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Residual entropy

Residual entropy is the finite measure of disorder that persists in certain physical systems at absolute zero temperature (0 K), arising from degeneracy or frozen-in configurational randomness in the ground state that cannot be resolved even as thermal energy vanishes. This phenomenon appears to challenge the Third Law of Thermodynamics, which asserts that the entropy of a perfect, pure crystalline substance approaches zero as temperature nears 0 K, reflecting a unique ground state with no accessible microstates.^[1]^[2] In practice, residual entropy manifests in systems like amorphous solids, spin glasses, and imperfect crystals, where multiple equivalent arrangements remain indistinguishable at low temperatures.^[1] The concept gained prominence through calorimetric measurements showing discrepancies between extrapolated and observed entropies at low temperatures, highlighting inherent structural imperfections. A seminal example is solid carbon monoxide (CO), where molecules can orient randomly as C≡O or O≡C in the lattice due to their similar atomic sizes, leading to a theoretical residual entropy of S = R \ln 2 \approx 5.76 J mol⁻¹ K⁻¹, though experimental values are slightly lower at about 4.7 J mol⁻¹ K⁻¹ owing to partial ordering.^[3] Similarly, in water ice, proton positions among oxygen atoms exhibit residual disorder constrained by the Bernal-Fowler rules of hydrogen bonding, resulting in a calculated residual entropy of S = R \ln (3/2) \approx 3.37 J mol⁻¹ K⁻¹, as derived by Linus Pauling in 1935 using a statistical approximation for the number of valid configurations.^[4] This Pauling entropy for ice has been verified through experiments and simulations, confirming its value within 0.1% accuracy.^[4] Beyond molecular crystals, residual entropy appears in frustrated magnetic systems like spin ice, where geometric constraints prevent full alignment of magnetic moments, yielding a macroscopic ground-state degeneracy analogous to Pauling's ice model and resulting in entropies on the order of (1/2) R \ln (3/2) per spin.^[5] In thermodynamics, residual entropy contributes to the total entropy budget and influences phase transitions, latent heats, and the interpretation of heat capacities at low temperatures; for instance, it explains why the entropy of fusion for associated liquids like water exceeds simple predictions.^[1] Quantitatively, it is often computed via the Boltzmann formula S = k \ln W, where W is the number of degenerate ground states and k is Boltzmann's constant, underscoring the statistical mechanical foundation of the phenomenon.^[4]

Basic Concepts

Definition

Residual entropy is defined as the non-zero entropy present in a substance at absolute zero temperature (0 K), which deviates from the ideal case of a perfect crystal where the entropy is exactly zero according to the Third Law of Thermodynamics.^[6] This residual value quantifies the inherent disorder or randomness that persists in the system's ground state.^[1] It arises from frozen-in disorder or degeneracy in the accessible microstates, where kinetic barriers prevent the system from reaching the unique ground state configuration even as temperature approaches zero.^[6] In thermodynamic terms, residual entropy represents the difference between the entropy of the real substance at 0 K and that of the hypothetical ideal perfect crystal:

S_{\text{residual}} = S_{\text{real}}(0 \, \text{K}) - S_{\text{crystal}}(0 \, \text{K}),

where S_{\text{crystal}}(0 \, \text{K}) = 0.^[1] The units of residual entropy are typically joules per mole per kelvin (J/mol·K), with representative values on the order of 3.4 J/mol·K illustrating the scale of this effect in certain systems.^[7]

