A field that assigns a single value to every point in space, unlike vector fields.A scalar field is a mathematical construct that assigns a single numerical value to every point in space and time. Unlike vector fields, which have both magnitude and direction, scalar fields are characterized by a simple number at each location. Examples include temperature distribution in a room, pressure in a fluid, or the potential energy in a gravitational field.
The concept of fields was introduced by Michael Faraday in the 19th century, and the formal mathematical treatment of scalar fields developed alongside vector calculus in the same era.
In physics, scalar fields are used to describe quantities that vary continuously through space. The field's value at each point can be measured or calculated, and its spatial variations often drive physical processes. For instance, gradients of a scalar field produce forces in vector form, linking the two concepts.
Scalar fields are fundamental in cosmology, where they model the inflaton field driving cosmic inflation, and in particle physics, where the Higgs field gives mass to particles. They are also used in computer graphics for rendering and in meteorology for mapping temperature and pressure.
The Higgs boson, discovered in 2012, is an excitation of the Higgs scalar field that permeates all of space, giving elementary particles their mass.
| V | variable | potential energy density — potential energy density joule per cubic metre |
| φ | variable | scalar field value — scalar field |
| λ | constant | decay rate of the potential — decay rate = varies |
| S | variable | Action of the theory — action joule second |
| g | variable | Determinant of the spacetime metric tensor — metric determinant |
| φ | variable | Scalar field non-minimally coupled to gravity — scalar field |
| R | variable | Ricci scalar curvature — ricci scalar per metre squared |
| ∂φ | variable | Gradient of the scalar field — field gradient per metre |
| ∫ d⁴x | operator | Integration over four-dimensional spacetime — four dimensional integral |
| √(-g) | operator | Volume element factor for curved spacetime — sqrt negative metric determinant |
| (∂φ)² | operator | Kinetic term of the scalar field, contraction of its gradient with itself — kinetic term |
| φ | variable | Scalar field configuration — scalar field |
| ∇² | operator | Laplacian (sum of second spatial derivatives) — laplacian operator |
| \varphi | variable | scalar field — scalar field |
| \rho | variable | source density — source density per cubic metre |
| \Box | operator | Lorentz-invariant second-order differential operator — d alembertian operator |
| m^* | variable | Effective nucleon mass in the medium — effective mass kilogram |
| m | variable | Bare nucleon mass (in vacuum) — mass kilogram |
| \sigma | variable | Scalar meson field expectation value — scalar field |
| g_\sigma | constant | Coupling constant between nucleons and the scalar sigma meson — coupling constant = varies (model-dependent) |
| V | variable | potential energy density of the scalar field — energy density joule per cubic metre |
| phi | variable | scalar field value — scalar field |
| lambda | constant | self-coupling constant of the scalar field — self coupling constant = 1.0 |



