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Cosmological implications of the Higgs mass measurement
Open accessAbstract
We assume the validity of the standard model up to an arbitrary high-energy scale and discuss what information on the early stages of the Universe can be extracted from a measurement of the Higgs mass. For , the Higgs potential can develop an instability at large-field values. From the absence of excessive thermal Higgs field fluctuations we derive a bound on the reheat temperature after inflation as a function of the Higgs and top masses. Then we discuss the interplay between the quantum Higgs fluctuations generated during the primordial stage of inflation and the cosmological perturbations, in the context of landscape scenarios in which the inflationary parameters scan. We show that, within the large-field models of inflation, it is highly improbable to obtain the observed cosmological perturbations in a Universe with a light Higgs. Moreover, independently of the inflationary model, the detection of primordial tensor perturbations through the B mode of CMB polarization and the discovery of a light Higgs can simultaneously occur only with exponentially small probability, unless there is new physics beyond the standard model.
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“For the observed values of the SM parameters, the latter effect is dominant and thermal corrections do not destabilise the electroweak vacuum, even when the reheating temperature is close to the Planck scale [14].”
From The cosmological Higgstory of the vacuum instability (2015) · cites this paper as [14]
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“(28) At t = 0, which corresponds to the top quark mass scale mT , the Higgs quadratic coupling λ(0) and the top Yukawa coupling yt (0) are determined by the pole masses and the vacuum expectation value v: λ(0) = m 2 H 2v2 [1 + ΔH (mH )] , yt (0) = √ 2mT v [1 + ΔT (mT )] , (29) where ΔH (mH ) and ΔT (mT ) are the corre…”
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“in [3, 12, 13], can prevent the Higgs from falling into the instability region of the SM potential (through quantum fluctuations during inflation), provided that the coupling ξ satisfies ξ(μ = mt) & 10−2, depending on the concrete value of H.”
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BackgroundStandard Model Higgs Peaks: a note on the Vacuum Instability during Inflation
Franciolini, G., Kehagias, A., & Riotto, A. W. (2026) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2026/07/014 · Cited by 2
“If instead one considers the opposite regime in which classical evolution dominates, the probability distribution becomes independent of N , P ( h ) ∼ exp( − 8 π 2 V ( h ) / 3 H 4 ) [7] (the same result is obtained considering the Hawking-Moss bounce [21]).”
Self-citationNonminimal Higgs Inflation and Initial Conditions in Cosmology
Barvinsky, A. O., & Kamenshchik, A. Y. (2023) · Springer eBooks · doi:10.1007/978-981-19-3079-9_13-1 · Cited by 5
Gravity, Cosmology, and Astrophysics
Betti Hartmann, A., & Kunz, J. (2023) · Lecture notes in physics · doi:10.1007/978-3-031-42096-2 · Cited by 3
Primordial Black Holes and Higgs Vacuum Decay
Gregory, R. (2023) · Lecture notes in physics · doi:10.1007/978-3-031-42096-2_12 · Cited by 3
“…𝜙 = | Φ | , and the potential is expressed in terms of an effective quartic coupling constant 𝜆 eff , Radiative corrections have been computed [32, 35, 22, 6, 28], and in [16, 17], were approximated by the analytic three-parameter fit which provides a good approximation to the exact results…”
MethodGauguin's questions in particle physics: Where are we coming from? What are we? Where are we going?
Ellis, J. R. (2008) · Journal of Physics Conference Series · doi:10.1088/1742-6596/110/1/012001 · Cited by 2
Simple mass estimates for resonance(s) being 6 top + 6 antitop bound states and combinations thereof
Nielsen, H. B. (2016) · International Journal of Modern Physics A · doi:10.1142/s0217751x16501682 · Cited by 2
Higgs domain walls in the thermal background
Krajewski, T., Zygmunt Lalak, A., Lewicki, M., & Olszewski, P. (2019) · Physics of the Dark Universe · doi:10.1016/j.dark.2019.100347 · Cited by 2
“As shown by many authors [7, 26, 17, 27, 22] the dynamics of the Higgs field in the thermal state differs significantly from the case of the vacuum for large enough temperatures.”
BackgroundInfluentialDecoupling of Higgs boson from the inflationary stage of Universe evolutionPreprint
Kiselev, V. V., & Timofeev, S. A. (2009) · arXiv (Cornell University) · doi:10.48550/arxiv.0906.4191 · Cited by 2
“These effects could be effectively taken into account by making use of renormalization group in SM [28] with an appropriate choice of renormalization point at the inflation stage, so that the whole effect would be reduced to the running of λ(μ) with the scale μ.”
BackgroundHiggs mass from cosmological and astrophysical measurementsPreprint
Popa, L. A. (2009) · arXiv (Cornell University) · doi:10.48550/arxiv.0910.5312 · Cited by 2
Hints of BSM physics in the SM effective potentialPreprint
Zygmunt Lalak, A., Lewicki, M., & Olszewski, P. (2015) · arXiv (Cornell University) · doi:10.48550/arxiv.1505.05505 · Cited by 2
Jangid, S., & Okada, H. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.109.015001 · Cited by 1
Nonminimal Higgs Inflation and Initial Conditions in Cosmology
Barvinsky, A. O., & Kamenshchik, A. Y. (2024) · Springer eBooks · doi:10.1007/978-981-99-7681-2_13 · Cited by 1
Mihaila, L. N., & Steinhauser, M. (2015) · Nuclear and Particle Physics Proceedings · doi:10.1016/j.nuclphysbps.2015.03.026 · Cited by 1
Theoretical Implications of the Higgs Discovery
Miró, J. E. (2015) · TDX (Tesis Doctorals en Xarxa) · Cited by 1
Асимптотическая безопасность гравитации и масса бозона Хиггса
Shaposhnikov, M. (2012) · Теоретическая и математическая физика · doi:10.4213/tmf6766 · Cited by 1
NEW PHYSICS WITHOUT NEW ENERGY SCALE
Shaposhnikov, M. (2011) · International Conference on Physics Beyond the Standard Models of Particles, Cosmology and Astrophysics (BEYOND) · doi:10.1142/9789814340861_0021 · Cited by 1
Metadata
- Authors
- Espinosa, J. R., Giudice, G. F., & Riotto, A.
- Affiliations
- Consejo Superior de Investigaciones Científicas (ES)
- European Organization for Nuclear Research (CH)
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova (IT)
- ORCID
- Riotto, A
- Venue
- Journal of Cosmology and Astroparticle Physics
- Publisher
- IOP Publishing
- Published
- 2008-05-06
- Volume
- 2008
- Issue
- 05
- Pages
- 002
- ISSN
- 1475-7508 (ISSN-L)
- 1475-7516
- OpenAlex
- W2029441706
- Cited by
- 342
- References
- 70
- Citations by year
- 2026: 5 · 2025: 5 · 2024: 9 · 2023: 12 · 2022: 14 · 2021: 11 · 2020: 14 · 2019: 23 · 2018: 33 · 2017: 30 · 2016: 36 · 2015: 49 · 2014: 28 · 2013: 22 · 2012: 25
- FWCI
- 4.98
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Journal of Cosmology and Astroparticle Physics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Funders
- CERN
- Comunidad de Madrid (P-ESP-00346)
- European Commission (MRTN-CT-2004-503369, MRTN-CT-2006-035863)
- 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 › Noncommutative and Quantum Gravity Theories
- Keywords
- Higgs boson mass, early universe, reheating temperature, inflation (cosmology), cosmological perturbations, landscape scenarios, large-field inflation, primordial tensor perturbations, CMB B-modes, top quark mass, beyond the Standard Model
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