approach includes correlations in the the equation of state self-consistently, satisfies sum rules
69 rmal conductivity and LEOS for Au/Al release equation-of-state show good agreement with data after 15
70 n three times that of stable nuclei, but not equations of state softened at higher densities because
71 ned by comparing predictions from the SESAME equation-of-state tables with those from the ideal gas e
74 ur results provide constraints on the carbon equation of state, which is of critical importance for d
75 AW-GGA can be described by a Birch-Murnaghan equation of state with = 687.4 A(3), = 51.7 GPa, and = 4
76 istic mean field theory and weakly repulsive equations of state with phase transitions at densities l
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