TY - JOUR
T1 - Quantum nature of the big bang
AU - Ashtekar, Abhay
AU - Pawlowski, Tomasz
AU - Singh, Parampreet
PY - 2006
Y1 - 2006
N2 - Some long-standing issues concerning the quantum nature of the big bang are resolved in the context of homogeneous isotropic models with a scalar field. Specifically, the known results on the resolution of the big-bang singularity in loop quantum cosmology are significantly extended as follows: (i) the scalar field is shown to serve as an internal clock, thereby providing a detailed realization of the "emergent time" idea; (ii) the physical Hilbert space, Dirac observables, and semiclassical states are constructed rigorously; (iii) the Hamiltonian constraint is solved numerically to show that the big bang is replaced by a big bounce. Thanks to the nonperturbative, background independent methods, unlike in other approaches the quantum evolution is deterministic across the deep Planck regime.
AB - Some long-standing issues concerning the quantum nature of the big bang are resolved in the context of homogeneous isotropic models with a scalar field. Specifically, the known results on the resolution of the big-bang singularity in loop quantum cosmology are significantly extended as follows: (i) the scalar field is shown to serve as an internal clock, thereby providing a detailed realization of the "emergent time" idea; (ii) the physical Hilbert space, Dirac observables, and semiclassical states are constructed rigorously; (iii) the Hamiltonian constraint is solved numerically to show that the big bang is replaced by a big bounce. Thanks to the nonperturbative, background independent methods, unlike in other approaches the quantum evolution is deterministic across the deep Planck regime.
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U2 - 10.1103/PhysRevLett.96.141301
DO - 10.1103/PhysRevLett.96.141301
M3 - Article
C2 - 16712061
AN - SCOPUS:33645776283
SN - 0031-9007
VL - 96
JO - Physical review letters
JF - Physical review letters
IS - 14
M1 - 141301
ER -