Relation to the Third Law of Thermodynamics

The Third Law of Thermodynamics states that the entropy of a perfect crystalline substance approaches zero as the temperature approaches absolute zero (0 K).^[8] This principle establishes an absolute zero point for entropy, resolving the arbitrary constant in thermodynamic entropy calculations and enabling the determination of absolute entropy values.^[8] The foundational basis for this law originated from Walther Nernst's heat theorem, proposed in the early 20th century, which asserts that as temperature approaches 0 K, the entropy change (ΔS) for any reversible isothermal process approaches zero.^[8] Nernst's theorem, derived from observations of heat capacities and reaction enthalpies at low temperatures, implied that chemical reactions at absolute zero occur without entropy change.^[8] Max Planck later generalized this in 1911–1912, extending it to the modern formulation of the Third Law, which posits that the entropy of all perfect crystals vanishes at 0 K, while also implying the unattainability of absolute zero temperature through any finite number of thermodynamic operations.^[9] This evolution from Nernst's empirical heat theorem to Planck's theoretical framework refined thermodynamics by linking low-temperature behavior to fundamental limits on entropy and temperature.^[9] In real materials, however, the Third Law's ideal condition of zero entropy at 0 K is often not realized due to kinetic trapping, where high activation energy barriers prevent atomic or molecular rearrangements, freezing in disordered configurations from higher temperatures.^[6] Residual entropy, defined as the non-zero entropy persisting at absolute zero in such systems, quantifies these deviations and highlights the practical distinction between idealized perfect crystals and actual substances that cannot equilibrate fully at low temperatures.^[6] The unattainability of absolute zero exacerbates this issue, as real systems remain out of equilibrium, with residual entropy representing latent configurational disorder that would require infinite time to resolve.^[10] Importantly, this residual entropy does not violate the Third Law, as the law pertains to equilibrated states; instead, it refines our understanding by emphasizing kinetic constraints in non-ideal systems.^[6] The implications of residual entropy extend to absolute entropy scales in calorimetry, where experimental determination of entropy involves integrating heat capacity (C_p) over temperature from near 0 K to the desired value, yielding S = ∫(C_p / T) dT + S_residual.^[6] For perfect crystals, the Third Law sets S_residual = 0, providing a baseline for absolute entropies; in real materials, however, the measured value includes this residual component, necessitating corrections for accurate thermodynamic predictions and comparisons with theoretical models.^[6] This approach has been crucial since the 1930s, when discrepancies between calorimetric and spectroscopic entropies first revealed residual entropy's role in bridging experimental data with the law's ideals.^[6]

Theoretical Foundations

Thermodynamic Perspective

In classical thermodynamics, the total entropy S(T) of a substance at temperature T is expressed as the sum of the thermal entropy, obtained from calorimetric measurements, and the residual entropy S_0 at absolute zero:

S(T) = \int_0^T \frac{C_p(T')}{T'} \, dT' + S_0,

where C_p is the heat capacity at constant pressure.^[11] This formulation accounts for the fact that, in systems with inherent disorder, such as imperfect crystals or glasses, S_0 > 0, representing configurational contributions that persist even as T \to 0 K.^[11] The thermal entropy term arises from reversible heat absorption during temperature changes, while S_0 reflects frozen-in disorder not removable by cooling. Calorimetric determination of entropy involves measuring C_p over a range of temperatures and extrapolating the integral to 0 K, yielding the thermal contribution alone. Discrepancies between this calorimetric entropy and values derived from spectroscopic data or theoretical models at higher temperatures reveal the presence of S_0. For example, for carbon monoxide gas at 298 K, calorimetric measurements yield an entropy of approximately 46.2 cal mol⁻¹ K⁻¹, while spectroscopic calculations predict 47.3 cal mol⁻¹ K⁻¹.^[12] The difference of about 1.1 cal mol⁻¹ K⁻¹ is attributed to the residual entropy of solid CO due to random molecular orientations, which is less than the theoretical maximum of R \ln 2 \approx 1.38 cal mol⁻¹ K⁻¹ (where R is the gas constant) owing to partial ordering.^[11] Such extrapolations highlight how residual entropy manifests as an additive constant in thermodynamic tables. Residual entropy influences the entropy changes \Delta S during phase transitions or cooling processes by reducing the apparent magnitude of ordering effects. In a freezing transition to a disordered solid, the measured \Delta S is smaller than for a fully ordered phase, as part of the configurational entropy remains in S_0, contributing to the overall process entropy. This affects the Gibbs free energy G = H - TS, where the -T S_0 term, though diminishing at low T, alters the temperature dependence of G and can stabilize disordered phases relative to ordered ones at intermediate low temperatures by lowering their free energy through the entropic contribution.^[11] Consequently, systems exhibiting residual entropy may show modified phase diagrams, with implications for low-temperature stability in materials like molecular solids.

