Entropy

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Entropy
Common symbols	S
SI unit	joules per kelvin (J⋅K−1)
In SI base units	kg⋅m2⋅s−2⋅K−1

Thermodynamics
The classical Carnot heat engine

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Entropy articles
Introduction History Classical entropy Statistical entropy

Entropy is a scientific concept as well as a measurable physical property that is most commonly associated with a state of disorder, randomness, or uncertainty. The term and the concept are used in diverse fields, from classical thermodynamics, where it was first recognized, to the microscopic description of nature in statistical physics, and to the principles of information theory. It has found far-ranging applications in chemistry and physics, in biological systems and their relation to life, in cosmology, economics, sociology, weather science, climate change, and information systems including the transmission of information in telecommunication.

The thermodynamic concept was referred to by Scottish scientist and engineer Macquorn Rankine in 1850 with the names thermodynamic function and heat-potential. In 1865, German physicist Rudolf Clausius, one of the leading founders of the field of thermodynamics, defined it as the quotient of an infinitesimal amount of heat to the instantaneous temperature. He initially described it as transformation-content, in German Verwandlungsinhalt, and later coined the term entropy from a Greek word for transformation. Referring to microscopic constitution and structure, in 1862, Clausius interpreted the concept as meaning disgregation.

A consequence of entropy is that certain processes are irreversible or impossible, aside from the requirement of not violating the conservation of energy, the latter being expressed in the first law of thermodynamics. Entropy is central to the second law of thermodynamics, which states that the entropy of isolated systems left to spontaneous evolution cannot decrease with time, as they always arrive at a state of thermodynamic equilibrium, where the entropy is highest.

Austrian physicist Ludwig Boltzmann explained entropy as the measure of the number of possible microscopic arrangements or states of individual atoms and molecules of a system that comply with the macroscopic condition of the system. He thereby introduced the concept of statistical disorder and probability distributions into a new field of thermodynamics, called statistical mechanics, and found the link between the microscopic interactions, which fluctuate about an average configuration, to the macroscopically observable behavior, in form of a simple logarithmic law, with a proportionality constant, the Boltzmann constant, that has become one of the defining universal constants for the modern International System of Units (SI).

In 1948, Bell Labs scientist Claude Shannon developed similar statistical concepts of measuring microscopic uncertainty and multiplicity to the problem of random losses of information in telecommunication signals. Upon John von Neumann's suggestion, Shannon named this entity of missing information in analogous manner to its use in statistical mechanics as entropy, and gave birth to the field of information theory. This description has been identified as a universal definition of the concept of entropy.

History

Rudolf Clausius (1822–1888), originator of the concept of entropy

 

Main article: History of entropy

In his 1803 paper, Fundamental Principles of Equilibrium and Movement, the French mathematician Lazare Carnot proposed that in any machine, the accelerations and shocks of the moving parts represent losses of moment of activity; in any natural process there exists an inherent tendency towards the dissipation of useful energy. In 1824, building on that work, Lazare's son, Sadi Carnot, published Reflections on the Motive Power of Fire, which posited that in all heat-engines, whenever "caloric" (what is now known as heat) falls through a temperature difference, work or motive power can be produced from the actions of its fall from a hot to cold body. He used an analogy with how water falls in a water wheel. That was an early insight into the second law of thermodynamics. Carnot based his views of heat partially on the early 18th-century "Newtonian hypothesis" that both heat and light were types of indestructible forms of matter, which are attracted and repelled by other matter, and partially on the contemporary views of Count Rumford, who showed in 1789 that heat could be created by friction, as when cannon bores are machined. Carnot reasoned that if the body of the working substance, such as a body of steam, is returned to its original state at the end of a complete engine cycle, "no change occurs in the condition of the working body".

The first law of thermodynamics, deduced from the heat-friction experiments of James Joule in 1843, expresses the concept of energy, and its conservation in all processes; the first law, however, is unsuitable to separately quantify the effects of friction and dissipation.

In the 1850s and 1860s, German physicist Rudolf Clausius objected to the supposition that no change occurs in the working body, and gave that change a mathematical interpretation, by questioning the nature of the inherent loss of usable heat when work is done, e.g., heat produced by friction. He described his observations as a dissipative use of energy, resulting in a transformation-content (Verwandlungsinhalt in German), of a thermodynamic system or working body of chemical species during a change of state. That was in contrast to earlier views, based on the theories of Isaac Newton, that heat was an indestructible particle that had mass. Clausius discovered that the non-usable energy increases as steam proceeds from inlet to exhaust in a steam engine. From the prefix en-, as in 'energy', and from the Greek word τροπή [tropē], which is translated in an established lexicon as turning or change and that he rendered in German as Verwandlung, a word often translated into English as transformation, in 1865 Clausius coined the name of that property as entropy. The word was adopted into the English language in 1868.

Later, scientists such as Ludwig Boltzmann, Josiah Willard Gibbs, and James Clerk Maxwell gave entropy a statistical basis. In 1877, Boltzmann visualized a probabilistic way to measure the entropy of an ensemble of ideal gas particles, in which he defined entropy as proportional to the natural logarithm of the number of microstates such a gas could occupy. The proportionality constant in this definition, called the Boltzmann constant, has become one of the defining universal constants for the modern International System of Units (SI). Henceforth, the essential problem in statistical thermodynamics has been to determine the distribution of a given amount of energy E over N identical systems. Constantin Carathéodory, a Greek mathematician, linked entropy with a mathematical definition of irreversibility, in terms of trajectories and integrability.

Etymology

In 1865, Clausius named the concept of "the differential of a quantity which depends on the configuration of the system," entropy (Entropie) after the Greek word for 'transformation'. He gave "transformational content" (Verwandlungsinhalt) as a synonym, paralleling his "thermal and ergonal content" (Wärme- und Werkinhalt) as the name of ${\displaystyle U}$, but preferring the term entropy as a close parallel of the word energy, as he found the concepts nearly "analogous in their physical significance." This term was formed by replacing the root of ἔργον ('ergon', 'work') by that of τροπή ('tropy', 'transformation').

In more detail, Clausius explained his choice of "entropy" as a name as follows:

I prefer going to the ancient languages for the names of important scientific quantities, so that they may mean the same thing in all living tongues. I propose, therefore, to call S the entropy of a body, after the Greek word "transformation". I have designedly coined the word entropy to be similar to energy, for these two quantities are so analogous in their physical significance, that an analogy of denominations seems to me helpful.

Leon Cooper added that in this way "he succeeded in coining a word that meant the same thing to everybody: nothing."

Definitions and descriptions

Any method involving the notion of entropy, the very existence of which depends on the second law of thermodynamics, will doubtless seem to many far-fetched, and may repel beginners as obscure and difficult of comprehension.

Willard Gibbs, Graphical Methods in the Thermodynamics of Fluids

The concept of entropy is described by two principal approaches, the macroscopic perspective of classical thermodynamics, and the microscopic description central to statistical mechanics. The classical approach defines entropy in terms of macroscopically measurable physical properties, such as bulk mass, volume, pressure, and temperature. The statistical definition of entropy defines it in terms of the statistics of the motions of the microscopic constituents of a system – modeled at first classically, e.g. Newtonian particles constituting a gas, and later quantum-mechanically (photons, phonons, spins, etc.). The two approaches form a consistent, unified view of the same phenomenon as expressed in the second law of thermodynamics, which has found universal applicability to physical processes.

State variables and functions of state

Many thermodynamic properties are defined by physical variables that define a state of thermodynamic equilibrium; these are state variables. State variables depend only on the equilibrium condition, not on the path evolution to that state. State variables can be functions of state, also called state functions, in a sense that one state variable is a mathematical function of other state variables. Often, if some properties of a system are determined, they are sufficient to determine the state of the system and thus other properties' values. For example, temperature and pressure of a given quantity of gas determine its state, and thus also its volume via the ideal gas law. A system composed of a pure substance of a single phase at a particular uniform temperature and pressure is determined, and is thus a particular state, and has not only a particular volume but also a specific entropy. The fact that entropy is a function of state makes it useful. In the Carnot cycle, the working fluid returns to the same state that it had at the start of the cycle, hence the change or line integral of any state function, such as entropy, over this reversible cycle is zero.

