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The flat FRW model coupled to the massless scalar field according to the improved, background scale independent version of Ashtekar, Pawlowski and Singh is considered.
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Kato T 1980, Perturbation Theory for Linear Operators, (Springer-Verlag)
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Bojowald M 2001, Loop quantum cosmology: III. Wheeler-DeWitt operators, Class. Quantum Grav. 18
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Rovelli C 2004, Quantum Gravity, (Cambridge Cambridge University Press) Thiemann T, Introduction to Modern Canonical Quantum General Relativity (Cambridge: Cambridge University Press), Ashtekar A and Lewandowski J 2004, Background independent quantum gravity: A status report, Class. Quant. Grav. 21
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Ashtekar A, Pawłowski T and Singh P 2006, Quantum Nature of Big Bang: Improved dynamics, Phys. Rev. D 7
2006
Cited alongside, same era.
Kamiński W, Lewandowski J, Pawłowski T and Szulc Ł 2006, Properties of the scalar constraint operator in LQC models, in preparation
2006
Cited alongside, same era.
Ashtekar A, Pawłowski T, Vandersloot K and Singh P 2006 Loop quantum cosmology of k = 1 k=1 FRW models 2007 Phys.Rev. D
2007
Cited alongside, same era.
Vandersloot K 2006, Loop quantum cosmology and the k = - 1 RW model, Preprint gr-qc/0612070 Szulc L 2007 Open FRW model in Loop Quantum Cosmology, gr-qc/0612101
2007
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Astekar A, Corichi A, Singh P 2007, contributed talk at IGC Inaugural Conference Aug 9-11, 2007, Penn State
2007
Closest in time.
Pawłowski T, contributed talk at IGC Inaugural Conference Aug 9-11, 2007, Penn State
2007
Closest in time.
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