math

natural logarithm

natural logarithm — from formula anatomy
6 related articles · 6 formulas

Description

The natural logarithm, denoted ln(x), is the logarithm to the base e, where e ≈ 2.71828 is Euler's number. It is the inverse function of the exponential function e^x. In physics, the natural logarithm appears wherever growth, decay, or entropy is involved: radioactive decay half-lives, the Boltzmann distribution in statistical mechanics, the entropy formula S = k ln W, and the definition of decibels and pH. It simplifies multiplicative relationships into additive ones, making it a fundamental tool in theoretical analysis.

History

The natural logarithm was introduced by John Napier in the early 17th century (though his logarithms were base 10-like), and the base e was recognized by Leonhard Euler in the 18th century. The notation 'ln' became standard in the 19th century.

How it works

The natural logarithm of a positive number x is the power to which e must be raised to obtain x. Its derivative is 1/x, which makes it the natural antiderivative of 1/x. It satisfies the properties ln(ab) = ln(a) + ln(b) and ln(a^b) = b ln(a). In physics, it often arises from integrating differential equations of the form dy/dx = y, or from the logarithm of a product of probabilities.

In practice

Used in calculating entropy changes, signal attenuation in electronics, and the age of materials via radioactive dating (e.g., carbon-14).

Fun fact

The natural logarithm of 2 (≈0.693) is the basis for the 'rule of 72' in finance, but in physics it appears as the half-life factor in exponential decay.

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Formulas

$$S = k_B \ln \Omega$$
Entropy equals Boltzmann constant times log of states.
What is in the formula
Svariableentropy of the system — entropy joule per kelvin
Ωvariablenumber of microstates corresponding to the macrostate — number of microstates
k_Bconstantrelates temperature to energy per degree of freedom — boltzmann constant = 1.380649e-23 joule per kelvin
lnoperatornatural logarithm — natural logarithm
$$S \leq k \ln W$$
Entropy is bounded by the logarithm of the number of states.
What is in the formula
SvariableEntropy — entropy joule per kelvin
WvariableNumber of microstates — number of states
kconstantRelates temperature to energy in statistical mechanics — boltzmann constant = 1.380649e-23 joule per kelvin
\leqoperatorIndicates an upper bound — less than or equal
\lnoperatorComputes the logarithm to base e — natural logarithm
$$| ext{squeezing}| ext{ grows as } rac{1}{2} ext{ln}(4ar{n})$$
Maximum squeezing increases logarithmically with mean photon number.
What is in the formula
squeezingvariablesqueezing parameter (magnitude) — squeezing parameter
n̄variablemean photon number — mean photon number
lnoperatornatural logarithm function — natural logarithm
$$S = -\operatorname{tr}(\rho \ln \rho)$$
Entropy of a quantum system given its density matrix ρ.
What is in the formula
Svariablevon Neumann entropy — entropy joule per kelvin
ρvariabledensity matrix of the quantum state — density matrix
troperatorsums diagonal elements of a matrix — trace operator
lnoperatortakes the natural logarithm — natural logarithm
$$t = \frac{1}{\lambda} \ln \left( \frac{N_0}{N} \right)$$
Time elapsed from initial to current isotope ratio.
What is in the formula
tvariableelapsed time — time second
λvariabledecay constant — decay constant per second
N_0variableinitial number of radioactive nuclei — number of nuclei
Nvariablecurrent number of radioactive nuclei — number of nuclei
lnoperatornatural logarithm of the ratio — natural logarithm
$$R_L \approx a \frac{0.49 q^{2/3}}{0.6 q^{2/3} + \ln(1+q^{1/3})}$$
Approximate size of the Roche lobe in binary systems.
What is in the formula
R_LvariableRoche lobe radius — radius metre
avariableorbital separation — length metre
qvariablemass ratio (M1/M2) — mass ratio
lnoperatornatural logarithm — natural logarithm

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