Statistical Mechanics Explanation

In statistical mechanics, residual entropy emerges from the degeneracy of the ground state at absolute zero temperature, where multiple microstates share the lowest energy level, preventing the system from achieving a unique configuration. Boltzmann's entropy formula, applied in the limit as temperature approaches 0 K, yields S = k \ln W, where k is Boltzmann's constant and W represents the number of accessible microstates corresponding to this degenerate ground state. This formulation highlights that residual entropy quantifies the inherent disorder encoded in the multiplicity of ground-state configurations, consistent with the third law of thermodynamics allowing non-zero entropy for systems with such degeneracy./21%3A_Entropy_and_the_Third_Law_of_Thermodynamics/21.02%3A_The_3rd_Law_of_Thermodynamics_Puts_Entropy_on_an_Absolute_Scale) Entropy in solids at low temperatures arises from both configurational and vibrational contributions. Vibrational entropy, stemming from quantized harmonic oscillations around equilibrium positions, diminishes to zero as T \to 0 K because higher-energy phonon modes become inaccessible, leaving only the zero-point energy. Residual entropy, however, persists due to configurational degeneracy—arising from unresolved positional or orientational disorder in the atomic or molecular arrangements—that cannot be eliminated without surmounting significant energy barriers. This configurational component reflects the system's inability to reach a singular ordered state, even in principle, due to the multiplicity of equivalent low-energy configurations.^[13] For systems exhibiting random disorder, such as independent units with frozen-in randomness, the residual entropy can be derived generally. Consider a system comprising N such units, each capable of occupying one of g equivalent ground states independently. The total number of microstates is then W = g^N, leading to the residual entropy S_\text{residual} = k \ln (g^N) = N k \ln g. This expression captures the extensive nature of the entropy, scaling linearly with system size, and applies to scenarios like randomly oriented dipoles or substitutional alloys where correlations are negligible.^[14] Quantum effects play a crucial role in sustaining this degeneracy by prohibiting classical relaxation pathways to a unique ground state. At finite but low temperatures, thermal activation over barriers is suppressed, and as T \to 0 K, quantum tunneling between degenerate states becomes the dominant mechanism; however, for macroscopic systems, tunneling rates are exponentially small, effectively freezing the disorder in place. This quantum prohibition ensures that the system remains distributed across the degenerate microstates, preserving the residual entropy.^[15]

