ライフサイエンスコーパス: equation of state

1 derived from a Cubic Plus Association (CPA) equation of state.

2 odynamic properties as encapsulated by their equation of state.

3 llowing for robust tests of the neutron star equation of state.

4 previously developed data-driven rheological equation of state.

5 ls of capillary pressure using Peng-Robinson equation of state.

6 are found to follow a lever rule and obey an equation of state.

7 use these to obtain the system's 2D osmotic equation of state.

8 ontrast with a standard extrapolation of the equation of state.

9 harge state distribution, opacity and plasma equation of state.

10 he cluster mass distribution and dark energy equation of state.

11 field theory, to constrain the neutron-star equation of state.

12 phase were calculated from the Peng-Robinson equation of state.

13 tion and could be described by a hard sphere equation of state.

14 tivity) do not require one to fix a specific equation of state.

15 f-state tables with those from the ideal gas equation-of-state.

16 are modeled with the cubic-plus-association equation-of-state.

17 ane coverage by ENTH, validating theoretical equations of state.

18 ent between the theoretical and experimental equations of state.

19 ligent models have high accuracy compared to equations of state.

20 rong correlations to the diamond and methane equations of state.

21 nary and on details of their largely unknown equation of state, a dynamically evolving and short-live

22 ssure scales based on the reduced shock-wave equations of state alone may predict pressure variations

23 mong rather than within molecular motors, an equation of state and an expression for energy output ca

24 r fractions calculated from the water virial equation of state and equilibrium constants.

25 )) has been achieved using the Peng-Robinson equation of state and ignoring all binary interactions w

26 Both processes substantially affect the equation of state and radiation transport and, therefore

27 n strongly constrain the neutron star matter equation of state and rule out theoretical models of the

28 acticality of this cell by studying: (1) the equation of state and second virial coefficients of conc

29 The measured equation of state and structural parameters have been co

30 rst and Second Laws seems derivable from the equation of state and the First Law's energy function.

31 namic properties are vital to build accurate equation of state and transport models.

32 g of white dwarf physics is sensitive to the equation of state and where models differ considerably.

33 ilica, alpha-quartz, and stishovite yielding equation-of-state and electronic conductivity data at un

34 , and composition based on the Peng-Robinson equation-of-state and the modified Henry's law (Krychevs

35 useful benchmarks for developing theoretical equation-of-state and transport models in the warm dense

36 pressures and temperatures, determined their equations of state and analyzed the evolution of the pol

37 ed hybrid paradigm is more reliable than the equations of state and available correlations in the lit

38 Our results provide the best constrained equations of state and phase boundaries available for si

39 The calculated lattice constants, equation of states, and atomic coordinates are in excell

40 Using a finite strain equation of state approach, the elastic bulk and shear m

41 calculations, the obtained melting curve and equation of state are valid up to at least 815 GPa, at w

42 particular, we demonstrate that equilibrium equations of state are also valid out of equilibrium, an

43 We determine the equation of state as a function of density, temperature,

44 The correct equation of state as well as nonlocality of interactions

45 A quasi-hydrostatic equation of state at ambient temperature has also been c

46 In addition, a quasi-hydrostatic equation of state at ambient temperature has been experi

47 urements, we observe scaling behavior of the equation of state at low temperatures, locate the quantu

48 consistent with three-dimensional Heisenberg equation of state calculations including a narrow distri

49 lications for the standard approaches to the equation of state calculations.

50 er pressure, implying that only a high-order equation of state can accurately describe the density ev

51 llow for direct quantitative measurements of equation-of-state, conductivity, opacity, and stopping p

52 muscle are immediately described by a muscle equation of state containing muscle force as a state var

53 Shock-compression equation-of-state data and optical reflectivities of the

54 These equation-of-state data can now be compared to first-prin

55 i-absolute, high-precision, pressure-density equation-of-state data for gold and platinum.

56 els using extrapolated or calculated thermal equation-of-state data without considering the effects o

57 We observed that the equation of state degenerates, and there is a universal

58 es.(4)(,)(5) A recently published ecological equation of state demonstrated a strong relationship bet

59 t cell vs pressure relation) into the atomic equation of states describing dependencies of atomic cha

60 ns are fundamental challenges for lanthanide equation of state development.

