quantity

decay rate

The rate at which the amplitude of a wave or oscillation decreases over time.
9 related articles · 6 formulas

Description

Decay rate describes how quickly the amplitude of a wave or oscillation diminishes over time. In physics, this concept applies to everything from a swinging pendulum losing energy to friction, to the exponential decay of radioactive particles, to the damping of electromagnetic waves in a medium. It quantifies how a system returns to equilibrium after being disturbed.

History

The mathematical formalism of exponential decay was established in the 17th century, but its application to wave damping and particle physics developed through the 19th and 20th centuries, notably with Rutherford's work on radioactivity.

How it works

The decay rate is typically expressed as a constant that appears in an exponential function, such as A(t) = A₀ e^(-λt), where λ is the decay rate. A higher λ means faster decay. The mechanism behind it varies: for mechanical oscillations, it's often friction or air resistance; for particles, it's quantum mechanical processes like spontaneous emission or nuclear instability.

In practice

Decay rates are used in medical imaging (e.g., PET scans), in dating archaeological artifacts via carbon-14, and in designing shock absorbers and damping systems for buildings and vehicles.

Fun fact

The decay rate of a pendulum in a vacuum is so small that it can swing for hours, but in air, it loses energy much faster due to air resistance.

Concept graph →

Formulas

$$V(\phi) \propto e^{-\lambda \phi}$$
A scalar field potential decaying exponentially with the field.
What is in the formula
Vvariablepotential energy density — potential energy density joule per cubic metre
φvariablescalar field value — scalar field
λconstantdecay rate of the potential — decay rate = varies
$$C = \frac{4g^2}{\kappa_1 \kappa_2}$$
Parameter quantifying coupling strength between two modes in cavity QED.
What is in the formula
gvariablecoupling strength between the two modes — coupling strength radian per second
κ₁variabledecay rate of the first mode — decay rate radian per second
κ₂variabledecay rate of the second mode — decay rate radian per second
$$P(t) = e^{-\Gamma t}$$
Survival probability decays exponentially with time.
What is in the formula
P(t)variableSurvival probability at time t — probability
tvariableTime — time second
ΓvariableDecay rate (inverse lifetime) — decay rate per second
$$\psi(t) = A e^{-\omega_I t} \cos(\omega_R t - \phi)$$
A damped oscillation describes the decay of quasinormal modes.
What is in the formula
ψvariableperturbation amplitude — wave function
Avariableinitial amplitude — amplitude
ω_Ivariableimaginary part of frequency (decay rate) — decay rate per second
ω_Rvariablereal part of frequency (oscillation frequency) — angular frequency per second
φvariablephase offset — phase
$$\tau = \frac{1}{\lambda}$$
The lifetime is the reciprocal of the decay rate constant.
What is in the formula
\tauvariablelifetime — lifetime second
\lambdavariabledecay rate constant — decay rate per second
$$T_{\text{rh}} \simeq \left(\frac{30}{\pi^2 g_*}\right)^{1/4} \sqrt{\Gamma M_P}$$
Temperature after inflation from decay rate and Planck mass.
What is in the formula
T_{\text{rh}}variableReheating temperature after inflation — temperature kelvin
g_*variableEffective number of relativistic degrees of freedom
\GammavariableInflaton decay rate — decay rate per second
M_PvariableReduced Planck mass — mass kilogram
\sqrt{}operatorTakes the square root of the argument — square root
\simeqoperatorIndicates approximate equality — approximate equality

Related articles · 9

General Relativity2026-08-091 minarXiv:2608.08863express
How Waves Fade into Infinity
A stone falls into a pond. Ripples spread, weaken, and soon vanish. But if the pond were infinite and the water perfect, the disturbance would last forever, gradually fading. In physics, such decaying remnants are called "tails"—they live long after the main wave has passed.
Quantum Physics2026-08-032 minarXiv:2608.02462express
A Pendulum That Feels Gravity Quantumly
A pendulum weighing a few grains of sand swings on a hair-thin glass fiber. Its motions are so faint that the thermal jostling of air molecules seems like a hurricane. Yet such a pendulum is the key to witnessing quantum wonders in the world of large objects.
The Snapping Cable of Reality: How Finite String Thickness Accelerates Quantum Decay and Reshapes the Gravitational Hum
Immediately after the Big Bang, in the seething cauldron of the cooling Universe, much like in unevenly hardening glass, stresses appeared — hairline cracks in reality, cosmic strings. Picture a tightrope walker balancing on an invisible cable stretched across the abyss of warped spacetime.
General Relativity2026-05-291 minarXiv:2606.00227express
The Universe Doesn't Remember Its Youth: The Echo of Quantum Gravity Can't Be Caught
Immediately after the Big Bang, space may have vibrated like a string from quantum effects. As these oscillations faded, they would have left a mark on the expansion of galaxies — a memory effect. The search for this echo in telescope data turned up nothing.
Atomic Physics2026-04-011 minarXiv:2604.01099express
Clocks That Hear the Silence
Atomic clocks are pendulums that tick at the frequency of light. Inside a trap, an aluminum ion hangs, and a laser probes it like a tuning fork. If the laser's frequency matches the atom's natural frequency, the atom responds. The clock's rate is checked against this response.
HEP Experiment2026-03-262 minarXiv:2603.25649express
How a Particle Decays: The Dance of Four Tracks
When a particle decays, it doesn't just vanish: it transforms into a whole set of other particles, and each transformation has its own script. Physicists from the BESIII collaboration have, for the first time, broken down the rare decay of the D0 meson step by step: it turns into two kaons and two pions.
HEP Experiment2026-03-241 minarXiv:2603.23081express
Photon Detective: How the J/psi Particle Decays
The J/psi particle lives for an instant and then decays into lighter particles, much like a snapped string scattering into pieces. Physicists from the BESIII collaboration caught over ten billion such decays to figure out exactly what 'pieces' are produced.
Quantum Physics2026-02-021 minarXiv:2602.01715express
Gravity Alters How Atoms Emit Light
An atom excited by light gives its energy back in an instant — it emits a photon. This process is like a tired runner dropping a heavy load. But if the runner is on a mountain slope, it's harder to pick up speed. Gravity acts on the atom similarly: near a massive body, time flows slower, and the atom emits differently.
Plasma Physics2026-01-262 minarXiv:2601.18495express
Solar Wind: Waves Give Birth to Radio Bursts
In the stream of charged particles that constantly blows from the Sun, radio bursts sometimes occur — short, powerful signals at frequencies you can pick up on an ordinary radio. Until now, it was unclear how exactly these signals are born in that stream.