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  Hamiltonian cosmological perturbation theory with loop quantum gravity corrections

Bojowald, M., Hernandez, H. H., Kagan, M., Singh, P., & Skirzewski, A. (2006). Hamiltonian cosmological perturbation theory with loop quantum gravity corrections. Physical Review D, 74: 123512. Retrieved from http://scitation.aip.org/getabs/servlet/GetabsServlet?prog=normal&id=PRVDAQ000074000012123512000001&idtype=cvips&gifs=yes.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4C63-D Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4C64-B
Genre: Journal Article

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0609057.pdf (Preprint), 268KB
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 Creators:
Bojowald, Martin, Author
Hernandez, Hector H.1, Author
Kagan, Mikhail, Author
Singh, Parampreet, Author
Skirzewski, Aureliano1, Author
Affiliations:
1Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24014              

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 Abstract: Cosmological perturbation equations are derived systematically in a canonical scheme based on Ashtekar variables. A comparison with the covariant derivation and various subtleties in the calculation and choice of gauges are pointed out. Nevertheless, the treatment is more systematic when correction terms of canonical quantum gravity are to be included. This is done throughout the paper for one characteristic modification expected from loop quantum gravity.

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 Dates: 2006
 Publication Status: Published in print
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Title: Physical Review D
Source Genre: Journal
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Pages: - Volume / Issue: 74 Sequence Number: 123512 Start / End Page: - Identifier: -