61 g, together with the corresponding empirical equation of state, effectively relates the phase diagram

62 Detailed study of the equation of state, elasticity, and hardness of selected

63 , and resolving the underlying parameterized equation of state (EoS) and crush porosity model paramet

64 re, offered a prototypical example of how an equation of state (EoS) can succinctly capture key prope

65 (MD) simulations are performed to derive an equation of state (EOS) for helium (He) bubbles in tungs

66 The equation of state (EOS) is essential for understanding m

67 We present structure and equation of state (EOS) measurements of biaxially orient

68 Here we report that the equation of state (EOS) of Mo is obtained by an integrat

69 symmetry, predicting a specific form for its equation of state (EoS), but it is currently unknown whe

70 as those characterizing material properties, equation of state (EOS), opacities, and initial conditio

71 tidal signature depends predominantly on the equation of state (EoS)-related tidal deformability para

72 his stress range and we have constrained its equation of state (EOS).

73 ly, R(s) was estimated using seven different equations of state (EoS).

74 Equations of state (EOSs) are limited in accurately pred

75 Also, five equations of state (EOSs) including Redlich-Kwong (RK),

76 ted, and the results were compared with four equations of state (EOSs), including Peng-Robinson (PR),

77 Moreover, three famous equations of state (EOSs), namely Peng-Robinson (PR), Va

78 solid-state materials are described by their equations of state (EOSs), which are often derived from

79 The 300 K equations of state fit to our P-V data collected on gold

80 priate set of state variables and extract an equation of state for laboratory midge swarms.

81 Sinhuber et al. formulated an equation of state for laboratory swarms of the non-bitin

82 The thermodynamic equation of state for liquid Fe84C16 is also obtained fr

83 The equation of state for m(e)(B) is w = -1, which implies t

84 We study also the equation of state for microstructure entropy.

85 l which, as only inputs, requires a reliable equation of state for the bulk free energy and the inter

86 riedmann-Robertson-Walker universe where the equation of state for the cosmological fluid is uncertai

87 An equation of state for the free energy of self-assembly f

88 Using the equation of state for the same sample, the shear-, compr

89 ss the quality of the Perdew-Burke-Ernzerhof equations of state for 71 elemental crystals.

90 Moreover, we show that the equations of state for a wide range of interaction stren

91 lusion is based on a limited set of possible equations of state for quark matter.

92 al results, Peng-Robinson, PC-SAFT, and GERG Equations of State for were validated CO2+CO under the c

93 yses, we rule out strongly repulsive nuclear equations of state from relativistic mean field theory a

94 e comprehensive set of proposed quark-matter equations of state from the literature, and conclude tha

95 rough the Fluctuation Theory-based Tait-like Equation of State (FT-EoS).

96 The thermal equation of state has been determined based upon the dat

97 this phenomenon, a general, first-principles equation of state has been developed by extending scaled

98 the phenomenon is intimately related to the equation of state; hence, an accurate treatment is cruci

99 cles via external stimuli, and show that our equation of state holds throughout.

100 The equation of state implies a mass-radius relation, while

101 d proxies, the performance of the ecological equation of state in predicting biomass varied systemati

102 ge of the Hubble constant, unless the cosmic equation of state is dominated by a component that viola

103 If the neutron-star equation of state is sufficiently stiff (that is, the pr

104 .e., the BMP+[Formula: see text] rheological equation-of-state, is used as a theoretical approach to

105 rrently proposed hyperon or boson condensate equations of state (M(middle dot in circle), solar mass)

106 en at significantly lower pressures, and the equation of state measured agrees with our findings.

107 From the equation-of-state measurement, we determine the molecula

108 The three desired properties of a general Equation of State model are adherence to the Laws of The

109 Equations of State model relations between thermodynamic

110 alculations and serve as key touchstones for equation of state modeling.

111 mmary of the physical property measurements, equations of state modeling, molecular simulations, sepa

112 r constraining both thermal conductivity and equation-of-state models.

