The DOI matches its Crossref record; 9 of the 9 references it cites were found in a registry or an index.
Scalar fields in cosmology with an exponential potential
Overview
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Citations
Cites
Linde, A. D. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)91219-9 · Cited by 6,405
Radiative Corrections as the Origin of Spontaneous Symmetry Breaking
Coleman, S., & Weinberg, E. (1973) · Physical Review D · doi:10.1103/physrevd.7.1888 · Cited by 4,263
Lucchin, F., & Matarrese, S. (1985) · Physical Review D · doi:10.1103/physrevd.32.1316 · Cited by 883
Chiral compactification on Minkowski × S2 of N = 2 Einstein-Maxwell supergravity in six dimensions
Salam, A., & Sezgin, E. (1984) · Physics Letters B · doi:10.1016/0370-2693(84)90589-6 · Cited by 282
Inflationary stages in cosmological models with a scalar field
Belinsky, V. A., Grishchuk, L. P., Khalatnikov, I. M., & Zeldovich, Y. B. (1985) · Physics Letters B · doi:10.1016/0370-2693(85)90644-6 · Cited by 247
Maeda, K., & Nishino, H. (1985) · Physics Letters B · doi:10.1016/0370-2693(85)90409-5 · Cited by 69
An attractor universe in six-dimensional N = 2 supergravity Kaluza-Klein theory
Maeda, K., & Nishino, H. (1985) · Physics Letters B · doi:10.1016/0370-2693(85)90437-x · Cited by 53
Cosmological evolution of degenerate vacua
Gibbons, G. W., & Townsend, P. K. (1987) · Nuclear Physics B · doi:10.1016/0550-3213(87)90700-0 · Cited by 44
A quantum cosmological approach to Kaluza-Klein theory and the boundary condition of 'no boundary'
Carow-Watamura, U., Inami, T., & Watamura, S. (1987) · Classical and Quantum Gravity · doi:10.1088/0264-9381/4/1/006 · Cited by 11
Cited by
Cosmological consequences of a rolling homogeneous scalar field
Ratra, B., & Peebles, P. J. E. (1988) · Physical Review D · doi:10.1103/physrevd.37.3406 · Cited by 4,310
Theory of cosmological perturbations
Mukhanov, V (1992) · Physics Reports · doi:10.1016/0370-1573(92)90044-z · Cited by 3,608
Exponential potentials and cosmological scaling solutions
Copeland, E. J., Liddle, A. R., & Wands, D. (1998) · Physical Review D · doi:10.1103/physrevd.57.4686 · Cited by 1,468
Linde, A. (1994) · Physical Review D · doi:10.1103/physrevd.49.748 · Cited by 1,314
Cosmology with a primordial scaling field
Ferreira, P. G., & Joyce, M. (1998) · Physical Review D · doi:10.1103/physrevd.58.023503 · Cited by 894
Metadata
- Authors
- Halliwell, J. J.
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 1987-02
- Volume
- 185
- Issue
- 3-4
- Pages
- 341-344
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2092554079
- Cited by
- 573
- References
- 9
- FWCI
- 17.30
- Type
- journal article
- Language
- en
- Open access
- closed
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Scalar fields in cosmology with an exponential potential. https://app.cochat.ai/papers/10.1016/0370-2693(87)91011-2
- The paper
- Halliwell, J. J. (1987). Scalar fields in cosmology with an exponential potential. Physics Letters B. https://doi.org/10.1016/0370-2693(87)91011-2
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.
