2012
DOI: 10.1103/physrevlett.108.021301
|View full text |Cite
|
Sign up to set email alerts
|

Quantum Gravitational Contributions to the Cosmic Microwave Background Anisotropy Spectrum

Abstract: We derive the primordial power spectrum of density fluctuations in the framework of quantum cosmology. For this purpose we perform a Born-Oppenheimer approximation to the Wheeler-DeWitt equation for an inflationary universe with a scalar field. In this way, we first recover the scale-invariant power spectrum that is found as an approximation in the simplest inflationary models. We then obtain quantum gravitational corrections to this spectrum and discuss whether they lead to measurable signatures in the cosmic… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

11
171
0

Year Published

2013
2013
2022
2022

Publication Types

Select...
6
3

Relationship

1
8

Authors

Journals

citations
Cited by 125 publications
(182 citation statements)
references
References 25 publications
11
171
0
Order By: Relevance
“…For example, applications of the covariant theory lead to detailed predictions for the cross sections of various scattering processes [8], but such phenomena (if any) occur at energy scales inaccessible to observations, and also the effects of Planck-scale physics on cosmology, e.g., the cosmic microwave background radiation and its anisotropy spectrum [9][10][11][12][13], are not yet easily accessible to observations, although cosmology offers possibly the best chances for testing quantum gravity [14].…”
Section: Introductionmentioning
confidence: 99%
“…For example, applications of the covariant theory lead to detailed predictions for the cross sections of various scattering processes [8], but such phenomena (if any) occur at energy scales inaccessible to observations, and also the effects of Planck-scale physics on cosmology, e.g., the cosmic microwave background radiation and its anisotropy spectrum [9][10][11][12][13], are not yet easily accessible to observations, although cosmology offers possibly the best chances for testing quantum gravity [14].…”
Section: Introductionmentioning
confidence: 99%
“…We observe that if one identifies Ψ = e ī h S , with S given by (17), and substitutes in Eq. (1) the results (18) and (19) …”
Section: Geometrodynamical Approachmentioning
confidence: 99%
“…The first geometrodynamical approach by Brizuela, Kiefer and Kramer (henceforth BKK) [16,17] is examined in detail in Section 2, in particular with the aim of comparing it with our, above mentioned, traditional BO method which, in contrast, does not suffer from unitarity violating difficulties.…”
Section: Introductionmentioning
confidence: 99%
“…Following the approach presented in [10,11], and also used in [12,13], the next step of the analysis involves a power expansion in the inverse of the squared Planck mass m 2 P . At leading order, one recovers the Hamilton-Jacobi equation, which encodes the classical dynamics of the system.…”
Section: Quantization and Semiclassical Approximationmentioning
confidence: 99%