Reversible process

Total entropy may be conserved during a reversible process. The entropy change ${\textstyle dS}$ of the system (not including the surroundings) is well-defined as heat ${\textstyle \delta Q_{\text{rev}}}$ transferred to the system divided by the system temperature ${\textstyle T}$, ${\textstyle dS={\frac {\delta Q_{\text{rev}}}{T}}}$. A reversible process is a quasistatic one that deviates only infinitesimally from thermodynamic equilibrium and avoids friction or other dissipation. Any process that happens quickly enough to deviate from thermal equilibrium cannot be reversible, total entropy increases, and the potential for maximum work to be done in the process is also lost. For example, in the Carnot cycle, while the heat flow from the hot reservoir to the cold reservoir represents an increase in entropy, the work output, if reversibly and perfectly stored in some energy storage mechanism, represents a decrease in entropy that could be used to operate the heat engine in reverse and return to the previous state; thus the total entropy change may still be zero at all times if the entire process is reversible. An irreversible process increases the total entropy of system and surroundings.

Carnot cycle

The concept of entropy arose from Rudolf Clausius's study of the Carnot cycle. In a Carnot cycle, heat Q_H is absorbed isothermally at temperature T_H from a 'hot' reservoir and given up isothermally as heat Q_C to a 'cold' reservoir at T_C. According to Carnot's principle, work can only be produced by the system when there is a temperature difference, and the work should be some function of the difference in temperature and the heat absorbed (Q_H). Carnot did not distinguish between Q_H and Q_C, since he was using the incorrect hypothesis that caloric theory was valid, and hence heat was conserved (the incorrect assumption that Q_H and Q_C were equal in magnitude) when, in fact, Q_H is greater than the magnitude of Q_C. Through the efforts of Clausius and Kelvin, it is now known that the maximum work that a heat engine can produce is the product of the Carnot efficiency and the heat absorbed from the hot reservoir:

$${\displaystyle W=\left({\frac {T_{\text{H}}-T_{\text{C}}}{T_{\text{H}}}}\right)Q_{\text{H}}=\left(1-{\frac {T_{\text{C}}}{T_{\text{H}}}}\right)Q_{\text{H}}}$$

(1)

To derive the Carnot efficiency, which is 1 − T_C/T_H (a number less than one), Kelvin had to evaluate the ratio of the work output to the heat absorbed during the isothermal expansion with the help of the Carnot–Clapeyron equation, which contained an unknown function called the Carnot function. The possibility that the Carnot function could be the temperature as measured from a zero point of temperature was suggested by Joule in a letter to Kelvin. This allowed Kelvin to establish his absolute temperature scale. It is also known that the net work W produced by the system in one cycle is the net heat absorbed, which is the sum (or difference of the magnitudes) of the heat Q_H > 0 absorbed from the hot reservoir and the waste heat Q_C < 0 given off to the cold reservoir:

$${\displaystyle W=Q_{\text{H}}+Q_{\text{C}}}$$

(2)

Since the latter is valid over the entire cycle, this gave Clausius the hint that at each stage of the cycle, work and heat would not be equal, but rather their difference would be the change of a state function that would vanish upon completion of the cycle. The state function was called the internal energy central to the first law of thermodynamics.

Now equating (1) and (2) gives

$${\displaystyle {\frac {Q_{\text{H}}}{T_{\text{H}}}}+{\frac {Q_{\text{C}}}{T_{\text{C}}}}=0}$$

This implies that there is a function of state whose change is Q/T and that is conserved over a complete cycle of the Carnot cycle. Clausius called this state function entropy. One can see that entropy was discovered through mathematics rather than through laboratory results. It is a mathematical construct and has no easy physical analogy. This makes the concept somewhat obscure or abstract, akin to how the concept of energy arose.

Clausius then asked what would happen if there should be less work produced by the system than that predicted by Carnot's principle. The right-hand side of the first equation would be the upper bound of the work output by the system, which would now be converted into an inequality

$${\displaystyle W<\left(1-{\frac {T_{\text{C}}}{T_{\text{H}}}}\right)Q_{\text{H}}}$$

When the second equation is used to express the work as a net or total heat exchanged in a cycle, we get

$${\displaystyle Q_{\text{H}}+Q_{\text{C}}<\left(1-{\frac {T_{\text{C}}}{T_{\text{H}}}}\right)Q_{\text{H}}}$$

or

$${\displaystyle |Q_{\text{C}}|>{\frac {T_{\text{C}}}{T_{\text{H}}}}Q_{\text{H}}}$$

So more heat is given up to the cold reservoir than in the Carnot cycle. If we denote the entropy changes by ΔS_i = Q_i/T_i for the two stages of the process, then the above inequality can be written as a decrease in the entropy

$${\displaystyle \Delta S_{\text{H}}+\Delta S_{\text{C}}<0}$$

or

$${\displaystyle \Delta S_{\text{H}}<-\Delta S_{\text{C}}=|\Delta S_{\text{C}}|}$$

The magnitude of the entropy that leaves the system is greater than the entropy that enters the system, implying that some irreversible process prevents the cycle from producing the maximum amount of work predicted by the Carnot equation.

The Carnot cycle and efficiency are useful because they define the upper bound of the possible work output and the efficiency of any classical thermodynamic heat engine. Other cycles, such as the Otto cycle, Diesel cycle and Brayton cycle, can be analyzed from the standpoint of the Carnot cycle. Any machine or cyclic process that converts heat to work and is claimed to produce an efficiency greater than the Carnot efficiency is not viable because it violates the second law of thermodynamics. For very small numbers of particles in the system, statistical thermodynamics must be used. The efficiency of devices such as photovoltaic cells requires an analysis from the standpoint of quantum mechanics.

Classical thermodynamics

Main article: Entropy (classical thermodynamics)

 

Conjugate variables of thermodynamics

Pressure Volume (Stress) (Strain) Temperature Entropy Chemical potential Particle number

The thermodynamic definition of entropy was developed in the early 1850s by Rudolf Clausius and essentially describes how to measure the entropy of an isolated system in thermodynamic equilibrium with its parts. Clausius created the term entropy as an extensive thermodynamic variable that was shown to be useful in characterizing the Carnot cycle. Heat transfer along the isotherm steps of the Carnot cycle was found to be proportional to the temperature of a system (known as its absolute temperature). This relationship was expressed in increments of entropy equal to the ratio of incremental heat transfer divided by temperature, which was found to vary in the thermodynamic cycle but eventually return to the same value at the end of every cycle. Thus it was found to be a function of state, specifically a thermodynamic state of the system.

While Clausius based his definition on a reversible process, there are also irreversible processes that change entropy. Following the second law of thermodynamics, entropy of an isolated system always increases for irreversible processes. The difference between an isolated system and closed system is that energy may not flow to and from an isolated system, but energy flow to and from a closed system is possible. Nevertheless, for both closed and isolated systems, and indeed, also in open systems, irreversible thermodynamics processes may occur.

According to the Clausius equality, for a reversible cyclic process: ${\textstyle \oint {\frac {\delta Q_{\text{rev}}}{T}}=0}$. This means the line integral ${\textstyle \int _{L}{\frac {\delta Q_{\text{rev}}}{T}}}$ is path-independent.

So we can define a state function S called entropy, which satisfies ${\textstyle dS={\frac {\delta Q_{\text{rev}}}{T}}}$.

To find the entropy difference between any two states of a system, the integral must be evaluated for some reversible path between the initial and final states. Since entropy is a state function, the entropy change of the system for an irreversible path is the same as for a reversible path between the same two states. However, the heat transferred to or from, and the entropy change of, the surroundings is different.

We can only obtain the change of entropy by integrating the above formula. To obtain the absolute value of the entropy, we need the third law of thermodynamics, which states that S = 0 at absolute zero for perfect crystals.

From a macroscopic perspective, in classical thermodynamics the entropy is interpreted as a state function of a thermodynamic system: that is, a property depending only on the current state of the system, independent of how that state came to be achieved. In any process where the system gives up energy ΔE, and its entropy falls by ΔS, a quantity at least T_R ΔS of that energy must be given up to the system's surroundings as heat (T_R is the temperature of the system's external surroundings). Otherwise the process cannot go forward. In classical thermodynamics, the entropy of a system is defined only if it is in physical thermodynamic equilibrium (but chemical equilibrium is not required: the entropy of a mixture of two moles of hydrogen and one mole of oxygen at 1 bar pressure and 298 K is well-defined).