Notable Examples

Water Ice

Hexagonal ice (Ih), the common form of ice at atmospheric pressure, exhibits residual entropy due to proton disorder within its crystalline structure. The oxygen atoms in ice Ih form a tetrahedral network connected by hydrogen bonds, where each water molecule consists of an oxygen atom bonded to two hydrogen atoms via covalent bonds and to two others via hydrogen bonds. This arrangement adheres to the Bernal-Fowler rules, which stipulate that (1) each oxygen atom has exactly two hydrogen atoms in close proximity (covalent bonds) and two farther away (hydrogen bonds), and (2) along each O-O bond, there is exactly one hydrogen atom. These rules permit multiple equivalent configurations for the positions of the protons (or deuterons in heavy ice), as the hydrogens can occupy different allowed positions without violating the local bonding constraints, leading to a macroscopic degeneracy at absolute zero temperature.^[16]^[17] In 1935, Linus Pauling provided an approximate calculation of this residual entropy by estimating the number of valid proton configurations. For a system of N water molecules, Pauling approximated the total number of configurations W as \left( \frac{3}{2} \right)^N, accounting for the fact that each oxygen has six possible ways to place its two hydrogens (out of 16 total orientations) while satisfying the ice rules on average across the lattice. The resulting residual entropy per mole is then given by the statistical mechanics relation S = R \ln W / N = R \ln \left( \frac{3}{2} \right), where R is the gas constant, yielding approximately 3.37 J/mol·K. This approximation assumes independence of local configurations and neglects long-range correlations, but it closely matches experimental observations.^[7] Calorimetric measurements confirm the presence of this residual entropy. In 1936, Giauque and Stout integrated the heat capacity of ice from low temperatures up to 273 K and found that the extrapolated entropy at 0 K is about 3.41 J/mol·K, slightly higher than Pauling's estimate due to subtle correlations in the proton arrangements. Modern simulations refine this further, showing the exact value for ice Ih to be around 3.414 J/mol·K.^[18]^[19] Other ice phases, such as cubic ice (Ic), display similar proton disorder but with slight differences arising from their distinct lattice geometries. While ice Ih has a wurtzite-like hexagonal stacking, ice Ic features a diamond-like cubic structure, leading to a residual entropy of approximately 3.41 J/mol·K, nearly identical to that of Ih, with only subtle differences arising from the distinct lattice geometries under the same Bernal-Fowler constraints. This comparison highlights how subtle structural variations influence the degree of frozen-in disorder.^[17]^[20]

Carbon Monoxide and Similar Diatomic Molecules

In the solid phase at low temperatures, carbon monoxide (CO) forms a cubic crystal structure in the Pa3 space group, characterized by nearly symmetric head-to-tail packing of the diatomic molecules. This arrangement permits random orientations of the CO dipoles, with each molecule able to point in one of two directions (C-O or O-C) without significant energetic preference, resulting in orientational disorder that persists to absolute zero.^[21] The residual entropy arising from this twofold degeneracy is theoretically S_\text{residual} = R \ln 2 \approx 5.76 J/mol·K, where R = 8.314 J/mol·K is the gas constant, reflecting the statistical weight of the two equally likely configurations per molecule.^[22] Experimentally, calorimetric measurements yield a value of approximately 4.6 J/mol·K for CO, slightly lower than the ideal prediction due to minor energetic differences between orientations but confirming the substantial disorder in the lattice.^[22] Quantum mechanical tunneling between the two orientations is possible but occurs at an exceedingly slow rate below 1 K, on the order of years or longer for reorientation, thereby preventing the system from reaching a fully ordered ground state and preserving the residual entropy at 0 K.^[23] Nitrous oxide (N₂O), another linear asymmetric diatomic-like molecule (N≡N–O), exhibits analogous behavior in its cubic crystal structure, where the lattice sites accommodate random head-to-tail disorder despite the molecular asymmetry. The two possible orientations (N₂O or O N₂) become nearly indistinguishable in the packed lattice, leading to a theoretical residual entropy of R \ln 2 \approx 5.76 J/mol·K.^[22] Experimental determination gives a value of about 5.8 J/mol·K, closely matching the prediction and highlighting the role of persistent orientational randomness.^[22] Like CO, quantum tunneling minimally resolves this disorder at cryogenic temperatures, ensuring nonzero entropy as T approaches 0 K.^[24]

