The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model
In the extended scalar sector of the SMASH (Standard Model - Axion-Seesaw-Higgs portal inflation) framework, we conduct a phenomenological investigation of the observable effects. In a suitable region of the SMASH scalar parameter spaces, we solve the vacuum metastability problem and discuss the one...
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author | C.R. Das Katri Huitu Timo J. Kärkkäinen |
author_facet | C.R. Das Katri Huitu Timo J. Kärkkäinen |
author_sort | C.R. Das |
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description | In the extended scalar sector of the SMASH (Standard Model - Axion-Seesaw-Higgs portal inflation) framework, we conduct a phenomenological investigation of the observable effects. In a suitable region of the SMASH scalar parameter spaces, we solve the vacuum metastability problem and discuss the one-loop correction to the triple Higgs coupling, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mrow><mi>H</mi><mi>H</mi><mi>H</mi></mrow></msub></semantics></math></inline-formula>. The <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mrow><mi>H</mi><mi>H</mi><mi>H</mi></mrow></msub></semantics></math></inline-formula> and SM Higgs quartic coupling <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mi>H</mi></msub></semantics></math></inline-formula> corrections are found to be proportional to the threshold correction. A large <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mrow><mi>H</mi><mi>H</mi><mi>H</mi></mrow></msub></semantics></math></inline-formula> correction (≳5%) implies vacuum instability in the model and thus limits the general class of theories that use threshold correction. We performed a full two-loop renormalization group analysis of the SMASH model. The SMASH framework has also been used to estimate the evolution of lepton asymmetry in the universe. |
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spelling | doaj.art-752f0151584b4722bfed9a5b2cfb2cec2023-12-01T00:59:23ZengMDPI AGUniverse2218-19972023-01-01914310.3390/universe9010043The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) ModelC.R. Das0Katri Huitu1Timo J. Kärkkäinen2Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research – International Intergovernmental Organization, Joliot-Curie 6, 141980 Dubna, Moscow Region, RussiaDepartment of Physics and Helsinki Institute of Physics, University of Helsinki, P.O. Box 64, FI-00014 Helsinki, FinlandLaboratory of High Energy and Computational Physics, National Institute of Chemical Physics and Biophysics, Rävala 10, 10143 Tallinn, EstoniaIn the extended scalar sector of the SMASH (Standard Model - Axion-Seesaw-Higgs portal inflation) framework, we conduct a phenomenological investigation of the observable effects. In a suitable region of the SMASH scalar parameter spaces, we solve the vacuum metastability problem and discuss the one-loop correction to the triple Higgs coupling, <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mrow><mi>H</mi><mi>H</mi><mi>H</mi></mrow></msub></semantics></math></inline-formula>. The <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mrow><mi>H</mi><mi>H</mi><mi>H</mi></mrow></msub></semantics></math></inline-formula> and SM Higgs quartic coupling <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mi>H</mi></msub></semantics></math></inline-formula> corrections are found to be proportional to the threshold correction. A large <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>λ</mi><mrow><mi>H</mi><mi>H</mi><mi>H</mi></mrow></msub></semantics></math></inline-formula> correction (≳5%) implies vacuum instability in the model and thus limits the general class of theories that use threshold correction. We performed a full two-loop renormalization group analysis of the SMASH model. The SMASH framework has also been used to estimate the evolution of lepton asymmetry in the universe.https://www.mdpi.com/2218-1997/9/1/43Higgs portal inflationbeyond the standard modelSMASHHiggs triple couplingHiggs trilinear coupling |
spellingShingle | C.R. Das Katri Huitu Timo J. Kärkkäinen The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model Universe Higgs portal inflation beyond the standard model SMASH Higgs triple coupling Higgs trilinear coupling |
title | The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model |
title_full | The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model |
title_fullStr | The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model |
title_full_unstemmed | The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model |
title_short | The Higgs Trilinear Coupling and the Scale of New Physics for the SM-Axion-Seesaw-Higgs Portal Inflation (SMASH) Model |
title_sort | higgs trilinear coupling and the scale of new physics for the sm axion seesaw higgs portal inflation smash model |
topic | Higgs portal inflation beyond the standard model SMASH Higgs triple coupling Higgs trilinear coupling |
url | https://www.mdpi.com/2218-1997/9/1/43 |
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