The starting state of a system, such as position and velocity, from which its evolution begins.Initial conditions are the complete specification of a system's state at the starting moment of its evolution — for a particle, this means its position and velocity; for a field, the values at every point. In deterministic physics, the initial conditions uniquely determine the entire future trajectory of a system through the equations of motion. However, in chaotic systems, tiny differences in initial conditions grow exponentially, making long-term prediction impossible even though the physics is fully deterministic — the famous 'butterfly effect'.
The concept of initial conditions became central to physics with Isaac Newton's formulation of classical mechanics in 1687, where the laws of motion require both position and velocity to predict the future. Pierre-Simon Laplace in 1814 famously articulated the idea of a 'demon' that, knowing all initial conditions and forces, could predict the entire future of the universe.
The evolution of any physical system is governed by differential equations that take the current state as input and produce the next state. The initial conditions provide the boundary values needed to solve these equations uniquely. In quantum mechanics, the initial wavefunction completely determines the probability distribution of all future measurements. In cosmology, the initial conditions of the universe — the density fluctuations present shortly after the Big Bang — are imprinted on the cosmic microwave background and seed the formation of all galaxies and large-scale structures we observe today.
Weather forecasting relies on measuring current atmospheric conditions as initial conditions for numerical models. In biology, the initial conditions of a bacterial colony — cell density and nutrient distribution — determine the spatial patterns of colony growth. In quantum computing, precise preparation of initial qubit states is essential for reliable computation.
The universe's initial conditions were so finely tuned that the density fluctuations were about one part in 100,000 — if they had been much larger, galaxies would have collapsed into black holes; much smaller, and no stars would have formed.