Amorphous Solids and Glasses

Glasses are non-crystalline solids formed when a supercooled liquid is cooled below its glass transition temperature without undergoing crystallization, resulting in a kinetically arrested structure that retains short-range order but lacks long-range periodicity.^[25] This process traps the material in a metastable state where atomic or molecular arrangements are fixed on experimental timescales, preventing equilibrium reconfiguration.^[26] In amorphous solids and glasses, the configurational entropy—arising from the multitude of possible structural arrangements—does not fully relax to zero as temperature approaches absolute zero; instead, the value at the glass transition temperature T_g becomes effectively frozen and persists as residual entropy at 0 K.^[27] This residual configurational entropy typically ranges on the order of several J/mol·K, reflecting the incomplete exploration of the potential energy landscape during rapid cooling.^[27] The presence of this residual entropy is intimately linked to the Kauzmann paradox, which arises from extrapolating the entropy of a supercooled liquid below T_g: without vitrification, the liquid's configurational entropy would eventually drop below that of the corresponding crystal, potentially leading to negative excess entropy, violating the third law of thermodynamics.^[28] However, the freezing of configurational entropy in glasses provides a resolution by maintaining a positive excess entropy at 0 K, avoiding the paradoxical "entropy catastrophe" while highlighting the non-ergodic nature of the glassy state.^[28] Representative examples illustrate the variability of residual entropy based on structural complexity. In silica glass (SiO₂), the residual entropy is approximately 1.66 J/mol·K, corresponding to a relatively constrained network of corner-sharing tetrahedra with limited configurational freedom.^[29] Metallic glasses, by contrast, exhibit higher values, such as about 2.2 J/mol·K in Cu₅₀Zr₅₀, due to the greater number of accessible atomic packing configurations in their disordered metallic bonding.^[13]

Historical Development

Early Observations

In the early 20th century, calorimetric investigations into the heat capacities of gases and solids at low temperatures began to uncover entropy discrepancies that foreshadowed the concept of residual entropy. Walther Nernst's heat theorem, initially proposed in 1906 and refined by 1912, asserted that entropy changes in isothermal processes approach zero as the temperature nears absolute zero, implying a zero entropy state for perfect crystals at 0 K.^[30] These foundational ideas set the stage for experimental tests, but measurements often revealed inconsistencies for certain systems, suggesting that the absolute entropy at 0 K might not always vanish. During the 1910s and 1920s, researchers including Nernst and Franz Simon advanced low-temperature calorimetry, enabling precise heat capacity determinations down to a few kelvin for various substances. Simon's work, for instance, demonstrated that the specific heats of metals like copper and lead conform to the theorem's expectations at very low temperatures, with heat capacities approaching zero proportionally to T^3 as predicted by the Debye model. However, for molecular solids and gases, the integrated entropy from heat capacity data frequently fell short of values derived from spectroscopic observations or chemical equilibrium studies, indicating unexplained entropy contributions persisting to 0 K. These discrepancies posed early puzzles, appearing as apparent violations of Nernst's theorem in seemingly simple systems. A key example emerged in the early 1930s with carbon monoxide (CO), where calorimetric and vapor pressure measurements suggested a non-zero entropy at absolute zero. Precise calorimetry by William F. Giauque and collaborators in 1932 confirmed this, measuring the heat capacity of solid CO from 13.5 K upward and finding the entropy at 0 K to be approximately 0.98 cal/K·mol (or about 71% of R \ln 2), attributable to residual orientational disorder in the crystal.^[31] Similar anomalies were noted for nitrous oxide (N₂O), another linear molecule, where entropy comparisons in the early 1930s revealed a shortfall in calorimetric values relative to band spectrum data, implying a residual entropy on the order of R \ln 2. These observations in diatomic and triatomic molecules underscored limitations in the Nernst theorem's application to imperfect crystals, prompting further scrutiny of molecular disorder at low temperatures without yet providing a theoretical resolution.^[32]

