9 Equations True Geeks Should Know
The world’s complexities and uncertainties are distilled and set in orderly figures, with a handful of characters sufficing to capture the universe itself.
For your enjoyment, the Wired Science team has gathered nine of our favorite equations. This article was published November 4, 2011. Some represent the universe; others, the nature of life. One represents the limit of equations.
1. Euler’s Identity
Also called Euler’s relation, or the Euler equation of complex analysis, this bit of mathematics enjoys accolades across geeky disciplines.
Swiss mathematician Leonhard Euler first wrote the equality, which links together geometry, algebra, and five of the most essential symbols in math — 0, 1, i, pi and e — that are essential tools in scientific work.
Theoretical physicist Richard Feynman was a huge fan and called it a “jewel” and a “remarkable” formula. Fans today refer to it as “the most beautiful equation.”
2. The Entire Universe in Figures: Friedmann Equations
Derived from Einstein’s theory of General Relativity, the two Friedmann equations describe the life of the entire universe, from fiery Big Bang birth to chilly accelerated expansion death.
3. Boltzmann’s Entropy Formula
Nature loves chaos when it pushes systems toward equilibrium, and geeks call this universal property entropy.
The equation describes the tight relationship between entropy (S), and the myriad ways particles in a system can be arranged (k log W). The last part is tricky. k is Boltzmann’s constant and W is the number of microscopic elements of a system (e.g. the momentum and position of individual atoms of gas) in a macroscopic system in a state of balance (e.g., gas sealed in a bottle).
4. Electricity and Magnetism: Maxwell’s Equations
Without these four equations, every lolcat on the Internet couldn’t exist. First put together by James Clerk Maxwell in 1861, the formulas describe all known behaviors of electricity and magnetism and show the relationship between the two forces. They state that a moving electric charge will generate a magnetic field while a shifting magnetic field similarly creates an electric field.
5. Certain Uncertainty: Schrödinger Equation
Erwin Schrödinger’s famous equation reigns supreme over the smallest objects in the universe. It illustrates how subatomic particles change with time when under the influence of a force. Any particular atom or molecule is described by its wavefunction, the probability of where and when the particle appears, represented by the Greek letter psi.
6. All Life Is an Island: Island Biogeography
Though physicists can describe the universe’s expansion in a few lines, the basic properties of life on Earth are far harder to quantify. During the latter half of the 20th century, biologists arrived at the theory of island biogeography, which described the dynamics of animal populations on islands.
7. The Essence of Evolution: Nowak’s Evolvability
At its most basic level, life is what replicates itself — but how did it begin? It’s the ultimate chicken-and-egg problem, and one that scientists studying what’s called pre-life try to answer. On the left side of the equation, proposed by Harvard University mathematical biologist Martin Nowak, is a symbol representing all possible strings of molecules; at right are the speed of chemical reactions, the tendency of shorter strings to be more common than longer strings, selection pressures and fitness ratings. As Nowak has shown, all that’s necessary for life to emerge are molecules subject to forces of selection and mutation. If those conditions are met, self-replication will emerge with the inexorability of gravity.
8. The Razor’s Edge of Outbreak: R-Nought
Brought to mainstream attention by the thriller Contagion, R0, pronounced R-nought, is a very simple figure: It refers to the average number of people an individual infected with a pathogen will go on to infect. If it’s less than one, the disease will burn itself out; if greater than one, it will spread. In a world where a flu virus from Mexico can infect millions of people around the world in a matter of months, this equation is as symbolic as it is straightforward.
9. Hot or Not: The (Limited) Mathematics of Beauty
Not everything can be quantified, especially when it comes to matters of the human heart and mind. For decades, psychologists and biologists have tried to represent physical beauty in formula form; but even if some tendencies emerge when hundreds of individual preferences are measured, what any one individual considers beautiful is impossible to predict.
At right is an equation from an unpublished attempty by Israeli computer scientists to design a program capable of quantifying the attractiveness of a face. “Y” is the empirical beauty score; at right, various measurements of how different features in a face compared to a baseline face. The program was brilliantly coded, but it didn’t work very well.
The largest balls in the world: the bush cricket Platycleis affinis, apparently, has the largest testicles around. 70 mg may not sound like much, but it’s an impressive fourteen percent of the cricket’s body mass. A little back-of-the-envelope calculation of what a human male would have to sport in order to compete: assuming the average male weighs 75 kg, he would have to have balls weighing 75/100*14 = 10.5 kilograms. If this mass were to be concentrated in an average pair of testicles, whose volume is about 36 cm3, the density would be 10500g/36cm3 = 292g/cm3. That’s twice as dense as the core of the Sun.
The guys who measured bush cricket balls didn’t do it just to settle who’s bigger. They found “that testis mass increased with the degree of polyandry, but decreased with increasing ejaculate mass.”
Spinoxy
So very very hot!! Sweet, this innocence, this brilliance!!
Page 1 of 2