Statistical mechanics

Main article: Entropy (statistical thermodynamics)

The statistical definition was developed by Ludwig Boltzmann in the 1870s by analyzing the statistical behavior of the microscopic components of the system. Boltzmann showed that this definition of entropy was equivalent to the thermodynamic entropy to within a constant factor—known as Boltzmann's constant. In summary, the thermodynamic definition of entropy provides the experimental definition of entropy, while the statistical definition of entropy extends the concept, providing an explanation and a deeper understanding of its nature.

The interpretation of entropy in statistical mechanics is the measure of uncertainty, disorder, or mixedupness in the phrase of Gibbs, which remains about a system after its observable macroscopic properties, such as temperature, pressure and volume, have been taken into account. For a given set of macroscopic variables, the entropy measures the degree to which the probability of the system is spread out over different possible microstates. In contrast to the macrostate, which characterizes plainly observable average quantities, a microstate specifies all molecular details about the system including the position and velocity of every molecule. The more such states are available to the system with appreciable probability, the greater the entropy. In statistical mechanics, entropy is a measure of the number of ways a system can be arranged, often taken to be a measure of "disorder" (the higher the entropy, the higher the disorder). This definition describes the entropy as being proportional to the natural logarithm of the number of possible microscopic configurations of the individual atoms and molecules of the system (microstates) that could cause the observed macroscopic state (macrostate) of the system. The constant of proportionality is the Boltzmann constant.

Boltzmann's constant, and therefore entropy, have dimensions of energy divided by temperature, which has a unit of joules per kelvin (J⋅K⁻¹) in the International System of Units (or kg⋅m²⋅s⁻²⋅K⁻¹ in terms of base units). The entropy of a substance is usually given as an intensive property – either entropy per unit mass (SI unit: J⋅K⁻¹⋅kg⁻¹) or entropy per unit amount of substance (SI unit: J⋅K⁻¹⋅mol⁻¹).

Specifically, entropy is a logarithmic measure of the number of system states with significant probability of being occupied:

${\displaystyle S=-k_{\mathrm {B} }\sum _{i}p_{i}\log p_{i},}$

(${\displaystyle p_{i}}$ is the probability that the system is in ${\displaystyle i}$th state, usually given by the Boltzmann distribution; if states are defined in a continuous manner, the summation is replaced by an integral over all possible states) or, equivalently, the expected value of the logarithm of the probability that a microstate is occupied

${\displaystyle S=-k_{\mathrm {B} }\langle \log p\rangle }$

where k_B is the Boltzmann constant, equal to 1.38065×10⁻²³ J/K. The summation is over all the possible microstates of the system, and p_i is the probability that the system is in the i-th microstate. This definition assumes that the basis set of states has been picked so that there is no information on their relative phases. In a different basis set, the more general expression is

${\displaystyle S=-k_{\mathrm {B} }\operatorname {Tr} ({\widehat {\rho }}\log({\widehat {\rho }})),}$

where ${\displaystyle {\widehat {\rho }}}$ is the density matrix, ${\displaystyle \operatorname {Tr} }$ is trace and ${\displaystyle \log }$ is the matrix logarithm. This density matrix formulation is not needed in cases of thermal equilibrium so long as the basis states are chosen to be energy eigenstates. For most practical purposes, this can be taken as the fundamental definition of entropy since all other formulas for S can be mathematically derived from it, but not vice versa.

In what has been called the fundamental assumption of statistical thermodynamics or the fundamental postulate in statistical mechanics, among system microstates of the same energy (degenerate microstates) each microstate is assumed to be populated with equal probability; this assumption is usually justified for an isolated system in equilibrium. Then for an isolated system p_i = 1/Ω, where Ω is the number of microstates whose energy equals the system's energy, and the previous equation reduces to

${\displaystyle S=k_{\mathrm {B} }\log \Omega .}$

In thermodynamics, such a system is one in which the volume, number of molecules, and internal energy are fixed (the microcanonical ensemble).

For a given thermodynamic system, the excess entropy is defined as the entropy minus that of an ideal gas at the same density and temperature, a quantity that is always negative because an ideal gas is maximally disordered. This concept plays an important role in liquid-state theory. For instance, Rosenfeld's excess-entropy scaling principle states that reduced transport coefficients throughout the two-dimensional phase diagram are functions uniquely determined by the excess entropy.

The most general interpretation of entropy is as a measure of the extent of uncertainty about a system. The equilibrium state of a system maximizes the entropy because it does not reflect all information about the initial conditions, except for the conserved variables. This uncertainty is not of the everyday subjective kind, but rather the uncertainty inherent to the experimental method and interpretative model.

The interpretative model has a central role in determining entropy. The qualifier "for a given set of macroscopic variables" above has deep implications: if two observers use different sets of macroscopic variables, they see different entropies. For example, if observer A uses the variables U, V and W, and observer B uses U, V, W, X, then, by changing X, observer B can cause an effect that looks like a violation of the second law of thermodynamics to observer A. In other words: the set of macroscopic variables one chooses must include everything that may change in the experiment, otherwise one might see decreasing entropy.

Entropy can be defined for any Markov processes with reversible dynamics and the detailed balance property.

In Boltzmann's 1896 Lectures on Gas Theory, he showed that this expression gives a measure of entropy for systems of atoms and molecules in the gas phase, thus providing a measure for the entropy of classical thermodynamics.

Entropy of a system

A thermodynamic system

 

A temperature–entropy diagram for steam. The vertical axis represents uniform temperature, and the horizontal axis represents specific entropy. Each dark line on the graph represents constant pressure, and these form a mesh with light gray lines of constant volume. (Dark-blue is liquid water, light-blue is liquid-steam mixture, and faint-blue is steam. Grey-blue represents supercritical liquid water.)

Entropy arises directly from the Carnot cycle. It can also be described as the reversible heat divided by temperature. Entropy is a fundamental function of state.

In a thermodynamic system, pressure and temperature tend to become uniform over time because the equilibrium state has higher probability (more possible combinations of microstates) than any other state.

As an example, for a glass of ice water in air at room temperature, the difference in temperature between the warm room (the surroundings) and the cold glass of ice and water (the system and not part of the room) decreases as portions of the thermal energy from the warm surroundings spread to the cooler system of ice and water. Over time the temperature of the glass and its contents and the temperature of the room become equal. In other words, the entropy of the room has decreased as some of its energy has been dispersed to the ice and water, of which the entropy has increased.

However, as calculated in the example, the entropy of the system of ice and water has increased more than the entropy of the surrounding room has decreased. In an isolated system such as the room and ice water taken together, the dispersal of energy from warmer to cooler always results in a net increase in entropy. Thus, when the "universe" of the room and ice water system has reached a temperature equilibrium, the entropy change from the initial state is at a maximum. The entropy of the thermodynamic system is a measure of how far the equalization has progressed.

Thermodynamic entropy is a non-conserved state function that is of great importance in the sciences of physics and chemistry. Historically, the concept of entropy evolved to explain why some processes (permitted by conservation laws) occur spontaneously while their time reversals (also permitted by conservation laws) do not; systems tend to progress in the direction of increasing entropy. For isolated systems, entropy never decreases. This fact has several important consequences in science: first, it prohibits "perpetual motion" machines; and second, it implies the arrow of entropy has the same direction as the arrow of time. Increases in the total entropy of system and surroundings correspond to irreversible changes, because some energy is expended as waste heat, limiting the amount of work a system can do.

Unlike many other functions of state, entropy cannot be directly observed but must be calculated. Absolute standard molar entropy of a substance can be calculated from the measured temperature dependence of its heat capacity. The molar entropy of ions is obtained as a difference in entropy from a reference state defined as zero entropy. The second law of thermodynamics states that the entropy of an isolated system must increase or remain constant. Therefore, entropy is not a conserved quantity: for example, in an isolated system with non-uniform temperature, heat might irreversibly flow and the temperature become more uniform such that entropy increases. Chemical reactions cause changes in entropy and system entropy, in conjunction with enthalpy, plays an important role in determining in which direction a chemical reaction spontaneously proceeds.

