Is it possible to create a universe in the laboratory by quantum tunneling?
Creators
- 1. Massachusetts Inst. of Tech., Cambridge (USA). Dept. of Physics
- 2. Massachusetts Inst. of Tech., Cambridge (USA). Center for Theoretical Physics
- 3. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)
- 4. Universidad Nacional Autonoma de Mexico, Mexico City (Mexico). Inst. de Ciencias Nucleares
Description
We explore the possibility that a new universe can be created by producing a small bubble of false vacuum. The initial bubble is small enough to be produced without an initial singularity, but classically it could not become a universe - instead it would reach a maximum radius and then collapse. We investigate the possibility that quantum effects allow the bubble to tunnel into a larger bubble, of the same mass, which would then classically evolve to become a new universe. The calculation of the tunneling amplitude is attempted, in lowest order semiclassical approximation (in the thin-wall limit), using both a canonical and a functional integral approach. The canonical approach is found to have flaws, attributable to our method of space-time slicing. The functional integral approach leads to a euclidean interpolating solution that is not a manifold. To describe it, we define an object which we call a 'pseudomanifold', and give a prescription to define its action. We conjecture that the tunneling probability to produce a new universe can be approximated using this action, and we show that this leads to a plausible result. (orig.)
Additional details
Publishing Information
- Journal Title
- Nuclear Physics B, Particle Physics
- Journal Volume
- 339
- Journal Issue
- 2
- Series
- Nucl. Phys. B, Part. Phys.
- Journal Page Range
- 417-490
- ISSN
- 0550-3213
- CODEN
- NUPBB
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 21088905
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACTION INTEGRAL; BUBBLES; CLASSICAL MECHANICS; COSMOLOGY; ENERGY-LEVEL TRANSITIONS; EQUATIONS OF MOTION; EUCLIDEAN SPACE; FEYNMAN PATH INTEGRAL; FIELD EQUATIONS; FUNCTIONAL ANALYSIS; HAMILTONIANS; INTERPOLATION; LAGRANGE EQUATIONS; LAGRANGIAN FIELD THEORY; MATHEMATICAL MANIFOLDS; METASTABLE STATES; QUANTUM MECHANICS; SCALAR FIELDS; SCHWARZSCHILD METRIC; SECOND QUANTIZATION; SEMICLASSICAL APPROXIMATION; SINGULARITY; SPACE-TIME; TRANSITION AMPLITUDES; TUNNEL EFFECT; UNIVERSE; VACUUM STATES
- Descriptors DEC
- AMPLITUDES; DIFFERENTIAL EQUATIONS; ENERGY LEVELS; EQUATIONS; EXCITED STATES; FIELD THEORIES; INTEGRALS; MATHEMATICAL OPERATORS; MATHEMATICAL SPACE; MATHEMATICS; MECHANICS; METRICS; NUMERICAL SOLUTION; PARTIAL DIFFERENTIAL EQUATIONS; QUANTIZATION; QUANTUM FIELD THEORY; QUANTUM OPERATORS; RIEMANN SPACE; SPACE
Optional Information
- Contract/Grant/Project number
- Contract DE-AC02-76ER03069; Grant NAGW-533