
A distinct configuration of a physical system, such as a superconductor's current-carrying condition.In physics, a state refers to a distinct configuration of a physical system, characterized by a specific set of properties. For example, a superconductor can exist in a state where it carries current without resistance, or in a normal resistive state. The concept of state is central to quantum mechanics, where a system's state is described by a wavefunction that contains all information about its properties. Different states can have vastly different behaviors, and transitions between states are often the focus of research.
The concept of state in physics evolved from classical thermodynamics, where it referred to the macroscopic condition of a system. In quantum mechanics, the notion of state was formalized by Erwin Schrödinger and Werner Heisenberg in the 1920s.
A state is defined by the values of observable quantities, such as energy, momentum, or spin. In quantum mechanics, a state is a vector in Hilbert space, and its evolution is governed by the Schrödinger equation. For macroscopic systems, states can be distinguished by order parameters, like the superconducting gap or the magnetization. Transitions between states can be continuous (phase transitions) or abrupt, and are often driven by external parameters like temperature, pressure, or magnetic field.
The concept of state is used in designing quantum computers, where qubits must be maintained in specific quantum states, and in materials science, where engineers seek to stabilize desirable states like superconductivity at higher temperatures.
In some materials, a single crystal can host two different superconducting states simultaneously, each with a different symmetry of the order parameter, a phenomenon known as 'two-gap superconductivity'.