One dictionary definition of entropy is that it is "a measure of thermal energy per unit temperature that is not available for useful work" in a cyclic process. For instance, a substance at uniform temperature is at maximum entropy and cannot drive a heat engine. A substance at non-uniform temperature is at a lower entropy (than if the heat distribution is allowed to even out) and some of the thermal energy can drive a heat engine.

A special case of entropy increase, the entropy of mixing, occurs when two or more different substances are mixed. If the substances are at the same temperature and pressure, there is no net exchange of heat or work – the entropy change is entirely due to the mixing of the different substances. At a statistical mechanical level, this results due to the change in available volume per particle with mixing.

Equivalence of definitions

Proofs of equivalence between the definition of entropy in statistical mechanics (the Gibbs entropy formula ${\textstyle S=-k_{\mathrm {B} }\sum _{i}p_{i}\log p_{i}}$) and in classical thermodynamics (${\textstyle dS={\frac {\delta Q_{\text{rev}}}{T}}}$ together with the fundamental thermodynamic relation) are known for the microcanonical ensemble, the canonical ensemble, the grand canonical ensemble, and the isothermal–isobaric ensemble. These proofs are based on the probability density of microstates of the generalized Boltzmann distribution and the identification of the thermodynamic internal energy as the ensemble average ${\displaystyle U=\left\langle E_{i}\right\rangle }$. Thermodynamic relations are then employed to derive the well-known Gibbs entropy formula. However, the equivalence between the Gibbs entropy formula and the thermodynamic definition of entropy is not a fundamental thermodynamic relation but rather a consequence of the form of the generalized Boltzmann distribution.

Furthermore, it has been shown that the definitions of entropy in statistical mechanics is the only entropy that is equivalent to the classical thermodynamics entropy under the following postulates:

1. The probability density function is proportional to some function of the ensemble parameters and random variables.
2. Thermodynamic state functions are described by ensemble averages of random variables.
3. At infinite temperature, all the microstates have the same probability.

Second law of thermodynamics

The second law of thermodynamics requires that, in general, the total entropy of any system does not decrease other than by increasing the entropy of some other system. Hence, in a system isolated from its environment, the entropy of that system tends not to decrease. It follows that heat cannot flow from a colder body to a hotter body without the application of work to the colder body. Secondly, it is impossible for any device operating on a cycle to produce net work from a single temperature reservoir; the production of net work requires flow of heat from a hotter reservoir to a colder reservoir, or a single expanding reservoir undergoing adiabatic cooling, which performs adiabatic work. As a result, there is no possibility of a perpetual motion machine. It follows that a reduction in the increase of entropy in a specified process, such as a chemical reaction, means that it is energetically more efficient.

It follows from the second law of thermodynamics that the entropy of a system that is not isolated may decrease. An air conditioner, for example, may cool the air in a room, thus reducing the entropy of the air of that system. The heat expelled from the room (the system), which the air conditioner transports and discharges to the outside air, always makes a bigger contribution to the entropy of the environment than the decrease of the entropy of the air of that system. Thus, the total of entropy of the room plus the entropy of the environment increases, in agreement with the second law of thermodynamics.

In mechanics, the second law in conjunction with the fundamental thermodynamic relation places limits on a system's ability to do useful work. The entropy change of a system at temperature ${\textstyle T}$ absorbing an infinitesimal amount of heat ${\textstyle \delta q}$ in a reversible way, is given by ${\textstyle \delta q/T}$. More explicitly, an energy ${\textstyle T_{R}S}$ is not available to do useful work, where ${\textstyle T_{R}}$ is the temperature of the coldest accessible reservoir or heat sink external to the system. For further discussion, see Exergy.

Statistical mechanics demonstrates that entropy is governed by probability, thus allowing for a decrease in disorder even in an isolated system. Although this is possible, such an event has a small probability of occurring, making it unlikely.

The applicability of a second law of thermodynamics is limited to systems in or sufficiently near equilibrium state, so that they have defined entropy. Some inhomogeneous systems out of thermodynamic equilibrium still satisfy the hypothesis of local thermodynamic equilibrium, so that entropy density is locally defined as an intensive quantity. For such systems, there may apply a principle of maximum time rate of entropy production. It states that such a system may evolve to a steady state that maximizes its time rate of entropy production. This does not mean that such a system is necessarily always in a condition of maximum time rate of entropy production; it means that it may evolve to such a steady state.

Applications

The fundamental thermodynamic relation

Main article: Fundamental thermodynamic relation

The entropy of a system depends on its internal energy and its external parameters, such as its volume. In the thermodynamic limit, this fact leads to an equation relating the change in the internal energy ${\displaystyle U}$ to changes in the entropy and the external parameters. This relation is known as the fundamental thermodynamic relation. If external pressure ${\displaystyle p}$ bears on the volume ${\displaystyle V}$ as the only external parameter, this relation is:

${\displaystyle dU=T\,dS-p\,dV}$

Since both internal energy and entropy are monotonic functions of temperature ${\displaystyle T}$, implying that the internal energy is fixed when one specifies the entropy and the volume, this relation is valid even if the change from one state of thermal equilibrium to another with infinitesimally larger entropy and volume happens in a non-quasistatic way (so during this change the system may be very far out of thermal equilibrium and then the whole-system entropy, pressure, and temperature may not exist).

The fundamental thermodynamic relation implies many thermodynamic identities that are valid in general, independent of the microscopic details of the system. Important examples are the Maxwell relations and the relations between heat capacities.

Entropy in chemical thermodynamics

Thermodynamic entropy is central in chemical thermodynamics, enabling changes to be quantified and the outcome of reactions predicted. The second law of thermodynamics states that entropy in an isolated system – the combination of a subsystem under study and its surroundings – increases during all spontaneous chemical and physical processes. The Clausius equation of ${\displaystyle \delta q_{\text{rev}}/T=\Delta S}$ introduces the measurement of entropy change, ${\displaystyle \Delta S}$. Entropy change describes the direction and quantifies the magnitude of simple changes such as heat transfer between systems – always from hotter to cooler spontaneously.

The thermodynamic entropy therefore has the dimension of energy divided by temperature, and the unit joule per kelvin (J/K) in the International System of Units (SI).

Thermodynamic entropy is an extensive property, meaning that it scales with the size or extent of a system. In many processes it is useful to specify the entropy as an intensive property independent of the size, as a specific entropy characteristic of the type of system studied. Specific entropy may be expressed relative to a unit of mass, typically the kilogram (unit: J⋅kg⁻¹⋅K⁻¹). Alternatively, in chemistry, it is also referred to one mole of substance, in which case it is called the molar entropy with a unit of J⋅mol⁻¹⋅K⁻¹.

Thus, when one mole of substance at about 0 K is warmed by its surroundings to 298 K, the sum of the incremental values of ${\textstyle q_{\text{rev}}/T}$ constitute each element's or compound's standard molar entropy, an indicator of the amount of energy stored by a substance at 298 K. Entropy change also measures the mixing of substances as a summation of their relative quantities in the final mixture.

Entropy is equally essential in predicting the extent and direction of complex chemical reactions. For such applications, ${\displaystyle \Delta S}$ must be incorporated in an expression that includes both the system and its surroundings, ${\displaystyle \Delta S_{\text{universe}}=\Delta S_{\text{surroundings}}+\Delta S_{\text{system}}}$. This expression becomes, via some steps, the Gibbs free energy equation for reactants and products in the system: ${\displaystyle \Delta G}$ [the Gibbs free energy change of the system] ${\displaystyle =\Delta H}$ [the enthalpy change] ${\displaystyle -T\,\Delta S}$ [the entropy change].

World's technological capacity to store and communicate entropic information

A 2011 study in Science (journal) estimated the world's technological capacity to store and communicate optimally compressed information normalized on the most effective compression algorithms available in the year 2007, therefore estimating the entropy of the technologically available sources. The author's estimate that human kind's technological capacity to store information grew from 2.6 (entropically compressed) exabytes in 1986 to 295 (entropically compressed) exabytes in 2007. The world's technological capacity to receive information through one-way broadcast networks was 432 exabytes of (entropically compressed) information in 1986, to 1.9 zettabytes in 2007. The world's effective capacity to exchange information through two-way telecommunication networks was 281 petabytes of (entropically compressed) information in 1986, to 65 (entropically compressed) exabytes in 2007.

