Ostrogradsky instability 1970-01-01
Ostrogradsky instability is a phenomenon that arises in the context of classical field theory and, more broadly, in the study of higher-derivative theories. It is named after the mathematician and physicist Mikhail Ostrogradsky, who is known for his work on the dynamics of systems described by higher-order differential equations. In classical mechanics, the equations of motion for a system are typically second-order in time.
Partial differential equation 1970-01-01
A partial differential equation (PDE) is a type of mathematical equation that involves partial derivatives of an unknown function with respect to two or more independent variables. Unlike ordinary differential equations (ODEs), which deal with functions of a single variable, PDEs allow for the modeling of phenomena where multiple variables are involved, such as time and space.
Pendulum (mechanics) 1970-01-01
A pendulum in mechanics is a weight (or bob) attached to a fixed point by a string or rod that swings back and forth under the influence of gravity. The simple pendulum is characterized by its motion that follows a periodic path, making it a classic example in physics for studying oscillatory motion.
Perturbation theory 1970-01-01
Perturbation theory is a mathematical technique used in various fields, including physics, chemistry, and engineering, to find an approximate solution to a problem that cannot be solved exactly. It is particularly useful in quantum mechanics, where systems can often be analyzed in terms of small changes (or "perturbations") to a known solvable system.
Perturbation theory (quantum mechanics) 1970-01-01
Perturbation theory in quantum mechanics is a mathematical method used to find an approximate solution to a problem that cannot be solved exactly. It is particularly useful when the Hamiltonian (the total energy operator) of a quantum system can be expressed as the sum of a solvable part and a "perturbing" part that represents a small deviation from that solvable system. ### Key Concepts 1.
Point source 1970-01-01
A "point source" refers to a distinct, identifiable source of environmental pollution or emissions that can be pinpointed to a specific location. In various contexts, it may denote: 1. **Environmental Science**: A point source of pollution typically refers to contaminants that are discharged from a single, identifiable location such as a factory, sewage treatment plant, or a specific point along a river.
Poisson's equation 1970-01-01
Poisson's equation is a fundamental partial differential equation in mathematical physics that relates the distribution of a scalar potential field to its sources. It is commonly used in electrostatics, gravitational theory, and fluid dynamics.
Potential theory 1970-01-01
Potential theory is a branch of mathematical analysis that deals with potentials and potential functions, typically in relation to fields such as electrostatics, gravitation, fluid dynamics, and various areas of applied mathematics. The theory is largely concerned with the behavior of harmonic functions and their properties. At its core, potential theory examines the concept of a potential function, which describes gravitational or electrostatic potentials in physics.
Pregeometry (physics) 1970-01-01
Pregeometry is a concept in theoretical physics that seeks to describe the fundamental structure of spacetime and matter in a way that is more primitive than the traditional notions of geometry used in classical and quantum physics. The idea is that the familiar geometric structure of spacetime, as described by general relativity, emerges from a more basic underlying framework that does not rely on pre-existing notions of points, lines, and surfaces.
Projection method (fluid dynamics) 1970-01-01
The projection method is a numerical technique used in fluid dynamics, particularly for solving incompressible Navier-Stokes equations. This method helps in efficiently predicting the flow of fluids by separating the velocity field from the pressure field in the numerical solution process. It is particularly notable for its ability to handle incompressible flows with a prescribed divergence-free condition for the velocity field.
Propagator 1970-01-01
A **propagator** is a concept used in various fields, particularly in physics and mathematics, with specific meanings depending on the context: 1. **Quantum Field Theory (QFT)**: In the context of quantum field theory, a propagator is a mathematical function that describes the behavior of particles as they propagate from one point to another in spacetime. It essentially provides a mechanism to account for the interactions and effects of fields and particles.
Quantization (physics) 1970-01-01
Quantization in physics refers to the process of transitioning from classical physics to quantum mechanics, where certain physical properties are restricted to discrete values rather than continuous ranges. This concept is foundational to quantum theory, which describes the behavior of matter and energy on very small scales, such as atoms and subatomic particles. Key aspects of quantization include: 1. **Energy Levels**: In quantum mechanics, systems like electrons in an atom can only occupy specific energy levels.
Quantum field theory 1970-01-01
Quantum Field Theory (QFT) is a fundamental theoretical framework that combines classical field theory, quantum mechanics, and special relativity. It describes how subatomic particles interact and behave as excitations or quanta of underlying fields that permeate space and time. Here are some key concepts: 1. **Fields**: In QFT, every type of particle is associated with a corresponding field. For example, electrons are excitations of the electron field, while photons are excitations of the electromagnetic field.
Quantum geometry 1970-01-01
Quantum geometry is a field of research that intersects quantum mechanics and geometry, focusing on the geometrical aspects of quantum theories. It seeks to understand the structure of spacetime at quantum scales and to explore how quantum principles affect the geometric properties of space and time. Here are some key concepts and areas associated with quantum geometry: 1. **Noncommutative Geometry**: Traditional geometry relies on the notion of points and continuous functions.
Quantum spacetime 1970-01-01
Quantum spacetime is a theoretical framework that seeks to reconcile the principles of quantum mechanics with the fabric of spacetime as described by general relativity. In classical physics, spacetime is treated as a smooth, continuous entity, where events occur at specific points in space and time. However, in quantum mechanics, the nature of reality is fundamentally probabilistic, leading to several challenges when trying to unify these two domains.
Quantum speed limit 1970-01-01
The quantum speed limit is a concept in quantum mechanics that sets a fundamental limit on how fast a quantum system can evolve from one state to another. It essentially describes the maximum rate at which quantum information can be processed or transmitted. The concept is analogous to the classical speed limit in physics, which governs how fast an object can move in space.
Quantum triviality 1970-01-01
Quantum triviality is a concept that arises in the context of quantum field theory, particularly in the study of certain types of quantum field theories and their behavior at different energy scales. The term often applies to theories that do not have the capacity to produce non-trivial dynamics or effective interactions in the quantum regime.
Radius of convergence 1970-01-01
The radius of convergence is a concept in mathematical analysis, particularly in the study of power series. It measures the range within which a power series converges to a finite value.
Random matrix 1970-01-01
A random matrix is a matrix whose elements are randomly generated according to some probability distribution. Random matrices are a central object of study in various fields, including mathematics, statistics, physics, and engineering, and they are used to model complex systems and phenomena in these areas.
Rarita–Schwinger equation 1970-01-01
The Rarita-Schwinger equation is a fundamental equation in theoretical physics that describes particles with spin 3/2, which are often referred to as "Rarita-Schwinger fields." It generalizes the Dirac equation, which describes spin-1/2 particles like electrons, to account for higher-spin fermionic fields. The equation is named after physicists Walter Rarita and Julian Schwinger, who introduced it in 1941.