The DOI matches its Crossref record.
First-order phase transition of a vacuum and the expansion of the Universe
Open accessAbstract
The progress of a first-order phase transition of a vacuum in the expanding Universe is investigated. The expansion of bubbles of a stable vacuum is calculated simultaneously with the cosmic expansion with the aid of the following two simplified nucleation rates of bubbles p: (i) p = pT Tcδ (T−Tc) in the hot Universe models, (ii) p = 0 for n > nc and p = pQ for n < nc in the cold Universe models, where T is the cosmic temperature, Tc the critical temperature, n the cosmic number density of the fermions coupled to the order parameter of the vacuum, nc the critical density, and pT and pQ are parameters. The following results are obtained: (1) If the nucleation rates are small and the vacuum stays at the metastable state for a long time, the Universe begins to expand exponentially. As a result, the progress of the phase transition is delayed more and more by the rapid cosmic expansion. In particular, in model (i), if pT is less than a critical value, the phase transition never finishes. (2) The lower limits of the nucleation parameter pT and pQ are obtained from observation of the number ratio of photons to baryons in the present Universe. (3) If the phase transition of the vacuum in SU(5) GUT is of first order or if there exists a hypothetical first-order phase transition of the vacuum in the very early stage in which baryon number is not conserved, the density and the velocity fluctuations created by the phase transition may account for the origin of galaxies.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
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?
The check wasn’t confident either way, so it gives no verdict — never disputed.
In the citing paper
“However, our universe, created by a single inflation event, likely includes more than 10100 Sun-like stars.”
From Emergence of life in an inflationary universe (2020) · cites this paper as [38]
Experimental — accuracy not yet measured
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
The publisher hasn’t deposited this paper’s reference list.
Research works printed but not linked: 4
- Kolb, E. W. & Wolfram, S., 1979. Preprint OAP-579.
- Press, W. H. & Vishniac, E. T., 1980. Harvard Univ. Preprint-1232.
- Weinberg, S., 1972. Gravitation and Cosmology, Wiley, New York.
- Weinberg, S., 1979. Lecture in the Symposium on the Universe at Large Redshift, Copenhagen, June.
Cited by
Sorted by citations
Items 101–200 of 1,001
Anisotropic power-law inflation
Kanno, S., Soda, J., & Watanabe, M.-A. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/12/024 · Cited by 173
Inflaton decay in supergravity
Endo, M., Takahashi, F., & Yanagida, T. T. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.083509 · Cited by 182
Quantum Brownian motion in a bath of parametric oscillators: A model for system-field interactions
Hu, B. L., & Matacz, A. (1994) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.49.6612 · Cited by 150
ALTERNATIVES TO THE INFLATIONARY PARADIGM OF STRUCTURE FORMATION
Brandenberger, R. (2011) · International Journal of Modern Physics Conference Series · doi:10.1142/s2010194511000109 · Cited by 150
Cosmological Magnetic Field: A Fossil of Density Perturbations in the Early Universe
Ichiki, K., Takahashi, K., Ohno, H., Hanayama, H., & Sugiyama, N. (2006) · Science · doi:10.1126/science.1120690 · Cited by 150
0 One-loop corrections to a scalar field during inflationPreprint
Seery, D. (2007) · Cited by 163
Exploring cosmic origins with CORE: Inflation
Finelli, F., Bucher, M., Achúcarro, A., Ballardini, M., Bartolo, N., Baumann, D., Clesse, S., Errard, J., Handley, W. J., Hindmarsh, M. B., et al. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/04/016 · Cited by 204
On perturbations of a quintom bounce
Cai, Y.-F., Qiu, T., Brandenberger, R., Piao, Y.-S., & Zhang, X. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/03/013 · Cited by 166
STRING GAS COSMOLOGY AND STRUCTURE FORMATION
Brandenberger, R., Nayeri, A., Patil, S. P., & Vafa, C. (2007) · International Journal of Modern Physics A · doi:10.1142/s0217751x07037159 · Cited by 148
“It is instructive to compare the background evolution of string gas cosmology with the background of inflationary cosmology [26, 27], the current paradigm of early Universe evolution.”
