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science Science is a systematic discipline that builds and organises knowledge in the form of testable hypotheses and predictions about the universe. Modern science is typically divided into twoor threemajor branches: the natural sciences, which stu ...
, ''e''-folding is the time interval in which an exponentially growing quantity increases or decreases by a factor of ''e''; it is the base-''e'' analog of doubling time. This term is often used in many areas of science, such as in
atmospheric chemistry Atmospheric chemistry is a branch of atmospheric science that studies the chemistry of the Earth's atmosphere and that of other planets. This multidisciplinary approach of research draws on environmental chemistry, physics, meteorology, comput ...
,
medicine Medicine is the science and Praxis (process), practice of caring for patients, managing the Medical diagnosis, diagnosis, prognosis, Preventive medicine, prevention, therapy, treatment, Palliative care, palliation of their injury or disease, ...
,
theoretical physics Theoretical physics is a branch of physics that employs mathematical models and abstractions of physical objects and systems to rationalize, explain, and predict List of natural phenomena, natural phenomena. This is in contrast to experimental p ...
, and
cosmology Cosmology () is a branch of physics and metaphysics dealing with the nature of the universe, the cosmos. The term ''cosmology'' was first used in English in 1656 in Thomas Blount's ''Glossographia'', with the meaning of "a speaking of the wo ...
. In
cosmology Cosmology () is a branch of physics and metaphysics dealing with the nature of the universe, the cosmos. The term ''cosmology'' was first used in English in 1656 in Thomas Blount's ''Glossographia'', with the meaning of "a speaking of the wo ...
the ''e''-folding time scale is the
proper time In relativity, proper time (from Latin, meaning ''own time'') along a timelike world line is defined as the time as measured by a clock following that line. The proper time interval between two events on a world line is the change in proper time ...
in which the length of a patch of
space Space is a three-dimensional continuum containing positions and directions. In classical physics, physical space is often conceived in three linear dimensions. Modern physicists usually consider it, with time, to be part of a boundless ...
or
spacetime In physics, spacetime, also called the space-time continuum, is a mathematical model that fuses the three dimensions of space and the one dimension of time into a single four-dimensional continuum. Spacetime diagrams are useful in visualiz ...
increases by the factor ''e''. In
finance Finance refers to monetary resources and to the study and Academic discipline, discipline of money, currency, assets and Liability (financial accounting), liabilities. As a subject of study, is a field of Business administration, Business Admin ...
, the logarithmic return or continuously compounded return, also known as
force of interest Compound interest is interest accumulated from a principal sum and previously accumulated interest. It is the result of reinvesting or retaining interest that would otherwise be paid out, or of the accumulation of debts from a borrower. Compo ...
, is the reciprocal of the ''e''-folding time. The process of evolving to equilibrium is often characterized by a time scale called the ''e''-folding time, ''τ''. This time is used for processes which evolve exponentially toward a final state (equilibrium). In other words, if we examine an observable, ''X'', associated with a system, (
temperature Temperature is a physical quantity that quantitatively expresses the attribute of hotness or coldness. Temperature is measurement, measured with a thermometer. It reflects the average kinetic energy of the vibrating and colliding atoms making ...
or
density Density (volumetric mass density or specific mass) is the ratio of a substance's mass to its volume. The symbol most often used for density is ''ρ'' (the lower case Greek letter rho), although the Latin letter ''D'' (or ''d'') can also be u ...
, for example) then after a time, ''τ'', the initial difference between the initial value of the observable and the equilibrium value, Δ''X''''i'', will have decreased to Δ''X''''i'' /''e'' where the number ''e'' ≈ 2.71828. :T_e = \frac = \frac = \frac * ''T''''e'' ''e''-folding time * ''N''(''t'') amount at time ''t'' * ''N''(0) initial amount * ''T''''d'' doubling time * ln(2) ≈ 0.693
natural logarithm of 2 In mathematics, the natural logarithm of 2 is the unique real number argument such that the exponential function equals two. It appears frequently in various formulas and is also given by the alternating harmonic series. The decimal value of th ...
* ''r''% growth rate in time ''t''


Example of lifetime as ''e''-folding time

The concept of ''e''-folding time may be used in the analysis of kinetics. Consider a chemical species A, which decays into another chemical species, B. We could depict this as an equation: : \rightarrow Let us assume that this reaction follows first order kinetics, meaning that the conversion of A into B depends only on the concentration of A, and the rate constant which dictates the velocity at which this happens, ''k''. We could write the following reaction to describe this first order kinetic process: : \frac=-k[] This ordinary differential equation states that a change (in this case the disappearance) of the concentration of A, ''d''[A]/''dt'', is equal to the rate constant ''k'' multiplied by the concentration of A. Consider what the units of ''k'' would be. On the left hand side, we have a concentration divided by a unit of time. The units for ''k'' would need to allow for these to be replicated on the right hand side. For this reason, the units of ''k'', here, would be 1/time. Because this is a
linear In mathematics, the term ''linear'' is used in two distinct senses for two different properties: * linearity of a '' function'' (or '' mapping''); * linearity of a '' polynomial''. An example of a linear function is the function defined by f(x) ...
,
homogeneous Homogeneity and heterogeneity are concepts relating to the uniformity of a substance, process or image. A homogeneous feature is uniform in composition or character (i.e., color, shape, size, weight, height, distribution, texture, language, i ...
and separable differential equation, we may separate the terms such that the equation becomes: : \frac = -k \,dt We may then integrate both sides of this equation, which results in the inclusion of the constant ''e'': : \begin & \int_^ \frac = \int_^t -k \, dt \\ pt& \ln[]_f - \ln[]_i = -kt - k(0) \\ pt& \ln\frac = -kt \\ pt& \frac = e^ \end where sub>''f'' and sub>''i'' are the final and initial concentrations of A. Upon comparing the ratio on the left hand side to the equation on the right hand side, we conclude that the ratio between the final and initial concentrations follows an exponential function, of which ''e'' is the base. As mentioned above, the units for ''k'' are inverse time. If we were to take the reciprocal of this, we would be left with units of time. For this reason, we often state that the lifetime of a species that undergoes first order decay is equal to the reciprocal of ''k''. Consider, now, what would happen if we were to set the time, ''t'', to the reciprocal of the rate constant, ''k'', i.e. ''t'' = 1/''k''. This would yield : \frac = e^ = e^ = \frac 1 e \approx 0.37 This states that after one lifetime (1/''k''), the ratio of final to initial concentrations is equal to about 0.37. Stated another way, after one lifetime, we have : \frac \approx \frac = 37\% which means that we have lost (1 − 0.37 = 0.63) 63% of A, with only 37% left. With this, we now know that if we have 1 lifetime passed, we have gone through 1 "e-folding". What would 2 "e-foldings" look like? After two lifetimes, we would have , which would result in : \frac = e^ = e^ = \frac 1 \approx 0.14 = 14\% which says that only about 14% of A remains. It is in this manner that ''e''-folding lends us an easy way to describe the number of lifetimes that have passed. After 1 lifetime, we have 1/''e'' remaining. After 2 lifetimes, we have 1/''e''2 remaining. One lifetime, therefore, is one ''e''-folding time, which is the most descriptive way of stating the decay.


See also

* Doubling time


References

{{DEFAULTSORT:E-Folding Inflation (cosmology) Temporal exponentials