Pauling's Contribution and Later Advances

In 1935, Linus Pauling provided a groundbreaking theoretical explanation for the residual entropy of ice by analyzing the positional disorder of hydrogen atoms in the crystal lattice. He proposed that the hydrogen positions must satisfy the Bernal-Fowler "ice rules," where each oxygen atom forms two short (covalent) and two long (hydrogen-bonded) O-H bonds with neighboring oxygens. Pauling estimated the number of valid configurations satisfying these local constraints across the entire lattice as approximately W = \left( \frac{3}{2} \right)^N, where N is the number of water molecules; this yields a residual entropy per mole of S = R \ln \frac{3}{2} \approx 3.37 J/mol·K, with R being the gas constant. This prediction was soon validated experimentally through low-temperature calorimetry. In 1936, William F. Giauque and John W. Stout measured the heat capacity of ice from 15 K to 273 K and extrapolated the entropy to absolute zero, obtaining a value of 3.42 ± 0.20 J/mol·K, which closely matches Pauling's theoretical estimate and confirms the presence of configurational disorder frozen in at low temperatures.^[18] Following Pauling's work, the concept of residual entropy was extended to other disordered systems in the post-1930s era. In the 1920s and 1930s, physicist Franz Simon applied similar ideas to amorphous solids and glasses, arguing that their kinetically arrested, non-equilibrium structures retain configurational entropy at 0 K, necessitating a reformulation of the third law to account for metastable states rather than perfect crystals.^[33] By the 1990s, advances in frustrated magnetism revived Pauling's ice model through the development of spin ice systems, such as the pyrochlore compound Ho₂Ti₂O₇ discovered in 1998, where rare-earth magnetic moments align according to analogous "2-in/2-out" ice rules on tetrahedral lattices, resulting in a macroscopic degeneracy and Pauling entropy of R \ln \frac{3}{2} per spin formula unit. Subsequent theoretical extensions in the 2000s incorporated quantum fluctuations into these models, predicting quantum residual entropy in systems like quantum spin ice, where tunneling between configurations modifies the ground-state degeneracy. Recent computational advances up to 2024 have further refined and confirmed Pauling's approximation for ice and its analogues. Multicanonical Monte Carlo simulations of ordinary ice Ih have yielded residual entropies within 0.1% of Pauling's value, accounting for long-range correlations neglected in the original estimate.^[34] Similarly, transfer-matrix methods and replica-exchange simulations applied to two-dimensional ice monolayers and artificial spin ice arrays have validated the entropy in constrained geometries, with deviations below 0.5% from the Pauling limit even in quantum analogues.^[20]

Implications and Applications

In Materials Science

In materials science, residual entropy plays a crucial role in the design and understanding of disordered materials, particularly amorphous solids where frozen-in configurational disorder persists at absolute zero, influencing macroscopic properties. This entropy arises from the inability of the system to reach complete equilibrium during cooling, leading to a non-zero configurational contribution that affects thermal and mechanical behaviors. For instance, in glasses, residual entropy contributes to abrupt changes in the thermal expansion coefficient at the glass transition temperature (Tg), where the material's volume response to temperature shifts due to the locked-in structural disorder, as observed in calorimetric and dilatometric studies of silicate and metallic glasses.^[35] The impact extends to mechanical strength, where the topological disorder associated with residual entropy enhances hardness and resistance to deformation in amorphous structures. In bulk metallic glasses (BMGs), such as Zr-based alloys, this disorder enables exceptional compressive strengths exceeding 2 GPa, far surpassing crystalline counterparts, by suppressing dislocation-mediated plasticity and promoting shear band formation under stress. Similarly, residual entropy influences supercooled liquid behavior by dictating relaxation kinetics; in these regimes, the frozen configurational states slow structural rearrangements, contributing to the non-Arrhenius viscosity increase near Tg. Systems exhibiting high residual entropy, like certain polymer and metallic glass-formers, often display fragile behavior, characterized by a steep drop in configurational entropy upon cooling, which correlates with rapid changes in transport properties and heightened sensitivity to temperature variations.^[36]^[35]^[37] Applications leverage these effects for advanced materials. Metallic glasses, with their inherent residual entropy, are employed in high-strength alloys for biomedical implants and aerospace components, where the amorphous structure provides superior wear resistance and elasticity without crystalline defects. In amorphous semiconductors, such as chalcogenide glasses used in phase-change memory devices, tailored residual entropy from compositional mixing optimizes electronic band gaps and switching speeds, enabling non-volatile electronics with low energy consumption. In 21st-century developments, entropy-stabilized oxides (e.g., (Mg,Co,Ni,Cu,Zn)O) and high-entropy alloys (HEAs) incorporate residual configurational contributions to enhance phase stability; in these multicomponent systems, the entropy term counteracts enthalpic instabilities, maintaining single-phase structures up to 1000°C and improving thermal barrier coatings for turbines. High-entropy metallic glasses further exemplify this, combining atomic disorder for robust mechanical performance in extreme environments. As noted in examples like water ice glasses, these principles underscore the broader utility of residual entropy in stabilizing amorphous phases.^[38]^[39]^[40]^[41]

