Wheeler-DeWitt equation

by Google AI

Wheeler-DeWitt equation is a fundamental equation in quantum gravity that describes the wave function of the universe, but it is “timeless” because it lacks an explicit time variable, which creates the “problem of time” in physics. This means the equation doesn’t inherently describe how a system changes over time, leading to challenges in understanding the transition from quantum to classical physics or how change occurs. Physicists are working on ways to resolve this by introducing a time-dependent description through various methods, such as using an “intrinsic time” or other formalisms to recover a sense of evolution. 

The timeless nature of the equation 

  • The Wheeler-DeWitt equation is derived from the Hamiltonian formulation of general relativity, and one of its key features is a constraint equation.
  • When the Hamiltonian operator is applied to the wave function of the universe, the result is zero, meaning the equation has no explicit time variable.
  • This is different from the Schrödinger equation in standard quantum mechanics, which clearly shows how a wave function evolves over time. 

The “problem of time” 

  • The lack of a time variable is known as the “problem of time” in quantum gravity, and it makes it difficult to connect the timeless Wheeler-DeWitt equation to our experience of a dynamic, evolving universe.
  • It implies that there is no universal clock or mechanism for change built into the fundamental equations. 

Current approaches to introduce time 

  • Introduce an intrinsic time: Some approaches reintroduce time by defining an “intrinsic time” from the gravitational field itself.
  • Use specific approximations: The Wheeler-DeWitt equation can be combined with approximations, like the WKB ansatz, to extract a time-dependent description from the timeless equation.
  • Alternative formulations: Researchers are developing new formalisms, such as the “Chronon-Adapted Wheeler-DeWitt Formalism,” to embed an intrinsic time function into the equation and recover a time-dependent description.
  • Relate it to boundary conditions: In some models, time evolution is not governed by the equation itself but by the boundary conditions of the universe, as discussed in studies of path integrals for quantum gravity. 

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