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Assigning Quantum-Mechanical Initial Conditions to Cosmological Perturbations
Quantum-mechanical initial conditions for the fluctuations of the geometry can be assigned in excess of a given physical wavelength. The two-point functions of the scalar and tensor modes of the geometry will then inherit corrections depending on which Hamiltonian is minimized at the initial stage o...
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| Lenguaje: | eng |
| Publicado: |
2003
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| Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/20/24/016 http://cds.cern.ch/record/636603 |