113 essure-viscosity coefficient and the assumed equation of state must limit the use of the classical fo

114 Nonetheless, the equation of state obtained by Sinhuber et al. is anomalo

115 We report the Hugoniot equation of state of a martian analog basalt and single-

116 stressed diamond anvils correlated with the equation of state of Au and does not require an addition

117 ults, it was possible to determine a thermal equation of state of chromium valid up to 65 GPa and 210

118 f neutron stars provide a direct test of the equation of state of cold nuclear matter, a relationship

119 TIP4P/2005, adding to the similarity in the equation of state of liquid water in both models.

120 Such large neutron star masses constrain the equation of state of matter at or beyond the nuclear equ

121 This is relevant for the equation of state of matter at pressures ranging from 10

122 studied the elasticity and pressure-density equation of state of MgO in diamond cells to 55 GPa and

123 The isothermal equation of state of silicon has been determined by sync

124 he NMMA code has allowed us to constrain the equation of state of supranuclear dense matter, to measu

125 diagrammatic Monte Carlo calculation of the equation of state of the 2D SU(N) Hubbard model in an ex

126 Quantitative analysis of the measured equation of state of the bundles revealed the contributi

127 Our results illuminate the equation of state of the white dwarf envelope (the regio

128 d to establish internally consistent thermal equations of state of Au, Pt, NaCl-B2, and solid Ne.

129 n ensured by first obtaining self-consistent equations of state of gold, platinum, and tungsten in st

130 antle depend on comparing laboratory-derived equations of state of mantle phases with seismically det

131 n theory, we obtain the thermal pressure and equations of state of silica phases up to Earth's core-m

132 e used either "from scratch" to learn a full Equation of State, or in conjunction with a pre-existing

133 e sun; for example, through the opacity, the equation of state, or wave motion.

134 but finite proper thickness l of fluid with equation of state p = +rho, replacing both the Schwarzsc

135 e current 2sigma contours on the dark energy equation-of-state parameter w(x) by approximately 30%.

136 s leads to 5% constraints on the dark energy equation-of-state parameter, and limits possible deviati

137 r, more proximal, seismic events to seek the equation of state parameters that best describe the liqu

138 nt Al2O3 has yielded different values of the equation of state parameters, with the bulk modulus bein

139 erties such as bandgaps, Curie temperatures, equation-of-state parameters and densities of states.

140 be the materials in terms of the density and equations of state rather than specific atomic structure

141 tigate how the performance of the ecological equation of state relates to expected ecosystem conditio

142 A theory-derived ecological equation of state relating biodiversity, productivity, a

143 The measurements test these equation-of-state relations that are used in the modelli

144 A fourth-order Birch-Murnaghan equation of state reproduces our experimental data over

145 HD approach includes correlations in the the equation of state self-consistently, satisfies sum rules

146 rmal conductivity and LEOS for Au/Al release equation-of-state show good agreement with data after 15

147 Moreover, four Equation of States [Soave-Redlich-Kwong, Peng-Robinson,

148 n three times that of stable nuclei, but not equations of state softened at higher densities because

149 Here, we investigate the equation of state, speciation, and transport properties

150 ost of our method open new opportunities for equation-of-state studies.

151 ned by comparing predictions from the SESAME equation-of-state tables with those from the ideal gas e

152 onditions differing from predictions by some equations of state tables, which underlines the influenc

153 differential performance was stronger in the equation of state than in correlative models fit to the

154 into a neural-network-based learning of the equations of state that allows for efficient constructio

155 or any reflector (VISAR) results extends the equation of state to over 800 GPa.

156 We fit the simulation data to a two-state equation of state to provide an estimate of the LLCP's l

157 e fitted remarkably well using the Two-State-Equation-of-State (TSEOS).

158 planets and calls for a reformulation of the equations of state used to model them.

159 rams calculated from the Peng-Robinson cubic equation-of-state using one-parameter mixing rules.

160 Additionally, we deconvoluted the equation of state (volume of the unit cell vs pressure r

161 ur results provide constraints on the carbon equation of state, which is of critical importance for d

162 AW-GGA can be described by a Birch-Murnaghan equation of state with = 687.4 A(3), = 51.7 GPa, and = 4

163 ive very similar third-order Birch-Murnaghan equations of state with bulk moduli of 182-185 GPa and r

164 istic mean field theory and weakly repulsive equations of state with phase transitions at densities l

165 We also measure equations of state with tunable dipolar interactions.

166 are compatible with extrapolated hydrostatic equations of state within 1% up to 4 Mbar.