cosmological constant

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cosmological constant

The cosmological constant is represented by the Greek letter lambda in Einstein's field equations.

Definition
  1. Noun:
    • An arbitrary constant in the equations of general relativity theory: A term introduced by Albert Einstein into his field equations of general relativity to allow for a static universe. It represents a uniform energy density (or negative pressure) inherent to space itself, which can cause the universe to expand or contract.
Usage Examples
  • Noun:
    • Einstein originally introduced the cosmological constant to achieve a static model of the universe.
    • Modern observations suggest the cosmological constant may be the simplest explanation for dark energy, driving the accelerated expansion of the universe.
Advanced Usage
  • "The cosmological constant problem": Refers to the significant discrepancy between the observed small value of the cosmological constant and the much larger value predicted by quantum field theory.
    • The cosmological constant problem remains one of the greatest unsolved mysteries in theoretical physics.
Variants and Related Words
  • Lambda (Λ): The Greek letter commonly used as the symbol for the cosmological constant in equations.
    • In the Friedmann equations, Lambda represents the cosmological constant term.
Synonyms
  • Vacuum energy: A concept in quantum mechanics often conceptually linked to the cosmological constant, representing the energy of empty space.
  • Dark energy: In modern cosmology, the cosmological constant is the leading candidate model for the dark energy causing cosmic acceleration.
Related Phrases
  • "Cosmological constant term": The specific component in an equation representing this constant.
    • The cosmological constant term in Einstein's equation can be moved to the right-hand side and interpreted as a fluid with negative pressure.
cosmological constant

The cosmological constant is represented by the Greek letter lambda in Einstein's field equations.

Noun
  1. an arbitrary constant in the equations of general relativity theory