quantity

decay probability

Decay probability is the likelihood that a particle will undergo a specific decay process within a given time.
5 related articles

Description

Decay probability is the likelihood that an unstable particle or quantum state will undergo a specific decay process within a given time interval. In quantum mechanics, decay is inherently probabilistic: an excited atom, a radioactive nucleus, or an unstable elementary particle has no definite 'lifetime' but rather a probability per unit time of decaying. This probability is governed by the transition rate, often calculated using Fermi's Golden Rule, which depends on the strength of the interaction causing the decay and the density of available final states. The concept is fundamental to nuclear physics, particle physics, and quantum optics, where it explains phenomena from radioactivity to spontaneous emission.

History

The probabilistic nature of decay was established in the early 20th century with the work of Rutherford and Soddy on radioactive decay (1902), who empirically found the exponential law. The quantum mechanical explanation was developed by Dirac (1927) and later formalized by Fermi (1950) in his Golden Rule, which remains the standard tool for calculating decay rates.

How it works

For a system in an initial state |i⟩, the decay probability to a final state |f⟩ per unit time is given by the transition rate Γ = (2π/ℏ) |⟨f|H'|i⟩|² ρ(E_f), where H' is the perturbing interaction and ρ(E_f) is the density of final states. The total decay probability over time t is then P(t) = 1 − exp(−Γt), assuming a constant Γ. This exponential behavior arises when the decay is Markovian—the system has no memory of its past. The decay probability is measured by preparing many identical particles and counting how many decay in successive time intervals, yielding the characteristic exponential decay curve.

In practice

Decay probability is used in radiocarbon dating, nuclear reactor design, particle physics experiments (e.g., measuring the Higgs boson's decay channels), and in quantum computing to predict qubit relaxation times and optimize error correction.

Fun fact

The decay probability of a single particle is constant per unit time, but if you watch it continuously, the quantum Zeno effect can suppress the decay—frequent measurements can freeze the particle in its initial state.

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Related articles · 5

HEP Phenomenology2026-05-022 minarXiv:2605.01618express
How a Star's Matter Takes the Hit
If you squeeze a handful of sand in your fist, it first compacts, but then starts to resist — the grains have nowhere left to go. In the depths of a neutron star, something similar happens, except instead of sand grains, you have elementary particles, and instead of your hand, you have monstrous gravity.
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.
The Prisoner's Paradox: The Old Bicycle of Classical Probability
Two accomplices are interrogated separately: betray or stay silent? If neither knows what the other will do, their choice breaks the classical rule of probability. It’s like riding an old bicycle over bumps — the hard seat jolts you off. The textbook rule, the classical model, fails. The authors of a new study found a simple fix: the cyclist needs a soft saddle.
Quantum Decay Tail: How the Memory of Birth Depends on Color
A quantum system, once born, does not forget it. Even after dozens of lifetimes, a trace of the initial state remains in its decay: a slowly decreasing power-law tail. For two fluorescent dyes, erythrosine B and eosin Y, this tail has been observed for the first time in two spectral channels simultaneously.
Symphony of Imaginary Frequencies: Quantum Decay of the Inverted Well
At the hilltop of classical physics, a particle is frozen in unstable equilibrium. The slightest nudge — and it rolls down with increasing speed. In the quantum universe, no nudge is needed: the uncertainty principle itself acts as an all-pervading wind, blowing the particle off the peak.