The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
Backreaction Problem for Cosmological Perturbations
Open accessAbstract
We derive the effective energy-momentum tensor for cosmological perturbations and prove its gauge invariance. The result is applied to study the influence of perturbations on the behavior of the Friedmann background in inflationary universe scenarios. We found that the back reaction of cosmological perturbations on the background can become important already at energies below the self-reproduction scale.
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Cites
Dynamical Theory of Groups and Fields
DeWitt, B. S., & Mullin, A. A. (1966) · American Journal of Physics · doi:10.1119/1.1953053 · Cited by 1,634
Cited by
Gauge-invariant perturbations at second order: multiple scalar fields on large scales
Malik, K. A. (2005) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2005/11/005 · Cited by 72
Conservation of second-order cosmological perturbations in a scalar field dominated universe
Vernizzi, F. (2005) · Physical Review D · doi:10.1103/physrevd.71.061301 · Cited by 57
Instability of de Sitter spacetime induced by quantum conformal anomaly
Matsui, H. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/01/003 · Cited by 18
Can backreaction prevent eternal inflation?
Brandenberger, R., Costa, R., & Franzmann, G. (2015) · Physical Review D · doi:10.1103/physrevd.92.043517 · Cited by 10
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Metadata
- Authors
- Mukhanov, V. F., Abramo, L. R. W., & Brandenberger, R. H.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 1997-03-03
- Volume
- 78
- Issue
- 9
- Pages
- 1624-1627
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W1568178795
- Cited by
- 307
- References
- 1
- FWCI
- 6.25
- Type
- journal article
- Language
- en
- Open access
- green
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