Entropy balance equation for open systems

During steady-state continuous operation, an entropy balance applied to an open system accounts for system entropy changes related to heat flow and mass flow across the system boundary.

In chemical engineering, the principles of thermodynamics are commonly applied to "open systems", i.e. those in which heat, work, and mass flow across the system boundary. Flows of both heat (${\displaystyle {\dot {Q}}}$) and work, i.e. ${\displaystyle {\dot {W}}_{\text{S}}}$ (shaft work) and ${\displaystyle P(dV/dt)}$ (pressure-volume work), across the system boundaries, in general cause changes in the entropy of the system. Transfer as heat entails entropy transfer ${\displaystyle {\dot {Q}}/T}$, where ${\displaystyle T}$ is the absolute thermodynamic temperature of the system at the point of the heat flow. If there are mass flows across the system boundaries, they also influence the total entropy of the system. This account, in terms of heat and work, is valid only for cases in which the work and heat transfers are by paths physically distinct from the paths of entry and exit of matter from the system.

To derive a generalized entropy balanced equation, we start with the general balance equation for the change in any extensive quantity ${\displaystyle \theta }$ in a thermodynamic system, a quantity that may be either conserved, such as energy, or non-conserved, such as entropy. The basic generic balance expression states that ${\displaystyle d\theta /dt}$, i.e. the rate of change of ${\displaystyle \theta }$ in the system, equals the rate at which ${\displaystyle \theta }$ enters the system at the boundaries, minus the rate at which ${\displaystyle \theta }$ leaves the system across the system boundaries, plus the rate at which ${\displaystyle \theta }$ is generated within the system. For an open thermodynamic system in which heat and work are transferred by paths separate from the paths for transfer of matter, using this generic balance equation, with respect to the rate of change with time ${\displaystyle t}$ of the extensive quantity entropy ${\displaystyle S}$, the entropy balance equation is:

${\displaystyle {\frac {dS}{dt}}=\sum _{k=1}^{K}{\dot {M}}_{k}{\hat {S}}_{k}+{\frac {\dot {Q}}{T}}+{\dot {S}}_{\text{gen}}}$

where

• ${\textstyle \sum _{k=1}^{K}{\dot {M}}_{k}{\hat {S}}_{k}}$ is the net rate of entropy flow due to the flows of mass into and out of the system (where ${\displaystyle {\hat {S}}}$ is entropy per unit mass).
• ${\textstyle {\frac {\dot {Q}}{T}}}$ is the rate of entropy flow due to the flow of heat across the system boundary.
• ${\textstyle {\dot {S}}_{\text{gen}}}$ is the rate of entropy production within the system. This entropy production arises from processes within the system, including chemical reactions, internal matter diffusion, internal heat transfer, and frictional effects such as viscosity occurring within the system from mechanical work transfer to or from the system.

If there are multiple heat flows, the term ${\displaystyle {\dot {Q}}/T}$ is replaced by ${\textstyle \sum {\dot {Q}}_{j}/T_{j},}$ where ${\displaystyle {\dot {Q}}_{j}}$ is the heat flow and ${\displaystyle T_{j}}$ is the temperature at the ${\displaystyle j}$th heat flow port into the system.

Note that the nomenclature "entropy balance" is misleading and often deemed inappropriate because entropy is not a conserved quantity. In other words, the term ${\displaystyle {\dot {S}}_{\text{gen}}}$ is never a known quantity but always a derived one based on the expression above. Therefore, the open system version of the second law is more appropriately described as the "entropy generation equation" since it specifies that ${\displaystyle {\dot {S}}_{\text{gen}}\geq 0}$, with zero for reversible processes or greater than zero for irreversible ones.

Entropy change formulas for simple processes

For certain simple transformations in systems of constant composition, the entropy changes are given by simple formulas.

Isothermal expansion or compression of an ideal gas

For the expansion (or compression) of an ideal gas from an initial volume ${\displaystyle V_{0}}$ and pressure ${\displaystyle P_{0}}$ to a final volume ${\displaystyle V}$ and pressure ${\displaystyle P}$ at any constant temperature, the change in entropy is given by:

${\displaystyle \Delta S=nR\ln {\frac {V}{V_{0}}}=-nR\ln {\frac {P}{P_{0}}}.}$

Here ${\displaystyle n}$ is the amount of gas (in moles) and ${\displaystyle R}$ is the ideal gas constant. These equations also apply for expansion into a finite vacuum or a throttling process, where the temperature, internal energy and enthalpy for an ideal gas remain constant.

Cooling and heating

For pure heating or cooling of any system (gas, liquid or solid) at constant pressure from an initial temperature ${\displaystyle T_{0}}$ to a final temperature ${\displaystyle T}$, the entropy change is

${\displaystyle \Delta S=nC_{P}\ln {\frac {T}{T_{0}}}.}$

provided that the constant-pressure molar heat capacity (or specific heat) C_P is constant and that no phase transition occurs in this temperature interval.

Similarly at constant volume, the entropy change is

${\displaystyle \Delta S=nC_{v}\ln {\frac {T}{T_{0}}},}$

where the constant-volume molar heat capacity C_v is constant and there is no phase change.

At low temperatures near absolute zero, heat capacities of solids quickly drop off to near zero, so the assumption of constant heat capacity does not apply.

Since entropy is a state function, the entropy change of any process in which temperature and volume both vary is the same as for a path divided into two steps – heating at constant volume and expansion at constant temperature. For an ideal gas, the total entropy change is

${\displaystyle \Delta S=nC_{v}\ln {\frac {T}{T_{0}}}+nR\ln {\frac {V}{V_{0}}}.}$

Similarly if the temperature and pressure of an ideal gas both vary,

${\displaystyle \Delta S=nC_{P}\ln {\frac {T}{T_{0}}}-nR\ln {\frac {P}{P_{0}}}.}$

Phase transitions

Reversible phase transitions occur at constant temperature and pressure. The reversible heat is the enthalpy change for the transition, and the entropy change is the enthalpy change divided by the thermodynamic temperature. For fusion (melting) of a solid to a liquid at the melting point T_m, the entropy of fusion is

${\displaystyle \Delta S_{\text{fus}}={\frac {\Delta H_{\text{fus}}}{T_{\text{m}}}}.}$

Similarly, for vaporization of a liquid to a gas at the boiling point T_b, the entropy of vaporization is

${\displaystyle \Delta S_{\text{vap}}={\frac {\Delta H_{\text{vap}}}{T_{\text{b}}}}.}$

Approaches to understanding entropy

As a fundamental aspect of thermodynamics and physics, several different approaches to entropy beyond that of Clausius and Boltzmann are valid.

Standard textbook definitions

The following is a list of additional definitions of entropy from a collection of textbooks:

• a measure of energy dispersal at a specific temperature.
• a measure of disorder in the universe or of the availability of the energy in a system to do work.
• a measure of a system's thermal energy per unit temperature that is unavailable for doing useful work.

In Boltzmann's analysis in terms of constituent particles, entropy is a measure of the number of possible microscopic states (or microstates) of a system in thermodynamic equilibrium.

Order and disorder

Main article: Entropy (order and disorder)

Entropy is often loosely associated with the amount of order or disorder, or of chaos, in a thermodynamic system. The traditional qualitative description of entropy is that it refers to changes in the status quo of the system and is a measure of "molecular disorder" and the amount of wasted energy in a dynamical energy transformation from one state or form to another. In this direction, several recent authors have derived exact entropy formulas to account for and measure disorder and order in atomic and molecular assemblies. One of the simpler entropy order/disorder formulas is that derived in 1984 by thermodynamic physicist Peter Landsberg, based on a combination of thermodynamics and information theory arguments. He argues that when constraints operate on a system, such that it is prevented from entering one or more of its possible or permitted states, as contrasted with its forbidden states, the measure of the total amount of "disorder" in the system is given by:

${\displaystyle {\text{Disorder}}={C_{\text{D}} \over C_{\text{I}}}.\,}$

Similarly, the total amount of "order" in the system is given by:

${\displaystyle {\text{Order}}=1-{C_{\text{O}} \over C_{\text{I}}}.\,}$

In which C_D is the "disorder" capacity of the system, which is the entropy of the parts contained in the permitted ensemble, C_I is the "information" capacity of the system, an expression similar to Shannon's channel capacity, and C_O is the "order" capacity of the system.