Dark Energy: Investigation and Modeling
Tsujikawa, S. (2011) · Astrophysics and space science library · doi:10.1007/978-90-481-8685-3_8 · Cited by 213
Non-commutative inflation and the CMB
Tsujikawa, S., Maartens, R., & Brandenberger, R. (2003) · Physics Letters B · doi:10.1016/j.physletb.2003.09.022 · Cited by 147
Bianchi type III models with anisotropic dark energyPreprint
Akarsu, Ö., & Kılınç, C. B. (2012) · Cited by 157
Ratra, B., & Peebles, P. J. E. (1995) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.52.1837 · Cited by 141
Saito, R., Jun’ichi Yokoyama, B., & Nagata, R. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/06/024 · Cited by 152
Martin, J., & Vennin, V. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.023505 · Cited by 139
Curvature perturbation spectrum in two-field inflation with a turning trajectory
Pi, S., & Sasaki, M. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/10/051 · Cited by 139
Two field matter bounce cosmology
Cai, Y.-F., McDonough, E., Duplessis, F., & Brandenberger, R. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/10/024 · Cited by 138
One-loop corrections to the curvature perturbation from inflation
Seery, D. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/02/006 · Cited by 138
“For some years, the theory of inflation [1, 2, 3, 4, 5, 6, 7] has represented our most successful approach to the very early universe.”
BackgroundWarm inflation as a way out of the swampland
Motaharfar, M., Kamali, V., & Ramos, R. O. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.99.063513 · Cited by 138
Open EFTs, IR effects & late-time resummations: systematic corrections in stochastic inflation
Burgess, C. P., Holman, R., & Tasinato, G. (2016) · Journal of High Energy Physics · doi:10.1007/jhep01(2016)153 · Cited by 137
“Part of the appeal of inflationary models is their ability to explain these as vacuum fluctuations enormously stretched by universal expansion until writ large across the sky [1–8].”
Improved estimation of radiated axions from cosmological axionic strings
Hiramatsu, T., Kawasaki, M., Sekiguchi, T., Yamaguchi, M., & Yokoyama, J. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.123531 · Cited by 136
A matter bounce by means of ghost condensation
Lin, C., Brandenberger, R., & Perreault-Levasseur, L. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/04/019 · Cited by 135
Revisiting non-Gaussianity from non-attractor inflation models
Cai, Y.-F., Chen, X., Namjoo, M. H., Sasaki, M., Wang, D.-G., & Wang, Z. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/05/012 · Cited by 135
Non-Gaussianity and the induced gravitational wave background
Adshead, P. J., Lozanov, K. D., & Weiner, Z. J. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/10/080 · Cited by 135
The Dark Matter Crisis: Falsification of the Current Standard Model of CosmologyPreprint
Kroupa, P. (2012) · Cited by 134
Thermalization after/during reheating
Harigaya, K., & Mukaida, K. (2014) · Journal of High Energy Physics · doi:10.1007/jhep05(2014)006 · Cited by 134
“Tracing back the history of the Universe to the past, we encounter an era in which the energy density of the Universe is dominated by a potential energy of a scalar field, such as an inflaton [4–6], a curvaton [7–10], and a moduli field [11–13], and hence the Universe is expected to be far from thermal equilibrium.”
