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The spatially closed Friedmann-Lema\^{i}tre-Robertson-Walker model in loop quantum cosmology admits two inequivalent consistent quantizations: one based on expressing the field strength in terms of the holonomies over closed loops, and, another using a connection operator and open holonomies.
Phys. Rev. D68
P. Singh, M. Sami, and N. Dadhich, · 2003
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Phys. Rev. D69
P. Singh and A. Toporensky, · 2004
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K. A. Meissner, Class. Quant. Grav. 21
2004
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Class. Quant. Grav. 22
P. Singh, · 2005
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Phys. Rev. Lett. 96
A. Ashtekar, T. Pawlowski, and P. Singh, · 2006
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Phys. Rev. D73
A. Ashtekar, T. Pawlowski, and P. Singh, · 2006
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Phys. Rev. D74
A. Ashtekar, T. Pawlowski, and P. Singh, · 2006
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Phys. Rev. D74
M. Sami, P. Singh, and S. Tsujikawa, · 2006
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Phys. Rev. D73
P. Singh, · 2006
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Phys. Rev. D75
A. Ashtekar, T. Pawlowski, P. Singh, and K. Vandersloot, · 2007
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Class. Quant. Grav. 24
L. Szulc, W. Kaminski, and J. Lewandowski, · 2007
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Phys. Rev. D75
K. Vandersloot, · 2007
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C. G. Boehmer and K. Vandersloot, · 2007
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D. Samart and B. Gumjudpai, · 2007
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T. Naskar and J. Ward, · 2007
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Phys. Rev. D76
J. Magueijo and P. Singh, · 2007
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A. Corichi and P. Singh, · 2008
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E. Bentivegna and T. Pawlowski, · 2008
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V. Taveras, · 2008
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B. Gupt and P. Singh, · 2012
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P. Diener, B. Gupt, and P. Singh, · 2014
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E. Wilson-Ewing, · 2010
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A. Corichi and E. Montoya, · 2011
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A. Joe and P. Singh, · 2015
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The Vertex Expansion in the Consistent Histories Formulation of Spin Foam Loop Quantum Cosmology,
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