Energy dispersal

Main article: Entropy (energy dispersal)

 

The concept of entropy can be described qualitatively as a measure of energy dispersal at a specific temperature. Similar terms have been in use from early in the history of classical thermodynamics, and with the development of statistical thermodynamics and quantum theory, entropy changes have been described in terms of the mixing or "spreading" of the total energy of each constituent of a system over its particular quantized energy levels.

Ambiguities in the terms disorder and chaos, which usually have meanings directly opposed to equilibrium, contribute to widespread confusion and hamper comprehension of entropy for most students. As the second law of thermodynamics shows, in an isolated system internal portions at different temperatures tend to adjust to a single uniform temperature and thus produce equilibrium. A recently developed educational approach avoids ambiguous terms and describes such spreading out of energy as dispersal, which leads to loss of the differentials required for work even though the total energy remains constant in accordance with the first law of thermodynamics (compare discussion in next section). Physical chemist Peter Atkins, in his textbook Physical Chemistry, introduces entropy with the statement that "spontaneous changes are always accompanied by a dispersal of energy or matter and often both".

Relating entropy to energy usefulness

Following on from the above, it is possible (in a thermal context) to regard lower entropy as an indicator or measure of the effectiveness or usefulness of a particular quantity of energy. This is because energy supplied at a higher temperature (i.e. with low entropy) tends to be more useful than the same amount of energy available at a lower temperature. Mixing a hot parcel of a fluid with a cold one produces a parcel of intermediate temperature, in which the overall increase in entropy represents a "loss" that can never be replaced.

Thus, the fact that the entropy of the universe is steadily increasing, means that its total energy is becoming less useful: eventually, this leads to the "heat death of the Universe."

Entropy and adiabatic accessibility

A definition of entropy based entirely on the relation of adiabatic accessibility between equilibrium states was given by E.H.Lieb and J. Yngvason in 1999. This approach has several predecessors, including the pioneering work of Constantin Carathéodory from 1909 and the monograph by R. Giles. In the setting of Lieb and Yngvason one starts by picking, for a unit amount of the substance under consideration, two reference states ${\displaystyle X_{0}}$ and ${\displaystyle X_{1}}$ such that the latter is adiabatically accessible from the former but not vice versa. Defining the entropies of the reference states to be 0 and 1 respectively the entropy of a state ${\displaystyle X}$ is defined as the largest number ${\displaystyle \lambda }$ such that ${\displaystyle X}$ is adiabatically accessible from a composite state consisting of an amount ${\displaystyle \lambda }$ in the state ${\displaystyle X_{1}}$ and a complementary amount, ${\displaystyle (1-\lambda )}$, in the state ${\displaystyle X_{0}}$. A simple but important result within this setting is that entropy is uniquely determined, apart from a choice of unit and an additive constant for each chemical element, by the following properties: It is monotonic with respect to the relation of adiabatic accessibility, additive on composite systems, and extensive under scaling.

Entropy in quantum mechanics

Main article: von Neumann entropy

In quantum statistical mechanics, the concept of entropy was developed by John von Neumann and is generally referred to as "von Neumann entropy",

${\displaystyle S=-k_{\mathrm {B} }\operatorname {Tr} (\rho \log \rho ),}$

where ρ is the density matrix and Tr is the trace operator.

This upholds the correspondence principle, because in the classical limit, when the phases between the basis states used for the classical probabilities are purely random, this expression is equivalent to the familiar classical definition of entropy,

${\displaystyle S=-k_{\mathrm {B} }\sum _{i}p_{i}\,\log \,p_{i},}$

i.e. in such a basis the density matrix is diagonal.

Von Neumann established a rigorous mathematical framework for quantum mechanics with his work Mathematische Grundlagen der Quantenmechanik. He provided in this work a theory of measurement, where the usual notion of wave function collapse is described as an irreversible process (the so-called von Neumann or projective measurement). Using this concept, in conjunction with the density matrix he extended the classical concept of entropy into the quantum domain.

Information theory

Main articles: Entropy (information theory), Entropy in thermodynamics and information theory, and Entropic uncertainty

I thought of calling it "information", but the word was overly used, so I decided to call it "uncertainty". [...] Von Neumann told me, "You should call it entropy, for two reasons. In the first place your uncertainty function has been used in statistical mechanics under that name, so it already has a name. In the second place, and more important, nobody knows what entropy really is, so in a debate you will always have the advantage."

Conversation between Claude Shannon and John von Neumann regarding what name to give to the attenuation in phone-line signals

When viewed in terms of information theory, the entropy state function is the amount of information in the system that is needed to fully specify the microstate of the system. Entropy is the measure of the amount of missing information before reception. Often called Shannon entropy, it was originally devised by Claude Shannon in 1948 to study the size of information of a transmitted message. The definition of information entropy is expressed in terms of a discrete set of probabilities ${\displaystyle p_{i}}$ so that

${\displaystyle H(X)=-\sum _{i=1}^{n}p(x_{i})\log p(x_{i}).}$

In the case of transmitted messages, these probabilities were the probabilities that a particular message was actually transmitted, and the entropy of the message system was a measure of the average size of information of a message. For the case of equal probabilities (i.e. each message is equally probable), the Shannon entropy (in bits) is just the number of binary questions needed to determine the content of the message.

Most researchers consider information entropy and thermodynamic entropy directly linked to the same concept, while others argue that they are distinct. Both expressions are mathematically similar. If ${\displaystyle W}$ is the number of microstates that can yield a given macrostate, and each microstate has the same a priori probability, then that probability is ${\displaystyle p=1/W}$. The Shannon entropy (in nats) is:

${\displaystyle H=-\sum _{i=1}^{W}p\log(p)=\log(W)}$ and if entropy is measured in units of ${\displaystyle k}$ per nat, then the entropy is given by:

${\displaystyle H=k\log(W)}$

which is the Boltzmann entropy formula, where ${\displaystyle k}$ is Boltzmann's constant, which may be interpreted as the thermodynamic entropy per nat. Some authors argue for dropping the word entropy for the ${\displaystyle H}$ function of information theory and using Shannon's other term, "uncertainty", instead.

Measurement

The entropy of a substance can be measured, although in an indirect way. The measurement, known as entropymetry, is done on a closed system (with particle number N and volume V being constants) and uses the definition of temperature in terms of entropy, while limiting energy exchange to heat (${\displaystyle dU\rightarrow dQ}$).

${\displaystyle T:=\left({\frac {\partial U}{\partial S}}\right)_{V,N}\Rightarrow \cdots \Rightarrow \;dS=dQ/T}$

The resulting relation describes how entropy changes ${\displaystyle dS}$ when a small amount of energy ${\displaystyle dQ}$ is introduced into the system at a certain temperature ${\displaystyle T}$.

The process of measurement goes as follows. First, a sample of the substance is cooled as close to absolute zero as possible. At such temperatures, the entropy approaches zero – due to the definition of temperature. Then, small amounts of heat are introduced into the sample and the change in temperature is recorded, until the temperature reaches a desired value (usually 25 °C). The obtained data allows the user to integrate the equation above, yielding the absolute value of entropy of the substance at the final temperature. This value of entropy is called calorimetric entropy.

Interdisciplinary applications

Although the concept of entropy was originally a thermodynamic concept, it has been adapted in other fields of study, including information theory, psychodynamics, thermoeconomics/ecological economics, and evolution.

Philosophy and theoretical physics

Entropy is the only quantity in the physical sciences that seems to imply a particular direction of progress, sometimes called an arrow of time. As time progresses, the second law of thermodynamics states that the entropy of an isolated system never decreases in large systems over significant periods of time. Hence, from this perspective, entropy measurement is thought of as a clock in these conditions.

Biology

Chiavazzo et al. proposed that where cave spiders choose to lay their eggs can be explained through entropy minimization.

Entropy has been proven useful in the analysis of base pair sequences in DNA. Many entropy-based measures have been shown to distinguish between different structural regions of the genome, differentiate between coding and non-coding regions of DNA, and can also be applied for the recreation of evolutionary trees by determining the evolutionary distance between different species.

Cosmology

Assuming that a finite universe is an isolated system, the second law of thermodynamics states that its total entropy is continually increasing. It has been speculated, since the 19th century, that the universe is fated to a heat death in which all the energy ends up as a homogeneous distribution of thermal energy so that no more work can be extracted from any source.