BackgroundHiggs inflation with loop corrections in the Palatini formulation
Räsänen, S., & Wahlman, L.-P. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/11/047 · Cited by 134
Supergravity-based inflation models: a review
Yamaguchi, M. (2011) · Classical and Quantum Gravity · doi:10.1088/0264-9381/28/10/103001 · Cited by 144
Multi-production of universes by first-order phase transition of a vacuum
Sato, K., Kodama, H., Sasaki, M., & Maeda, K.-I. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)91152-2 · Cited by 133
Self-citationBianchi Type-V Cosmology in f(R,T) Gravity with Λ(T)
Ahmed, N., & Pradhan, A. (2013) · International Journal of Theoretical Physics · doi:10.1007/s10773-013-1809-7 · Cited by 131
Limits on anisotropic inflation from the Planck data
Kim, J., & Komatsu, E. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.101301 · Cited by 130
Inflation in the mixed Higgs- R 2 model
He, M., Starobinsky, A. A., & Yokoyama, J. (2018) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2018/05/064 · Cited by 129
Primordial non-gaussianities in general modified gravitational models of inflation
Felice, A. D., & Tsujikawa, S. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/04/029 · Cited by 129
Quantum corrections to slow roll inflation and new scaling of superhorizon fluctuations
Boyanovsky, D., de Vega, H. J., & Sanchez, N. G. (2006) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2006.04.010 · Cited by 136
Inflationary Cosmology: Progress and Problems
Brandenberger, R. (2000) · Astrophysics and space science library · doi:10.1007/978-94-011-4175-8_4 · Cited by 205
One-loop corrections to a scalar field during inflation
Seery, D. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/11/025 · Cited by 128
“P 11(2007)025 Keywords: cosmological perturbation theory, inflation, quantum field theory on curved space, physics of the early universe ArXiv ePrint: 0707.3377 c©2007 IOP Publishing Ltd and SISSA 1475-7516/07/11025+32$30.00 JC A P 11(2007)025 Contents”
BackgroundInfluentialRenormalization group for nonrenormalizable theories: Einstein gravity with a scalar field
Barvinsky, A. O., Kamenshchik, A. Y., & Karmazin, I. P. (1993) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.48.3677 · Cited by 129
Difficulties with Inflationary Cosmology a
PENROSE, R. (1989) · Annals of the New York Academy of Sciences · doi:10.1111/j.1749-6632.1989.tb50513.x · Cited by 165
Relaxing cosmological tensions with a sign switching cosmological constant
Akarsu, Ö., Kumar, S., Özülker, E., & Vazquez, J. A. (2021) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.104.123512 · Cited by 125
LRS Bianchi Type I Models with Anisotropic Dark Energy and Constant Deceleration ParameterPreprint
Akarsu, Ö. (2012) · Cited by 144
Cosmic no-hair theorem in power-law inflation
Kitada, Y., & Maeda, K.-I. (1992) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.45.1416 · Cited by 128
Observational neutrino astrophysics
Koshiba, M. (1992) · Physics Reports · doi:10.1016/0370-1573(92)90083-c · Cited by 126
Initial conditions for inflation — A short review
Brandenberger, R. (2016) · International Journal of Modern Physics D · doi:10.1142/s0218271817400028 · Cited by 144
“The inflationary scenario provides a theory for the origin of structure in the universe which can explain CMB anisotropies and the distribution of galaxies on large scales [5] (see also [6, 7]).”
BackgroundAxion inflation with an SU(2) gauge field: detectable chiral gravity waves
Maleknejad, A. (2016) · Journal of High Energy Physics · doi:10.1007/jhep07(2016)104 · Cited by 122
Constraining Primordial Black Hole Formation from Single-Field Inflation
Kristiano, J., & Yokoyama, J. (2024) · Physical Review Letters · doi:10.1103/physrevlett.132.221003 · Cited by 138
Observational tests of inflation with a field derivative coupling to gravity
Tsujikawa, S. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.85.083518 · Cited by 124
Figueroa, D. G., Raatikainen, S., Räsänen, S., & Tomberg, E. (2021) · Physical Review Letters · doi:10.1103/physrevlett.127.101302 · Cited by 119
D-branes in standard model building, gravity and cosmology
KIRITSIS, E. B. (2005) · Physics Reports · doi:10.1016/j.physrep.2005.09.001 · Cited by 118
The Matter Bounce Alternative to Inflationary CosmologyPreprint
Brandenberger, R. (2012) · arXiv (Cornell University) · doi:10.48550/arxiv.1206.4196 · Cited by 229
“[7] K.”