Measurement Challenges and Modern Techniques

Measuring residual entropy poses significant challenges due to the fundamental limitations of experimental techniques and the nature of the systems involved. The primary method relies on integrating the heat capacity C_p divided by temperature T from near 0 K to higher temperatures, but absolute zero cannot be reached in practice, necessitating extrapolation of C_p data to 0 K. This extrapolation introduces errors, particularly when C_p approaches zero at low temperatures, as small inaccuracies in the Debye or other model fits can lead to substantial uncertainties in the residual entropy value. Additionally, distinguishing the configurational contribution to residual entropy from vibrational, electronic, or magnetic components is difficult, as the total C_p encompasses all these effects, requiring sophisticated deconvolution that may not fully isolate the disorder-related term. The classical approach to quantifying residual entropy employs adiabatic calorimetry, where samples are cooled stepwise while minimizing heat exchange with the surroundings to measure C_p accurately from approximately 1 K upward. Pioneering measurements on ice demonstrated a residual entropy of about R \ln(3/2) \approx 3.37 J/mol·K by integrating C_p/T from 15 K to 273 K and extrapolating below, revealing proton disorder frozen at low temperatures. Similar calorimetry on solid carbon monoxide yielded a residual entropy of roughly 5 J/mol·K, attributed to orientational disorder of the molecules, with integration starting from the freezing point down to 15 K via extrapolation. These techniques, while foundational, are limited by thermal equilibration times and sample purity at ultra-low temperatures.^[18]^[31] Modern techniques have extended measurements to millikelvin (mK) regimes using dilution refrigerators combined with relaxation or AC calorimetry, enabling more precise C_p data near 0 K and reducing extrapolation errors for systems like amorphous solids. Neutron scattering complements calorimetry by visualizing atomic or spin disorder directly; for instance, diffuse scattering patterns in spin ice materials reveal correlations consistent with Pauling's predicted residual entropy, without relying on thermal integration. In glasses, inelastic neutron scattering probes vibrational spectra to separate configurational disorder from lattice contributions, aiding in entropy deconvolution. Computational density functional theory (DFT) predicts the degeneracy W of ground-state configurations by optimizing structures and estimating disorder entropy via S = k \ln W, as demonstrated in ice where DFT confirms near-degeneracy of hydrogen-bond networks leading to S \approx R \ln(3/2).^[42] In the 2020s, quantum simulators have emerged to mimic and directly measure residual entropy in artificial systems, overcoming classical measurement limits. Rydberg atom arrays configured as three-dimensional pyrochlore lattices simulate quantum spin ice, where site-resolved readout quantifies spin configurations and extracts entropy from the degeneracy of the emergent U(1) spin liquid ground state, matching theoretical predictions without thermal equilibration issues. These platforms allow controlled probing of disorder dynamics, providing benchmarks for natural materials like ice or glasses.^[43]

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Dec 29, 2020 · The most fragile glasses are those exhibiting low hopping barriers and, more importantly, dramatic drops of entropies upon cooling toward the glass transition ...Missing: residual | Show results with:residual
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In each case, a different amount of residual entropy will remain trapped in the glass as part of its thermal history. ... entropy trapped in pure glasses.
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The calculated entropy of the transition is 91% of the ideal configurational entropy associated with H-bond disordering compared with experimentally reported ...
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Feb 6, 2025 · This paper proposes a U(1) quantum spin liquid in 3D using Rydberg atoms in a pyrochlore lattice, where spins fail to order due to quantum ...Missing: 2020s | Show results with:2020s