The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Equilibrium state of a self-interacting scalar field in the de Sitter background
Open accessAbstract
The behavior of a weakly self-interacting scalar field with a small mass in the de Sitter background is investigated using the stochastic approach (including the case of a double-well interaction potential). The existence of the de Sitter-invariant equilibrium quantum state of the scalar field in the presence of the interaction is shown for any sign of the mass term. The stochastic approach is further developed to produce a method of calculating an arbitrary anomalously large correlation function of the scalar field in the de Sitter background, and expressions for the two-point correlation function in the equilibrium state, correlation time, and spatial physical correlation radius are presented. The latter does not depend on time, which implies that the characteristic size of domains with positive and negative values of the scalar field remains the same on average in the equilibrium state in spite of the expansion of the t=const hypersurface of the de Sitter space-time.
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the absence of a large Higgs mass term, the evolution of the long wavelength modes of the h field is controlled by the Langevin equation.
“In the absence of a large Higgs mass term, the evolution of the long wavelength modes of the h field is controlled by the Langevin equation [48]”
From The cosmological Higgstory of the vacuum instability (2015) · cites this paper as [48]
Citations
Cites
Birth of inflationary universes
Vilenkin, A. (1983) · Physical Review D · doi:10.1103/physrevd.27.2848 · Cited by 998
Supercooled phase transitions in the very early universe
Hawking, S. W., & Moss, I. L. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)90946-7 · Cited by 816
Flagged first, then by citations
Research works printed but not linked: 24
- N. A. Chernikov, 1968, Ann. Inst. Henri Poincaré, 9A, 109
- E. A. Tagirov, 1973, Ann. Phys. (N.Y.), 76, 561, 10.1016/0003-4916(73)90047-X · DOI
- T. S. Bunch, 1978, Proc. R. Soc. London, A360, 117, 10.1098/rspa.1978.0060 · DOI
- A. D. Linde, 1982, Phys. Lett., 116B, 335, 10.1016/0370-2693(82)90293-3 · DOI
- A. A. Starobinsky, 1982, Phys. Lett., 117B, 175, 10.1016/0370-2693(82)90541-X · DOI
- A. Vilenkin, 1982, Phys. Rev. D, 26, 1231, 10.1103/PhysRevD.26.1231 · DOI
- B. Allen, 1985, Phys. Rev. D, 32, 3136, 10.1103/PhysRevD.32.3136 · DOI
- G. W. Gibbons, 1977, Phys. Rev. D, 15, 2738, 10.1103/PhysRevD.15.2738 · DOI · Paper page
- M. Sasaki, 1993, Class. Quantum Grav., 10, L55, 10.1088/0264-9381/10/5/003 · DOI
- H. Suzuki, 1994, Int. J. Mod. Phys. A, 9, 221, 10.1142/S0217751X9400011X · DOI
- A. A. Starobinsky, 1984, Fundamental Interactions
- A. A. Starobinsky, 1986, Field Theory, Quantum Gravity and Strings
- F. Cooper, 1994, Phys. Rev. D, 50, 2848, 10.1103/PhysRevD.50.2848 · DOI
- A. S. Goncharov, 1987, Sov. Phys. JETP, 65, 635
- A. S. Goncharov, 1987, Int. J. Mod. Phys. A, 2, 561, 10.1142/S0217751X87000211 · DOI · Paper page
- M. Sasaki, 1988, Phys. Lett. B, 209, 197, 10.1016/0370-2693(88)90932-X · DOI
- K. Nakao, 1988, Prog. Theor. Phys., 80, 1041, 10.1143/PTP.80.1041 · DOI
- M. Mijić, 1990, Phys. Rev. D, 42, 2469, 10.1103/PhysRevD.42.2469 · DOI
- H. Risken, 1984, The Fokker Planck Equation, 10.1007/978-3-642-96807-5 · DOI
- D. H. Lyth, 1992, Phys. Rev. D, 46, 532, 10.1103/PhysRevD.46.532 · DOI
- L. D. Landau, 1965, Quantum Mechanics, 2nd ed.
- A. D. Linde, 1994, Phys. Lett. B, 327, 208, 10.1016/0370-2693(94)90719-6 · DOI
- A. D. Linde, 1994, Phys. Rev. D, 50, 2456, 10.1103/PhysRevD.50.2456 · DOI
- A. Vilenkin, 1994, Phys. Rev. Lett., 72, 3137, 10.1103/PhysRevLett.72.3137 · DOI
Cited by
Sorted by citations
The cosmological Higgstory of the vacuum instability
Espinosa, J. R., Giudice, G. F., Morgante, E., Riotto, A., Senatore, L., Strumia, A., & Tetradis, N. (2015) · Journal of High Energy Physics · doi:10.1007/jhep09(2015)174 · Cited by 247
Nonlocal Models of Cosmic Acceleration
Woodard, R. P. (2014) · Foundations of Physics · doi:10.1007/s10701-014-9780-6 · Cited by 127
Is a Higgs vacuum instability fatal for high-scale inflation?
Kearney, J., Yoo, H., & Zurek, K. M. (2015) · Physical Review D · doi:10.1103/physrevd.91.123537 · Cited by 97
Metadata
- Authors
- Starobinsky, A. A., & Yokoyama, J.
- Affiliations
- Landau Institute for Theoretical Physics (RU)
- Kyoto University (JP)
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1994-11-15
- Volume
- 50
- Issue
- 10
- Pages
- 6357-6368
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2595209810
- Cited by
- 809
- References
- 2
- Citations by year
- 2026: 40 · 2025: 57 · 2024: 62 · 2023: 60 · 2022: 57 · 2021: 45 · 2020: 61 · 2019: 50 · 2018: 62 · 2017: 33 · 2016: 40 · 2015: 35 · 2014: 21 · 2013: 22 · 2012: 32
- FWCI
- 0.49
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Noncommutative and Quantum Gravity Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Keywords
- self-interacting scalar field, de Sitter space, stochastic approach, double-well potential, two-point correlation function, correlation time, correlation radius, de Sitter expansion
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.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review