BackgroundChallenges of the Standard Cosmological Model
Di Valentino, E. (2022) · Universe · doi:10.3390/universe8080399 · Cited by 125
Inhomogeneous baryogenesis, cosmic antimatter, and dark matter
Dolgov, A. D., Kawasaki, M., & Kevlishvili, N. (2008) · Nuclear Physics B · doi:10.1016/j.nuclphysb.2008.08.029 · Cited by 133
Non-Gaussianity in a matter bounce
Cai, Y.-F., Wei Xue, B., Brandenberger, R., & Zhang, X. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/05/011 · Cited by 125
Gravitational perturbations from oscillons and transients after inflation
Lozanov, K. D., & Amin, M. A. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.99.123504 · Cited by 114
Ultra-slow-roll inflation with quantum diffusion
Pattison, C., Vennin, V., Wands, D., & Assadullahi, H. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/04/080 · Cited by 114
Ccat Collaboration, Aravena, M., Austermann, J., Basu, K., Battaglia, N., Beringue, B., Bertoldi, F., Bigiel, F., Bond, J., Breysse, P., et al. (2021) · Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ac9838 · Cited by 92
“Inflation models predict a period of rapid expansion in the early universe (Guth 1981; Sato 1981; Albrecht & Steinhardt 1982; Linde 1982), and the generation of both scalar (Mukhanov & Chibisov 1981; Guth & Pi 1982; Hawking 1982; Starobinsky 1982; Bardeen et al. 1983) and tensor perturbations…”
BackgroundBartolo, N., & Orlando, G. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/07/034 · Cited by 113
Considerations in optimizing CMB polarization experiments to constrain inflationary physics
Verde, L., Peiris, H. V., & Jiménez, R. (2006) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2006/01/019 · Cited by 113
The art of simulating the early universe. Part I. Integration techniques and canonical cases
Figueroa, D. G., Florio, A., Torrentí, F., & Valkenburg, W. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/04/035 · Cited by 112
Nakama, T., Harada, T., Polnarev, A. G., & Yokoyama, J. (2014) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2014/01/037 · Cited by 112
Secondary anisotropies of the CMB
Aghanim, N., Majumdar, S., & Silk, J. I. (2008) · Reports on Progress in Physics · doi:10.1088/0034-4885/71/6/066902 · Cited by 108
“Most, and indeed the simplest, inflationary scenarios (e.g. Guth 1981, Sato 1981) predict that the temperature anisotropy field obeys Gaussian statistics to first order.”
BackgroundRevisiting non-Gaussianity from non-attractor inflation models
Cai, Y.-F., Chen, X., Namjoo, M. H., Sasaki, M., Wang, D.-G., & Wang, Z. (2018) · DSpace@MIT (Massachusetts Institute of Technology) · Cited by 108
Non-Gaussianity from the inflationary trispectrum
Seery, D., & Lidsey, J. E. (2007) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2007/01/008 · Cited by 108
“universe. Non-gaussianity from the inflationary trispectrum 2 1. Introduction Recent observations of the cosmic microwave background (CMB) have provided strong evidence [1, 2, 3] thatan era ofinflation [4,5, 6,7, 8,9, 10] occurred in the early history of the universe. During inflation, the universe underwent a phase of a…”
BackgroundPre-inflationary universe in loop quantum cosmology
Zhu, T., Wang, A., Cleaver, G., Kirsten, K., & Sheng, Q. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.083520 · Cited by 114
Natural inflation: consistency with cosmic microwave background observations of Planck and BICEP2
Katherine Freese, B., & Kinney, W. H. (2015) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2015/03/044 · Cited by 106