If the universe can be considered to have generally increasing entropy, then – as Roger Penrose has pointed out – gravity plays an important role in the increase because gravity causes dispersed matter to accumulate into stars, which collapse eventually into black holes. The entropy of a black hole is proportional to the surface area of the black hole's event horizon. Jacob Bekenstein and Stephen Hawking have shown that black holes have the maximum possible entropy of any object of equal size. This makes them likely end points of all entropy-increasing processes, if they are totally effective matter and energy traps. However, the escape of energy from black holes might be possible due to quantum activity (see Hawking radiation).

The role of entropy in cosmology remains a controversial subject since the time of Ludwig Boltzmann. Recent work has cast some doubt on the heat death hypothesis and the applicability of any simple thermodynamic model to the universe in general. Although entropy does increase in the model of an expanding universe, the maximum possible entropy rises much more rapidly, moving the universe further from the heat death with time, not closer. This results in an "entropy gap" pushing the system further away from the posited heat death equilibrium. Other complicating factors, such as the energy density of the vacuum and macroscopic quantum effects, are difficult to reconcile with thermodynamical models, making any predictions of large-scale thermodynamics extremely difficult.

Current theories suggest the entropy gap to have been originally opened up by the early rapid exponential expansion of the universe.

Economics

See also: Nicholas Georgescu-Roegen § The relevance of thermodynamics to economics, and Ecological economics § Methodology

Romanian American economist Nicholas Georgescu-Roegen, a progenitor in economics and a paradigm founder of ecological economics, made extensive use of the entropy concept in his magnum opus on The Entropy Law and the Economic Process. Due to Georgescu-Roegen's work, the laws of thermodynamics now form an integral part of the ecological economics school. Although his work was blemished somewhat by mistakes, a full chapter on the economics of Georgescu-Roegen has approvingly been included in one elementary physics textbook on the historical development of thermodynamics.

In economics, Georgescu-Roegen's work has generated the term 'entropy pessimism'. Since the 1990s, leading ecological economist and steady-state theorist Herman Daly – a student of Georgescu-Roegen – has been the economics profession's most influential proponent of the entropy pessimism position.

A Beautiful Planet

From Wikipedia, the free encyclopedia

https://en.wikipedia.org/wiki/A_Beautiful_Planet 

 

A Beautiful Planet
Theatrical release poster
Directed by	Toni Myers
Written by	Toni Myers
Produced by	Toni Myers
Narrated by	Jennifer Lawrence
Cinematography	James Neihouse
Edited by	Toni Myers
Music by	Micky Erbe Maribeth Solomon
Production companies	IMAX Entertainment NASA
Distributed by	IMAX Entertainment
Release date	April 29, 2016 (United States)
Running time	46 minutes
Country	United States
Language	English
Box office	$25.7 million

Most of the reviews for A Beautiful Planet admired the singular perspectives that can be seen from the ISS, like this image of southern lights. (The Space Station's solar panels are visible at the upper right.)

A Beautiful Planet is a 2016 American documentary film directed, written, and produced by Toni Myers, and narrated by actress Jennifer Lawrence. It was originally released exclusively for IMAX theatres. Created in cooperation with the National Aeronautics and Space Administration (NASA), the documentary utilizes footage recorded by astronauts aboard the International Space Station (ISS) over the course of fifteen months. The documentary examines the daily lives and work of astronauts representing the respective space agencies of the United States, Russia, Europe, and Japan.

The documentary premiered in Manhattan on April 16, 2016 and made its theatrical debut on April 29, 2016. The film was first aired domestically in the United States, grossing $15.6 million. It was later aired in the United Kingdom, Australia, New Zealand and Russia/CIS.

Content overview

A Beautiful Planet utilizes large-scale cinema screens to display capital cities illuminated by skyglow, lightning storms seen from above clouds, Super Typhoon Maysak as seen from its eye, polar auroras viewed from low Earth orbit, the Great Lakes of North America locked in ice and snow, and reefs below the surface of the Caribbean Sea.

The big picture

The film depicts space-views from the International Space Station (ISS) of geographical formations that may not be visible from land such as annular lake, Lake Manicouagan in Quebec, Canada.

Scenes from the documentary show a snow-capped segment of South America's Andes, the longest continental mountain range in the world. The Andes stretch from Venezuela north of the Equator, through the Tropics, and down to southern Argentina, containing "some of the most extreme climate zones on Earth, from ice fields to deserts". The Andean Mountains includes Aconcagua, the highest peak in The Americas, as well as the highest in the Southern Hemisphere.

The Iberian Peninsula seen from the Space Station's vantage point in low Earth orbit. This photo shows all of Portugal, Spain and Gibraltar, and parts of Morocco, Algeria, France, the Mediterranean, and the Atlantic.

The movie presents Earth's driest and wettest areas with an overhead sequence of the Namib Desert on the east cleft by the Atlantic Ocean's Skeleton Coast on the west. The film repeats the consensus that the Namib is the "oldest desert" on Earth, having a desert climate longer than any other region in the world, and being around tens of millions of year longer than the Sahara.

The film begins with a light-years-long, computer-generated trip through swarms of stars in the Milky Way; the compressed trip ends with the Solar System.

Mount Fuji in Honshu, Japan, was photographed in February, 2016, using the most powerful camera lens then aboard the ISS. The photograph shows details of Japan's famous volcano, including switchbacks in the trail leading to the summit crater and features of the Hōei flank crater.

The film uses time-lapse photography to depict how Earth's warming climate is causing the Greenland ice sheet to melt, using footage of the Jakobshavn Glacier calving.

A Beautiful Planet also presents images of large-scale deforestation in Madagascar. The film shows how this island suffers from widespread soil erosion and habitat destruction of the island's native wildlife, such as the lemur. A Beautiful Planet also shows images of the burning of the Brazilian rainforest.

The film depicts multiple scenes of climate change and environmental degradation. Filmmaker Toni Myers told the Los Angeles Times, "I wanted to inspire people especially as to how beautiful the planet is, how fragile it is, how complex and diverse and varied it is ... Most of all I wanted to show why we want to find solutions to look after our planet. It's our only one."

Exoplanet Kepler-186f

The final scenes of A Beautiful Planet briefly examine an extrasolar planet (a planet outside of our planetary system) which was discovered in 2014. The planet, Kepler-186f, was the first approximately-Earth-sized planet found to be orbiting within its star's habitable zone, or orbital area where liquid water could conceivably exist without freezing or vaporizing. It was the first discovery of an Earth-sized planet on which life could reside.

An artist's conception of the Kepler-186 planetary system, with the Earth-sized planet Kepler-186f shown on the right, the system's red dwarf star at the lower left, and the four other known planets in the system faintly visible in orbits closer to the host star.

The name "Kepler" comes from its discovery by the Kepler Space Telescope, or "NASA Discovery Mission Number 10," a spacecraft observatory which is designed to find exoplanets in our region of the Milky Way Galaxy that are Earth-size and smaller, and that are within the habitable zone. The planet orbits Kepler-186, a red dwarf star about half the size and mass of the Sun which lies in the direction of the constellation Cygnus, about 500 light-years away. The number "186" in the planet's name refers to the order in which its planetary system was discovered while scientists processed all of the data produced by the Kepler Space Telescope.

Although the idea of interstellar travel to another planetary system like Kepler-186 is not feasible given current astronautics technology, some spaceflight futurists (like Samantha Cristoforetti) find value in speculating about the currently-impossible.

The astronauts

The film's cast consist of ISS crew from many nations. The astronauts who appeared in the movie included: Scott Kelly (NASA / USA), who spent an 11-month uninterrupted stint aboard the International Space Station; Samantha Cristoforetti (European Space Agency / Italy), who has spent more time in an uninterrupted spaceflight than any other European astronaut; Barry "Butch" Wilmore (NASA / USA), commander of the 42nd expedition to the ISS from November 10, 2014 to March 11, 2015; Terry Virts (NASA / USA), commander of the 43rd expedition to the ISS from March 11, 2015 to June 11, 2015; Anton Shkaplerov (Roscosmos / Russia), the commander of the Soyuz spacecraft that brought Cristoforetti and Virts to the Space Station; Kjell Lindgren (NASA / USA), a medical doctor who had previously worked as a flight surgeon supporting medical operations and space-station training at NASA's Johnson Space Center, and Kimiya Yui (Japan Aerospace Exploration Agency / Japan), a space explorer who was made Head of the JAXA Astronaut Group after he returned from his stay on the Space Station.

