Hamiltonian cosmological perturbation theory with loop quantum gravity 
corrections

Bojowald, Martin; Hernandez, Hector H.; Kagan, Mikhail; Singh, Parampreet; Skirzewski, Aureliano

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Hamiltonian cosmological perturbation theory with loop quantum gravity corrections

MPS-Authors

Hernandez, Hector H.
Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Skirzewski, Aureliano
Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

0609057.pdf
(Preprint), 268KB

prd74_123512.pdf
(Publisher version), 209KB

Supplementary Material (public)

There is no public supplementary material available

Citation

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.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-4C63-D

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.