Large tensor non-Gaussianity from axion-gauge field dynamics
Agrawal, A., Fujita, T., & Komatsu, E. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.97.103526 · Cited by 106
Escrivà, A., Kühnel, F., & Tada, Y. (2024) · Elsevier eBooks · doi:10.1016/b978-0-32-395636-9.00012-8 · Cited by 149
Kamada, K., Kobayashi, T., Takahashi, T., Yamaguchi, M., & Yokoyama, J. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.86.023504 · Cited by 105
Planck constraints on single-field inflation
Tsujikawa, S., Ohashi, J., Kuroyanagi, S., & Felice, A. D. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.88.023529 · Cited by 105
Bounce inflation in f ( T ) cosmology: A unified inflaton-quintessence field
Bamba, K., NASHED, G. G. L., Hanafy, W. E., & Sh.K., I. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.94.083513 · Cited by 109
Inflation with multiple sound speeds: A model of multiple DBI type actions and non-Gaussianities
Cai, Y.-F., & Xia, H.-Y. (2009) · Physics Letters B · doi:10.1016/j.physletb.2009.05.047 · Cited by 107
Seery, D., Lidsey, J. E., & Sloth, M. S. (2006) · CERN Document Server (European Organization for Nuclear Research) · Cited by 102
The Beginning and Evolution of the Universe
Ratra, B., & Vogeley, M. S. (2008) · Publications of the Astronomical Society of the Pacific · doi:10.1086/529495 · Cited by 118
Measuring the spectrum of primordial gravitational waves with CMB, PTA and laser interferometers
Campeti, P., Komatsu, E., Poletti, D., & Baccigalupi, C. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/01/012 · Cited by 101
“The cosmic inflation paradigm [1–5] predicts the primordial Stochastic Background of Gravitational Waves (hereafter SGWB) [6, 7].”
BackgroundOn applications of Campbell's embedding theorem
Lidsey, J. E., Romero, C., Tavakol, R., & Rippl, S. (1997) · Classical and Quantum Gravity · doi:10.1088/0264-9381/14/4/005 · Cited by 106
Stochastic inflation in phase space: is slow roll a stochastic attractor?
Grain, J., & Vennin, V. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/05/045 · Cited by 113
Open EFTs, IR effects & late-time resummations: systematic corrections in stochastic inflation
Burgess, C. P. (2022) · OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) · doi:10.1007/jhep01%282016%29153 · Cited by 100
Inflation in generalized Einstein theories
Berkin, A. L., & Maeda, K.-I. (1991) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.44.1691 · Cited by 100
Inflation and nonminimal scalar-curvature coupling in gravity and supergravity
Ketov, S. V., & Starobinsky, A. A. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/08/022 · Cited by 98
Probing non-Gaussianities with the high frequency tail of induced gravitational waves
Atal, V., & Domènech, G. (2021) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2021/06/001 · Cited by 98
Brandenberger, R. (2009) · doi:10.1002/9783527628063.ch6 · Cited by 97
The Universe of General Relativity
Kox, A. J., & Eisenstaedt, J. (2005) · Birkhäuser Boston eBooks · doi:10.1007/0-8176-4454-7 · Cited by 100
Space-based gravitational-wave detectors can determine the thermal history of the early Universe
Nakayama, K., Saito, S., Suwa, Y., & Yokoyama, J. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.124001 · Cited by 97
Czerny, M., & Takahashi, F. (2014) · Physics Letters B · doi:10.1016/j.physletb.2014.04.039 · Cited by 107
Does string theory lead to extended inflation?