Research lab

The International Space Station is a scientific laboratory, and many of the experiments on the ISS have the astronauts themselves as research participants to determine how spaceflight affects the human body. On March 28, 2015 Scott Kelly and Mikhail Kornienko arrived at the Space Station to commence a much-discussed one year mission to study the health effects of long-term space travel. Scientists hoped to analyze their mission and discover ways future space explorers might adjust to the effects of weightlessness, isolation, radiation exposure, and stress they would encounter in a 30-month-round-trip expedition to Mars, or in an even longer trip beyond Mars. Shortly after Kelly's arrival at the Space Station, A Beautiful Planet shows him participating in an initial examination of his eye, to study and correct any vision decline reported by many astronauts.

Former astronauts Scott Kelly (right) and Mark Kelly are the subjects of a twin study on the health effects of long-term space travel. Both cooperated with numerous medical tests during and after Scott's year long mission aboard the ISS.

Scott Kelly has an identical twin, Mark Kelly, who is also a retired NASA astronaut. The brothers agreed to be the subjects of an unprecedented twin study; Mark stayed on Earth during Scott's eleven months aboard the ISS so that researchers could examine how an extended spaceflight affected Scott's body compared to Mark's. While Scott was in space and then continuing after he returned, both twins gave periodic blood samples and DNA swabs, and they underwent body scans and many other medical tests. In the epilogue to his 2017 book about the year long mission, Scott wrote that the very preliminary assessments of the data from the mission and from the twin study were promising:

The data is still being analyzed as I write this, and the scientists are excited about what they are seeing so far. The genetic differences between my brother and me from this year could unlock new knowledge, not only about what spaceflight does to our bodies, but also about how we age here on Earth. The Fluid Shifts study Misha [Mikhail] and I did is promising in terms of improving astronauts' health on long missions. The studies I did on my eyes - which don't seem to have degraded further during this mission - could help solve the mystery of what causes damage to astronauts' vision, as well as helping us understand more about the anatomy and disease processes of the eye in general.

— Scott Kelly, Endurance: A Year in Space, a Lifetime of Discovery (2017)

In the taste test phase of an experiment with space farming, Kelly and his fellow Expedition 44 crew-members Kjell Lindgren and Kimiya Yui are shown sampling red romaine lettuce that was grown in the Space Station's "Veggie" (or Vegetable Production) System. The Veggie series of experiments are designed to ensure that future explorers visiting the Moon, Mars or an asteroid have access to fresh produce, and also to provide them with an opportunity for relaxation and relief from stress or boredom.

Earth observatory

ESA astronaut Samantha Cristoforetti in the Space Station's Cupola module, where many of the movie's scenes of Earth were filmed.

A Beautiful Planet provides close-up footage of the Cupola, a domed, 360 degree observation bay on the nadir (Earth-facing) side of the Station's Tranquility module / Node 3. It has seven windows in total, with six outwardly-angled windows arranged around a central, circular window which faces directly toward Earth. The circular window measures 80 centimeters in diameter; it is the largest window ever sent into space. Many scenes were filmed from the Cupola, and the astronauts themselves are shown taking photographs and gazing through its windows at views of Earth.

The Cupola was constructed by the European Space Agency for the utilitarian purpose of giving astronauts a workstation where they could observe the Earth, the exterior of the Station, visiting vehicles, and the operation of the ISS robotic arms. It also serves as a rejuvenation area where astronauts can relax and seek inspiration, including communicating with other crew members.

Training facility

Much of the "training facility" aspect of the ISS mission is geared toward providing practical experience so that astronauts, space agencies, aerospace engineers and scientists are prepared for much longer space missions, including a possible human presence on Mars or the Moon.

Astronauts on the Space Station are required to spend approximately two hours each day engaged in physical training to prevent loss of bone density, muscle atrophy, and weightlessness. In the documentary, Terry Virts is shown receiving a cardiovascular workout by running on an ISS treadmill and Samantha Cristoforetti does strength training using an ISS exercise machine that mimics weightlifting exercises. Both machines have adaptations that permit them to function in a micro-g environment. The treadmill has a harness and bungee cord straps that keep astronaut runners from floating away from it, and the "weightlifting" machine replaces the weights (which don't "weigh" anything in orbit) with two canisters that create small vacuums against which exercising astronauts can pull.

Barry "Butch" Wilmore conducting a spacewalk in 2015, with Earth visible in the background. Terry Virts accompanied Wilmore on this EVA; the inverted reflection of Virts is visible in the visor of Wilmore's EMU space suit.

The Space Station is positioned in low Earth orbit. This is just outside of the Earth's appreciable atmosphere, and provides a training area in which astronauts can put on space suits, leave the ISS life support systems behind, and conduct spacewalks - or "Extravehicular activity (EVA)." An EVA may be undertaken to make repairs, reconfigure the Station to accommodate new modules and deploy new equipment. The ISS orbits high enough to permit an astronaut and their sponsoring nation to gain an EVA experience outside of the atmosphere. However, it is low enough to avoid the increased radiation exposure and prevent difficulties associated with climbing further out of Earth's gravity well. (If the Earth is compared to a 16-inch beach ball, the orbit of the ISS would be about half an inch above the beach ball's surface.)

Butch Wilmore and Terry Virts performed three spacewalks over a nine-day period from February 21 to March 1, 2015. The film depicts some of their EVA activities outside the Space Station. While they worked, both explorers were cognizant of the dangers associated with spacewalks. Virts explains that a puncture to their EMU spacesuits was a particular concern because "you 'walk around' by grabbing onto things with your gloves ... The outside of the Space Station [is] a jungle of wires and equipment and metal bars and trusses. If you accidentally sliced your glove or your spacesuit on one of the sharp edges, that could create a leak, and if that leak were big enough, you would die." Describing some of the other EVA hazards, Wilmore elaborates that the temperature is "almost 300 degrees [Fahrenheit] on the Sun side of the Space Station, [but when] you get in the shade, it's minus 275 degrees. You feel that inside the suit. My fingertips in the sunlight would feel like they were on fire almost ... [Also,] you have a safety tether attached to the Station, and it's on a reel ... You can be upside down, twisted, inverted; you can completely lose your spatial awareness about where you are and what your attitude is, and you can easily get tangled up in that safety tether if you're not cautious. Every single movement you make, you're making an effort to think [things] through."

Production

A Beautiful Planet was written, produced, and directed by Toni Myers, who has created seven other space-themed IMAX films including Hubble 3D and Space Station 3D. The film premiered in Manhattan on April 16, 2016, and was released in cinemas on April 29, 2016. Despite being announced as distributor, Walt Disney Studios later removed association with the film prior to its release.

Digital IMAX cameras

The astronauts who filmed the movie used digital IMAX cameras, and much of the footage they produced was shot through the seven window panes on the Space Station's domed Cupola module. The use of digital cameras permitted cinematographer James Neihouse to review image sequences almost immediately and make suggestions for retakes, and was a lightweight alternative to using IMAX film which can be developed only when returned from space.

This night photograph of the American Midwest was taken from ISS Expedition 46. The city of Chicago is visible on the shore of Lake Michigan, as are Earth's atmosphere, part of the Space Station, and the approaching sunrise.

Myers and Neihouse coordinated with their astronaut camera crew to make use of the digital cameras' augmented capacity for filming in dim light. According to Myers, "We would not have the nighttime scenes without the digital dynamic range ... What the digital capture did was totally open up that night world to us, with stars, cities at night, lightning and other phenomena that you see at night, like aurora."

Reception

This movie received a 100% rating on Rotten Tomatoes and a 79% audience-enjoyment rating from the 13 reviews.

The film's ratings and reviews were mostly centered around its cinematography. A review in the British newspaper, The Guardian called it a "large-format eye-opener [which] achieves a breathtaking new perspective on Earthly life," while another appraisal in The New York Times asked, "how can your eyes not bug out when given 3-D views of Earth, taken from space, on a stories-high [IMAX] screen?"