Campbell, B. A., Linde, A. D., & Olive, K. A. (1991) · Nuclear Physics B · doi:10.1016/0550-3213(91)90307-j · Cited by 96
A new algorithm for calculating the curvature perturbations in stochastic inflation
Fujita, T., Kawasaki, M., Tada, Y., & Takesako, T. (2013) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2013/12/036 · Cited by 112
Polynomial chaotic inflation in the Planck era
Nakayama, K., Takahashi, F., & Yanagida, T. T. (2013) · Physics Letters B · doi:10.1016/j.physletb.2013.06.050 · Cited by 97
Anomaly-induced inflaton decay and gravitino-overproduction problem
Endo, M., Takahashi, F., & Yanagida, T. T. (2007) · Physics Letters B · doi:10.1016/j.physletb.2007.09.019 · Cited by 110
Baryon asymmetry and gravitational waves from pseudoscalar inflation
Tejero, D. J., Kamada, K., Schmitz, K., & Xu, X.-J. (2017) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2017/12/011 · Cited by 95
Bouncing cosmological solutions from $$f(\mathsf{R,T})$$ f ( R , T ) gravity
Shabani, H., & Ziaie, A. H. (2018) · The European Physical Journal C · doi:10.1140/epjc/s10052-018-5886-x · Cited by 95
Palatini side of inflationary attractors
Järv, L., Racioppi, A., & Tenkanen, T. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.97.083513 · Cited by 99
Stochastic inflation beyond slow roll
Pattison, C., Vennin, V., Assadullahi, H., & Wands, D. (2019) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2019/07/031 · Cited by 95
Creation of Schwarzschild-de Sitter wormholes by a cosmological first-order phase transition
Maeda, K.-I., Sato, K., Sasaki, M., & Kodama, H. (1982) · Physics Letters B · doi:10.1016/0370-2693(82)91151-0 · Cited by 95
Self-citationCosmology of the Very Early Universe
Brandenberger, R., Dupke, R. A., Alcaniz, J. S., Reza, R. D. L., & Daflon, S. (2010) · AIP conference proceedings · doi:10.1063/1.3483879 · Cited by 100
“In the context of a Universe with a de Sitter phase, the quantum origin of cosmological fluctuations was first discussed in [5] and also [4, 6] for earlier ideas.”
BackgroundEvolution of metric perturbations in a model of nonsingular inflationary cosmology
Cai, Y.-F., & Zhang, X. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2009/06/003 · Cited by 107
The pseudo-conformal universe: scale invariance from spontaneous breaking of conformal symmetry
Hinterbichler, K., & Khoury, J. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/04/023 · Cited by 93
Eternal Inflation and the Refined Swampland Conjecture
Kinney, W. H. (2019) · Physical Review Letters · doi:10.1103/physrevlett.122.081302 · Cited by 96
Running spectral index from inflation with modulations
Kobayashi, T., & Takahashi, F. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/01/026 · Cited by 92
Primordial non-Gaussianity from G inflation
Kobayashi, T., Yamaguchi, M., & Yokoyama, J. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.83.103524 · Cited by 92
A complete FFT-based decomposition formalism for the redshift-space bispectrum
Sugiyama, N. S., Saito, S., Beutler, F., & Seo, H. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty3249 · Cited by 91
“1 IN T RO D U C T I O N In the current picture of structure formation, the standard theory of inflation (Starobinsky 1980; Guth 1981; Sato 1981; Albrecht & Steinhardt 1982; Linde 1982) predicts primordial density perturbations that are nearly Gaussian.”
BackgroundInflation with Gauss-Bonnet coupling
Yi, Z., Gong, Y., & Sabir, M. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.083521 · Cited by 91
Metadata
- Authors
- Sato, K.
- Affiliations
- Kyoto University (JP)
- Corresponding author
- Sato, K.
- ORCID
- Sato, K.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 1981-07-01
- Volume
- 195
- Issue
- 3
- Pages
- 467-479
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2118084428
- Semantic Scholar
- 4996c653cfb125af342b7f3f7a40e15311999ba7
- Cited by
- 1,792
- References
- 0
- Citations by year
- 2026: 57 · 2025: 101 · 2024: 102 · 2023: 91 · 2022: 110 · 2021: 95 · 2020: 91 · 2019: 114 · 2018: 94 · 2017: 86 · 2016: 92 · 2015: 94 · 2014: 93 · 2013: 53 · 2012: 46
- FWCI
- 12.39
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- HighWire Press Open Archive (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- first-order phase transition, vacuum phase transition, bubble nucleation, cosmic expansion, metastable vacuum, nucleation rate, critical temperature, SU(5) grand unification, baryon number violation, density fluctuations, galaxy formation, early universe
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